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hep-ph/0204147
Jusak Tandean
Jusak Tandean, S. Gardner
Nonresonant Contributions in B->rho pi Decay
15 pages, 3 figures; minor changes, version to appear in Phys. Rev. D
Phys.Rev.D66:034019,2002
10.1103/PhysRevD.66.034019
SLAC-PUB-9199, UK/TP-2002-05
hep-ph hep-ex
null
We consider nonresonant contributions in the Dalitz plot analysis of B->rho pi->pi^+ pi^- pi^0 decay and their potential impact on the extraction of the CKM parameter alpha. In particular, we examine the role of the heavy mesons B^* and B_0, via the process B->pi (B^*, B_0)->pi^+ pi^- pi^0, and their interference with resonant contributions in the rho-mass region. We discuss the inherent uncertainties and suggest that the effects may be substantially smaller than previously indicated.
[ { "created": "Mon, 15 Apr 2002 00:37:45 GMT", "version": "v1" }, { "created": "Mon, 22 Jul 2002 13:52:19 GMT", "version": "v2" } ]
2008-11-26
[ [ "Tandean", "Jusak", "" ], [ "Gardner", "S.", "" ] ]
We consider nonresonant contributions in the Dalitz plot analysis of B->rho pi->pi^+ pi^- pi^0 decay and their potential impact on the extraction of the CKM parameter alpha. In particular, we examine the role of the heavy mesons B^* and B_0, via the process B->pi (B^*, B_0)->pi^+ pi^- pi^0, and their interference with resonant contributions in the rho-mass region. We discuss the inherent uncertainties and suggest that the effects may be substantially smaller than previously indicated.
2010.09762
Satyanarayan Mukhopadhyay
Disha Bhatia, Satyanarayan Mukhopadhyay
Unitarity limits on thermal dark matter in (non-)standard cosmologies
21 pages, 10 figures; v2: minor additions to text, version as published in JHEP
JHEP03(2021)133
10.1007/JHEP03(2021)133
null
hep-ph astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Using the upper bound on the inelastic reaction cross-section implied by S-matrix unitarity, we derive the thermally averaged maximum dark matter (DM) annihilation rate for general $k \rightarrow 2$ number-changing reactions, with $k \geq 2$, taking place either entirely within the dark sector, or involving standard model fields. This translates to a maximum mass of the particle saturating the observed DM abundance, which, for dominantly $s$-wave annihilations, is obtained to be around $130$ TeV, $1$ GeV, $7$ MeV and $110$ keV, for $k=2,3,4$ and $5$, respectively, in a radiation dominated Universe, for a real or complex scalar DM stabilized by a minimal symmetry. For modified thermal histories in the pre-big bang nucleosynthesis era, with an intermediate period of matter domination, values of reheating temperature higher than $\mathcal{O}(200)$ GeV for $k \geq 4$, $\mathcal{O}(1)$ TeV for $k=3$ and $\mathcal{O}(50)$ TeV for $k=2$ are strongly disfavoured by the combined requirements of unitarity and DM relic abundance, for DM freeze-out before reheating.
[ { "created": "Mon, 19 Oct 2020 18:03:23 GMT", "version": "v1" }, { "created": "Mon, 15 Mar 2021 06:22:40 GMT", "version": "v2" } ]
2021-03-17
[ [ "Bhatia", "Disha", "" ], [ "Mukhopadhyay", "Satyanarayan", "" ] ]
Using the upper bound on the inelastic reaction cross-section implied by S-matrix unitarity, we derive the thermally averaged maximum dark matter (DM) annihilation rate for general $k \rightarrow 2$ number-changing reactions, with $k \geq 2$, taking place either entirely within the dark sector, or involving standard model fields. This translates to a maximum mass of the particle saturating the observed DM abundance, which, for dominantly $s$-wave annihilations, is obtained to be around $130$ TeV, $1$ GeV, $7$ MeV and $110$ keV, for $k=2,3,4$ and $5$, respectively, in a radiation dominated Universe, for a real or complex scalar DM stabilized by a minimal symmetry. For modified thermal histories in the pre-big bang nucleosynthesis era, with an intermediate period of matter domination, values of reheating temperature higher than $\mathcal{O}(200)$ GeV for $k \geq 4$, $\mathcal{O}(1)$ TeV for $k=3$ and $\mathcal{O}(50)$ TeV for $k=2$ are strongly disfavoured by the combined requirements of unitarity and DM relic abundance, for DM freeze-out before reheating.
2111.12156
Hugues Beauchesne
Hugues Beauchesne and Giovanni Grilli di Cortona
Event-level variables for semivisible jets using anomalous jet tagging
Contribution to Snowmass 2022, 16 pages, 8 figures
null
null
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Semivisible jets are a characteristic signature of many confining dark sectors and consist of jets of visible hadrons intermixed with invisible stable particles. Since their initial proposal, considerable progress has been made in developing techniques for tagging anomalous jets. In this paper, we show that the ability to tag semivisible jets can be used to define new event-level variables which use generally ignored kinematic information and can considerably increase our ability to discover dark confining sectors. In practice, our best results are obtained by using the coefficients of the decomposition of the missing transverse momentum in terms of the transverse momenta of the jets tagged as anomalous. A benchmark scenario is introduced and the increase in significance due to these new variables is studied over some of its parameter space.
[ { "created": "Tue, 23 Nov 2021 21:15:52 GMT", "version": "v1" } ]
2021-11-25
[ [ "Beauchesne", "Hugues", "" ], [ "di Cortona", "Giovanni Grilli", "" ] ]
Semivisible jets are a characteristic signature of many confining dark sectors and consist of jets of visible hadrons intermixed with invisible stable particles. Since their initial proposal, considerable progress has been made in developing techniques for tagging anomalous jets. In this paper, we show that the ability to tag semivisible jets can be used to define new event-level variables which use generally ignored kinematic information and can considerably increase our ability to discover dark confining sectors. In practice, our best results are obtained by using the coefficients of the decomposition of the missing transverse momentum in terms of the transverse momenta of the jets tagged as anomalous. A benchmark scenario is introduced and the increase in significance due to these new variables is studied over some of its parameter space.
1511.00683
Andrew Kobach
Andr\'e de Gouv\^ea, Andrew Kobach
Global Constraints on a Heavy Neutrino
19 pages, 13 figures, 3 tables. Typographical errors corrected, results and conclusions unchanged
Phys. Rev. D 93, 033005 (2016)
10.1103/PhysRevD.93.033005
NUHEP-TH/15-03
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We estimate constraints on the existence of a heavy, mostly sterile neutrino with mass between 10 eV and 1 TeV. We improve upon previous analyses by performing a global combination and expanding the experimental inputs to simultaneously include tests for lepton universality, lepton-flavor-violating processes, electroweak precision data, dipole moments, and neutrinoless double beta decay. Assuming the heavy neutrino and its decay products are invisible to detection, we further include, in a self-consistent manner, constraints from direct kinematic searches, the kinematics of muon decay, cosmology, and neutrino oscillations, in order to estimate constraints on the values of $|U_{e4}|^2$, $|U_{\mu4}|^2$, and $|U_{\tau4}|^2$.
[ { "created": "Mon, 2 Nov 2015 21:00:00 GMT", "version": "v1" }, { "created": "Mon, 9 Nov 2015 22:01:27 GMT", "version": "v2" }, { "created": "Fri, 12 Feb 2016 17:39:53 GMT", "version": "v3" } ]
2016-02-17
[ [ "de Gouvêa", "André", "" ], [ "Kobach", "Andrew", "" ] ]
We estimate constraints on the existence of a heavy, mostly sterile neutrino with mass between 10 eV and 1 TeV. We improve upon previous analyses by performing a global combination and expanding the experimental inputs to simultaneously include tests for lepton universality, lepton-flavor-violating processes, electroweak precision data, dipole moments, and neutrinoless double beta decay. Assuming the heavy neutrino and its decay products are invisible to detection, we further include, in a self-consistent manner, constraints from direct kinematic searches, the kinematics of muon decay, cosmology, and neutrino oscillations, in order to estimate constraints on the values of $|U_{e4}|^2$, $|U_{\mu4}|^2$, and $|U_{\tau4}|^2$.
1901.00157
Chung Kao
Rishabh Jain and Chung Kao
Charming Top Decays with Flavor Changing Neutral Higgs Boson and WW at Hadron Colliders
15 pages, 7 figures, version to appear in Physical Review D. arXiv admin note: text overlap with arXiv:1112.1707
Phys. Rev. D 99, 055036 (2019)
10.1103/PhysRevD.99.055036
OU-HEP-181222
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate the prospects for discovering a top quark decaying into one light Higgs boson ($h^0$) along with a charm quark ($c$) in top quark pair production at the CERN Large Hadron Collider (LHC) and future hadron colliers. A general two Higgs doublet model is adopted to study the signature of flavor changing neutral Higgs (FCNH) interactions with $t \to c h^0$, followed by $h^0 \to WW^* \to \ell^+ \ell^- +\notE_T$, where $h^0$ is the CP-even Higgs boson and $\notE_T$ stands for missing transverse energy from neutrinos. We study the discovery potential for this FCNH signal and physics background from dominant processes with realistic acceptance cuts as well as tagging and mistagging efficiencies. Promising results are found for the LHC running at 13 TeV and 14 TeV center-of-mass energy as well as future pp colliders at 27 TeV and 100 TeV.
[ { "created": "Tue, 1 Jan 2019 14:33:47 GMT", "version": "v1" }, { "created": "Wed, 27 Feb 2019 02:35:41 GMT", "version": "v2" } ]
2019-04-03
[ [ "Jain", "Rishabh", "" ], [ "Kao", "Chung", "" ] ]
We investigate the prospects for discovering a top quark decaying into one light Higgs boson ($h^0$) along with a charm quark ($c$) in top quark pair production at the CERN Large Hadron Collider (LHC) and future hadron colliers. A general two Higgs doublet model is adopted to study the signature of flavor changing neutral Higgs (FCNH) interactions with $t \to c h^0$, followed by $h^0 \to WW^* \to \ell^+ \ell^- +\notE_T$, where $h^0$ is the CP-even Higgs boson and $\notE_T$ stands for missing transverse energy from neutrinos. We study the discovery potential for this FCNH signal and physics background from dominant processes with realistic acceptance cuts as well as tagging and mistagging efficiencies. Promising results are found for the LHC running at 13 TeV and 14 TeV center-of-mass energy as well as future pp colliders at 27 TeV and 100 TeV.
hep-ph/9406342
null
D. Ghilencea, L. Micu
Structure Dependence in $\pi \to \bf\ell\nu, \pi\ to \ell\nu\gamma$ and $\pi^0\ to \gamma\gamma$ Decays
no. pages 16 + 6 pages with figures by request, LATEX
Phys.Rev. D52 (1995) 1577-1587
10.1103/PhysRevD.52.1577
IFA-FT-395-1994
hep-ph
null
The amplitudes of $\pi$-meson decays are calculated in a relativistic nonperturbative quark model which assumes that mesons are made of a quark antiquark pair and of a scalar neutral component representing the contribution of the nonelementary fluctuations of the quark gluonic field. The experimental data can be fitted in a satisfactory manner using current quark masses $m_u\approx1.5\ MeV, m_d\approx9\ MeV$.
[ { "created": "Mon, 20 Jun 1994 11:24:00 GMT", "version": "v1" } ]
2009-10-28
[ [ "Ghilencea", "D.", "" ], [ "Micu", "L.", "" ] ]
The amplitudes of $\pi$-meson decays are calculated in a relativistic nonperturbative quark model which assumes that mesons are made of a quark antiquark pair and of a scalar neutral component representing the contribution of the nonelementary fluctuations of the quark gluonic field. The experimental data can be fitted in a satisfactory manner using current quark masses $m_u\approx1.5\ MeV, m_d\approx9\ MeV$.
2302.07165
Harleen Dahiya Dr.
Shubham Sharma, Narinder Kumar and Harleen Dahiya
Sub-leading twist transverse momentum dependent parton distributions in the light-front quark-diquark model
37 Pages, 12 Figures, 6 Tables, accepted for publication in Nuclear Physics B, arXiv admin note: text overlap with arXiv:2301.09536
Nucl. Phys. B, 992, 116247 (2023)
10.1016/j.nuclphysb.2023.116247
null
hep-ph
http://creativecommons.org/licenses/by/4.0/
In this study, the T-even sub-leading twist transverse momentum dependent distributions (TMDs) of proton in the light-front quark-diquark model (LFQDM) have been investigated. We have derived the overlap form of the light-front wave functions (LFWFs) for the sub-leading twist proton TMDs by detangling the un-integrated quark-quark correlator for the semi-inclusive deep inelastic scattering (SIDIS). We have obtained the explicit expressions of TMDs for both the cases of the diquark being a scalar or a vector and analysed their relationships with leading twist TMDs within the same model. Average transverse momenta and average square transverse momenta for the TMDs have been tabulated and compared with the results from the light-front bag model and the light-front constituent quark model (LFCQM). In addition to this, we have also compared our results for the PDF $e(x)$ with the recent CLAS collaboration results.
[ { "created": "Tue, 14 Feb 2023 16:27:19 GMT", "version": "v1" }, { "created": "Thu, 25 May 2023 10:01:51 GMT", "version": "v2" } ]
2023-08-01
[ [ "Sharma", "Shubham", "" ], [ "Kumar", "Narinder", "" ], [ "Dahiya", "Harleen", "" ] ]
In this study, the T-even sub-leading twist transverse momentum dependent distributions (TMDs) of proton in the light-front quark-diquark model (LFQDM) have been investigated. We have derived the overlap form of the light-front wave functions (LFWFs) for the sub-leading twist proton TMDs by detangling the un-integrated quark-quark correlator for the semi-inclusive deep inelastic scattering (SIDIS). We have obtained the explicit expressions of TMDs for both the cases of the diquark being a scalar or a vector and analysed their relationships with leading twist TMDs within the same model. Average transverse momenta and average square transverse momenta for the TMDs have been tabulated and compared with the results from the light-front bag model and the light-front constituent quark model (LFCQM). In addition to this, we have also compared our results for the PDF $e(x)$ with the recent CLAS collaboration results.
1202.3300
Wei Wang
Chuan-Hung Chen, Chao-Qiang Geng, Wei Wang
CP violation in $D^0 \to (K^- K^+, \pi^- \pi^+)$ from diquarks
9 pages, 3 figures, reference added
Phys. Rev. D 85, 077702 (2012)
10.1103/PhysRevD.85.077702
DESY 12-027
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The explanation of the large CP asymmetries in $D^0\to (\pi^+\pi^-, K^+K^-)$ decays observed by the LHCb collaboration is likely to call for new physics beyond the CKM paradigm. We explore new contributions caused by the color-sextet scalar diquark, and demonstrate that the diquark with the mass of order 1 TeV and nominal couplings with quarks can generate the CP asymmetries at the percent level. Using the experimental data on branching ratios and CP asymmetries of $D^0\to (\pi^+\pi^-, K^+K^-)$, we derive the constraints on the diquark mass and couplings, which can be further examined on hadron colliders in the dijet final states.
[ { "created": "Wed, 15 Feb 2012 13:21:35 GMT", "version": "v1" }, { "created": "Mon, 20 Feb 2012 15:07:21 GMT", "version": "v2" } ]
2012-04-20
[ [ "Chen", "Chuan-Hung", "" ], [ "Geng", "Chao-Qiang", "" ], [ "Wang", "Wei", "" ] ]
The explanation of the large CP asymmetries in $D^0\to (\pi^+\pi^-, K^+K^-)$ decays observed by the LHCb collaboration is likely to call for new physics beyond the CKM paradigm. We explore new contributions caused by the color-sextet scalar diquark, and demonstrate that the diquark with the mass of order 1 TeV and nominal couplings with quarks can generate the CP asymmetries at the percent level. Using the experimental data on branching ratios and CP asymmetries of $D^0\to (\pi^+\pi^-, K^+K^-)$, we derive the constraints on the diquark mass and couplings, which can be further examined on hadron colliders in the dijet final states.
hep-ph/0610302
Zhenyu Han
Zhenyu Han
Electroweak Constraints on Effective Theories
To appear in Proceedings of SUSY06, the 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006
AIPConf.Proc.903:435-438,2007
10.1063/1.2735217
null
hep-ph
null
We discuss electroweak constraints on TeV scale extensions of the standard model. To obtain model-independent results, effective theory approach is adopted. Constraints are given on arbitrary linear combinations of a set of dimension-6 operators that respect the SM gauge symmetry, as well as CP, lepton and baryon number conservation. Applications of the results are also discussed.
[ { "created": "Mon, 23 Oct 2006 22:52:06 GMT", "version": "v1" } ]
2008-11-26
[ [ "Han", "Zhenyu", "" ] ]
We discuss electroweak constraints on TeV scale extensions of the standard model. To obtain model-independent results, effective theory approach is adopted. Constraints are given on arbitrary linear combinations of a set of dimension-6 operators that respect the SM gauge symmetry, as well as CP, lepton and baryon number conservation. Applications of the results are also discussed.
1001.1652
Zhi-Gang Wang
Zhi-Gang Wang
Analysis of the ${1\over 2}^{\pm}$ flavor antitriplet heavy baryon states with QCD sum rules
11 pages, 16 figures, published version
Eur.Phys.J.C68:479-486,2010
10.1140/epjc/s10052-010-1365-8
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this article, we study the masses and pole residues of the ${1\over 2}^\pm$ flavor antitriplet heavy baryon states ($\Lambda_c^+$, $\Xi_c^+,\Xi_c^0)$ and ($\Lambda_b^0$, $\Xi_b^0,\Xi_b^-)$ by subtracting the contributions from the corresponding ${1\over 2}^\mp$ heavy baryon states with the QCD sum rules, and observe the masses are in good agreement with the experimental data and make reasonable predictions for the unobserved ${1\over 2}^-$ bottom baryon states. Once reasonable values of the pole residues $\lambda_{\Lambda}$ and $\lambda_{\Xi}$ are obtained, we can take them as basic parameters to study the revelent hadronic processes with the QCD sum rules.
[ { "created": "Mon, 11 Jan 2010 13:24:50 GMT", "version": "v1" }, { "created": "Sat, 27 Feb 2010 12:31:47 GMT", "version": "v2" }, { "created": "Sun, 21 Mar 2010 12:49:53 GMT", "version": "v3" }, { "created": "Tue, 8 Jun 2010 08:15:46 GMT", "version": "v4" } ]
2010-08-09
[ [ "Wang", "Zhi-Gang", "" ] ]
In this article, we study the masses and pole residues of the ${1\over 2}^\pm$ flavor antitriplet heavy baryon states ($\Lambda_c^+$, $\Xi_c^+,\Xi_c^0)$ and ($\Lambda_b^0$, $\Xi_b^0,\Xi_b^-)$ by subtracting the contributions from the corresponding ${1\over 2}^\mp$ heavy baryon states with the QCD sum rules, and observe the masses are in good agreement with the experimental data and make reasonable predictions for the unobserved ${1\over 2}^-$ bottom baryon states. Once reasonable values of the pole residues $\lambda_{\Lambda}$ and $\lambda_{\Xi}$ are obtained, we can take them as basic parameters to study the revelent hadronic processes with the QCD sum rules.
hep-ph/9803294
Sven Heinemeyer
S. Heinemeyer
Two-loop calculations in the MSSM
16 pages, 8 figures, Talk given at the workshop ``Quantum Effects in the MSSM'', Sept. 1997, Barcelona, Spain
null
null
KA-TP-18-1997
hep-ph
null
Recent results on two--loop calculations in the MSSM are reviewed. The computation of the QCD corrections to \Delta\rho, \Delta r and to the mass of the lightest Higgs boso in the MSSM are presented.
[ { "created": "Tue, 10 Mar 1998 13:48:06 GMT", "version": "v1" } ]
2007-05-23
[ [ "Heinemeyer", "S.", "" ] ]
Recent results on two--loop calculations in the MSSM are reviewed. The computation of the QCD corrections to \Delta\rho, \Delta r and to the mass of the lightest Higgs boso in the MSSM are presented.
hep-ph/0703245
Patricia Ball
Patricia Ball
Basics of D0-\bar D0 Mixing
Quasi-Impromptu Talk given at XLIInd Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, Italy, March 2007; typos removed; acknowledgements added
null
null
IPPP/07/09
hep-ph
null
Complementing the presentations, at this conference, of the first experimental evidence for $D$ mixing found at BaBar and Belle, I discuss the theoretical status of $D$ mixing.
[ { "created": "Thu, 22 Mar 2007 18:25:08 GMT", "version": "v1" }, { "created": "Fri, 30 Mar 2007 17:18:13 GMT", "version": "v2" } ]
2007-05-23
[ [ "Ball", "Patricia", "" ] ]
Complementing the presentations, at this conference, of the first experimental evidence for $D$ mixing found at BaBar and Belle, I discuss the theoretical status of $D$ mixing.
0903.1889
Muneyuki Ishida
Muneyuki Ishida and Keiji Igi
Test of Universal Rise of Hadronic Total Cross Sections based on pi p, Kp and pbar p,pp Scatterings
32 pages, 12 figures. to be published in Phys. Rev. D
Phys.Rev.D79:096003,2009
10.1103/PhysRevD.79.096003
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Recently there are several evidences of the hadronic total cross section sigma(tot) to be proportional to B (log s)2 consistent with the Froissart unitarity bound. The COMPETE collaborations have further assumed sigma(tot) = B (log s/s0)2 + Z to extend its universal rise with the common value of B and s0 for all hadronic scatterings to reduce the number of adjustable parameters. The coefficient B was suggested to be universal in the arguments of colour glass condensate (CGC) of QCD in recent years. There has been, however, no rigorous proof yet based only on QCD. We attempt to investigate the value of B for pi+- p, K+- p and pbar p,pp scatterings respectively through the search for the simultaneous best fit to the experimental sigma(tot) and rho ratios at high energies. The sigma(tot) at the resonance and intermediate energy regions has also been exploited as a duality constraint based on the special form of finite-energy sum rule(FESR). We estimate the values of B, s0 and Z individually for pi+- p, K+- p and pbar p,pp scatterings without using the universality hypothesis. It turs out that the values of B are mutually consistent within one standard deviation. It has to be stressed that we cannot obtain such a definite conclusion without the duality constraint. It is also interesting to note that the values of Z for pi p, Kp and pbar(p)p approximately satisfy the ratio 2:2:3 predicted by the quark model. The obtained value of B for pbar(p)p is Bpp = 0.280 +- 0.015 mb, which predicts sigma(tot)(pp) =108.0 +- 1.9mb and rho(pp) =0.131+- 0.0025 at the LHC energy s^0.5 =14 TeV.
[ { "created": "Wed, 11 Mar 2009 02:03:11 GMT", "version": "v1" }, { "created": "Sun, 26 Apr 2009 23:25:07 GMT", "version": "v2" } ]
2009-10-29
[ [ "Ishida", "Muneyuki", "" ], [ "Igi", "Keiji", "" ] ]
Recently there are several evidences of the hadronic total cross section sigma(tot) to be proportional to B (log s)2 consistent with the Froissart unitarity bound. The COMPETE collaborations have further assumed sigma(tot) = B (log s/s0)2 + Z to extend its universal rise with the common value of B and s0 for all hadronic scatterings to reduce the number of adjustable parameters. The coefficient B was suggested to be universal in the arguments of colour glass condensate (CGC) of QCD in recent years. There has been, however, no rigorous proof yet based only on QCD. We attempt to investigate the value of B for pi+- p, K+- p and pbar p,pp scatterings respectively through the search for the simultaneous best fit to the experimental sigma(tot) and rho ratios at high energies. The sigma(tot) at the resonance and intermediate energy regions has also been exploited as a duality constraint based on the special form of finite-energy sum rule(FESR). We estimate the values of B, s0 and Z individually for pi+- p, K+- p and pbar p,pp scatterings without using the universality hypothesis. It turs out that the values of B are mutually consistent within one standard deviation. It has to be stressed that we cannot obtain such a definite conclusion without the duality constraint. It is also interesting to note that the values of Z for pi p, Kp and pbar(p)p approximately satisfy the ratio 2:2:3 predicted by the quark model. The obtained value of B for pbar(p)p is Bpp = 0.280 +- 0.015 mb, which predicts sigma(tot)(pp) =108.0 +- 1.9mb and rho(pp) =0.131+- 0.0025 at the LHC energy s^0.5 =14 TeV.
2004.10359
Hoang Bao Tran Tan
V. V. Flambaum, I. B. Samsonov and H. B. Tran Tan
Limits on $CP$-violating hadronic interactions and proton EDM from paramagnetic molecules
27 pages. V2: major corrections, V3: comments on uncertainties and other minor corrections, journal version
null
10.1007/JHEP10(2020)077
null
hep-ph nucl-th physics.atom-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Experiments with paramagnetic ground or metastable excited states of molecules (ThO, HfF$^+$, YbF, YbOH, BaF, PbO, etc.) provide strong constraints on electron electric dipole moment (EDM) and coupling constant $C_{SP}$ of contact semileptonic interaction. We compute new contributions to $C_{SP}$ arising from the nucleon EDMs due to combined electric and magnetic electron-nucleon interaction. This allows us to improve limits from the experiments with paramagnetic molecules on the $CP$-violating parameters, such as the proton EDM, $|d_p|< 1.1\times 10^{-23} e\cdot $cm, the QCD vacuum angle, $|\bar \theta|<1.4\times 10^{-8}$, as well as the quark chromo-EDMs and $\pi$-meson-nucleon couplings. Our results may also be used to search for the axion dark matter which produces oscillating $\bar\theta$.
[ { "created": "Wed, 22 Apr 2020 01:34:31 GMT", "version": "v1" }, { "created": "Wed, 29 Apr 2020 01:11:06 GMT", "version": "v2" }, { "created": "Mon, 27 Jul 2020 03:59:35 GMT", "version": "v3" }, { "created": "Fri, 18 Sep 2020 01:44:53 GMT", "version": "v4" } ]
2020-10-28
[ [ "Flambaum", "V. V.", "" ], [ "Samsonov", "I. B.", "" ], [ "Tan", "H. B. Tran", "" ] ]
Experiments with paramagnetic ground or metastable excited states of molecules (ThO, HfF$^+$, YbF, YbOH, BaF, PbO, etc.) provide strong constraints on electron electric dipole moment (EDM) and coupling constant $C_{SP}$ of contact semileptonic interaction. We compute new contributions to $C_{SP}$ arising from the nucleon EDMs due to combined electric and magnetic electron-nucleon interaction. This allows us to improve limits from the experiments with paramagnetic molecules on the $CP$-violating parameters, such as the proton EDM, $|d_p|< 1.1\times 10^{-23} e\cdot $cm, the QCD vacuum angle, $|\bar \theta|<1.4\times 10^{-8}$, as well as the quark chromo-EDMs and $\pi$-meson-nucleon couplings. Our results may also be used to search for the axion dark matter which produces oscillating $\bar\theta$.
hep-ph/9906466
Colin Froggatt
C.D. Froggatt and H. B. Nielsen
Why do we have parity violation?
10 page LaTeX file; updated version of invited talk published in the Proceedings of the International Workshop on {\it What comes beyond the Standard Model}, Bled, Slovenia, 29 June - 9 July 1998 (DMFA - zalo\u{z}ni\u{s}tvo, Ljubljana)
null
null
GUTPA/99/05/2
hep-ph
null
We discuss here two of the questions posed at the beginning of the Bled 1998 workshop: Why is the weak charge dependent on handedness? Why do we have parity violation in the Standard Model? It is argued that the quarks and leptons must be protected from gaining a fundamental mass, very large compared to the electroweak scale, by gauge invariance and hence that their gauge charges must depend on handedness. Furthermore we argue that it is the conservation of parity in the electromagnetic and strong interactions rather than parity violation in the weak interactions that needs an explanation. We derive this parity conservation and indeed the whole system of Weyl fermion representations in the Standard Model from a few simple assumptions: Mass protection, small representations, anomaly cancellation and the Standard Model gauge group $S(U(2)\times U(3))$.
[ { "created": "Wed, 23 Jun 1999 13:39:49 GMT", "version": "v1" } ]
2007-05-23
[ [ "Froggatt", "C. D.", "" ], [ "Nielsen", "H. B.", "" ] ]
We discuss here two of the questions posed at the beginning of the Bled 1998 workshop: Why is the weak charge dependent on handedness? Why do we have parity violation in the Standard Model? It is argued that the quarks and leptons must be protected from gaining a fundamental mass, very large compared to the electroweak scale, by gauge invariance and hence that their gauge charges must depend on handedness. Furthermore we argue that it is the conservation of parity in the electromagnetic and strong interactions rather than parity violation in the weak interactions that needs an explanation. We derive this parity conservation and indeed the whole system of Weyl fermion representations in the Standard Model from a few simple assumptions: Mass protection, small representations, anomaly cancellation and the Standard Model gauge group $S(U(2)\times U(3))$.
2204.08440
Tom Tong
Vincenzo Cirigliano, Wouter Dekens, Jordy de Vries, Emanuele Mereghetti, Tom Tong
Beta-decay implications for the W-boson mass anomaly
null
null
10.1103/PhysRevD.106.075001
INT-PUB-22-014
hep-ph nucl-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We point out the necessity to consider $\beta$-decay observables in resolutions of the $W$-boson anomaly in the Standard Model Effective Field Theory that go beyond pure oblique corrections. We demonstrate that present global analyses that explain the $W$-boson mass anomaly predict a large, percent-level, violation of first-row CKM unitarity. We investigate what solutions to the $W$-boson mass anomaly survive after including $\beta$-decay constraints.
[ { "created": "Mon, 18 Apr 2022 17:52:41 GMT", "version": "v1" } ]
2022-10-19
[ [ "Cirigliano", "Vincenzo", "" ], [ "Dekens", "Wouter", "" ], [ "de Vries", "Jordy", "" ], [ "Mereghetti", "Emanuele", "" ], [ "Tong", "Tom", "" ] ]
We point out the necessity to consider $\beta$-decay observables in resolutions of the $W$-boson anomaly in the Standard Model Effective Field Theory that go beyond pure oblique corrections. We demonstrate that present global analyses that explain the $W$-boson mass anomaly predict a large, percent-level, violation of first-row CKM unitarity. We investigate what solutions to the $W$-boson mass anomaly survive after including $\beta$-decay constraints.
0807.1082
Redamy Perez Ramos
Wlofgang Ochs (MPI), Redamy Perez Ramos
Particle Multiplicity in Jets and Sub-jets with Jet Axis from Color Current
null
Phys.Rev.D78:034010,2008
10.1103/PhysRevD.78.034010
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the particle multiplicity in a jet or sub-jet as derived from an energy-multiplicity 2-particle correlation. This definition avoids the notion of a globally fixed jet axis and allows for the study of smaller jet cone openings in a more stable way. The results are sensitive to the mean color current $<C >_{A_0} $ in the jet from primary parton $A_0$ which takes into account intermediate partonic processes in the sub-jet production where $C_F< < C >_{A_0} < N_c$ at high energies. We generalize previous calculations in Leading Logarithmic Approximation (LLA). The size of the effects related to this jet axis definition are computed for multiplicities in sub-jets with different opening angles and energies by including contributions from the Modified LLA (MLLA) and Next-to-MLLA to the leading order QCD results.
[ { "created": "Mon, 7 Jul 2008 18:17:50 GMT", "version": "v1" } ]
2008-11-26
[ [ "Ochs", "Wlofgang", "", "MPI" ], [ "Ramos", "Redamy Perez", "" ] ]
We study the particle multiplicity in a jet or sub-jet as derived from an energy-multiplicity 2-particle correlation. This definition avoids the notion of a globally fixed jet axis and allows for the study of smaller jet cone openings in a more stable way. The results are sensitive to the mean color current $<C >_{A_0} $ in the jet from primary parton $A_0$ which takes into account intermediate partonic processes in the sub-jet production where $C_F< < C >_{A_0} < N_c$ at high energies. We generalize previous calculations in Leading Logarithmic Approximation (LLA). The size of the effects related to this jet axis definition are computed for multiplicities in sub-jets with different opening angles and energies by including contributions from the Modified LLA (MLLA) and Next-to-MLLA to the leading order QCD results.
hep-ph/0110224
Kenichiro Aoki
Kenichiro Aoki and Dimitri Kusnezov
Violations of local equilibrium and linear response in classical lattice theories
7pp, 4figs, talk given by KA at "Thermal field theory and applications" workshop 2001
Phys.Lett. A309 (2003) 377-381
10.1016/S0375-9601(03)00293-7
null
hep-ph
null
We study the dynamics of $\phi^4$ theory and the FPU $\beta$ model under thermal gradients, from first principles. We analyze quantitatively how local equilibrium and linear response are violated, paying special care to how we find observables that unambiguously display these violations. Relations between these quantities to equations of state are also examined. Further, we discuss how we can approach similar dynamical problems in continuum quantum field theory. We analyze how close we are to obtaining the continuum results.
[ { "created": "Wed, 17 Oct 2001 08:04:20 GMT", "version": "v1" } ]
2009-11-07
[ [ "Aoki", "Kenichiro", "" ], [ "Kusnezov", "Dimitri", "" ] ]
We study the dynamics of $\phi^4$ theory and the FPU $\beta$ model under thermal gradients, from first principles. We analyze quantitatively how local equilibrium and linear response are violated, paying special care to how we find observables that unambiguously display these violations. Relations between these quantities to equations of state are also examined. Further, we discuss how we can approach similar dynamical problems in continuum quantum field theory. We analyze how close we are to obtaining the continuum results.
hep-ph/0309305
Leonardo Rastelli
Nissan Itzhaki, Igor R. Klebanov, Peter Ouyang, and Leonardo Rastelli
Is Theta+(1540) a Kaon--Skyrmion Resonance?
22 pages. More details on SU(2)_I excitations of Theta+, version published on NPB
Nucl.Phys. B684 (2004) 264-280
10.1016/j.nuclphysb.2004.02.004
PUPT-2097
hep-ph
null
We reconsider the relationship between the bound state and the SU(3) rigid rotator approaches to strangeness in the Skyrme model. For non-exotic S=-1 baryons the bound state approach matches for small m_K onto the rigid rotator approach, and the bound state mode turns into the rotator zero-mode. However, for small m_K, we find no S=+1 kaon bound states or resonances in the spectrum, confirming previous work. This suggests that, at least for large N and small m_K, the exotic state may be an artifact of the rigid rotator approach to the Skyrme model. An S=+1 near-threshold state comes into existence only for sufficiently large SU(3) breaking. If such a state exists, then it has the expected quantum numbers of Theta+: I=0, J=1/2 and positive parity. Other exotic states with (I=1, J^P=3/2+), (I=1,J^P=1/2+), (I=2, J^P=5/2+) and (I=2,J^P=3/2+) appear as its SU(2) rotator excitations. As a test of our methods, we also identify a D-wave S=-1 near-threshold resonance that, upon SU(2) collective coordinate quantization, reproduces the mass splittings of the observed states Lambda(1520), Sigma(1670) and Sigma(1775) with good accuracy.
[ { "created": "Fri, 26 Sep 2003 19:48:13 GMT", "version": "v1" }, { "created": "Sat, 4 Oct 2003 21:34:24 GMT", "version": "v2" }, { "created": "Wed, 15 Oct 2003 15:08:47 GMT", "version": "v3" }, { "created": "Fri, 24 Oct 2003 20:25:39 GMT", "version": "v4" }, { "cr...
2010-04-05
[ [ "Itzhaki", "Nissan", "" ], [ "Klebanov", "Igor R.", "" ], [ "Ouyang", "Peter", "" ], [ "Rastelli", "Leonardo", "" ] ]
We reconsider the relationship between the bound state and the SU(3) rigid rotator approaches to strangeness in the Skyrme model. For non-exotic S=-1 baryons the bound state approach matches for small m_K onto the rigid rotator approach, and the bound state mode turns into the rotator zero-mode. However, for small m_K, we find no S=+1 kaon bound states or resonances in the spectrum, confirming previous work. This suggests that, at least for large N and small m_K, the exotic state may be an artifact of the rigid rotator approach to the Skyrme model. An S=+1 near-threshold state comes into existence only for sufficiently large SU(3) breaking. If such a state exists, then it has the expected quantum numbers of Theta+: I=0, J=1/2 and positive parity. Other exotic states with (I=1, J^P=3/2+), (I=1,J^P=1/2+), (I=2, J^P=5/2+) and (I=2,J^P=3/2+) appear as its SU(2) rotator excitations. As a test of our methods, we also identify a D-wave S=-1 near-threshold resonance that, upon SU(2) collective coordinate quantization, reproduces the mass splittings of the observed states Lambda(1520), Sigma(1670) and Sigma(1775) with good accuracy.
2406.01209
En Wang
Ying Li, Si-Wei Liu, En Wang, De-Min Li, Li-Sheng Geng, and Ju-Jun Xie
Theoretical study of $N(1535)$ and $\Sigma^*(1/2^-)$ in the Cabibbo-favored process $\Lambda_c^+ \to p \bar{K}^0\eta$
9 pages, 5 figures, comments are welcome!
null
null
null
hep-ph
http://creativecommons.org/licenses/by/4.0/
Motivated by the recent experimental measurements, we have investigated the Cabibbo-favored process $\Lambda_c^+ \to p \bar{K}^0\eta$, where the $N(1535)$ resonance is dynamically generated from the $S$-wave pseudoscalar meson-octet baryon interactions within the chiral unitary approach. The contributions from the intermediate $N(1650)$ and the predicted low-lying baryon $\Sigma^*(1/2^-)$ are also considered. In addition, a Breit-Wigner amplitude for the $N(1535)$ resonance is checked. By comparing with the measured $\eta p$, $\bar{K}^0 \eta$, and $p \bar{K}^0$ invariant mass squared distributions, our results support the interpretation of $N(1535)$ as a dynamically generated state. Furthermore, we demonstrate that, with the contribution from $\Sigma^*(1/2^-)$ taken into account, the calculated invariant mass spectrum agrees with the Belle measurements. Future precise measurements of the $\Lambda_c^+\to p \bar{K}^0\eta$ process can further elucidate the existence of the low-lying baryon $\Sigma^*(1/2^-)$.
[ { "created": "Mon, 3 Jun 2024 11:21:05 GMT", "version": "v1" } ]
2024-06-04
[ [ "Li", "Ying", "" ], [ "Liu", "Si-Wei", "" ], [ "Wang", "En", "" ], [ "Li", "De-Min", "" ], [ "Geng", "Li-Sheng", "" ], [ "Xie", "Ju-Jun", "" ] ]
Motivated by the recent experimental measurements, we have investigated the Cabibbo-favored process $\Lambda_c^+ \to p \bar{K}^0\eta$, where the $N(1535)$ resonance is dynamically generated from the $S$-wave pseudoscalar meson-octet baryon interactions within the chiral unitary approach. The contributions from the intermediate $N(1650)$ and the predicted low-lying baryon $\Sigma^*(1/2^-)$ are also considered. In addition, a Breit-Wigner amplitude for the $N(1535)$ resonance is checked. By comparing with the measured $\eta p$, $\bar{K}^0 \eta$, and $p \bar{K}^0$ invariant mass squared distributions, our results support the interpretation of $N(1535)$ as a dynamically generated state. Furthermore, we demonstrate that, with the contribution from $\Sigma^*(1/2^-)$ taken into account, the calculated invariant mass spectrum agrees with the Belle measurements. Future precise measurements of the $\Lambda_c^+\to p \bar{K}^0\eta$ process can further elucidate the existence of the low-lying baryon $\Sigma^*(1/2^-)$.
hep-ph/0401053
Arata Hayashigaki
Arata Hayashigaki and Kazuhiro Tanaka
Transverse quark motion inside charmonia in diffractive photo- and electroproductions
REVTeX4 17 pages, 14 figures
null
null
null
hep-ph nucl-th
null
We reexamine the Fermi motion effects on the diffractive photo- and electroproductions of heavy vector-mesons, J/psi and psi', off a nucleon in the leading ln(Q^2/Lambda_QCD^2) approximation (LLA) of QCD. We take into account all the Fermi motion corrections arising from the relative motion of quarks inside the charmonium, which is treated as a nonrelativistic bound state of c and \bar{c}. Our key ingredients are the correct spin structure for the ^3S_1 c\bar{c} bound state, the off-shellness in the c\bar{c} \to J/psi (psi') hadronization vertex, and the modification of the gluon's longitudinal momentum fraction probed by the process, due to the relative motion between c and \bar{c}. We demonstrate that these three contributions produce the new Fermi motion effects in the LLA diffractive amplitude in QCD. It is found that our new effects moderate the strong suppression of the diffractive J/psi (psi') production cross sections, which was reported in the previous works on the Fermi motion effects. We emphasize the role of the transverse quark motion for the heavy meson production, and also discuss the strong helicity dependence of the Fermi motion effects and its implication in the longitudinal to transverse production ratio, sigma_L/sigma_T.
[ { "created": "Fri, 9 Jan 2004 16:10:17 GMT", "version": "v1" } ]
2007-05-23
[ [ "Hayashigaki", "Arata", "" ], [ "Tanaka", "Kazuhiro", "" ] ]
We reexamine the Fermi motion effects on the diffractive photo- and electroproductions of heavy vector-mesons, J/psi and psi', off a nucleon in the leading ln(Q^2/Lambda_QCD^2) approximation (LLA) of QCD. We take into account all the Fermi motion corrections arising from the relative motion of quarks inside the charmonium, which is treated as a nonrelativistic bound state of c and \bar{c}. Our key ingredients are the correct spin structure for the ^3S_1 c\bar{c} bound state, the off-shellness in the c\bar{c} \to J/psi (psi') hadronization vertex, and the modification of the gluon's longitudinal momentum fraction probed by the process, due to the relative motion between c and \bar{c}. We demonstrate that these three contributions produce the new Fermi motion effects in the LLA diffractive amplitude in QCD. It is found that our new effects moderate the strong suppression of the diffractive J/psi (psi') production cross sections, which was reported in the previous works on the Fermi motion effects. We emphasize the role of the transverse quark motion for the heavy meson production, and also discuss the strong helicity dependence of the Fermi motion effects and its implication in the longitudinal to transverse production ratio, sigma_L/sigma_T.
1212.3249
Stefan Liebler
Robert V. Harlander, Stefan Liebler, Hendrik Mantler
SusHi: A program for the calculation of Higgs production in gluon fusion and bottom-quark annihilation in the Standard Model and the MSSM
28 pages, 4 figures; v2: typos corrected, reference added, version published in CPC
Computer Physics Communications 184 (2013) pp. 1605-1617
10.1016/j.cpc.2013.02.006
WUB/12-28, LPN12-134
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This article describes the code SusHi (for "Supersymmetric Higgs") which calculates the cross sections $pp/p\bar{p}\rightarrow\phi+X$ in gluon fusion and bottom-quark annihilation in the SM and the MSSM, where $\phi$ is any of the neutral Higgs bosons within these models. Apart from inclusive cross sections up to NNLO QCD, differential cross sections with respect to the Higgs' transverse momentum $p_T$ and (pseudo-)rapidity $y(\eta)$ can be calculated through NLO QCD. In case of gluon fusion, SusHi contains NLO QCD contributions from the third family of quarks and squarks, NNLO corrections due to top-quarks, approximate NNLO corrections due to top-squarks, and electro-weak effects. It supports various renormalization schemes for the sbottom sector and the bottom Yukawa coupling, as well as resummation effects of higher order $\tan\beta$-enhanced sbottom contributions. SusHi provides a link to FeynHiggs for the calculation of the Higgs masses.
[ { "created": "Thu, 13 Dec 2012 18:16:23 GMT", "version": "v1" }, { "created": "Tue, 19 Mar 2013 17:00:49 GMT", "version": "v2" } ]
2013-03-20
[ [ "Harlander", "Robert V.", "" ], [ "Liebler", "Stefan", "" ], [ "Mantler", "Hendrik", "" ] ]
This article describes the code SusHi (for "Supersymmetric Higgs") which calculates the cross sections $pp/p\bar{p}\rightarrow\phi+X$ in gluon fusion and bottom-quark annihilation in the SM and the MSSM, where $\phi$ is any of the neutral Higgs bosons within these models. Apart from inclusive cross sections up to NNLO QCD, differential cross sections with respect to the Higgs' transverse momentum $p_T$ and (pseudo-)rapidity $y(\eta)$ can be calculated through NLO QCD. In case of gluon fusion, SusHi contains NLO QCD contributions from the third family of quarks and squarks, NNLO corrections due to top-quarks, approximate NNLO corrections due to top-squarks, and electro-weak effects. It supports various renormalization schemes for the sbottom sector and the bottom Yukawa coupling, as well as resummation effects of higher order $\tan\beta$-enhanced sbottom contributions. SusHi provides a link to FeynHiggs for the calculation of the Higgs masses.
1311.7173
Piero Nicolini
Antonia M. Frassino, Piero Nicolini and Orlando Panella
Unparticle Casimir effect
13 pages, 3 figures; v2: improved discussion, additional references, v3: title slightly changed, version matching that in press on Physics Letters B
Physics Letters B 772 (2017) 675--680
10.1016/j.physletb.2017.07.029
null
hep-ph hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper we present the un-Casimir effect, namely the study of the Casimir energy in the presence of an unparticle component in addition to the electromagnetic field contribution. The distinctive feature of the un-Casimir effect is a fractalization of metallic plates. This result emerges through a new dependence of the Casimir energy on the plate separation that scales with a continuous power controlled by the unparticle dimension. As long as the perfect conductor approximation is valid, we find bounds on the unparticle scale that are independent of the effective coupling constant between the scale invariant sector and ordinary matter. We find regions of the parameter space such that for plate distances around $5\mu$m and larger the un-Casimir bound wins over the other bounds.
[ { "created": "Wed, 27 Nov 2013 23:01:15 GMT", "version": "v1" }, { "created": "Tue, 4 Mar 2014 21:00:30 GMT", "version": "v2" }, { "created": "Mon, 17 Jul 2017 21:04:08 GMT", "version": "v3" } ]
2017-07-27
[ [ "Frassino", "Antonia M.", "" ], [ "Nicolini", "Piero", "" ], [ "Panella", "Orlando", "" ] ]
In this paper we present the un-Casimir effect, namely the study of the Casimir energy in the presence of an unparticle component in addition to the electromagnetic field contribution. The distinctive feature of the un-Casimir effect is a fractalization of metallic plates. This result emerges through a new dependence of the Casimir energy on the plate separation that scales with a continuous power controlled by the unparticle dimension. As long as the perfect conductor approximation is valid, we find bounds on the unparticle scale that are independent of the effective coupling constant between the scale invariant sector and ordinary matter. We find regions of the parameter space such that for plate distances around $5\mu$m and larger the un-Casimir bound wins over the other bounds.
hep-ph/0406276
Shevchenko
V.I.Shevchenko, Yu.A.Simonov (ITEP)
Current correlators in QCD: OPE versus large distance dynamics
LaTeX, 25 pages, 13 figures
Phys.Rev. D70 (2004) 074012
10.1103/PhysRevD.70.074012
null
hep-ph
null
We analyse the structure of current-current correlators in coordinate space in large $N_c$ limit when the corresponding spectral density takes the form of an infinite sum over hadron poles. The latter are computed in the QCD string model with quarks at the ends, including the lowest states, for all channels. The corresponding correlators demonstrate reasonable qualitative agreement with the lattice data without any additional fits. Different issues concerning the structure of the short distance OPE are discussed.
[ { "created": "Thu, 24 Jun 2004 14:50:31 GMT", "version": "v1" } ]
2009-11-10
[ [ "Shevchenko", "V. I.", "", "ITEP" ], [ "Simonov", "Yu. A.", "", "ITEP" ] ]
We analyse the structure of current-current correlators in coordinate space in large $N_c$ limit when the corresponding spectral density takes the form of an infinite sum over hadron poles. The latter are computed in the QCD string model with quarks at the ends, including the lowest states, for all channels. The corresponding correlators demonstrate reasonable qualitative agreement with the lattice data without any additional fits. Different issues concerning the structure of the short distance OPE are discussed.
1603.06664
Huey-Wen Lin
Jiunn-Wei Chen, Saul D. Cohen, Xiangdong Ji, Huey-Wen Lin, and Jian-Hui Zhang
Nucleon Helicity and Transversity Parton Distributions from Lattice QCD
21 pages, 6 figures
null
10.1016/j.nuclphysb.2016.07.033
MIT-CTP/4776,INT-PUB-16-009
hep-ph hep-lat
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We present the first lattice-QCD calculation of the isovector polarized parton distribution functions (both helicity and transversity) using the large-momentum effective field theory (LaMET) approach for direct Bjorken-$x$ dependence. We first review the detailed steps of the procedure in the unpolarized case, then generalize to the helicity and transversity cases. We also derive a new mass-correction formulation for all three cases. We then compare the effects of each finite-momentum correction using lattice data calculated at $M_\pi\approx 310$ MeV. Finally, we discuss the implications of these results for the poorly known antiquark structure and predict the sea-flavor asymmetry in the transversely polarized nucleon.
[ { "created": "Tue, 22 Mar 2016 02:53:42 GMT", "version": "v1" } ]
2016-09-21
[ [ "Chen", "Jiunn-Wei", "" ], [ "Cohen", "Saul D.", "" ], [ "Ji", "Xiangdong", "" ], [ "Lin", "Huey-Wen", "" ], [ "Zhang", "Jian-Hui", "" ] ]
We present the first lattice-QCD calculation of the isovector polarized parton distribution functions (both helicity and transversity) using the large-momentum effective field theory (LaMET) approach for direct Bjorken-$x$ dependence. We first review the detailed steps of the procedure in the unpolarized case, then generalize to the helicity and transversity cases. We also derive a new mass-correction formulation for all three cases. We then compare the effects of each finite-momentum correction using lattice data calculated at $M_\pi\approx 310$ MeV. Finally, we discuss the implications of these results for the poorly known antiquark structure and predict the sea-flavor asymmetry in the transversely polarized nucleon.
0712.4053
Mayumi Aoki
Mayumi Aoki (Tokyo U., ICRR), Shinya Kanemura (Toyama U.)
Unitarity bounds in the Higgs model including triplet fields with custodial symmetry
1+15 pages, Version to be published in Phys. Rev. D
Phys.Rev.D77:095009,2008
10.1103/PhysRevD.77.095009
null
hep-ph
null
We study bounds on Higgs boson masses from perturbative unitarity in the Georgi-Machacek model, whose Higgs sector is composed of a scalar isospin doublet, a real and a complex isospin triplet fields. This model can be compatible with the electroweak precision data without fine tuning because of the imposed global SU(2)_R symmetry in the Higgs potential, by which the electroweak rho parameter is unity at the tree level. All possible two-body elastic-scattering channels are taken into account to evaluate the S-wave amplitude matrix, and then the condition of perturbative unitarity is imposed on the eigenvalues to obtain constraint on the Higgs parameters. Masses of all scalar bosons turn out to be bounded from above, some of which receive more strict upper bounds as compared to that in the standard model (712 GeV). In particular, the upper bound of the lightest scalar boson, whatever it would be, is about 270 GeV.
[ { "created": "Tue, 25 Dec 2007 08:51:00 GMT", "version": "v1" }, { "created": "Wed, 9 Apr 2008 06:09:42 GMT", "version": "v2" } ]
2008-11-26
[ [ "Aoki", "Mayumi", "", "Tokyo U., ICRR" ], [ "Kanemura", "Shinya", "", "Toyama U." ] ]
We study bounds on Higgs boson masses from perturbative unitarity in the Georgi-Machacek model, whose Higgs sector is composed of a scalar isospin doublet, a real and a complex isospin triplet fields. This model can be compatible with the electroweak precision data without fine tuning because of the imposed global SU(2)_R symmetry in the Higgs potential, by which the electroweak rho parameter is unity at the tree level. All possible two-body elastic-scattering channels are taken into account to evaluate the S-wave amplitude matrix, and then the condition of perturbative unitarity is imposed on the eigenvalues to obtain constraint on the Higgs parameters. Masses of all scalar bosons turn out to be bounded from above, some of which receive more strict upper bounds as compared to that in the standard model (712 GeV). In particular, the upper bound of the lightest scalar boson, whatever it would be, is about 270 GeV.
1609.02386
Alexei Smirnov Yu
A. Yu. Smirnov
Solar neutrinos: Oscillations or No-oscillations?
19 pages, 12 figures, Comments and 1 figure added
null
null
null
hep-ph astro-ph.SR hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The Nobel prize in physics 2015 has been awarded "... for the discovery of neutrino oscillations which show that neutrinos have mass". While SuperKamiokande (SK), indeed, has discovered oscillations, SNO observed effect of the adiabatic (almost non-oscillatory) flavor conversion of neutrinos in the matter of the Sun. Oscillations are irrelevant for solar neutrinos apart from small $\nu_e$ regeneration inside the Earth. Both oscillations and adiabatic conversion do not imply masses uniquely and further studies were required to show that non-zero neutrino masses are behind the SNO results. Phenomena of oscillations (phase effect) and adiabatic conversion (the MSW effect driven by the change of mixing in matter) are described in pedagogical way.
[ { "created": "Thu, 8 Sep 2016 11:56:07 GMT", "version": "v1" }, { "created": "Tue, 19 Sep 2017 11:51:10 GMT", "version": "v2" } ]
2017-09-20
[ [ "Smirnov", "A. Yu.", "" ] ]
The Nobel prize in physics 2015 has been awarded "... for the discovery of neutrino oscillations which show that neutrinos have mass". While SuperKamiokande (SK), indeed, has discovered oscillations, SNO observed effect of the adiabatic (almost non-oscillatory) flavor conversion of neutrinos in the matter of the Sun. Oscillations are irrelevant for solar neutrinos apart from small $\nu_e$ regeneration inside the Earth. Both oscillations and adiabatic conversion do not imply masses uniquely and further studies were required to show that non-zero neutrino masses are behind the SNO results. Phenomena of oscillations (phase effect) and adiabatic conversion (the MSW effect driven by the change of mixing in matter) are described in pedagogical way.
1709.08649
Ambresh Shivaji
Fabio Maltoni, Davide Pagani, Ambresh Shivaji, Xiaoran Zhao
Trilinear Higgs coupling determination via single-Higgs differential measurements at the LHC
31 pages, 15 figures, 5 tables; Matches the journal version
Eur. Phys. J. C (2017) 77: 887
10.1140/epjc/s10052-017-5410-8
CP3-17-37, TUM-HEP-1099/17, MCnet-17-18
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study one-loop effects induced by an anomalous Higgs trilinear coupling on total and differential rates for the $H\to 4\ell$ decay and some of the main single-Higgs production channels at the LHC, namely, VBF, $VH$, $t\bar tH$ and $tHj$. Our results are based on a public code that calculates these effects by simply reweighting samples of Standard-Model-like events for a given production channel. For $VH$ and $t\bar tH$ production, where differential effects are particularly relevant, we include Standard Model electroweak corrections, which have similar sizes but different kinematic dependences. Finally, we study the sensitivity of future LHC runs to determine the trilinear coupling via inclusive and differential measurements, considering also the case where the Higgs couplings to vector bosons and the top quark is affected by new physics. We find that the constraints on the couplings and the relevance of differential distributions critically depend on the expected experimental and theoretical uncertainties.
[ { "created": "Mon, 25 Sep 2017 18:01:33 GMT", "version": "v1" }, { "created": "Tue, 6 Feb 2018 22:51:06 GMT", "version": "v2" } ]
2018-02-08
[ [ "Maltoni", "Fabio", "" ], [ "Pagani", "Davide", "" ], [ "Shivaji", "Ambresh", "" ], [ "Zhao", "Xiaoran", "" ] ]
We study one-loop effects induced by an anomalous Higgs trilinear coupling on total and differential rates for the $H\to 4\ell$ decay and some of the main single-Higgs production channels at the LHC, namely, VBF, $VH$, $t\bar tH$ and $tHj$. Our results are based on a public code that calculates these effects by simply reweighting samples of Standard-Model-like events for a given production channel. For $VH$ and $t\bar tH$ production, where differential effects are particularly relevant, we include Standard Model electroweak corrections, which have similar sizes but different kinematic dependences. Finally, we study the sensitivity of future LHC runs to determine the trilinear coupling via inclusive and differential measurements, considering also the case where the Higgs couplings to vector bosons and the top quark is affected by new physics. We find that the constraints on the couplings and the relevance of differential distributions critically depend on the expected experimental and theoretical uncertainties.
1011.5154
Paula Tuzon
Martin Jung, Antonio Pich and Paula Tuz\'on
The B -> Xs gamma Rate and CP Asymmetry within the Aligned Two-Higgs-Doublet Model
12 pages, 6 figures. Submitted to Phys.Rev.D
Phys.Rev.D83:074011,2011
10.1103/PhysRevD.83.074011
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In the two-Higgs-doublet model the alignment of the Yukawa matrices in flavour space guarantees the absence of flavour-changing neutral currents at tree level, while introducing new sources for CP violation parametrized in a very economical way. This implies potentially large influence in a number of processes, b -> s gamma being a prominent example where rather high experimental and theoretical precision meet. We analyze the CP rate asymmetry in this inclusive decay and determine the resulting constraints on the model parameters. We demonstrate the compatibility with previously obtained limits. Moreover we extend the phenomenological analysis of the branching ratio, and examine the influence of resulting correlations on the like-sign dimuon charge asymmetry in B decays.
[ { "created": "Tue, 23 Nov 2010 16:39:01 GMT", "version": "v1" }, { "created": "Fri, 17 Dec 2010 19:42:03 GMT", "version": "v2" } ]
2011-04-22
[ [ "Jung", "Martin", "" ], [ "Pich", "Antonio", "" ], [ "Tuzón", "Paula", "" ] ]
In the two-Higgs-doublet model the alignment of the Yukawa matrices in flavour space guarantees the absence of flavour-changing neutral currents at tree level, while introducing new sources for CP violation parametrized in a very economical way. This implies potentially large influence in a number of processes, b -> s gamma being a prominent example where rather high experimental and theoretical precision meet. We analyze the CP rate asymmetry in this inclusive decay and determine the resulting constraints on the model parameters. We demonstrate the compatibility with previously obtained limits. Moreover we extend the phenomenological analysis of the branching ratio, and examine the influence of resulting correlations on the like-sign dimuon charge asymmetry in B decays.
hep-ph/0403078
Yue-Liang Wu
Y.B Zuo, Y.a Yan, Y.L Wu and W.Y Wang
Lifetime Difference and Endpoint effect in the Inclusive Bottom Hadron Decays
11 pages, Revtex, 10 figures, 6 tables, published version
Int.J.Mod.Phys. A19 (2004) 3685-3706
10.1142/S0217751X04018476
null
hep-ph
null
The lifetime differences of bottom hadrons are known to be properly explained within the framework of heavy quark effective field theory(HQEFT) of QCD via the inverse expansion of the dressed heavy quark mass. In general, the spectrum around the endpoint region is not well behaved due to the invalidity of $1/m_Q$ expansion near the endpoint. The curve fitting method is adopted to treat the endpoint behavior. It turns out that the endpoint effects are truly small and the explanation on the lifetime differences in the HQEFT of QCD is then well justified. The inclusion of the endpoint effects makes the prediction on the lifetime differences and the extraction on the CKM matrix element $|V_{cb}|$ more reliable.
[ { "created": "Mon, 8 Mar 2004 06:55:41 GMT", "version": "v1" } ]
2009-11-10
[ [ "Zuo", "Y. B", "" ], [ "Yan", "Y. a", "" ], [ "Wu", "Y. L", "" ], [ "Wang", "W. Y", "" ] ]
The lifetime differences of bottom hadrons are known to be properly explained within the framework of heavy quark effective field theory(HQEFT) of QCD via the inverse expansion of the dressed heavy quark mass. In general, the spectrum around the endpoint region is not well behaved due to the invalidity of $1/m_Q$ expansion near the endpoint. The curve fitting method is adopted to treat the endpoint behavior. It turns out that the endpoint effects are truly small and the explanation on the lifetime differences in the HQEFT of QCD is then well justified. The inclusion of the endpoint effects makes the prediction on the lifetime differences and the extraction on the CKM matrix element $|V_{cb}|$ more reliable.
1601.06394
Cheng-Wei Chiang
Cheng-Wei Chiang and An-Li Kuo
Can the 750-GeV diphoton resonance be the singlet Higgs boson of custodial Higgs triplet model?
14 pages, 2 figures, and 2 tables; bugs in numerical calculations fixed, and discussions and conclusions changed; typo corrected; 16 pages, expanded with more detailed discussions, updated figures and tables, version to appear in the journal
null
10.1016/j.physletb.2016.07.045
null
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The observation of diphoton excess around the mass of 750 GeV in LHC Run-II motivates us to consider whether the singlet Higgs boson in the custodial Higgs triplet model can serve as a good candidate because an earlier study of comprehensive parameter scan shows that it can have the right mass in the viable mass spectra. By assuming the singlet Higgs mass at 750 GeV, its total width less than 50 GeV and imposing constraints from the LHC 8-TeV data, we identify an approximately linear region on the $(v_\Delta, \alpha)$ plane along which the exotic Higgs boson masses satisfy a specific hierarchy and have lower possible spectra, where $v_\Delta$ denotes the triplet vacuum expectation value and $\alpha$ is the mixing angle between the singlet Higgs boson and the standard model-like Higgs boson. Although the diphoton decay rate can be enhanced by charged Higgs bosons running in the loop in this region, it is mostly orders of magnitude smaller than that required for the observed production rate, except for the small $v_\Delta$ region when the diphoton fusion production mechanism becomes dominant. Nonetheless, this part of parameter space suffers from the problems of breakdown of perturbativity and large uncertainties in the photon parton distribution function of proton.
[ { "created": "Sun, 24 Jan 2016 15:15:15 GMT", "version": "v1" }, { "created": "Wed, 3 Feb 2016 09:15:52 GMT", "version": "v2" }, { "created": "Fri, 26 Feb 2016 09:34:25 GMT", "version": "v3" }, { "created": "Wed, 20 Jul 2016 05:12:22 GMT", "version": "v4" } ]
2016-07-27
[ [ "Chiang", "Cheng-Wei", "" ], [ "Kuo", "An-Li", "" ] ]
The observation of diphoton excess around the mass of 750 GeV in LHC Run-II motivates us to consider whether the singlet Higgs boson in the custodial Higgs triplet model can serve as a good candidate because an earlier study of comprehensive parameter scan shows that it can have the right mass in the viable mass spectra. By assuming the singlet Higgs mass at 750 GeV, its total width less than 50 GeV and imposing constraints from the LHC 8-TeV data, we identify an approximately linear region on the $(v_\Delta, \alpha)$ plane along which the exotic Higgs boson masses satisfy a specific hierarchy and have lower possible spectra, where $v_\Delta$ denotes the triplet vacuum expectation value and $\alpha$ is the mixing angle between the singlet Higgs boson and the standard model-like Higgs boson. Although the diphoton decay rate can be enhanced by charged Higgs bosons running in the loop in this region, it is mostly orders of magnitude smaller than that required for the observed production rate, except for the small $v_\Delta$ region when the diphoton fusion production mechanism becomes dominant. Nonetheless, this part of parameter space suffers from the problems of breakdown of perturbativity and large uncertainties in the photon parton distribution function of proton.
hep-ph/9604275
Jerry Franklin
Jerrold Franklin
Application of Sum rules to heavy baryon masses
5 pages Latex. The replacement clarifies the discussion on the first two pages
Phys.Rev. D55 (1997) 423-424
10.1103/PhysRevD.55.423
TUHE-9641
hep-ph
null
Model independent sum rules are applied to recent measurements of heavy c-baryon and d-baryon masses. The sum rules are generally satisfied to the same degree as for the light (u,d,s) baryons.
[ { "created": "Tue, 9 Apr 1996 18:18:07 GMT", "version": "v1" }, { "created": "Wed, 10 Apr 1996 17:58:03 GMT", "version": "v2" } ]
2009-10-28
[ [ "Franklin", "Jerrold", "" ] ]
Model independent sum rules are applied to recent measurements of heavy c-baryon and d-baryon masses. The sum rules are generally satisfied to the same degree as for the light (u,d,s) baryons.
2211.08885
Anderson Kohara
Anderson Kendi Kohara
Observation of two zeros of the real amplitude in pp scattering at LHC energies
4 pages and 4 figures
null
null
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Elastic scattering of charged hadrons is described by the combination of nuclear and Coulomb amplitudes. It is well know that at the very forward range the nuclear real and Coulomb parts interplay a crucial role in the determination of the magnitude of the real part at $|t|=0$. However, beyond $|t|=0$ the real and imaginary nuclear amplitudes have different $t$ dependencies and we show that at LHC energies the zeros formed by the combination $T_C(t)+T_R^N(s,t)=0$ in pp process can be potentially observed when the background due to the imaginary part is removed. This observation constrains the real part at this forward range.
[ { "created": "Wed, 16 Nov 2022 12:47:44 GMT", "version": "v1" }, { "created": "Mon, 16 Jan 2023 08:40:47 GMT", "version": "v2" } ]
2023-01-18
[ [ "Kohara", "Anderson Kendi", "" ] ]
Elastic scattering of charged hadrons is described by the combination of nuclear and Coulomb amplitudes. It is well know that at the very forward range the nuclear real and Coulomb parts interplay a crucial role in the determination of the magnitude of the real part at $|t|=0$. However, beyond $|t|=0$ the real and imaginary nuclear amplitudes have different $t$ dependencies and we show that at LHC energies the zeros formed by the combination $T_C(t)+T_R^N(s,t)=0$ in pp process can be potentially observed when the background due to the imaginary part is removed. This observation constrains the real part at this forward range.
hep-ph/9507421
Lev F. M.
Felix M. Lev
Effect of Binding in Deep Inelastic Scattering Revisited
41 pages. The revised version is self-contained and additional arguments that perturbative QCD does not apply to DIS are given
null
null
null
hep-ph
null
In the Bjorken limit of the present theory of deep inelastic scattering (DIS) the structure functions (up to anomalous dimensions and perturbative QCD corrections) are described by the parton model. However the current operator in the parton model does not properly commute with the representation operators corresponding to the Lorentz group, space reflection and time reversal. To investigate the violation of these symmetries in the parton model we consider a model in which the current operator explicitly satisfies extended Poincare invariance and current conservation. It is shown that due to binding of quarks in the nucleon the Bjorken variable x no longer can be interpreted as the internal light cone momentum fraction $\xi$ even in the Bjorken limit. As a result, the data on DIS alone do not make it possible to determine the $\xi$ distribution of quarks in the nucleon. We also consider a qualitative explanation of the fact that in the parton model the values given by the sum rules exceed the corresponding experimental quantities while the quark contribution to the nucleon momentum and spin is underestimated.
[ { "created": "Wed, 26 Jul 1995 11:53:35 GMT", "version": "v1" }, { "created": "Wed, 6 Nov 1996 13:10:14 GMT", "version": "v2" } ]
2008-02-03
[ [ "Lev", "Felix M.", "" ] ]
In the Bjorken limit of the present theory of deep inelastic scattering (DIS) the structure functions (up to anomalous dimensions and perturbative QCD corrections) are described by the parton model. However the current operator in the parton model does not properly commute with the representation operators corresponding to the Lorentz group, space reflection and time reversal. To investigate the violation of these symmetries in the parton model we consider a model in which the current operator explicitly satisfies extended Poincare invariance and current conservation. It is shown that due to binding of quarks in the nucleon the Bjorken variable x no longer can be interpreted as the internal light cone momentum fraction $\xi$ even in the Bjorken limit. As a result, the data on DIS alone do not make it possible to determine the $\xi$ distribution of quarks in the nucleon. We also consider a qualitative explanation of the fact that in the parton model the values given by the sum rules exceed the corresponding experimental quantities while the quark contribution to the nucleon momentum and spin is underestimated.
0707.3342
S. Weinzierl
Stefan Weinzierl
Automated calculations for multi-leg processes
43 pages, plenary talk given at the ACAT 07 conference, Amsterdam, 2007; v2: references added
PoS ACAT:005,2007
null
null
hep-ph
null
The search for signals of new physics at the forthcoming LHC experiments involves the analysis of final states characterised by a high number of hadronic jets or identified particles. Precise theoretical predictions for these processes require the computation of scattering amplitudes with a large number of external particles and beyond leading order in perturbation theory. The complexity of a calculation grows with the number of internal loops as well as with the number of external legs. Automatisation of at least next-to-leading order calculations for LHC processes is therefore a timely task. I will discuss various approaches.
[ { "created": "Mon, 23 Jul 2007 09:26:46 GMT", "version": "v1" }, { "created": "Thu, 26 Jul 2007 12:07:13 GMT", "version": "v2" } ]
2009-04-16
[ [ "Weinzierl", "Stefan", "" ] ]
The search for signals of new physics at the forthcoming LHC experiments involves the analysis of final states characterised by a high number of hadronic jets or identified particles. Precise theoretical predictions for these processes require the computation of scattering amplitudes with a large number of external particles and beyond leading order in perturbation theory. The complexity of a calculation grows with the number of internal loops as well as with the number of external legs. Automatisation of at least next-to-leading order calculations for LHC processes is therefore a timely task. I will discuss various approaches.
0802.1209
Hanqing Zheng
Hanqing Zheng
Low Lying Scalar Resonances and Chiral Symmetry
Invited plenary talk given at CHIRAL 2007, Nov. 13-16, 2007, RCNP, Osaka, Japan
Mod.Phys.Lett.A23:2218-2225,2008
10.1142/S021773230802906X
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Current theoretical studies on the $\sigma$ and $\kappa$ resonances are reviewed. It is emphasized that all evidences accumulated so far are consistent with the picture that the $\sigma$ meson is the chiral partner of the Nambu--Goldstone bosons in a linear realization of chiral symmetry.
[ { "created": "Fri, 8 Feb 2008 20:52:04 GMT", "version": "v1" } ]
2008-11-26
[ [ "Zheng", "Hanqing", "" ] ]
Current theoretical studies on the $\sigma$ and $\kappa$ resonances are reviewed. It is emphasized that all evidences accumulated so far are consistent with the picture that the $\sigma$ meson is the chiral partner of the Nambu--Goldstone bosons in a linear realization of chiral symmetry.
1411.2780
Jambul Gegelia
J. Gegelia, U.-G. Mei{\ss}ner
Properties of effective massive Yang-Mills theory in the limit of vanishing vector boson mass
12 pages, 4 figures
null
10.1140/epja/i2014-14174-x
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Two-loop corrections to the pole mass of the vector boson and the pole masses and the magnetic moments of fermions are calculated in the framework of an effective field theory of massive Yang-Mills fields interacting with fermions. It is shown that the limit of vanishing vector boson mass is finite for all these quantities. Implications of the obtained results are discussed.
[ { "created": "Tue, 11 Nov 2014 12:36:43 GMT", "version": "v1" } ]
2015-06-23
[ [ "Gegelia", "J.", "" ], [ "Meißner", "U. -G.", "" ] ]
Two-loop corrections to the pole mass of the vector boson and the pole masses and the magnetic moments of fermions are calculated in the framework of an effective field theory of massive Yang-Mills fields interacting with fermions. It is shown that the limit of vanishing vector boson mass is finite for all these quantities. Implications of the obtained results are discussed.
2009.07193
Zhun Lu
Hui Li, Xiaoyu Wang, Yongliang Yang, Zhun Lu
The transverse polarization of $\Lambda$ hyperons in $e^+e^-\to\Lambda^\uparrow h X$ processes within TMD factorization
Title changed
Eur.Phys.J. C81 (2021) no.4, 289
10.1140/epjc/s10052-021-09064-1
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate the transverse polarization of the $\Lambda$ hyperon in the processes $e^+e^-\to\Lambda^\uparrow \pi^\pm X$ and $e^+e^-\to\Lambda^\uparrow K^\pm X$ within the framework of the transverse momentum dependent~(TMD) factorization. The transverse polarization is contributed by the convolution of the transversely polarizing fragmentation function~(PFF) $D_{1T}^\perp$ of the lambda hyperon and the unpolarized fragmentation function $D_1$ of pion/kaon. We adopt the spectator diquark model result for $D_{1T}^{\perp}$ to numerically estimate the transverse polarization in $e^+e^-\to\Lambda^\uparrow h X$ process at the kinematical region of Belle Collaboration. To implement the TMD evolution formalism of the fragmentation functions, we apply two different parametrizations on the nonperturbative Sudakov form factors associated with the fragmentation functions of the $\Lambda$, pion and kaon. It is found that our prediction on the polarization in the $\Lambda \pi^+$ production and $\bar{\Lambda} \pi^-$ is consistent with the recent Belle measurement in size and sign, while the model predictions on the polarizations in $\Lambda\pi^-$ and $\Lambda K^\pm$ productions show strong disagreement with the Belle data. The reason for the discrepancies is discussed and possible approaches to improve the calculation in the future are also discussed.
[ { "created": "Tue, 15 Sep 2020 16:01:30 GMT", "version": "v1" }, { "created": "Tue, 6 Apr 2021 02:28:39 GMT", "version": "v2" }, { "created": "Fri, 23 Apr 2021 12:32:40 GMT", "version": "v3" } ]
2021-04-26
[ [ "Li", "Hui", "" ], [ "Wang", "Xiaoyu", "" ], [ "Yang", "Yongliang", "" ], [ "Lu", "Zhun", "" ] ]
We investigate the transverse polarization of the $\Lambda$ hyperon in the processes $e^+e^-\to\Lambda^\uparrow \pi^\pm X$ and $e^+e^-\to\Lambda^\uparrow K^\pm X$ within the framework of the transverse momentum dependent~(TMD) factorization. The transverse polarization is contributed by the convolution of the transversely polarizing fragmentation function~(PFF) $D_{1T}^\perp$ of the lambda hyperon and the unpolarized fragmentation function $D_1$ of pion/kaon. We adopt the spectator diquark model result for $D_{1T}^{\perp}$ to numerically estimate the transverse polarization in $e^+e^-\to\Lambda^\uparrow h X$ process at the kinematical region of Belle Collaboration. To implement the TMD evolution formalism of the fragmentation functions, we apply two different parametrizations on the nonperturbative Sudakov form factors associated with the fragmentation functions of the $\Lambda$, pion and kaon. It is found that our prediction on the polarization in the $\Lambda \pi^+$ production and $\bar{\Lambda} \pi^-$ is consistent with the recent Belle measurement in size and sign, while the model predictions on the polarizations in $\Lambda\pi^-$ and $\Lambda K^\pm$ productions show strong disagreement with the Belle data. The reason for the discrepancies is discussed and possible approaches to improve the calculation in the future are also discussed.
hep-ph/9904395
Jose Espinosa
J. A. Casas, J. R. Espinosa, A. Ibarra and I. Navarro
Naturalness of nearly degenerate neutrinos
25 pages, LaTeX, 6 ps figures, psfig.sty. Typos, references and minor details corrected. Additional condition for the MSW mechanism incorporated. New viable textures added
Nucl.Phys. B556 (1999) 3-22
10.1016/S0550-3213(99)00383-1
null
hep-ph
null
If neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal mixing scenario, finding that (i) the vacuum oscillations solution to the solar neutrino problem is always excluded; (ii) if the mass matrix is produced by a see-saw mechanism, there are large regions of the parameter space consistent with the large angle MSW solution, providing a natural origin for the $\Delta m^2_{sol} << \Delta m^2_{atm}$ hierarchy; (iii) the bimaximal structure becomes then stable under radiative corrections. We also provide analytical expressions for the mass splittings and mixing angles and present a particularly simple see-saw ansatz consistent with all observations.
[ { "created": "Mon, 19 Apr 1999 17:49:20 GMT", "version": "v1" }, { "created": "Mon, 3 May 1999 17:07:08 GMT", "version": "v2" } ]
2009-10-31
[ [ "Casas", "J. A.", "" ], [ "Espinosa", "J. R.", "" ], [ "Ibarra", "A.", "" ], [ "Navarro", "I.", "" ] ]
If neutrinos are to play a relevant cosmological role, they must be essentially degenerate. We study whether radiative corrections can or cannot be responsible for the small mass splittings, in agreement with all the available experimental data. We perform an exhaustive exploration of the bimaximal mixing scenario, finding that (i) the vacuum oscillations solution to the solar neutrino problem is always excluded; (ii) if the mass matrix is produced by a see-saw mechanism, there are large regions of the parameter space consistent with the large angle MSW solution, providing a natural origin for the $\Delta m^2_{sol} << \Delta m^2_{atm}$ hierarchy; (iii) the bimaximal structure becomes then stable under radiative corrections. We also provide analytical expressions for the mass splittings and mixing angles and present a particularly simple see-saw ansatz consistent with all observations.
hep-ph/9708232
Peter Gosdzinsky
J. Bijnens, P. Gosdzinsky and P. Talavera
Matching the Heavy Vector Meson Theory
11 pages, 2 figures, revtex
JHEP 9801:014,1998
10.1088/1126-6708/1998/01/014
LU TP 97/16; NORDITA-97/50 N/P
hep-ph
null
We show how to obtain a ``heavy'' meson effective lagrangian for the case where the number of heavy particles is not conserved. We apply the method in a simple example at tree level and perform then the reduction for the case of vector mesons in Chiral Perturbation Theory in a manifestly chiral invariant fashion. Some examples showing that ``heavy'' meson effective theory also works at the one-loop level are included.
[ { "created": "Mon, 4 Aug 1997 14:09:48 GMT", "version": "v1" } ]
2010-02-03
[ [ "Bijnens", "J.", "" ], [ "Gosdzinsky", "P.", "" ], [ "Talavera", "P.", "" ] ]
We show how to obtain a ``heavy'' meson effective lagrangian for the case where the number of heavy particles is not conserved. We apply the method in a simple example at tree level and perform then the reduction for the case of vector mesons in Chiral Perturbation Theory in a manifestly chiral invariant fashion. Some examples showing that ``heavy'' meson effective theory also works at the one-loop level are included.
1906.09475
Sandeep Joshi
Sandeep Joshi, Sudhir R. Jain
Neutrino spin-flavor oscillations in solar environment
Published in Res.Astron.Astrophys
RAA 2020 Vol. 20 No. 8, 123(10pp)
10.1088/1674-4527/20/8/123
null
hep-ph astro-ph.SR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the phenomenon of neutrino spin-flavor oscillations due to solar magnetic fields. This allows us to examine how significantly the electron neutrinos produced in the solar interior undergo a resonant spin-flavor conversion. We construct analytical models for the solar magnetic field in all the three regions of the Sun. Neutrino spin-flavor oscillations in these magnetic fields are examined by studying the level crossing phenomenon and comparing the two cases of zero and non-zero vacuum mixing respectively. Results from the Borexino experiment are used to place an upper limit on the magnetic field in the solar core. Related phenomena such as effects of matter on neutrino spin transitions and differences between Dirac and Majorana transitions in the solar magnetic fields are also discussed.
[ { "created": "Sat, 22 Jun 2019 17:47:17 GMT", "version": "v1" }, { "created": "Fri, 7 Feb 2020 12:55:17 GMT", "version": "v2" }, { "created": "Mon, 10 Feb 2020 18:51:24 GMT", "version": "v3" }, { "created": "Tue, 18 Aug 2020 15:36:58 GMT", "version": "v4" } ]
2020-09-02
[ [ "Joshi", "Sandeep", "" ], [ "Jain", "Sudhir R.", "" ] ]
We study the phenomenon of neutrino spin-flavor oscillations due to solar magnetic fields. This allows us to examine how significantly the electron neutrinos produced in the solar interior undergo a resonant spin-flavor conversion. We construct analytical models for the solar magnetic field in all the three regions of the Sun. Neutrino spin-flavor oscillations in these magnetic fields are examined by studying the level crossing phenomenon and comparing the two cases of zero and non-zero vacuum mixing respectively. Results from the Borexino experiment are used to place an upper limit on the magnetic field in the solar core. Related phenomena such as effects of matter on neutrino spin transitions and differences between Dirac and Majorana transitions in the solar magnetic fields are also discussed.
hep-ph/0210191
Isabela Porto Cavalcante
Isabela P. Cavalcante, J. Sa Borges
Unitarized pion-nucleon scattering amplitude from inverse amplitude method
6 pages, 3 figures
Nucl.Phys. A720 (2003) 87-94
10.1016/S0375-9474(03)00669-9
null
hep-ph
null
In a recent work on low energy pion-nucleon scattering, instead of using chiral perturbation theory (ChPT) amplitude, we started from a pion-nucleon {\it soft-pion} result and used elastic unitarity directly as a dynamical constraint to construct first-order unitarity corrected amplitudes. The resulting amplitudes are crossing symmetric but, as the ChPT ones, satisfy only approximate unitarity relation. In the present work, we reconsider our approach and we apply the inverse amplitude method (IAM) in order to access the energy resonance region. We present the resulting S- and P-wave phase shifts that are shown to be in qualitative agreement with experimental data.
[ { "created": "Sat, 12 Oct 2002 16:27:58 GMT", "version": "v1" }, { "created": "Thu, 30 Jan 2003 19:07:51 GMT", "version": "v2" } ]
2009-11-07
[ [ "Cavalcante", "Isabela P.", "" ], [ "Borges", "J. Sa", "" ] ]
In a recent work on low energy pion-nucleon scattering, instead of using chiral perturbation theory (ChPT) amplitude, we started from a pion-nucleon {\it soft-pion} result and used elastic unitarity directly as a dynamical constraint to construct first-order unitarity corrected amplitudes. The resulting amplitudes are crossing symmetric but, as the ChPT ones, satisfy only approximate unitarity relation. In the present work, we reconsider our approach and we apply the inverse amplitude method (IAM) in order to access the energy resonance region. We present the resulting S- and P-wave phase shifts that are shown to be in qualitative agreement with experimental data.
hep-ph/0010149
J.-Alexis Rodriguez L.
R. Diaz, R. Martinez and J.-Alexis Rodriguez
Lepton Flavor Violation in the Two Higgs Doublet Model type III
7 pages RevTeX4, 4 figures postscript, new section added and some new references
Phys.Rev.D63:095007,2001
10.1103/PhysRevD.63.095007
null
hep-ph
null
We consider the Two Higgs Doublet Model (2HDM) of type III which leads to Flavour Changing Neutral Currents (FCNC) at tree level in the leptonic sector. In the framework of this model we can have, in principle, two situations: the case (a) when both doublets acquire a vacuum expectation value different from zero and the case (b) when only one of them is not zero. In addition, we show that we can make two types of rotations for the flavor mixing matrices which generates four types of lagrangians, with the rotation of type I we recover the case (b) from the case (a) in the limit $\tan \beta \to \infty $, and with the rotation of type II we obtain the case (b) from (a) in the limit $\tan \beta \to 0. $Moreover, two of the four possible lagrangians correspond to the models of types I and II plus Flavor Changing (FC) interactions. The analitical expressions of the partial lepton number violating widths $\Gamma (\mu \to eee) $ and $\Gamma (\mu \to e\gamma) $are derived for the cases (a) and (b) and both types of rotations.$ $In all cases these widths go asymptotically to zero in the decoupling limit for all Higgses. We present from our analysis upper bounds for the flavour changing transition $\mu \to e,$ and we show that such bounds are sensitive to the VEV structure and the type of rotation utilized.
[ { "created": "Sat, 14 Oct 2000 23:03:27 GMT", "version": "v1" }, { "created": "Fri, 22 Dec 2000 17:24:54 GMT", "version": "v2" } ]
2014-11-17
[ [ "Diaz", "R.", "" ], [ "Martinez", "R.", "" ], [ "Rodriguez", "J. -Alexis", "" ] ]
We consider the Two Higgs Doublet Model (2HDM) of type III which leads to Flavour Changing Neutral Currents (FCNC) at tree level in the leptonic sector. In the framework of this model we can have, in principle, two situations: the case (a) when both doublets acquire a vacuum expectation value different from zero and the case (b) when only one of them is not zero. In addition, we show that we can make two types of rotations for the flavor mixing matrices which generates four types of lagrangians, with the rotation of type I we recover the case (b) from the case (a) in the limit $\tan \beta \to \infty $, and with the rotation of type II we obtain the case (b) from (a) in the limit $\tan \beta \to 0. $Moreover, two of the four possible lagrangians correspond to the models of types I and II plus Flavor Changing (FC) interactions. The analitical expressions of the partial lepton number violating widths $\Gamma (\mu \to eee) $ and $\Gamma (\mu \to e\gamma) $are derived for the cases (a) and (b) and both types of rotations.$ $In all cases these widths go asymptotically to zero in the decoupling limit for all Higgses. We present from our analysis upper bounds for the flavour changing transition $\mu \to e,$ and we show that such bounds are sensitive to the VEV structure and the type of rotation utilized.
2111.14884
Zahra Tabrizi
Varun Mathur, Ian M. Shoemaker and Zahra Tabrizi
Using DUNE to Shed Light on the Electromagnetic Properties of Neutrinos
17 pages, 8 figures, 1 table
null
10.1007/JHEP10(2022)041
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study future DUNE sensitivity to various electromagnetic couplings of neutrinos, including magnetic moments, milli-charges, and charge radii. The DUNE PRISM capabilities play a crucial role in constraining the electron flavored couplings. We find that DUNE will be able to place the strongest terrestrial constraint on the muon-neutrino magnetic moment by improving on LSND's bounds by roughly a factor of two, although Borexino's solar constraint will still be stronger. For the muon neutrino milli-charge DUNE can place the leading experimental bound, with two orders of magnitude improvement compared to the existing COHERENT constraint. Finally, DUNE may be able to test the SM prediction for the muon neutrino charge radius, by placing a constraint two times better than CHARM-II and CCFR experiments.
[ { "created": "Mon, 29 Nov 2021 19:00:38 GMT", "version": "v1" } ]
2022-10-26
[ [ "Mathur", "Varun", "" ], [ "Shoemaker", "Ian M.", "" ], [ "Tabrizi", "Zahra", "" ] ]
We study future DUNE sensitivity to various electromagnetic couplings of neutrinos, including magnetic moments, milli-charges, and charge radii. The DUNE PRISM capabilities play a crucial role in constraining the electron flavored couplings. We find that DUNE will be able to place the strongest terrestrial constraint on the muon-neutrino magnetic moment by improving on LSND's bounds by roughly a factor of two, although Borexino's solar constraint will still be stronger. For the muon neutrino milli-charge DUNE can place the leading experimental bound, with two orders of magnitude improvement compared to the existing COHERENT constraint. Finally, DUNE may be able to test the SM prediction for the muon neutrino charge radius, by placing a constraint two times better than CHARM-II and CCFR experiments.
hep-ph/0107267
Matsuoka Takeo
Y. Abe, C. Hattori, M. Ito, M. Matsuda, M. Matsunaga and T. Matsuoka
Flavor Symmetry on Non-Commutative Compact Space and $SU(6) \times SU(2)_R$ Model
28pages, Latex, no figures, Revised version includes some details
Prog.Theor.Phys. 106 (2001) 1275-1295
10.1143/PTP.106.1275
AUE-01-01/KGKU-01-01/MIE01-01
hep-ph
null
In the four-dimensional effective theory from string compactification discrete flavor symmetries arise from symmetric structure of the compactified space and generally contain both the $R$ symmetry and non-$R$ symmetry. We point out that a new type of non-Abelian flavor symmetry can also appear if the compact space is non- commutative. Introducing the dihedral group $D_4$ as such a new type of flavor symmetry together with the $R$ symmetry and non-$R$ symmetry in $SU(6) \times SU(2)_R$ model, we explain not only fermion mass hierarchies but also hierarchical energy scales including the breaking scale of the GUT-type gauge symmetry, intermediate Majorana masses of R-handed neutrinos and the scale of $\mu$-term.
[ { "created": "Thu, 26 Jul 2001 01:47:23 GMT", "version": "v1" }, { "created": "Thu, 11 Oct 2001 06:05:30 GMT", "version": "v2" } ]
2009-11-07
[ [ "Abe", "Y.", "" ], [ "Hattori", "C.", "" ], [ "Ito", "M.", "" ], [ "Matsuda", "M.", "" ], [ "Matsunaga", "M.", "" ], [ "Matsuoka", "T.", "" ] ]
In the four-dimensional effective theory from string compactification discrete flavor symmetries arise from symmetric structure of the compactified space and generally contain both the $R$ symmetry and non-$R$ symmetry. We point out that a new type of non-Abelian flavor symmetry can also appear if the compact space is non- commutative. Introducing the dihedral group $D_4$ as such a new type of flavor symmetry together with the $R$ symmetry and non-$R$ symmetry in $SU(6) \times SU(2)_R$ model, we explain not only fermion mass hierarchies but also hierarchical energy scales including the breaking scale of the GUT-type gauge symmetry, intermediate Majorana masses of R-handed neutrinos and the scale of $\mu$-term.
2312.05619
Ai-Jun Ma
Ai-Jun Ma, Wen-Fei Wang
Contributions of the subprocess $K^*_0(1430) \to K\eta^{\prime}$ in the charmless three-body $B$ meson decays
10 pages, 2 figures and 4 tables. Matching the published version in PRD
Phys. Rev. D 109, 056017 (2024)
10.1103/PhysRevD.109.056017
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the contributions for $K\eta^{\prime}$ pair originating from the scalar intermediate state $K_0^{*}(1430)$ in the three-body decays $B\to K\eta^{\prime} h$ ($h=\pi, K$) within the perturbative QCD approach. The contribution of $K^*_0(1430)\to K\eta^{\prime}$ is described by the Flatt${\rm \acute{e}}$ formula with coupled channels $K\pi$, $K\eta$ and $K\eta^{\prime}$. The strong coupling constants $g_{K^*_0K\eta^{(\prime)}}$ are extracted from $g_{K^*_0 K\pi}$ within flavor SU$(3)$ symmetry. In spite of the strong depression by phase space near the threshold of $K\eta^\prime$, the $CP$ averaged branching fractions for the $B\to K^*_0(1430) h \to K\eta^\prime h$ decays are predicted to be on the order of $10^{-8}$ to $10^{-5}$, which are non-negligible for the corresponding three-body $B$ decays. Since the K$\eta$ system is almost decoupled from the even-spin strange mesons under flavor SU$(3)$ symmetry, those quasi-two-body $B$ decays with subprocess $K^*_0(1430) \to K \eta$ shall have quite small branching ratios and are not taken into account in this work. We also estimate that the branching fraction for $K_0^{*}(1430)\to K\eta^{\prime}$ is about one fifth of that for $K_0^{*}(1430)\to K\pi$. The predictions for the relevant decays are expected to be tested by the LHCb and Belle-II experiments in the future.
[ { "created": "Sat, 9 Dec 2023 17:24:00 GMT", "version": "v1" }, { "created": "Wed, 20 Mar 2024 09:21:58 GMT", "version": "v2" } ]
2024-03-21
[ [ "Ma", "Ai-Jun", "" ], [ "Wang", "Wen-Fei", "" ] ]
We study the contributions for $K\eta^{\prime}$ pair originating from the scalar intermediate state $K_0^{*}(1430)$ in the three-body decays $B\to K\eta^{\prime} h$ ($h=\pi, K$) within the perturbative QCD approach. The contribution of $K^*_0(1430)\to K\eta^{\prime}$ is described by the Flatt${\rm \acute{e}}$ formula with coupled channels $K\pi$, $K\eta$ and $K\eta^{\prime}$. The strong coupling constants $g_{K^*_0K\eta^{(\prime)}}$ are extracted from $g_{K^*_0 K\pi}$ within flavor SU$(3)$ symmetry. In spite of the strong depression by phase space near the threshold of $K\eta^\prime$, the $CP$ averaged branching fractions for the $B\to K^*_0(1430) h \to K\eta^\prime h$ decays are predicted to be on the order of $10^{-8}$ to $10^{-5}$, which are non-negligible for the corresponding three-body $B$ decays. Since the K$\eta$ system is almost decoupled from the even-spin strange mesons under flavor SU$(3)$ symmetry, those quasi-two-body $B$ decays with subprocess $K^*_0(1430) \to K \eta$ shall have quite small branching ratios and are not taken into account in this work. We also estimate that the branching fraction for $K_0^{*}(1430)\to K\eta^{\prime}$ is about one fifth of that for $K_0^{*}(1430)\to K\pi$. The predictions for the relevant decays are expected to be tested by the LHCb and Belle-II experiments in the future.
hep-ph/9812338
Nikolaos Irges
Nikolaos Irges
Anomalous U(1), holomorphy, supersymmetry breaking and dilaton stabilization
14 pages, no figures; wording of the abstract is changed
Phys.Rev. D59 (1999) 115008
10.1103/PhysRevD.59.115008
null
hep-ph
null
We argue that in certain models with family symmetries the implementation of the alignment mechanism for the supression of the flavor changing neutral currents requires mass matrices with holomorphic zeros in the down quark sector. Holomorphic zeros typically open flat directions that potentially spoil the uniqueness of the supersymmetric vacuum. We then present an anomalous U(1) model without holomorphic zeros in the quark sector that can reproduce the fermion mass hierarchies, provided that $\tan{\beta}$ is of order one. To avoid undesired flavor changing neutral currents we propose a supersymmetry breaking mechanism and a dilaton stabilization scenario that result in degenerate squarks at $M\sim M_{GUT}$ and a calculable low energy spectrum. We present the numerical predictions of this model for the Higgs mass for different values of $M$ and $\tan{\beta}$.
[ { "created": "Fri, 11 Dec 1998 20:32:09 GMT", "version": "v1" }, { "created": "Tue, 16 Feb 1999 16:16:58 GMT", "version": "v2" }, { "created": "Wed, 14 Apr 1999 14:35:04 GMT", "version": "v3" }, { "created": "Sat, 17 Jul 2004 07:21:42 GMT", "version": "v4" } ]
2009-10-31
[ [ "Irges", "Nikolaos", "" ] ]
We argue that in certain models with family symmetries the implementation of the alignment mechanism for the supression of the flavor changing neutral currents requires mass matrices with holomorphic zeros in the down quark sector. Holomorphic zeros typically open flat directions that potentially spoil the uniqueness of the supersymmetric vacuum. We then present an anomalous U(1) model without holomorphic zeros in the quark sector that can reproduce the fermion mass hierarchies, provided that $\tan{\beta}$ is of order one. To avoid undesired flavor changing neutral currents we propose a supersymmetry breaking mechanism and a dilaton stabilization scenario that result in degenerate squarks at $M\sim M_{GUT}$ and a calculable low energy spectrum. We present the numerical predictions of this model for the Higgs mass for different values of $M$ and $\tan{\beta}$.
hep-ph/0110259
Carl Albright
Carl H. Albright (Fermilab/Northern Illinois U.)
SO(10) SUSY GUT Model with a U(1) x Z_2 x Z_2 Flavor Symmetry
3 pages including 2 figures submitted for proceedings of the Snowmass Workshop on the Future of Particle Physics, 30 June - 21 July 2001
eConfC010630:P203,2001
null
FERMILAB-Conf-01/306-T
hep-ph
null
An SO(10) SUSY GUT model which leads to maximal atmospheric neutrino mixing and the LMA solar neutrino solution, developed in collaboration with S.M. Barr, is briefly described. Since the model is quantitatively predictive, it can be used to assess the need for a neutrino factory, as shown in collaboration with S. Geer.
[ { "created": "Thu, 18 Oct 2001 16:53:25 GMT", "version": "v1" } ]
2008-11-26
[ [ "Albright", "Carl H.", "", "Fermilab/Northern Illinois U." ] ]
An SO(10) SUSY GUT model which leads to maximal atmospheric neutrino mixing and the LMA solar neutrino solution, developed in collaboration with S.M. Barr, is briefly described. Since the model is quantitatively predictive, it can be used to assess the need for a neutrino factory, as shown in collaboration with S. Geer.
1101.5326
Shinya Matsuzaki
Ki-Young Choi, Deog Ki Hong and Shinya Matsuzaki
Techni-dilaton as Dark Matter
6 pages, 2 figures; version to appear in PLB
null
10.1016/j.physletb.2011.11.013
PNUTP-11-A01
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We propose a new dark matter candidate, {\it light decoupled techni-dilaton}, which arises from the almost scale-invariant/conformal (walking) technicolor. We investigate its characteristic nature and discuss several cosmological and astrophysical constraints. It turns out that techni-dilatons are extremely weakly interacting and produced dominantly by the non-thermal mechanism to be the main component of dark matter with mass range between around 0.01 eV and 500 eV for typical walking technicolor scenarios.
[ { "created": "Thu, 27 Jan 2011 16:19:42 GMT", "version": "v1" }, { "created": "Tue, 1 Feb 2011 05:24:50 GMT", "version": "v2" }, { "created": "Mon, 25 Apr 2011 06:32:11 GMT", "version": "v3" }, { "created": "Sat, 5 Nov 2011 05:59:16 GMT", "version": "v4" } ]
2015-05-27
[ [ "Choi", "Ki-Young", "" ], [ "Hong", "Deog Ki", "" ], [ "Matsuzaki", "Shinya", "" ] ]
We propose a new dark matter candidate, {\it light decoupled techni-dilaton}, which arises from the almost scale-invariant/conformal (walking) technicolor. We investigate its characteristic nature and discuss several cosmological and astrophysical constraints. It turns out that techni-dilatons are extremely weakly interacting and produced dominantly by the non-thermal mechanism to be the main component of dark matter with mass range between around 0.01 eV and 500 eV for typical walking technicolor scenarios.
hep-ph/0212365
Mairi Sakellariadou
Mairi Sakellariadou (University of Athens)
The role of topologigal defects in cosmology
Invited lectures in the NATO ASI / COSLAB (ESF) School ``Patterns of symmetry breaking'', September 2002 (Cracow). 28 pages
null
null
null
hep-ph astro-ph gr-qc
null
Topological defects are involved in a plethora of physical and astrophysical phenomena. In these lectures, I will review the r\^ ole they could play in the large-scale structure formation and the anisotropies of the cosmic microwave background, as well as in various high energy phenomena, including baryon number asymmetry, ultra-high energy cosmic rays, and gamma ray bursts. I will then summarize the gravitational effects of cosmic strings. Finally, I will briefly discuss the r\^ ole of topological defects in brane world cosmology.
[ { "created": "Wed, 25 Dec 2002 17:40:00 GMT", "version": "v1" } ]
2007-05-23
[ [ "Sakellariadou", "Mairi", "", "University of Athens" ] ]
Topological defects are involved in a plethora of physical and astrophysical phenomena. In these lectures, I will review the r\^ ole they could play in the large-scale structure formation and the anisotropies of the cosmic microwave background, as well as in various high energy phenomena, including baryon number asymmetry, ultra-high energy cosmic rays, and gamma ray bursts. I will then summarize the gravitational effects of cosmic strings. Finally, I will briefly discuss the r\^ ole of topological defects in brane world cosmology.
hep-ph/0410298
Jose Ramon Espinosa
J.A. Casas, J.R. Espinosa and I. Hidalgo
Implications for New Physics from Fine-Tuning Arguments: I. Application to SUSY and Seesaw Cases
24 pages, LaTeX, 5 ps figures
JHEP0411:057,2004
10.1088/1126-6708/2004/11/057
IFT-UAM/CSIC-04-57
hep-ph
null
We revisit the standard argument to estimate the scale of new physics (NP) beyond the SM, based on the sensitivity of the Higgs mass to quadratic divergences. Although this argument is arguably naive, the corresponding estimate, Lambda_SM < 2-3 TeV, works reasonably well in most cases and should be considered a conservative bound, as it ignores other contributions to the Higgs mass which are potentially large. Besides, the possibility of an accidental Veltman-like cancellation does not raise significantly Lambda_SM. One can obtain more precise implications from fine-tuning arguments in specific examples of NP. Here we consider SUSY and right-handed (seesaw) neutrinos. SUSY is a typical example for which the previous general estimate is indeed conservative: the MSSM is fine-tuned a few %, even for soft masses of a few hundred GeV. In contrast, other SUSY scenarios, in particular those with low-scale SUSY breaking, can easily saturate the general bound on Lambda_SM. The seesaw mechanism requires large fine-tuning if M_R > 10^7 GeV, unless there is additional NP (SUSY being a favourite option).
[ { "created": "Thu, 21 Oct 2004 17:10:35 GMT", "version": "v1" } ]
2008-11-26
[ [ "Casas", "J. A.", "" ], [ "Espinosa", "J. R.", "" ], [ "Hidalgo", "I.", "" ] ]
We revisit the standard argument to estimate the scale of new physics (NP) beyond the SM, based on the sensitivity of the Higgs mass to quadratic divergences. Although this argument is arguably naive, the corresponding estimate, Lambda_SM < 2-3 TeV, works reasonably well in most cases and should be considered a conservative bound, as it ignores other contributions to the Higgs mass which are potentially large. Besides, the possibility of an accidental Veltman-like cancellation does not raise significantly Lambda_SM. One can obtain more precise implications from fine-tuning arguments in specific examples of NP. Here we consider SUSY and right-handed (seesaw) neutrinos. SUSY is a typical example for which the previous general estimate is indeed conservative: the MSSM is fine-tuned a few %, even for soft masses of a few hundred GeV. In contrast, other SUSY scenarios, in particular those with low-scale SUSY breaking, can easily saturate the general bound on Lambda_SM. The seesaw mechanism requires large fine-tuning if M_R > 10^7 GeV, unless there is additional NP (SUSY being a favourite option).
1501.00012
Ya-Juan Zheng
Xiao-Gang He, Guan-Nan Li, Ya-Juan Zheng
Probing Higgs Boson $CP$ Properties with $t\bar{t}H$ at the LHC and the 100 TeV $pp$ Collider
7 pages, 4 figures. v2: typos corrected and references added
null
10.1142/S0217751X15501560
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The Higgs boson $H$ has the largest coupling to the top quark $t$ among the standard model (SM) fermions. This is one of the ideal places to investigate new physics beyond SM. In this work, we study the potential of determining Higgs boson $CP$ properties at the LHC and future 33 TeV and 100 TeV $pp$ colliders by analysing various operators formed from final states variables in $t\bar{t}H$ production. The discrimination power from SM coupling is obtained with Higgs boson reconstructed from $ H\to \gamma \gamma$ and $ H\to b \bar{b}$. We find that $t\bar{t}b\bar{b}$ process can provide more than 3$\sigma$ discrimination power with 300 $fb^{-1}$ integrated luminosity in a wide range of allowed Higgs to top couplings for the LHC, the 33 TeV and 100 TeV colliders. For $t\bar{t}\gamma\gamma$ the discrimination power will be below 3$\sigma$ at the LHC, while for 33 TeV and 100 TeV colliders, more than 3$\sigma$ sensitivity can be reached.
[ { "created": "Tue, 30 Dec 2014 21:00:33 GMT", "version": "v1" }, { "created": "Sat, 10 Jan 2015 04:27:38 GMT", "version": "v2" } ]
2015-09-30
[ [ "He", "Xiao-Gang", "" ], [ "Li", "Guan-Nan", "" ], [ "Zheng", "Ya-Juan", "" ] ]
The Higgs boson $H$ has the largest coupling to the top quark $t$ among the standard model (SM) fermions. This is one of the ideal places to investigate new physics beyond SM. In this work, we study the potential of determining Higgs boson $CP$ properties at the LHC and future 33 TeV and 100 TeV $pp$ colliders by analysing various operators formed from final states variables in $t\bar{t}H$ production. The discrimination power from SM coupling is obtained with Higgs boson reconstructed from $ H\to \gamma \gamma$ and $ H\to b \bar{b}$. We find that $t\bar{t}b\bar{b}$ process can provide more than 3$\sigma$ discrimination power with 300 $fb^{-1}$ integrated luminosity in a wide range of allowed Higgs to top couplings for the LHC, the 33 TeV and 100 TeV colliders. For $t\bar{t}\gamma\gamma$ the discrimination power will be below 3$\sigma$ at the LHC, while for 33 TeV and 100 TeV colliders, more than 3$\sigma$ sensitivity can be reached.
hep-ph/0605023
Michal Czakon
R. Boughezal, M. Czakon, T. Schutzmeier
Charm and Bottom Quark Masses from Perturbative QCD
5 pages, 2 figures, final version as published
Phys.Rev.D74:074006,2006
10.1103/PhysRevD.74.074006
null
hep-ph
null
Using a new result for the first moment of the hadronic production cross section at order ${\cal O}(\alpha_s^3)$, and new data on the $J/\psi$ and $\psi'$ resonances for the charm quark, we determine the \msb masses of the charm and bottom quarks to be $\bar{m}_c(\bar{m}_c) = 1.295 \pm 0.015$ GeV and $\bar{m}_b(\bar{m}_b) = 4.205 \pm 0.058$ GeV. We assume that the continuum contribution to the sum rules is adequately described by pQCD. While we observe a large reduction of the perturbative error, the shifts induced by the theoretical input are very small. The main change in the central value of $m_c$ is related to the experimental data. On the other hand, the value of $m_b$ is not changed by our calculation to the assumed precision.
[ { "created": "Mon, 1 May 2006 19:16:45 GMT", "version": "v1" }, { "created": "Thu, 4 May 2006 13:52:14 GMT", "version": "v2" }, { "created": "Fri, 13 Oct 2006 21:03:39 GMT", "version": "v3" } ]
2008-11-26
[ [ "Boughezal", "R.", "" ], [ "Czakon", "M.", "" ], [ "Schutzmeier", "T.", "" ] ]
Using a new result for the first moment of the hadronic production cross section at order ${\cal O}(\alpha_s^3)$, and new data on the $J/\psi$ and $\psi'$ resonances for the charm quark, we determine the \msb masses of the charm and bottom quarks to be $\bar{m}_c(\bar{m}_c) = 1.295 \pm 0.015$ GeV and $\bar{m}_b(\bar{m}_b) = 4.205 \pm 0.058$ GeV. We assume that the continuum contribution to the sum rules is adequately described by pQCD. While we observe a large reduction of the perturbative error, the shifts induced by the theoretical input are very small. The main change in the central value of $m_c$ is related to the experimental data. On the other hand, the value of $m_b$ is not changed by our calculation to the assumed precision.
hep-ph/0106185
Sandipan Mohanty
Bo Andersson, Sandipan Mohanty, Fredrik Soderberg
The Lund Fragmentation Process for a Multi-gluon String According to the Area Law
1 title page + 36 pages, 20 figures
Eur.Phys.J.C21:631-647,2001
10.1007/s100520100757
LU TP 01-22
hep-ph
null
The Lund Area Law describes the probability for the production of a set of colourless hadrons from an initial set of partons, in the Lund string fragmentation model. In this paper we will present a general method to implement the Area Law for a multi-gluon string state. The partonic states are in general given by a perturbative QCD cascade and are consequently defined only down to a cutoff in the energy momentum fluctuations. We will show that our method defines the states down to the hadronic mass scale inside an analytically calculable scenario. We will then show that there is a differential version of our process which is closely related to the generalised rapidity range \lambda, which has been used as a measure on the partonic states. We identify \lambda as the area spanned between the directrix curve (the curve given by the parton energy momentum vectors laid out in colour order, which determines the string surface) and the average curve (to be called the P-curve) of the stochastic X-curves (curves obtained when the hadronic energy-momentum vectors are laid out in rank order). Finally we show that from the X-curve corresponding to a particular stochastic fragmentation situation it is possible to reproduce the directrix curve (up to one starting vector and a set of sign choices, one for each hadron).
[ { "created": "Sat, 16 Jun 2001 23:11:40 GMT", "version": "v1" } ]
2016-09-06
[ [ "Andersson", "Bo", "" ], [ "Mohanty", "Sandipan", "" ], [ "Soderberg", "Fredrik", "" ] ]
The Lund Area Law describes the probability for the production of a set of colourless hadrons from an initial set of partons, in the Lund string fragmentation model. In this paper we will present a general method to implement the Area Law for a multi-gluon string state. The partonic states are in general given by a perturbative QCD cascade and are consequently defined only down to a cutoff in the energy momentum fluctuations. We will show that our method defines the states down to the hadronic mass scale inside an analytically calculable scenario. We will then show that there is a differential version of our process which is closely related to the generalised rapidity range \lambda, which has been used as a measure on the partonic states. We identify \lambda as the area spanned between the directrix curve (the curve given by the parton energy momentum vectors laid out in colour order, which determines the string surface) and the average curve (to be called the P-curve) of the stochastic X-curves (curves obtained when the hadronic energy-momentum vectors are laid out in rank order). Finally we show that from the X-curve corresponding to a particular stochastic fragmentation situation it is possible to reproduce the directrix curve (up to one starting vector and a set of sign choices, one for each hadron).
2303.04022
Xiang Liu
Si-Qiang Luo, Xiang Liu
The newly observed $\Omega_c(3327)$: A good candidate for a $D$-wave charmed baryon
6 pages, 4 tables, 3 figures. Accepted by PRD
Phys. Rev. D 107, 074041 (2023)
10.1103/PhysRevD.107.074041
null
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The newly observed $\Omega_c(3327)$ gives us a good chance to construct the $\Omega_c$ charmed baryon family. In this work, we carry out the mass spectrum analysis by a non-relativistic potential model using Gaussian Expansion Method, and the study of its two-body Okubo-Zweig-Iizuka allowed strong decay behavior. Our results imply that the $\Omega_c(3327)$ is good candidate of $\Omega_c(1D)$ state with $J^P=5/2^+$. We also predict the spectroscopy behavior of other $\Omega_c(1D)$ states, which may provide further clues to their search.
[ { "created": "Tue, 7 Mar 2023 16:38:14 GMT", "version": "v1" }, { "created": "Wed, 5 Apr 2023 11:53:55 GMT", "version": "v2" } ]
2023-05-01
[ [ "Luo", "Si-Qiang", "" ], [ "Liu", "Xiang", "" ] ]
The newly observed $\Omega_c(3327)$ gives us a good chance to construct the $\Omega_c$ charmed baryon family. In this work, we carry out the mass spectrum analysis by a non-relativistic potential model using Gaussian Expansion Method, and the study of its two-body Okubo-Zweig-Iizuka allowed strong decay behavior. Our results imply that the $\Omega_c(3327)$ is good candidate of $\Omega_c(1D)$ state with $J^P=5/2^+$. We also predict the spectroscopy behavior of other $\Omega_c(1D)$ states, which may provide further clues to their search.
hep-ph/0003097
Peter Kroll
P. Kroll (Wuppertal Univ.)
The b-u skewed parton distributions
8 pages, 3 figures (using epsfig.sty, espcrc1.sty)
Nucl.Phys. A680 (2000) 37-42
10.1016/S0375-9474(00)00384-5
WU-B 00-05
hep-ph
null
The b - u skewed parton distributions (SPDs) are discussed. The SPDs allow an unambigous superposition of overlap and resonsance contributions and their zeroth order moments represent the B - pi transition form factors. The values of the form factors at maximum recoil are found to be F+(0)=F0(0)=0.22 with an error of 0.05 in agreement with measurements of the B - pi pi branching ratio. The branching ratios for the semi-leptonic B - pi decays are evaluated too.
[ { "created": "Fri, 10 Mar 2000 13:43:45 GMT", "version": "v1" } ]
2009-10-31
[ [ "Kroll", "P.", "", "Wuppertal Univ." ] ]
The b - u skewed parton distributions (SPDs) are discussed. The SPDs allow an unambigous superposition of overlap and resonsance contributions and their zeroth order moments represent the B - pi transition form factors. The values of the form factors at maximum recoil are found to be F+(0)=F0(0)=0.22 with an error of 0.05 in agreement with measurements of the B - pi pi branching ratio. The branching ratios for the semi-leptonic B - pi decays are evaluated too.
0909.2937
Seong Chan Park
Seong Chan Park, Kai Wang and Tsutomu T. Yanagida (Tokyo U., IPMU)
Neutrino mass from a hidden world and its phenomenological implications
11 pages, 2 figures
Phys.Lett.B685:309-312,2010
10.1016/j.physletb.2010.01.070
IPMU-09-0104
hep-ph
http://creativecommons.org/licenses/by/3.0/
We propose a model of neutrino mass generation in extra dimension. Allowing a large lepton number violation on a distant brane spatially separated from the standard model brane, a small neutrino mass is naturally generated due to an exponential suppression of the messenger field in the 5D bulk. The model accommodates a large Yukawa coupling with the singlet neutrino (n_R) which may change the standard Higgs search and can simultaneously accommodate visible lepton number violation at the electroweak scale, which leads to very interesting phenomenology at the CERN Large Hadron Collider.
[ { "created": "Wed, 16 Sep 2009 11:38:14 GMT", "version": "v1" } ]
2010-03-02
[ [ "Park", "Seong Chan", "", "Tokyo U., IPMU" ], [ "Wang", "Kai", "", "Tokyo U., IPMU" ], [ "Yanagida", "Tsutomu T.", "", "Tokyo U., IPMU" ] ]
We propose a model of neutrino mass generation in extra dimension. Allowing a large lepton number violation on a distant brane spatially separated from the standard model brane, a small neutrino mass is naturally generated due to an exponential suppression of the messenger field in the 5D bulk. The model accommodates a large Yukawa coupling with the singlet neutrino (n_R) which may change the standard Higgs search and can simultaneously accommodate visible lepton number violation at the electroweak scale, which leads to very interesting phenomenology at the CERN Large Hadron Collider.
0809.1301
Stefano Actis
S. Actis, G. Passarino, C. Sturm, S. Uccirati
NLO Electroweak Corrections to Higgs Boson Production at Hadron Colliders
LaTeX, 11 pages, 3 figures
Phys.Lett.B670:12-17,2008
10.1016/j.physletb.2008.10.018
PITHA 08/20, SFB/CPP-08-62, TTP08-38
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Results for the complete NLO electroweak corrections to Standard Model Higgs production via gluon fusion are included in the total cross section for hadronic collisions. Artificially large threshold effects are avoided working in the complex-mass scheme. The numerical impact at LHC (Tevatron) energies is explored for Higgs mass values up to 500 GeV (200 GeV). Assuming a complete factorization of the electroweak corrections, one finds a +5 % shift with respect to the NNLO QCD cross section for a Higgs mass of 120 GeV both at the LHC and the Tevatron. Adopting two different factorization schemes for the electroweak effects, an estimate of the corresponding total theoretical uncertainty is computed.
[ { "created": "Mon, 8 Sep 2008 09:41:54 GMT", "version": "v1" } ]
2008-12-18
[ [ "Actis", "S.", "" ], [ "Passarino", "G.", "" ], [ "Sturm", "C.", "" ], [ "Uccirati", "S.", "" ] ]
Results for the complete NLO electroweak corrections to Standard Model Higgs production via gluon fusion are included in the total cross section for hadronic collisions. Artificially large threshold effects are avoided working in the complex-mass scheme. The numerical impact at LHC (Tevatron) energies is explored for Higgs mass values up to 500 GeV (200 GeV). Assuming a complete factorization of the electroweak corrections, one finds a +5 % shift with respect to the NNLO QCD cross section for a Higgs mass of 120 GeV both at the LHC and the Tevatron. Adopting two different factorization schemes for the electroweak effects, an estimate of the corresponding total theoretical uncertainty is computed.
1803.05466
Patrick Foldenauer
Martin Bauer, Patrick Foldenauer, Joerg Jaeckel
Hunting All the Hidden Photons
44 pages, 20 figures, 4 tables, v2: added limits from BaBar/KLOE invisibles searches, added COHERENT limits from elastic neutrino-nucleus scattering, updated references v3: minor corrections: updated Electron beam dump limits (E137, E141, E774, Orsay) in Fig. 12, corrected discussion of hadron beam bumps, improved discussion of beam dump calculation in appendix
J. High Energ. Phys. (2018) 2018: 94
10.1007/JHEP07(2018)094
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We explore constraints on gauge bosons of a weakly coupled $U(1)_{B-L}$, $U(1)_{L_\mu-L_e}$, $U(1)_{L_e-L_\tau}$ and $U(1)_{L_\mu-L_\tau}$. To do so we apply the full constraining power of experimental bounds derived for a hidden photon of a secluded $U(1)_{X}$ and translate them to the considered gauge groups. In contrast to the secluded hidden photon that acquires universal couplings to charged Standard Model particles through kinetic mixing with the photon, for these gauge groups the couplings to the different Standard Model particles can vary widely. We take finite, computable loop-induced kinetic mixing effects into account, which provide additional sensitivity in a range of experiments. In addition, we collect and extend limits from neutrino experiments as well as astrophysical and cosmological observations and include new constraints from white dwarf cooling. We discuss the reach of future experiments in searching for these gauge bosons.
[ { "created": "Wed, 14 Mar 2018 18:33:37 GMT", "version": "v1" }, { "created": "Mon, 16 Jul 2018 12:57:02 GMT", "version": "v2" }, { "created": "Thu, 26 Sep 2019 12:03:42 GMT", "version": "v3" } ]
2019-09-27
[ [ "Bauer", "Martin", "" ], [ "Foldenauer", "Patrick", "" ], [ "Jaeckel", "Joerg", "" ] ]
We explore constraints on gauge bosons of a weakly coupled $U(1)_{B-L}$, $U(1)_{L_\mu-L_e}$, $U(1)_{L_e-L_\tau}$ and $U(1)_{L_\mu-L_\tau}$. To do so we apply the full constraining power of experimental bounds derived for a hidden photon of a secluded $U(1)_{X}$ and translate them to the considered gauge groups. In contrast to the secluded hidden photon that acquires universal couplings to charged Standard Model particles through kinetic mixing with the photon, for these gauge groups the couplings to the different Standard Model particles can vary widely. We take finite, computable loop-induced kinetic mixing effects into account, which provide additional sensitivity in a range of experiments. In addition, we collect and extend limits from neutrino experiments as well as astrophysical and cosmological observations and include new constraints from white dwarf cooling. We discuss the reach of future experiments in searching for these gauge bosons.
1608.04239
Dirk Rollmann
David E. Miller and Dirk Rollmann
Motion of Confined Particles
6 pages, 3 figures
Acta Physica Polonica B Proceedings Supplement, Vol. 10 Number 3 (2017) 699-673
10.5506/APhysPolBSupp.10.669
BI-TP 2016/07
hep-ph hep-th
http://creativecommons.org/licenses/by/4.0/
We carry out numerical evaluations of the motion of classical particles in Minkowski Space $\mathbb{M}^{4}$ which are confined to the inside of a bag. In particular, we analyze the structure of the paths evolving from the breaking of the dilatation symmetry, the conformal symmetry and the combination of both together. The confining forces arise directly from the corresponding nonconserved currents. We demonstrate in our evaluations that these particles under certain initial conditions move toward the interior of the bag.
[ { "created": "Mon, 15 Aug 2016 11:30:02 GMT", "version": "v1" }, { "created": "Tue, 5 Dec 2017 13:32:55 GMT", "version": "v2" } ]
2017-12-06
[ [ "Miller", "David E.", "" ], [ "Rollmann", "Dirk", "" ] ]
We carry out numerical evaluations of the motion of classical particles in Minkowski Space $\mathbb{M}^{4}$ which are confined to the inside of a bag. In particular, we analyze the structure of the paths evolving from the breaking of the dilatation symmetry, the conformal symmetry and the combination of both together. The confining forces arise directly from the corresponding nonconserved currents. We demonstrate in our evaluations that these particles under certain initial conditions move toward the interior of the bag.
1303.6636
Juan Rojo
Maxime Gouzevitch, Alexandra Oliveira, Juan Rojo, Rogerio Rosenfeld, Gavin P. Salam, Veronica Sanz
Scale-invariant resonance tagging in multijet events and new physics in Higgs pair production
38 pages, 17 figures, accepted for publication in JHEP
null
10.1007/JHEP07(2013)148
CERN-PH-TH/2012-311, ICTP-SAIFR/2013-003
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study resonant pair production of heavy particles in fully hadronic final states by means of jet substructure techniques. We propose a new resonance tagging strategy that smoothly interpolates between the highly boosted and fully resolved regimes, leading to uniform signal efficiencies and background rejection rates across a broad range of masses. Our method makes it possible to efficiently replace independent experimental searches, based on different final state topologies, with a single common analysis. As a case study, we apply our technique to pair production of Higgs bosons decaying into $b\bar{b}$ pairs in generic New Physics scenarios. We adopt as benchmark models radion and massive KK graviton production in warped extra dimensions. We find that despite the overwhelming QCD background, the $4b$ final state has enough sensitivity to provide a complementary handle in searches for enhanced Higgs pair production at the LHC.
[ { "created": "Tue, 26 Mar 2013 20:00:02 GMT", "version": "v1" }, { "created": "Tue, 9 Jul 2013 07:09:49 GMT", "version": "v2" } ]
2015-06-15
[ [ "Gouzevitch", "Maxime", "" ], [ "Oliveira", "Alexandra", "" ], [ "Rojo", "Juan", "" ], [ "Rosenfeld", "Rogerio", "" ], [ "Salam", "Gavin P.", "" ], [ "Sanz", "Veronica", "" ] ]
We study resonant pair production of heavy particles in fully hadronic final states by means of jet substructure techniques. We propose a new resonance tagging strategy that smoothly interpolates between the highly boosted and fully resolved regimes, leading to uniform signal efficiencies and background rejection rates across a broad range of masses. Our method makes it possible to efficiently replace independent experimental searches, based on different final state topologies, with a single common analysis. As a case study, we apply our technique to pair production of Higgs bosons decaying into $b\bar{b}$ pairs in generic New Physics scenarios. We adopt as benchmark models radion and massive KK graviton production in warped extra dimensions. We find that despite the overwhelming QCD background, the $4b$ final state has enough sensitivity to provide a complementary handle in searches for enhanced Higgs pair production at the LHC.
hep-ph/9308366
null
R. Casalbuoni, S. De Curtis and M. Grazzini
One Loop Calculation of the $\epsilon_3$ Parameter within the Extended Bess Model
p. 9, LATEX, DFF 186/7/1993
Phys.Lett. B317 (1993) 151-158
10.1016/0370-2693(93)91585-B
null
hep-ph
null
The existence of a strongly interacting sector responsible for the electroweak symmetry breaking is assumed. As a consequence vector and axial-vector bound states may be formed. These resonances mix with the Standard Model gauge bosons and are of primary phenomenological importance for the LEP physics. The extended BESS model is an effective scheme based on the symmetry group $SU(8)_L\otimes SU(8)_R$, describing in a consistent way the interactions among the pseudo-Goldstone bosons, vector and axial-vector resonances and the standard gauge bosons. In a previous paper, the contribution from extended BESS to the electroweak oblique corrections was evaluated. However, only an estimate of the effects coming from mass and wave function renormalization of the new resonances, was given. Here we complete the evaluation by computing explicitly these effects. We confirm the previous result, that is, in spite of the great precision of the present LEP measurements, the extended BESS parameter space is not very much constrained.
[ { "created": "Tue, 31 Aug 1993 09:47:40 GMT", "version": "v1" } ]
2009-10-22
[ [ "Casalbuoni", "R.", "" ], [ "De Curtis", "S.", "" ], [ "Grazzini", "M.", "" ] ]
The existence of a strongly interacting sector responsible for the electroweak symmetry breaking is assumed. As a consequence vector and axial-vector bound states may be formed. These resonances mix with the Standard Model gauge bosons and are of primary phenomenological importance for the LEP physics. The extended BESS model is an effective scheme based on the symmetry group $SU(8)_L\otimes SU(8)_R$, describing in a consistent way the interactions among the pseudo-Goldstone bosons, vector and axial-vector resonances and the standard gauge bosons. In a previous paper, the contribution from extended BESS to the electroweak oblique corrections was evaluated. However, only an estimate of the effects coming from mass and wave function renormalization of the new resonances, was given. Here we complete the evaluation by computing explicitly these effects. We confirm the previous result, that is, in spite of the great precision of the present LEP measurements, the extended BESS parameter space is not very much constrained.
1507.01256
Andrey Lobanov
A. E. Lobanov
Particle quantum states with indefinite mass and neutrino oscillations
22 pages, LaTeX. Final version
Annals of Physics 403, 82-105 (2019)
10.1016/j.aop.2019.02.001
null
hep-ph hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this work we develop a mathematical formalism which allows obtaining oscillation formula for neutrino of any energy. We demonstrate that in the ultra-relativistic limit the results obtained in this new approach agree with the previously used phenomenological theory which is only applicable to ultra-relativistic neutrinos. To this end we do the following. The Hilbert spaces of particle states are constructed in such a way that the neutrinos are combined in a multiplet with its components being considered as different quantum states of a single particle. The same is done for the charged leptons and the down- and up-type quarks. In the theory based on the Lagrangian of the fermion sector of the Standard Model modified in accordance with this construction, the phenomenon of neutrino oscillations arises as a direct consequence of the general principles of quantum field theory. Using the example of the pion decay, when the resulting neutrino has to be ultra-relativistic, it is shown that the neutrino states produced in the decay process can be described by a superposition of states with different masses and identical canonical momenta with very high accuracy.
[ { "created": "Sun, 5 Jul 2015 18:57:35 GMT", "version": "v1" }, { "created": "Sat, 9 Apr 2016 19:08:37 GMT", "version": "v2" }, { "created": "Mon, 5 Dec 2016 21:55:31 GMT", "version": "v3" }, { "created": "Sat, 9 Dec 2017 15:25:21 GMT", "version": "v4" }, { "creat...
2019-06-28
[ [ "Lobanov", "A. E.", "" ] ]
In this work we develop a mathematical formalism which allows obtaining oscillation formula for neutrino of any energy. We demonstrate that in the ultra-relativistic limit the results obtained in this new approach agree with the previously used phenomenological theory which is only applicable to ultra-relativistic neutrinos. To this end we do the following. The Hilbert spaces of particle states are constructed in such a way that the neutrinos are combined in a multiplet with its components being considered as different quantum states of a single particle. The same is done for the charged leptons and the down- and up-type quarks. In the theory based on the Lagrangian of the fermion sector of the Standard Model modified in accordance with this construction, the phenomenon of neutrino oscillations arises as a direct consequence of the general principles of quantum field theory. Using the example of the pion decay, when the resulting neutrino has to be ultra-relativistic, it is shown that the neutrino states produced in the decay process can be described by a superposition of states with different masses and identical canonical momenta with very high accuracy.
1312.2796
Vladimir Sauli
Vladimir Sauli
Lattice data inspired but Minkowski space calculated QCD fundamental propagator
Explanatory section redone, split an enlarged into two new Sections, new simplify results added for LA, typos corrected the 26 pp, 6 figs
null
null
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the Dyson-Schwinger equation for the quark propagator in Minkowski space. In order to have analytical behaviour at the timelike axis of momenta under control, we use the Stieltjes and the Hilbert transformation for the interaction kernels and discuss the solution from the perspective of these transformations. In addition, a lattice fit for the gluon propagator and approximation for quark-gluon vertex are employed, and within the model the quark propagator is obtained through the solution of Dyson-Schwinger equation in Minkowski space. The resulting propagators in all studied cases do not show up particle like pole and production thresholds. Instead of, the quark propagator satisfies Hilbert transformation and the associated dynamical mass function becomes complex without a presence of particle like branch point.
[ { "created": "Tue, 10 Dec 2013 13:46:32 GMT", "version": "v1" }, { "created": "Mon, 13 Jan 2014 09:34:06 GMT", "version": "v2" }, { "created": "Tue, 1 Apr 2014 13:40:15 GMT", "version": "v3" } ]
2014-04-02
[ [ "Sauli", "Vladimir", "" ] ]
We study the Dyson-Schwinger equation for the quark propagator in Minkowski space. In order to have analytical behaviour at the timelike axis of momenta under control, we use the Stieltjes and the Hilbert transformation for the interaction kernels and discuss the solution from the perspective of these transformations. In addition, a lattice fit for the gluon propagator and approximation for quark-gluon vertex are employed, and within the model the quark propagator is obtained through the solution of Dyson-Schwinger equation in Minkowski space. The resulting propagators in all studied cases do not show up particle like pole and production thresholds. Instead of, the quark propagator satisfies Hilbert transformation and the associated dynamical mass function becomes complex without a presence of particle like branch point.
hep-ph/0101060
Eugene Levin
S. Bondarenko, E. Gotsman, E. Levin and U. Maor (Tel Aviv U.)
An Inclusive Cross Section for the Nucleus - Nucleus Interaction at RHIC Energies
9 pages, 11 pictures in eps files
null
null
TAUP 2663-2001
hep-ph
null
We discuss the saturation of the parton density in heavy ion collisions at RHIC energiesusing a Pomeron approach. Our predictions for the particle density in ion-ion collisions at RHIC energies can be utilized as the background for the observation of possible quark-gluon plasma production.
[ { "created": "Mon, 8 Jan 2001 11:17:34 GMT", "version": "v1" }, { "created": "Wed, 17 Jan 2001 13:08:52 GMT", "version": "v2" } ]
2007-05-23
[ [ "Bondarenko", "S.", "", "Tel Aviv U." ], [ "Gotsman", "E.", "", "Tel Aviv U." ], [ "Levin", "E.", "", "Tel Aviv U." ], [ "Maor", "U.", "", "Tel Aviv U." ] ]
We discuss the saturation of the parton density in heavy ion collisions at RHIC energiesusing a Pomeron approach. Our predictions for the particle density in ion-ion collisions at RHIC energies can be utilized as the background for the observation of possible quark-gluon plasma production.
2208.01319
Yang Zhang
Peter Athron, Csaba Balazs, Andrew Fowlie, Lachlan Morris, Graham White, Yang Zhang
How arbitrary are perturbative calculations of the electroweak phase transition?
45 pages, 16 figures and 2 tables; version accepted for publication in JHEP; Correct the signs of mu in Table 2
null
10.1007/JHEP01(2023)050
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate the extent to which perturbative calculations of the electroweak phase transition are arbitrary and uncertain, owing to their gauge, renormalisation scale and scheme dependence, as well as treatments of the Goldstone catastrophe and daisy diagrams. Using the complete parameter space of the Standard Model extended by a real scalar singlet with a $\mathbb{Z}_2$ symmetry as a test, we explore the properties of the electroweak phase transition in general $R_\xi$ and covariant gauges, OS and $\overline{\text{MS}}$ renormalisation schemes, and for common treatments of the Goldstone catastrophe and daisy diagrams. Reassuringly, we find that different renormalisation schemes and different treatments of the Goldstone catastrophe and daisy diagrams typically lead to only modest changes in predictions for the critical temperature and strength of the phase transition. On the other hand, the gauge and renormalisation scale dependence may be significant, and often impact the existence of the phase transition altogether.
[ { "created": "Tue, 2 Aug 2022 08:59:49 GMT", "version": "v1" }, { "created": "Thu, 11 Aug 2022 01:47:26 GMT", "version": "v2" }, { "created": "Thu, 22 Dec 2022 17:04:47 GMT", "version": "v3" }, { "created": "Wed, 19 Apr 2023 02:58:50 GMT", "version": "v4" } ]
2023-04-20
[ [ "Athron", "Peter", "" ], [ "Balazs", "Csaba", "" ], [ "Fowlie", "Andrew", "" ], [ "Morris", "Lachlan", "" ], [ "White", "Graham", "" ], [ "Zhang", "Yang", "" ] ]
We investigate the extent to which perturbative calculations of the electroweak phase transition are arbitrary and uncertain, owing to their gauge, renormalisation scale and scheme dependence, as well as treatments of the Goldstone catastrophe and daisy diagrams. Using the complete parameter space of the Standard Model extended by a real scalar singlet with a $\mathbb{Z}_2$ symmetry as a test, we explore the properties of the electroweak phase transition in general $R_\xi$ and covariant gauges, OS and $\overline{\text{MS}}$ renormalisation schemes, and for common treatments of the Goldstone catastrophe and daisy diagrams. Reassuringly, we find that different renormalisation schemes and different treatments of the Goldstone catastrophe and daisy diagrams typically lead to only modest changes in predictions for the critical temperature and strength of the phase transition. On the other hand, the gauge and renormalisation scale dependence may be significant, and often impact the existence of the phase transition altogether.
2002.01217
Anton Motornenko
Anton Motornenko, Jan Steinheimer, Volodymyr Vovchenko, Stefan Schramm, and Horst Stoecker
QCD equation of state at vanishing and high baryon density: Chiral Mean Field model
4 pages, 2 figures, Proceedings of the XXVIIIth International Conference on Ultrarelativistic Nucleus-Nucleus Collisions (Quark Matter 2019), Wuhan, China, November 3-9 2019
null
10.1016/j.nuclphysa.2020.121836
null
hep-ph astro-ph.HE nucl-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The thermodynamic properties of high temperature and high density QCD-matter are studied using the Chiral SU(3)-flavor parity-doublet Polyakov-loop quark-hadron mean-field model, CMF. The CMF model provides a proper description of lattice QCD data, heavy-ions physics, and static neutron stars. The behavior of lines of constant pressure with increase of baryon density is discussed. The rapid change of pressure behavior at $\mu_B/T\approx3$ suggests a strong contribution of baryons to thermodynamic properties at this region. The position of this region is very close to the radius of convergence for a Taylor expansion of the QCD pressure. The role of mesons and unstable hadrons in the hydrodynamic expansion of strongly interacting matter is also discussed.
[ { "created": "Tue, 4 Feb 2020 10:46:05 GMT", "version": "v1" } ]
2021-02-03
[ [ "Motornenko", "Anton", "" ], [ "Steinheimer", "Jan", "" ], [ "Vovchenko", "Volodymyr", "" ], [ "Schramm", "Stefan", "" ], [ "Stoecker", "Horst", "" ] ]
The thermodynamic properties of high temperature and high density QCD-matter are studied using the Chiral SU(3)-flavor parity-doublet Polyakov-loop quark-hadron mean-field model, CMF. The CMF model provides a proper description of lattice QCD data, heavy-ions physics, and static neutron stars. The behavior of lines of constant pressure with increase of baryon density is discussed. The rapid change of pressure behavior at $\mu_B/T\approx3$ suggests a strong contribution of baryons to thermodynamic properties at this region. The position of this region is very close to the radius of convergence for a Taylor expansion of the QCD pressure. The role of mesons and unstable hadrons in the hydrodynamic expansion of strongly interacting matter is also discussed.
hep-ph/9610430
Markus Diehl
M. Diehl
Azimuthal angles in diffractive ep collisions
38 pages including 6 figures, LaTeX, uses epsf.sty. Text shortened, physics unchanged. To appear in Z. Phys. C
Z.Phys.C76:499-514,1997
10.1007/s002880050573
CPTH-S472-1096 and DAMTP-96-91
hep-ph
null
We investigate azimuthal correlations in deep inelastic diffractive scattering, e + p -> e + \tilde{p} + X. The dependence of the ep cross section on the angle between the lepton plane and some direction in the hadronic final state can be written in a simple form; its measurement can be used to constrain the cross section for longitudinally polarised photons. Using the model of nonperturbative two-gluon exchange of Landshoff and Nachtmann we calculate the distribution of the azimuthal jet angle in diffractive dijet production and find that useful bounds on the longitudinal cross section for such events might be obtained from its measurement. We then discuss the predictions of this model for the dependence of the ep cross section on the azimuthal angle of the proton remnant \tilde{p}, which contains information about the helicity content of the pomeron.
[ { "created": "Mon, 21 Oct 1996 17:19:26 GMT", "version": "v1" }, { "created": "Mon, 15 Sep 1997 09:14:23 GMT", "version": "v2" } ]
2011-07-19
[ [ "Diehl", "M.", "" ] ]
We investigate azimuthal correlations in deep inelastic diffractive scattering, e + p -> e + \tilde{p} + X. The dependence of the ep cross section on the angle between the lepton plane and some direction in the hadronic final state can be written in a simple form; its measurement can be used to constrain the cross section for longitudinally polarised photons. Using the model of nonperturbative two-gluon exchange of Landshoff and Nachtmann we calculate the distribution of the azimuthal jet angle in diffractive dijet production and find that useful bounds on the longitudinal cross section for such events might be obtained from its measurement. We then discuss the predictions of this model for the dependence of the ep cross section on the azimuthal angle of the proton remnant \tilde{p}, which contains information about the helicity content of the pomeron.
1911.06477
Marco Merchand
Marco Merchand, Marc Sher
Constraints on the Parameter Space in an Inert Doublet Model with two Active Doublets
Matches version to appear in JHEP. Significant modifications were made including a discussion of lifting the dark democracy assumption of the quartic couplings
null
10.1007/JHEP03(2020)108
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study a three Higgs doublet model where one doublet is inert and the other two doublets are active. Flavor changing neutral currents are avoided at tree-level by imposing a softly broken $Z'_2$ symmetry and we consider type I and type II Yukawa structures. The lightest inert scalar is a viable Dark Matter (DM) candidate. A numerical scan of the free parameters is performed taking into account theoretical constraints such as positivity of the scalar potential and unitarity of $2 \rightarrow 2$ scattering amplitudes. The model is further constrained by experimental results such as $B$ physics lower limits on charged Higgs masses, Electroweak Precision Observables, LEP II, LHC Higgs measurements, Planck measurement of the DM relic abundance and WIMP direct searches by the LUX and XENON1T experiments. The model predictions for mono-jet, mono Z and mono Higgs final states are studied and tested against current LHC data and we find the model to be allowed. We also discuss the effects of abandoning the "dark democracy" assumption common in studies of inert models. Projected sensitivities of direct detection experiments will leave only a tiny window in the DM mass versus coupling plane that is compliant with relic density bounds.
[ { "created": "Fri, 15 Nov 2019 04:52:36 GMT", "version": "v1" }, { "created": "Tue, 17 Mar 2020 15:26:53 GMT", "version": "v2" } ]
2020-04-22
[ [ "Merchand", "Marco", "" ], [ "Sher", "Marc", "" ] ]
We study a three Higgs doublet model where one doublet is inert and the other two doublets are active. Flavor changing neutral currents are avoided at tree-level by imposing a softly broken $Z'_2$ symmetry and we consider type I and type II Yukawa structures. The lightest inert scalar is a viable Dark Matter (DM) candidate. A numerical scan of the free parameters is performed taking into account theoretical constraints such as positivity of the scalar potential and unitarity of $2 \rightarrow 2$ scattering amplitudes. The model is further constrained by experimental results such as $B$ physics lower limits on charged Higgs masses, Electroweak Precision Observables, LEP II, LHC Higgs measurements, Planck measurement of the DM relic abundance and WIMP direct searches by the LUX and XENON1T experiments. The model predictions for mono-jet, mono Z and mono Higgs final states are studied and tested against current LHC data and we find the model to be allowed. We also discuss the effects of abandoning the "dark democracy" assumption common in studies of inert models. Projected sensitivities of direct detection experiments will leave only a tiny window in the DM mass versus coupling plane that is compliant with relic density bounds.
hep-ph/9906352
Benaoum Hachemi
H.B. Benaoum (Mainz Uni.)
More on triangular mass matrices for fermions
8 pages, latex; Submitted to Phys. Lett. B
null
null
MZ-TH/98-37
hep-ph
null
A direct proof is given here which shows that instead of 6 complex numbers, the triangular mass matrix for each sector could just be expressed in terms of 5 by performing a specific weak basis transformation, leading therefore to a new textures for triangular mass matrices. Furthermore, starting with the set of 20 real parameters for both sectors, it can shown that 6 redundant parameters can be removed by using the rephasing freedom.
[ { "created": "Sun, 13 Jun 1999 15:33:58 GMT", "version": "v1" } ]
2007-05-23
[ [ "Benaoum", "H. B.", "", "Mainz Uni." ] ]
A direct proof is given here which shows that instead of 6 complex numbers, the triangular mass matrix for each sector could just be expressed in terms of 5 by performing a specific weak basis transformation, leading therefore to a new textures for triangular mass matrices. Furthermore, starting with the set of 20 real parameters for both sectors, it can shown that 6 redundant parameters can be removed by using the rephasing freedom.
1207.3068
Sanjin Beni\'c
S. Benic, D. Horvatic, D. Kekez, D. Klabucar
Restoration of singlet axial symmetry at finite temperature
null
null
null
null
hep-ph nucl-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
To accomodate recent RHIC data on eta prime multiplicity, we propose a minimal modification of the Witten-Veneziano relation at high temperature. This renders a significant drop of eta prime mass at high temperature signaling a restoration of the U(1)A, and the Goldstone character of etaprime.
[ { "created": "Thu, 12 Jul 2012 19:24:17 GMT", "version": "v1" } ]
2012-07-13
[ [ "Benic", "S.", "" ], [ "Horvatic", "D.", "" ], [ "Kekez", "D.", "" ], [ "Klabucar", "D.", "" ] ]
To accomodate recent RHIC data on eta prime multiplicity, we propose a minimal modification of the Witten-Veneziano relation at high temperature. This renders a significant drop of eta prime mass at high temperature signaling a restoration of the U(1)A, and the Goldstone character of etaprime.
hep-ph/9606421
null
Edmond L. Berger and Harry Contopanagos (Argonne National Laboratory)
Calculation of the Cross Section for Top Quark Production
13 pages, LaTeX, including 6 ps files of figures. Invited paper presented by E. L. Berger at the XIth Topical Workshop on Hadron Collider Physics, Abano Terme, Padova, Italy, May, 1996
null
null
ANL-HEP-CP-96-51
hep-ph
null
We summarize calculations of the cross section for top quark production at hadron colliders within the context of perturbative quantum chromodynamics, including resummation of the effects of initial-state soft gluon radiation to all orders in the strong coupling strength. In our approach we resum the universal leading-logarithm contributions, and we restrict the calculation to the region of phase space that is demonstrably perturbative. We compare our approach with other methods. We present predictions of the physical cross section as a function of the top quark mass in proton-antiproton reactions at center-of-mass energies of 1.8 and 2.0 TeV, and we discuss estimated uncertainties.
[ { "created": "Mon, 24 Jun 1996 23:21:21 GMT", "version": "v1" } ]
2007-05-23
[ [ "Berger", "Edmond L.", "", "Argonne National Laboratory" ], [ "Contopanagos", "Harry", "", "Argonne National Laboratory" ] ]
We summarize calculations of the cross section for top quark production at hadron colliders within the context of perturbative quantum chromodynamics, including resummation of the effects of initial-state soft gluon radiation to all orders in the strong coupling strength. In our approach we resum the universal leading-logarithm contributions, and we restrict the calculation to the region of phase space that is demonstrably perturbative. We compare our approach with other methods. We present predictions of the physical cross section as a function of the top quark mass in proton-antiproton reactions at center-of-mass energies of 1.8 and 2.0 TeV, and we discuss estimated uncertainties.
1003.2570
Joel Walker
Tianjun Li, Dimitri V. Nanopoulos, Joel W. Walker
Elements of F-ast Proton Decay
V2, As published in Nuclear Physics B; 57 pages, 7 figures, 12 tables
Nucl.Phys.B846:43-99,2011
10.1016/j.nuclphysb.2010.12.014
ACT-03-10, MIFPA-10-09
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Gauge coupling unification in the Minimal Supersymmetric Standard Model (MSSM) strongly suggests the existence of a Grand Unified Theory (GUT), which could be probed by the observation of proton decay. Proton lifetime in the p \to (e+|mu+) pi0 dimension six mode is proportional in the fourth power to the GUT mass scale, and inversely proportional in the fourth power to the GUT coupling. We provide an updated dictionary of solutions for the relevant unification parameters with generic beta-function coefficients, significantly upgrading the level of detail with which second order effects are treated, and correcting subtle published errors. F-lipped SU(5) with strict MSSM field content is known to survive existing null detection limits for proton decay approaching 10^34 years, and indeed, the lifetime predicted by prior studies can be so long that successful detection is not currently plausible. Recently studied classes of F-theory derived GUT models postulate additional vector-like multiplets at the TeV scale which modify the renormalization group to yield a substantial increase in the SU(3)_C X SU(2)_L unified coupling. We find the conjunction of these models with the F-resh analysis employed to be comparatively F-ast proton decay, only narrowly evading existing detection limits, and likely falling within the observable range of proposed next generation detectors such as DUSEL and Hyper-Kamiokande. The TeV-scale vector multiplets are themselves suitable for cross correlation by the Large Hadron Collider. Their presence moreover magnifies the gap between the dual mass scales of Flipped SU(5), allowing for an elongated second stage renormalization, pushing grand unification to the doorstep of the reduced Planck mass.
[ { "created": "Fri, 12 Mar 2010 16:08:18 GMT", "version": "v1" }, { "created": "Thu, 31 Mar 2011 17:59:03 GMT", "version": "v2" } ]
2015-03-13
[ [ "Li", "Tianjun", "" ], [ "Nanopoulos", "Dimitri V.", "" ], [ "Walker", "Joel W.", "" ] ]
Gauge coupling unification in the Minimal Supersymmetric Standard Model (MSSM) strongly suggests the existence of a Grand Unified Theory (GUT), which could be probed by the observation of proton decay. Proton lifetime in the p \to (e+|mu+) pi0 dimension six mode is proportional in the fourth power to the GUT mass scale, and inversely proportional in the fourth power to the GUT coupling. We provide an updated dictionary of solutions for the relevant unification parameters with generic beta-function coefficients, significantly upgrading the level of detail with which second order effects are treated, and correcting subtle published errors. F-lipped SU(5) with strict MSSM field content is known to survive existing null detection limits for proton decay approaching 10^34 years, and indeed, the lifetime predicted by prior studies can be so long that successful detection is not currently plausible. Recently studied classes of F-theory derived GUT models postulate additional vector-like multiplets at the TeV scale which modify the renormalization group to yield a substantial increase in the SU(3)_C X SU(2)_L unified coupling. We find the conjunction of these models with the F-resh analysis employed to be comparatively F-ast proton decay, only narrowly evading existing detection limits, and likely falling within the observable range of proposed next generation detectors such as DUSEL and Hyper-Kamiokande. The TeV-scale vector multiplets are themselves suitable for cross correlation by the Large Hadron Collider. Their presence moreover magnifies the gap between the dual mass scales of Flipped SU(5), allowing for an elongated second stage renormalization, pushing grand unification to the doorstep of the reduced Planck mass.
hep-ph/9505383
null
Carl H. Albright and Satyanarayan Nandi
An Explicit SO(10) x U(1)_F Model of the Yukawa Interactions
15 pages, latex with style files attached, 1 figure in uuencoded postscript file
Mod.Phys.Lett. A11 (1996) 737-748
10.1142/S0217732396000746
FERMILAB-PUB-95/107-T and OSU preprint 303
hep-ph
null
We construct an explicit $SO(10) \times U(1)_F$ model of the Yukawa interactions by using as a guide previous phenomenological results obtained from a bottom-up approach to quark and lepton mass matrices. The global $U(1)_F$ family symmetry group sets the textures for the Majorana and generic Dirac mass matrices by restricting the type and number of Higgs diagrams which can contribute to each matrix element, while the $SO(10)$ group relates each particular element of the up, down, neutrino and charged lepton Dirac matrices. The Yukawa couplings and vacuum expectation values associated with pairs of {\bf 1,~45, 10,} and {\bf 126} Higgs representations successfully correlate all the quark and lepton masses and mixings in the scenario incorporating the nonadiabatic solar neutrino and atmospheric neutrino depletion effects.
[ { "created": "Thu, 25 May 1995 22:03:26 GMT", "version": "v1" }, { "created": "Fri, 26 May 1995 17:00:51 GMT", "version": "v2" } ]
2009-10-28
[ [ "Albright", "Carl H.", "" ], [ "Nandi", "Satyanarayan", "" ] ]
We construct an explicit $SO(10) \times U(1)_F$ model of the Yukawa interactions by using as a guide previous phenomenological results obtained from a bottom-up approach to quark and lepton mass matrices. The global $U(1)_F$ family symmetry group sets the textures for the Majorana and generic Dirac mass matrices by restricting the type and number of Higgs diagrams which can contribute to each matrix element, while the $SO(10)$ group relates each particular element of the up, down, neutrino and charged lepton Dirac matrices. The Yukawa couplings and vacuum expectation values associated with pairs of {\bf 1,~45, 10,} and {\bf 126} Higgs representations successfully correlate all the quark and lepton masses and mixings in the scenario incorporating the nonadiabatic solar neutrino and atmospheric neutrino depletion effects.
1203.6679
Vasile Topor Pop N
V. Topor Pop (McGill Univ., Montreal), M. Gyulassy (Columbia University, NY), J. Barrette (McGill Univ, Montreal), C. Gale (McGill Univ., Montreal), and A. Warburton (McGill Univ, Montreal)
Hyperon/meson ratios in rare high-multiplicity $pp$ collisions at energies available at the Large Hadron Collider, and potential signatures for mini-quark-gluon plasma formation
version2, text modifications,new figures and references added; 22 pages, 8 figures. Accepted for publication, Phys. Rev. C
Phys.Rev.C 86 (2012) 044902
10.1103/PhysRevC.86.044902
null
hep-ph hep-ex nucl-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We use the framework of the HIJING/B\=B v2.0 model to simulate high-multiplicity (HM) $p+p$ collision events at the Large Hadron Collider (LHC) to study observables sensitive to possible collective phenomena, such as strong longitudinal color fields (SLCF) modeled by an enhanced string tension ($\kappa$). We focus on the hyperon/meson yield ratios at center-of-mass (c.m.) energy $\sqrt{s}$ = 7 TeV, in the transverse momentum region, $1 < p_T < 4 $ GeV/{\it c}. For minimum bias events these ratios are well described assuming an energy dependence $\kappa = \kappa(s)= \kappa_{0} (s/s_{0})^{0.04} {\rm GeV/fm}$ ($\kappa_{0}$= 1 GeV/fm), giving a value $\kappa = 2$ GeV/fm at $\sqrt{s}$ = 7 TeV. We compare minimum bias (MB) events to simulated HM events assuming that $\kappa(MB)=2$ GeV/fm could grow to an extreme value of $\kappa(HM)=5$ GeV/fm that saturates the strangeness suppression factor. With this assumption the model predicts a very strong enhancement of (multi)strange baryon/meson ratios in HM events. If observed, such an enhancement could be also interpreted as a possible signature for formation in HM $p+p$ collision events of a deconfined but out of local thermal equilibrium {\em mini quark-gluon plasma} (mQGP).
[ { "created": "Thu, 29 Mar 2012 21:59:23 GMT", "version": "v1" }, { "created": "Wed, 26 Sep 2012 10:47:17 GMT", "version": "v2" } ]
2012-10-23
[ [ "Pop", "V. Topor", "", "McGill Univ., Montreal" ], [ "Gyulassy", "M.", "", "Columbia\n University, NY" ], [ "Barrette", "J.", "", "McGill Univ, Montreal" ], [ "Gale", "C.", "", "McGill Univ.,\n Montreal" ], [ "Warburton", "A...
We use the framework of the HIJING/B\=B v2.0 model to simulate high-multiplicity (HM) $p+p$ collision events at the Large Hadron Collider (LHC) to study observables sensitive to possible collective phenomena, such as strong longitudinal color fields (SLCF) modeled by an enhanced string tension ($\kappa$). We focus on the hyperon/meson yield ratios at center-of-mass (c.m.) energy $\sqrt{s}$ = 7 TeV, in the transverse momentum region, $1 < p_T < 4 $ GeV/{\it c}. For minimum bias events these ratios are well described assuming an energy dependence $\kappa = \kappa(s)= \kappa_{0} (s/s_{0})^{0.04} {\rm GeV/fm}$ ($\kappa_{0}$= 1 GeV/fm), giving a value $\kappa = 2$ GeV/fm at $\sqrt{s}$ = 7 TeV. We compare minimum bias (MB) events to simulated HM events assuming that $\kappa(MB)=2$ GeV/fm could grow to an extreme value of $\kappa(HM)=5$ GeV/fm that saturates the strangeness suppression factor. With this assumption the model predicts a very strong enhancement of (multi)strange baryon/meson ratios in HM events. If observed, such an enhancement could be also interpreted as a possible signature for formation in HM $p+p$ collision events of a deconfined but out of local thermal equilibrium {\em mini quark-gluon plasma} (mQGP).
hep-ph/0002087
Hendrik van Hees
Hendrik van Hees, J\"orn Knoll
Finite pion width effects on the rho-meson and di-lepton spectra
Invited talk given at International Workshop "Gross properties of Nuclei and Nuclear Exitations", Hirschegg, Austria, 16-22.01.2000, Latex, 7 pages
null
null
null
hep-ph nucl-th
null
Within a field theoretical model where all damping width effects are treated self-consistently we study the changes of the spectral properties of rho-mesons due to the finite damping width of the pions in dense hadronic matter at finite temperature. The corresponding effects in the di-lepton yields are presented. Some problems concerning the self consistent treatment of vector or gauge bosons are discussed.
[ { "created": "Tue, 8 Feb 2000 14:52:51 GMT", "version": "v1" } ]
2007-05-23
[ [ "van Hees", "Hendrik", "" ], [ "Knoll", "Jörn", "" ] ]
Within a field theoretical model where all damping width effects are treated self-consistently we study the changes of the spectral properties of rho-mesons due to the finite damping width of the pions in dense hadronic matter at finite temperature. The corresponding effects in the di-lepton yields are presented. Some problems concerning the self consistent treatment of vector or gauge bosons are discussed.
0710.2394
Stefan Scherer
Stefan Scherer (Johannes Gutenberg University, Mainz)
Recent Progress in Effective Field Theory in the One-Nucleon Sector
6 pages, 2 figures, invited parallel session lead talk given at the 20th European Conference on Few-Body Problems in Physics (EFB20), Pisa, Italy, 10-14 September 2007
Few Body Syst.43:179-184,2008
10.1007/s00601-008-0229-3
MKPH-T-07-14
hep-ph
null
Chiral perturbation theory (ChPT) is the effective field theory of the strong interactions at low energies. We will address the issue of a consistent power counting scheme in a manifestly Lorentz-invariant formulation of baryon ChPT. As applications we show how the inclusion of vector and axial-vector mesons in the calculation of the nucleon electromagnetic and axial form factors, respectively, lead to an improved description of the empirical data. Finally, we will outline a systematic implementation of the Delta(1232) resonance into the effective field theory program.
[ { "created": "Fri, 12 Oct 2007 06:56:58 GMT", "version": "v1" } ]
2009-01-08
[ [ "Scherer", "Stefan", "", "Johannes Gutenberg University, Mainz" ] ]
Chiral perturbation theory (ChPT) is the effective field theory of the strong interactions at low energies. We will address the issue of a consistent power counting scheme in a manifestly Lorentz-invariant formulation of baryon ChPT. As applications we show how the inclusion of vector and axial-vector mesons in the calculation of the nucleon electromagnetic and axial form factors, respectively, lead to an improved description of the empirical data. Finally, we will outline a systematic implementation of the Delta(1232) resonance into the effective field theory program.
hep-ph/0212271
Antonio Vairo
Antonio Vairo (CERN)
Heavy Quarkonium Inclusive Decays: Theoretical Status and Perspectives
10 pages, uses modified ws-procs9x6.cls (ws-procs9x6-notrim.cls), Plenary talk presented at The 5th International Conference Quark Confinement and the Hadron Spectrum, Gargnano, Italy 10-14 September, 2002
null
10.1142/9789812704269_0007
CERN-TH/2002-376
hep-ph
null
I review some recent progress and open problems in the calculation of heavy-quarkonium inclusive decay widths into light particles in the framework of QCD non-relativistic effective field theories.
[ { "created": "Wed, 18 Dec 2002 19:48:09 GMT", "version": "v1" } ]
2017-08-23
[ [ "Vairo", "Antonio", "", "CERN" ] ]
I review some recent progress and open problems in the calculation of heavy-quarkonium inclusive decay widths into light particles in the framework of QCD non-relativistic effective field theories.
1505.06981
Yu-Jie Zhang Dr.
Guang-Zhi Xu, Gang Li, Yi-Jie Li, Kui-Yong Liu, and Yu-Jie Zhang
Interference effects on Higgs mass measurement in $e^+e^-\to H(\gamma\gamma) Z$ at CEPC
Comments and suggestions are welcome
Chinese Physics C Vol. 40, No. 3 (2016) 033101
10.1088/1674-1137/40/3/033101
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A high luminosity Circular Electron Positron Collider (CEPC) as a Higgs Factory will be helpful to the precision measurement of the Higgs mass. The signal-background interference effect is carefully studied for the Higgs diphoton decay mode in the associated Z boson production at the future $e^+e^-$ colliders at energy $246 {\rm GeV}$. The mass shifts go up from about $20 {\rm MeV}$ to $50 {\rm MeV}$ for the experimental mass resolution ranging from $0.8 {\rm GeV}$ to $2 {\rm GeV}$.
[ { "created": "Sat, 23 May 2015 10:35:57 GMT", "version": "v1" } ]
2016-01-08
[ [ "Xu", "Guang-Zhi", "" ], [ "Li", "Gang", "" ], [ "Li", "Yi-Jie", "" ], [ "Liu", "Kui-Yong", "" ], [ "Zhang", "Yu-Jie", "" ] ]
A high luminosity Circular Electron Positron Collider (CEPC) as a Higgs Factory will be helpful to the precision measurement of the Higgs mass. The signal-background interference effect is carefully studied for the Higgs diphoton decay mode in the associated Z boson production at the future $e^+e^-$ colliders at energy $246 {\rm GeV}$. The mass shifts go up from about $20 {\rm MeV}$ to $50 {\rm MeV}$ for the experimental mass resolution ranging from $0.8 {\rm GeV}$ to $2 {\rm GeV}$.
1907.13477
Narmin Huseynova
Narmin Huseynova, Shahin Mamedov
$a_1$ meson-baryon coupling constants in the framework of soft-wall and hard-wall AdS/QCD models
16 pages. arXiv admin note: text overlap with arXiv:1408.5496 version published in IJMPA
null
10.1142/S0217751X19502403
null
hep-ph hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We calculate the $a_1$ meson-nucleon coupling constant in the framework of soft-wall and hard-wall AdS/QCD models. In the bulk of AdS space were written bulk interaction Lagrangians for a minimal gauge coupling, a magnetic gauge coupling and a triple coupling. To use AdS/CFT correspondence and these bulk interaction Lagrangians we calculate the $a_1$ axial-vector meson-nucleon coupling constant in the boundary of AdS space within both models. We observe that the numerical values for the $g_{a_1 NN}$ coupling constant in the framework of both models are more close to the experimental value than results in other works. We also calculate the $g_{a_1 \Delta \Delta}$ axial-vector meson-$\Delta$-baryon coupling constant in the framework of hard-wall AdS/QCD model.
[ { "created": "Tue, 30 Jul 2019 09:38:38 GMT", "version": "v1" }, { "created": "Tue, 4 Feb 2020 10:43:12 GMT", "version": "v2" } ]
2020-02-19
[ [ "Huseynova", "Narmin", "" ], [ "Mamedov", "Shahin", "" ] ]
We calculate the $a_1$ meson-nucleon coupling constant in the framework of soft-wall and hard-wall AdS/QCD models. In the bulk of AdS space were written bulk interaction Lagrangians for a minimal gauge coupling, a magnetic gauge coupling and a triple coupling. To use AdS/CFT correspondence and these bulk interaction Lagrangians we calculate the $a_1$ axial-vector meson-nucleon coupling constant in the boundary of AdS space within both models. We observe that the numerical values for the $g_{a_1 NN}$ coupling constant in the framework of both models are more close to the experimental value than results in other works. We also calculate the $g_{a_1 \Delta \Delta}$ axial-vector meson-$\Delta$-baryon coupling constant in the framework of hard-wall AdS/QCD model.
hep-ph/9904272
Ignatios Antoniadis
I. Antoniadis (Ecole Polytechnique)
On Possible Modifications of Gravitation in the (sub)millimeter range
7 pages, LaTeX, needs moriond2.sty, one eps figure, references added Invited talk given at the XXXIV Rencontres de Moriond on Gravitational Waves and Experimental Gravity, Les Arcs, France, January 23-30, 1999
null
null
CPHT-PC715.0499
hep-ph gr-qc hep-th
null
I discuss possible modifications of gravitation at short distances in string theories with large internal dimensions and low string scale. The modifications are due to the change of Newton's law in the presence of (sub)millimeter-size transverse dimensions, or due to the existence of light scalars with masses as small as 10^{-3} eV, related to the mechanism of supersymmetry breaking, mediating new Yukawa-type forces with strength comparable to gravity. These modifications are testable in "tabletop" experiments that measure gravity at such short distances.
[ { "created": "Thu, 8 Apr 1999 09:03:21 GMT", "version": "v1" }, { "created": "Wed, 14 Apr 1999 21:35:06 GMT", "version": "v2" } ]
2007-05-23
[ [ "Antoniadis", "I.", "", "Ecole Polytechnique" ] ]
I discuss possible modifications of gravitation at short distances in string theories with large internal dimensions and low string scale. The modifications are due to the change of Newton's law in the presence of (sub)millimeter-size transverse dimensions, or due to the existence of light scalars with masses as small as 10^{-3} eV, related to the mechanism of supersymmetry breaking, mediating new Yukawa-type forces with strength comparable to gravity. These modifications are testable in "tabletop" experiments that measure gravity at such short distances.
hep-ph/0503248
Brooks Thomas
Brooks Thomas
Requirements to Detect the Monoenergetic Photon Signature of Thermal Cold Dark Matter in PeV-Scale Split Supersymmetry
16 pages, 6 figures
Phys.Rev. D72 (2005) 023519
10.1103/PhysRevD.72.023519
MCTP-05-66
hep-ph
null
Split supersymmetry scenarios with PeV-scale scalar masses circumvent many of the restrictions on supersymmetry coming from experimental limits on CP violation, flavor-changing neutral currents, and the Higgs boson mass. We consider the situation where the LSP is either a Wino or Higgsino and the majority of its cold dark matter relic density is of thermal origin, in which case its mass is specified to be 2.3 TeV for a Wino or 1.1 TeV for a Higgsino. We examine the potential for indirect detection, at present and future gamma-ray telescopes, of the monoenergetic photon lines that would result from the annihilation of these particles near the galactic center. We show how the possibility for detection depends on the precise form of the galactic dark-matter halo profile and examine what performance attributes a gamma-ray detector would need in order to register a 5-sigma discovery.
[ { "created": "Thu, 24 Mar 2005 04:54:06 GMT", "version": "v1" } ]
2009-11-11
[ [ "Thomas", "Brooks", "" ] ]
Split supersymmetry scenarios with PeV-scale scalar masses circumvent many of the restrictions on supersymmetry coming from experimental limits on CP violation, flavor-changing neutral currents, and the Higgs boson mass. We consider the situation where the LSP is either a Wino or Higgsino and the majority of its cold dark matter relic density is of thermal origin, in which case its mass is specified to be 2.3 TeV for a Wino or 1.1 TeV for a Higgsino. We examine the potential for indirect detection, at present and future gamma-ray telescopes, of the monoenergetic photon lines that would result from the annihilation of these particles near the galactic center. We show how the possibility for detection depends on the precise form of the galactic dark-matter halo profile and examine what performance attributes a gamma-ray detector would need in order to register a 5-sigma discovery.
1703.05255
Fernando Febres Cordero
S. Abreu, F. Febres Cordero, H. Ita, M. Jaquier and B. Page
Subleading Poles in the Numerical Unitarity Method at Two Loops
18 pages, 4 figures. v2: Minor text improvements; added reference; matches published version
Phys. Rev. D 95, 096011 (2017)
10.1103/PhysRevD.95.096011
FR-PHENO-2017-002
hep-ph hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We describe the unitarity approach for the numerical computation of two-loop integral coefficients of scattering amplitudes. It is well known that the leading propagator singularities of an amplitude's integrand are related to products of tree amplitudes. At two loops, Feynman diagrams with doubled propagators appear naturally, which lead to subleading pole contributions. In general, it is not known how these contributions can be directly expressed in terms of a product of on-shell tree amplitudes. We present a universal algorithm to extract these subleading pole terms by releasing some of the on-shell conditions. We demonstrate the new approach by numerically computing two-loop four-gluon integral coefficients.
[ { "created": "Wed, 15 Mar 2017 16:56:17 GMT", "version": "v1" }, { "created": "Tue, 6 Jun 2017 07:17:53 GMT", "version": "v2" } ]
2017-06-07
[ [ "Abreu", "S.", "" ], [ "Cordero", "F. Febres", "" ], [ "Ita", "H.", "" ], [ "Jaquier", "M.", "" ], [ "Page", "B.", "" ] ]
We describe the unitarity approach for the numerical computation of two-loop integral coefficients of scattering amplitudes. It is well known that the leading propagator singularities of an amplitude's integrand are related to products of tree amplitudes. At two loops, Feynman diagrams with doubled propagators appear naturally, which lead to subleading pole contributions. In general, it is not known how these contributions can be directly expressed in terms of a product of on-shell tree amplitudes. We present a universal algorithm to extract these subleading pole terms by releasing some of the on-shell conditions. We demonstrate the new approach by numerically computing two-loop four-gluon integral coefficients.
2109.06618
C. Pallis
C Pallis
SU(2,1) / (SU(2) x U(1)) B-L Higgs Inflation
Prepared for the Proceedings of HEP 2021, Thessaloniki, Greece
J.Phys.Conf.Ser. 2105 (2021) 12, 012007
10.1088/1742-6596/2105/1/012007
null
hep-ph astro-ph.CO hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We present a realization of Higgs inflation within Supergravity which is largely tied to the existence of a pole of order two in the kinetic term of the inflaton field. This pole arises due to the selected Kaehler potential which parameterizes the SU(2,1) / (SU(2) x U(1)) manifold with scalar curvature R_{21}=-6/N. The associated superpotential includes, in addition to the Higgs superfields, a stabilizer superfield, respects a B-L gauge and an R symmetries and contains the first allowed nonrenormalizable term. If the coefficient of this term is almost equal to that of the others within about 10^-5 and N=2, the inflationary observables can be done compatible with the present data. The tuning can be eluded if we modify the Kaehler potential associated with the manifold above. In this case, inflation can be realized with just renormalizable superpotential terms and results to higher tensor-to-scalar ratios as N approaches its maximum at N~80.
[ { "created": "Tue, 14 Sep 2021 12:14:46 GMT", "version": "v1" } ]
2021-11-30
[ [ "Pallis", "C", "" ] ]
We present a realization of Higgs inflation within Supergravity which is largely tied to the existence of a pole of order two in the kinetic term of the inflaton field. This pole arises due to the selected Kaehler potential which parameterizes the SU(2,1) / (SU(2) x U(1)) manifold with scalar curvature R_{21}=-6/N. The associated superpotential includes, in addition to the Higgs superfields, a stabilizer superfield, respects a B-L gauge and an R symmetries and contains the first allowed nonrenormalizable term. If the coefficient of this term is almost equal to that of the others within about 10^-5 and N=2, the inflationary observables can be done compatible with the present data. The tuning can be eluded if we modify the Kaehler potential associated with the manifold above. In this case, inflation can be realized with just renormalizable superpotential terms and results to higher tensor-to-scalar ratios as N approaches its maximum at N~80.
hep-ph/0012161
null
I.I. Bigi
Heavy Flavour Physics: On Its More Than 50 Years Of History, Its Future And The Rio Manifesto
32 pages, LATEX, no figures; Summary Talk given at HQ2K `Heavy Quarks at Fixed Target 2000', Rio de Janeiro, Brazil, Oct. 9 -12, 2000. A clarification about the Beneke et al. approach has been added as has been a reference on penguins on Rio's beaches
null
null
UND-HEP-00-BIG 11
hep-ph
null
After a reminder about how $\Delta S\neq 0$ physics has been instrumental for the development of the Standard Model I sketch theoretical technologies for dealing with nonperturbative QCD in heavy flavour decays and state predictions for CP odd effects as they were made in 1998. I review the exciting developments in heavy flavour physics as presented at this conference. A central message is presented in the `Rio Manifesto' where I recapitulate the lessons we have learnt from charm physics, point out the special role future dedicated charm studies can play in revealing the presence of New Physics and give an introduction to the relevant phenomenology focussed on CP studies.
[ { "created": "Wed, 13 Dec 2000 21:27:33 GMT", "version": "v1" }, { "created": "Sat, 23 Dec 2000 05:22:43 GMT", "version": "v2" } ]
2007-05-23
[ [ "Bigi", "I. I.", "" ] ]
After a reminder about how $\Delta S\neq 0$ physics has been instrumental for the development of the Standard Model I sketch theoretical technologies for dealing with nonperturbative QCD in heavy flavour decays and state predictions for CP odd effects as they were made in 1998. I review the exciting developments in heavy flavour physics as presented at this conference. A central message is presented in the `Rio Manifesto' where I recapitulate the lessons we have learnt from charm physics, point out the special role future dedicated charm studies can play in revealing the presence of New Physics and give an introduction to the relevant phenomenology focussed on CP studies.
2302.03383
Shahin Mamedov
Minaya Allahverdiyeva and Shahin Mamedov
Vector Meson Gravitational Form Factors and Generalized Parton Distributions at finite temperature within the soft-wall AdS/QCD Model
19 pages, 9 figures, added references, numerical analysis extended, match to published version
null
null
null
hep-ph
http://creativecommons.org/licenses/by/4.0/
We investigate the vector meson's gravitational form factors (GFFs) and generalized parton distributions (GPDs) at finite temperatures within the soft-wall AdS/ QCD model. The plotted soft-wall GFFs graphs at zero temperature are close to the hard-wall results [1]. The dependence on temperature of the GFFs and GPDs is studied using the thermal dilaton approach in the soft-wall model. Plots of thermal GFFs show that they decrease in temperature increase. Also, the gravitational radius of $\rho$ meson decreases in temperature growth and becomes zero around the critical temperature $T_c=0.2 {\rm\ GeV}$. GPDs at zero skewness are plotted and analyzed at zero and finite temperature cases.
[ { "created": "Tue, 7 Feb 2023 10:42:38 GMT", "version": "v1" }, { "created": "Tue, 14 Feb 2023 11:14:06 GMT", "version": "v2" }, { "created": "Mon, 3 Jul 2023 10:21:26 GMT", "version": "v3" } ]
2023-07-04
[ [ "Allahverdiyeva", "Minaya", "" ], [ "Mamedov", "Shahin", "" ] ]
We investigate the vector meson's gravitational form factors (GFFs) and generalized parton distributions (GPDs) at finite temperatures within the soft-wall AdS/ QCD model. The plotted soft-wall GFFs graphs at zero temperature are close to the hard-wall results [1]. The dependence on temperature of the GFFs and GPDs is studied using the thermal dilaton approach in the soft-wall model. Plots of thermal GFFs show that they decrease in temperature increase. Also, the gravitational radius of $\rho$ meson decreases in temperature growth and becomes zero around the critical temperature $T_c=0.2 {\rm\ GeV}$. GPDs at zero skewness are plotted and analyzed at zero and finite temperature cases.
1210.3297
Steven D. Bass
Steven D. Bass
The cosmological constant puzzle: Vacuum energies from QCD to dark energy
10 pages, presented at the Symposium "Quantum Chromodynamics: History and Prospects", Oberwoelz, Austria, September 3-8, 2012
null
null
null
hep-ph astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The accelerating expansion of the Universe points to a small positive vacuum energy density and negative vacuum pressure. A strong candidate is the cosmological constant in Einstein's equations of General Relativity. The vacuum dark energy density extracted from astrophysics is 10^56 times smaller than the value expected from the Higgs potential in Standard Model particle physics. The dark energy scale is however close to the range of possible values expected for the light neutrino mass. We investigate this physics in a simple toy model where the chirality of the neutrino is treated by analogy as an Ising-like "spin" degree of freedom.
[ { "created": "Thu, 11 Oct 2012 16:49:03 GMT", "version": "v1" } ]
2012-10-12
[ [ "Bass", "Steven D.", "" ] ]
The accelerating expansion of the Universe points to a small positive vacuum energy density and negative vacuum pressure. A strong candidate is the cosmological constant in Einstein's equations of General Relativity. The vacuum dark energy density extracted from astrophysics is 10^56 times smaller than the value expected from the Higgs potential in Standard Model particle physics. The dark energy scale is however close to the range of possible values expected for the light neutrino mass. We investigate this physics in a simple toy model where the chirality of the neutrino is treated by analogy as an Ising-like "spin" degree of freedom.
1307.2253
Andrea De Simone
Giorgio Busoni, Andrea De Simone, Enrico Morgante, Antonio Riotto
On the Validity of the Effective Field Theory for Dark Matter Searches at the LHC
16 pages, 7 figures. References added and minor corrections made to match published version
Physics Letters B 728C (2014)
10.1016/j.physletb.2013.11.069
CERN-PH-TH/2013-151, SISSA 29/2013/FISI
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We discuss the limitations to the use of the effective field theory approach to study dark matter at the LHC. We introduce and study a few quantities, some of them independent of the ultraviolet completion of the dark matter theory, which quantify the error made when using effective operators to describe processes with very high momentum transfer. Our criteria indicate up to what cutoff energy scale, and with what precision, the effective description is valid, depending on the dark matter mass and couplings.
[ { "created": "Mon, 8 Jul 2013 20:05:08 GMT", "version": "v1" }, { "created": "Thu, 19 Dec 2013 14:54:02 GMT", "version": "v2" } ]
2013-12-20
[ [ "Busoni", "Giorgio", "" ], [ "De Simone", "Andrea", "" ], [ "Morgante", "Enrico", "" ], [ "Riotto", "Antonio", "" ] ]
We discuss the limitations to the use of the effective field theory approach to study dark matter at the LHC. We introduce and study a few quantities, some of them independent of the ultraviolet completion of the dark matter theory, which quantify the error made when using effective operators to describe processes with very high momentum transfer. Our criteria indicate up to what cutoff energy scale, and with what precision, the effective description is valid, depending on the dark matter mass and couplings.
hep-ph/0008058
Michael Dine
Alexey Anisimov and Michael Dine
Some Issues in Flat Direction Baryogenesis
Latex, 14 pages. Typos and some minor errors fixed
Nucl.Phys. B619 (2001) 729-740
10.1016/S0550-3213(01)00550-8
SCIPP-00/26
hep-ph
null
Motivated by recent developments, we explore some issues in Affleck-Dine baryogenesis. We consider in greater detail the role of thermal effects in the production of baryon number. We find that these effects are important even for rather flat potentials, and obtain somewhat different estimates of the baryon asymmetry than those in the literature. We also consider the decay of the condensate, and possible implications of these observations for the formation of Q-balls.
[ { "created": "Mon, 7 Aug 2000 16:55:43 GMT", "version": "v1" }, { "created": "Wed, 15 Aug 2001 22:12:45 GMT", "version": "v2" } ]
2009-10-31
[ [ "Anisimov", "Alexey", "" ], [ "Dine", "Michael", "" ] ]
Motivated by recent developments, we explore some issues in Affleck-Dine baryogenesis. We consider in greater detail the role of thermal effects in the production of baryon number. We find that these effects are important even for rather flat potentials, and obtain somewhat different estimates of the baryon asymmetry than those in the literature. We also consider the decay of the condensate, and possible implications of these observations for the formation of Q-balls.
2311.16920
Dian-Yong Chen
Quan-Yun Guo, Zi-Li Yue, Dian-Yong Chen
$\Xi(1620)$ production in $K^- p$ scattering process
5 pages, 5 figures
null
null
null
hep-ph hep-ex
http://creativecommons.org/licenses/by/4.0/
In the present work, the production of $\Xi(1620)$ in the $K^- p$ scattering process is investigated by using an effective Lagrangian approach, where $\Xi(1620)$ is considered as a $\bar{K} \Lambda$ molecular state. Our estimations indicate that the cross sections for $K^-p\to K^+ \Xi(1620)^-$ are $(1.48 ^{+ 1.12}_{-0.69}) \ \mathrm{\mu b}$ at $P_K=2.8 \ \mathrm{GeV}$, where the uncertainties are resulted from the variation of the model parameter. As for the $K^-p\to K^+ \pi^0 \Xi^-$ process, the cross sections are estimated to be $(0.61 ^{+0.47}_{-0.29})\ \mathrm{\mu b}$ at $P_K =2.8 \ \mathrm{GeV}$, which is consistent with the experimental measurements.
[ { "created": "Tue, 28 Nov 2023 16:24:57 GMT", "version": "v1" } ]
2023-11-29
[ [ "Guo", "Quan-Yun", "" ], [ "Yue", "Zi-Li", "" ], [ "Chen", "Dian-Yong", "" ] ]
In the present work, the production of $\Xi(1620)$ in the $K^- p$ scattering process is investigated by using an effective Lagrangian approach, where $\Xi(1620)$ is considered as a $\bar{K} \Lambda$ molecular state. Our estimations indicate that the cross sections for $K^-p\to K^+ \Xi(1620)^-$ are $(1.48 ^{+ 1.12}_{-0.69}) \ \mathrm{\mu b}$ at $P_K=2.8 \ \mathrm{GeV}$, where the uncertainties are resulted from the variation of the model parameter. As for the $K^-p\to K^+ \pi^0 \Xi^-$ process, the cross sections are estimated to be $(0.61 ^{+0.47}_{-0.29})\ \mathrm{\mu b}$ at $P_K =2.8 \ \mathrm{GeV}$, which is consistent with the experimental measurements.
1503.00530
Malin Sjodahl
Yi-Jian Du, Malin Sjodahl and Johan Thoren
Recursion in multiplet bases for tree-level MHV gluon amplitudes
Version published in JHEP, reference updated
null
null
LU TP 15-07, MCnet-15-02
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate the construction of tree-level MHV gluon amplitudes in multiplet bases using BCFW recursion. The multiplet basis decomposition can either be obtained by decomposing results derived in (for example) the DDM basis or by formulating the recursion directly in the multiplet basis. We focus on the latter approach and show how to efficiently deal with the color structure appearing in the recursion. For illustration, we also explicitly calculate the four-, five- and six-gluon amplitudes.
[ { "created": "Mon, 2 Mar 2015 14:03:57 GMT", "version": "v1" }, { "created": "Mon, 5 Oct 2015 12:18:02 GMT", "version": "v2" } ]
2015-10-06
[ [ "Du", "Yi-Jian", "" ], [ "Sjodahl", "Malin", "" ], [ "Thoren", "Johan", "" ] ]
We investigate the construction of tree-level MHV gluon amplitudes in multiplet bases using BCFW recursion. The multiplet basis decomposition can either be obtained by decomposing results derived in (for example) the DDM basis or by formulating the recursion directly in the multiplet basis. We focus on the latter approach and show how to efficiently deal with the color structure appearing in the recursion. For illustration, we also explicitly calculate the four-, five- and six-gluon amplitudes.
1805.01866
Sumit Ghosh
Bhaskar Dutta, Sumit Ghosh, Ilia Gogoladze, Tianjun Li
Three-loop neutrino masses via new massive gauge bosons from $E_6$ GUT
13 pages, 2 figure
Phys. Rev. D 98, 055028 (2018)
10.1103/PhysRevD.98.055028
MI-TH-1882
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We propose an $SU(3)_C\times SU(2)_L \times SU(2)_N \times U(1)_Y$ model arising from $E_6$ grand unified theory. We show that the tiny neutrino masses in this model can be generated at the three-loop involving the $SU(2)_N$ gauge bosons. With Yukawa couplings around 0.01 or larger and TeV-scale $SU(2)_N$ gauge bosons, we show that the neutrino oscillation data can be explained naturally by presenting a concrete benchmark set of input parameters. All new particles are around the TeV scale. Thus our model can be tested at the ongoing/future collider experiments.
[ { "created": "Fri, 4 May 2018 17:21:06 GMT", "version": "v1" }, { "created": "Sun, 7 Oct 2018 02:13:11 GMT", "version": "v2" }, { "created": "Wed, 12 Jun 2019 02:16:14 GMT", "version": "v3" } ]
2019-06-13
[ [ "Dutta", "Bhaskar", "" ], [ "Ghosh", "Sumit", "" ], [ "Gogoladze", "Ilia", "" ], [ "Li", "Tianjun", "" ] ]
We propose an $SU(3)_C\times SU(2)_L \times SU(2)_N \times U(1)_Y$ model arising from $E_6$ grand unified theory. We show that the tiny neutrino masses in this model can be generated at the three-loop involving the $SU(2)_N$ gauge bosons. With Yukawa couplings around 0.01 or larger and TeV-scale $SU(2)_N$ gauge bosons, we show that the neutrino oscillation data can be explained naturally by presenting a concrete benchmark set of input parameters. All new particles are around the TeV scale. Thus our model can be tested at the ongoing/future collider experiments.
1210.7817
Matthew McCullough
Francesco D'Eramo, Matthew McCullough, and Jesse Thaler
Multiple Gamma Lines from Semi-Annihilation
15 pages of text, 8 figures. v2: refs added
null
10.1088/1475-7516/2013/04/030
MIT-CTP-4408; UCB-PTH-12/18
hep-ph astro-ph.HE
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Hints in the Fermi data for a 130 GeV gamma line from the galactic center have ignited interest in potential gamma line signatures of dark matter. Explanations of this line based on dark matter annihilation face a parametric tension since they often rely on large enhancements of loop-suppressed cross sections. In this paper, we pursue an alternative possibility that dark matter gamma lines could arise from "semi-annihilation" among multiple dark sector states. The semi-annihilation reaction with a single final state photon is typically enhanced relative to ordinary annihilation into photon pairs. Semi-annihilation allows for a wide range of dark matter masses compared to the fixed mass value required by annihilation, opening the possibility to explain potential dark matter signatures at higher energies. The most striking prediction of semi-annihilation is the presence of multiple gamma lines, with as many as order N^3 lines possible for N dark sector states, allowing for dark sector spectroscopy. A smoking gun signature arises in the simplest case of degenerate dark matter, where a strong semi-annihilation line at 130 GeV would be accompanied by a weaker annihilation line at 173 GeV. As a proof of principle, we construct two explicit models of dark matter semi-annihilation, one based on non-Abelian vector dark matter and the other based on retrofitting Rayleigh dark matter.
[ { "created": "Mon, 29 Oct 2012 20:01:00 GMT", "version": "v1" }, { "created": "Fri, 9 Nov 2012 19:53:05 GMT", "version": "v2" } ]
2015-06-11
[ [ "D'Eramo", "Francesco", "" ], [ "McCullough", "Matthew", "" ], [ "Thaler", "Jesse", "" ] ]
Hints in the Fermi data for a 130 GeV gamma line from the galactic center have ignited interest in potential gamma line signatures of dark matter. Explanations of this line based on dark matter annihilation face a parametric tension since they often rely on large enhancements of loop-suppressed cross sections. In this paper, we pursue an alternative possibility that dark matter gamma lines could arise from "semi-annihilation" among multiple dark sector states. The semi-annihilation reaction with a single final state photon is typically enhanced relative to ordinary annihilation into photon pairs. Semi-annihilation allows for a wide range of dark matter masses compared to the fixed mass value required by annihilation, opening the possibility to explain potential dark matter signatures at higher energies. The most striking prediction of semi-annihilation is the presence of multiple gamma lines, with as many as order N^3 lines possible for N dark sector states, allowing for dark sector spectroscopy. A smoking gun signature arises in the simplest case of degenerate dark matter, where a strong semi-annihilation line at 130 GeV would be accompanied by a weaker annihilation line at 173 GeV. As a proof of principle, we construct two explicit models of dark matter semi-annihilation, one based on non-Abelian vector dark matter and the other based on retrofitting Rayleigh dark matter.
2107.07251
Jiri Hosek
Jiri Hosek
London model of dual color superconductor
null
null
10.1051/epjconf/202227402001
null
hep-ph hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Following closely the logic of the London phenomenological macroscopic theory of the Meissner effect in superconductors we describe the origin of the short-range behavior of the chromo-electric field, the necessary ingredient for color confinement in QCD. The genuinely non-Abelian model is specified by the strong-coupling colored-gluon current. Its first term, as the superconductivity current, is proportional to the gauge potential. The new term is simply related to the chromo-magnetic pseudo-vector current of the non-Abelian Bianchi identity. We suggest that this London dual color superconductivity current is responsible for the observed almost perfect fluidity in droplets of the strongly interacting quark-gluon plasma. Its chromo-magnetic component should have a specific experimental manifestation.
[ { "created": "Thu, 15 Jul 2021 11:21:38 GMT", "version": "v1" } ]
2023-01-11
[ [ "Hosek", "Jiri", "" ] ]
Following closely the logic of the London phenomenological macroscopic theory of the Meissner effect in superconductors we describe the origin of the short-range behavior of the chromo-electric field, the necessary ingredient for color confinement in QCD. The genuinely non-Abelian model is specified by the strong-coupling colored-gluon current. Its first term, as the superconductivity current, is proportional to the gauge potential. The new term is simply related to the chromo-magnetic pseudo-vector current of the non-Abelian Bianchi identity. We suggest that this London dual color superconductivity current is responsible for the observed almost perfect fluidity in droplets of the strongly interacting quark-gluon plasma. Its chromo-magnetic component should have a specific experimental manifestation.
1808.07492
Julian Heeck
Julian Heeck, Daniele Teresi
Pati-Salam explanations of the B-meson anomalies
26 pages, includes discussion of RGEs; to appear in JHEP
JHEP 12 (2018) 103
10.1007/JHEP12(2018)103
ULB-TH/18-11, UCI-TR-2018-13
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We provide a combined explanation of the increasingly tantalizing $B$-meson anomalies, both in $R_{K^{(*)}}$ and $R_{D^{(*)}}$, in the Pati-Salam model with minimal matter content. This well-known model, based on the gauge group $SU(4)_{LC} \times SU(2)_L \times SU(2)_R$, naturally contains a variety of scalar leptoquarks with related and restricted couplings. In particular we show that the seesaw-motivated scalar leptoquark within the representation $(\overline{10}, 3, 1)$ and its right-handed parity partner $(\overline{10}, 1, 3)$ can solve both anomalies while making testable predictions for related observables such as $B \to K\nu\nu$ and $B \to K \mu\tau$. The solution of the $R_{K^{(*)}}$ anomaly alone can be related to a type-II seesaw neutrino mass structure. Explaining also $R_{D^{(*)}}$ requires the existence of a light right-handed neutrino, which constrains the UV structure of the model.
[ { "created": "Wed, 22 Aug 2018 18:00:05 GMT", "version": "v1" }, { "created": "Wed, 12 Dec 2018 17:51:34 GMT", "version": "v2" } ]
2018-12-18
[ [ "Heeck", "Julian", "" ], [ "Teresi", "Daniele", "" ] ]
We provide a combined explanation of the increasingly tantalizing $B$-meson anomalies, both in $R_{K^{(*)}}$ and $R_{D^{(*)}}$, in the Pati-Salam model with minimal matter content. This well-known model, based on the gauge group $SU(4)_{LC} \times SU(2)_L \times SU(2)_R$, naturally contains a variety of scalar leptoquarks with related and restricted couplings. In particular we show that the seesaw-motivated scalar leptoquark within the representation $(\overline{10}, 3, 1)$ and its right-handed parity partner $(\overline{10}, 1, 3)$ can solve both anomalies while making testable predictions for related observables such as $B \to K\nu\nu$ and $B \to K \mu\tau$. The solution of the $R_{K^{(*)}}$ anomaly alone can be related to a type-II seesaw neutrino mass structure. Explaining also $R_{D^{(*)}}$ requires the existence of a light right-handed neutrino, which constrains the UV structure of the model.
hep-ph/9901453
John McDonald
John McDonald
B-ball Baryogenesis and D-term Inflation
14 pages LaTeX. Talk presented at SEWM'98, NORDITA, Copenhagen
null
null
null
hep-ph astro-ph
null
The MSSM has flat directions in its scalar potential, along which it is natural for Bose condensates of squarks to form in the early Universe. A baryon asymmetry can be induced in these condensates via Affleck-Dine baryogenesis. The condensates are unstable with respect to fragmentation to "B-balls", solitons made of squarks and carrying baryon number, which, if they survive thermalization, fill the Universe down to low temperatures, much lower than that of the electroweak phase transition, with interesting cosmological consequences. In particular, their decay implies a similar number density of baryons and dark matter neutralinos, in accordance with observations. Evasion of thermalization and the ability to account for the observed baryon asymmetry requires a very low reheating temperature, which, it is argued, is a natural feature of presently favoured D-term inflation models.
[ { "created": "Fri, 29 Jan 1999 18:21:53 GMT", "version": "v1" }, { "created": "Mon, 1 Feb 1999 11:55:23 GMT", "version": "v2" }, { "created": "Fri, 5 Feb 1999 17:30:40 GMT", "version": "v3" } ]
2007-05-23
[ [ "McDonald", "John", "" ] ]
The MSSM has flat directions in its scalar potential, along which it is natural for Bose condensates of squarks to form in the early Universe. A baryon asymmetry can be induced in these condensates via Affleck-Dine baryogenesis. The condensates are unstable with respect to fragmentation to "B-balls", solitons made of squarks and carrying baryon number, which, if they survive thermalization, fill the Universe down to low temperatures, much lower than that of the electroweak phase transition, with interesting cosmological consequences. In particular, their decay implies a similar number density of baryons and dark matter neutralinos, in accordance with observations. Evasion of thermalization and the ability to account for the observed baryon asymmetry requires a very low reheating temperature, which, it is argued, is a natural feature of presently favoured D-term inflation models.
1810.10524
Qin Qin
Shan Cheng and Qin Qin
$Z \to \pi^+\pi^-, K^+K^-$: A touchstone of the PQCD approach
matches published version
Phys. Rev. D 99, 016019 (2019)
10.1103/PhysRevD.99.016019
SI-HEP-2018-30, QFET-2018-19
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study two rare decays, $Z \to \pi^+\pi^-$ and $K^+K^-$, in the perturbative QCD approach up to the next-to-leading order of the strong coupling and the leading power of $1/m_Z$, $m_Z$ being the $Z$ boson mass. The branching ratios $\mathcal{B}(Z\to \pi^+\pi^-) = (0.83 \pm 0.02 \pm 0.02 \pm 0.04)\times 10^{-12}$ and $\mathcal{B}(Z\to K^+K^-) = (1.74^{+0.03}_{-0.05} \pm 0.04 \pm 0.02)\times 10^{-12}$ are obtained and can be measured at a tera-$Z$ factory. Because the subleading-power contributions to the branching ratios are negligible, and the leading one does not depend on any free parameter, the two channels can serve as a touchstone for the applicability of the perturbative QCD approach.
[ { "created": "Wed, 24 Oct 2018 17:59:46 GMT", "version": "v1" }, { "created": "Sun, 3 Feb 2019 09:34:18 GMT", "version": "v2" } ]
2019-02-06
[ [ "Cheng", "Shan", "" ], [ "Qin", "Qin", "" ] ]
We study two rare decays, $Z \to \pi^+\pi^-$ and $K^+K^-$, in the perturbative QCD approach up to the next-to-leading order of the strong coupling and the leading power of $1/m_Z$, $m_Z$ being the $Z$ boson mass. The branching ratios $\mathcal{B}(Z\to \pi^+\pi^-) = (0.83 \pm 0.02 \pm 0.02 \pm 0.04)\times 10^{-12}$ and $\mathcal{B}(Z\to K^+K^-) = (1.74^{+0.03}_{-0.05} \pm 0.04 \pm 0.02)\times 10^{-12}$ are obtained and can be measured at a tera-$Z$ factory. Because the subleading-power contributions to the branching ratios are negligible, and the leading one does not depend on any free parameter, the two channels can serve as a touchstone for the applicability of the perturbative QCD approach.
1912.09862
Patrick Blackstone
Patrick Blackstone, Matteo Fael, Emilie Passemar
$\tau \to \mu\mu\mu$ at a rate of one out of $10^{14}$ tau decays?
6 pages, 2 figures, 1 table. v2 version published in EPJC, minor changes
null
10.1140/epjc/s10052-020-8059-7
null
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We present in a full analytic form the partial widths for the lepton flavour violating decays $\mu^\pm \to e^\pm e^+ e^-$ and $\tau^\pm \to \ell^\pm \ell'^{+} \ell'^{-}$, with $\ell,\ell'=\mu,e$, mediated by neutrino oscillations in the one-loop diagrams. Compared to the first result by Petcov in [1], obtained in the zero momentum limit $\mathcal{P}\ll m_{\nu} \ll M_W$, we retain full dependence on $\mathcal{P}$, the momenta and masses of external particles, and we determine the branching ratios in the physical limit $m_\nu \ll \mathcal{P} \ll M_W$. We show that the claim presented in [2] that the $\tau \to \ell \ell' \ell'$ branching ratios could be as large as $10^{-14}$, as a consequence of keeping the $\mathcal{P}$ dependence, is flawed. We find rates of order $10^{-55}$, even smaller than those obtained in the zero momentum limit, as the latter prediction contains an unphysical logarithmic enhancement.
[ { "created": "Fri, 20 Dec 2019 15:04:39 GMT", "version": "v1" }, { "created": "Tue, 9 Jun 2020 15:05:51 GMT", "version": "v2" } ]
2020-07-15
[ [ "Blackstone", "Patrick", "" ], [ "Fael", "Matteo", "" ], [ "Passemar", "Emilie", "" ] ]
We present in a full analytic form the partial widths for the lepton flavour violating decays $\mu^\pm \to e^\pm e^+ e^-$ and $\tau^\pm \to \ell^\pm \ell'^{+} \ell'^{-}$, with $\ell,\ell'=\mu,e$, mediated by neutrino oscillations in the one-loop diagrams. Compared to the first result by Petcov in [1], obtained in the zero momentum limit $\mathcal{P}\ll m_{\nu} \ll M_W$, we retain full dependence on $\mathcal{P}$, the momenta and masses of external particles, and we determine the branching ratios in the physical limit $m_\nu \ll \mathcal{P} \ll M_W$. We show that the claim presented in [2] that the $\tau \to \ell \ell' \ell'$ branching ratios could be as large as $10^{-14}$, as a consequence of keeping the $\mathcal{P}$ dependence, is flawed. We find rates of order $10^{-55}$, even smaller than those obtained in the zero momentum limit, as the latter prediction contains an unphysical logarithmic enhancement.
1710.01585
Peter Cox
Peter Cox, Chengcheng Han, Tsutomu T. Yanagida
Right-handed Neutrino Dark Matter in a U(1) Extension of the Standard Model
10 two-column pages, 2 figures; v2: version published in JCAP
JCAP 01 (2018) 029
10.1088/1475-7516/2018/01/029
IPMU17-0138
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We consider minimal $U(1)$ extensions of the Standard Model in which one of the right-handed neutrinos is charged under the new gauge symmetry and plays the role of dark matter. In particular, we perform a detailed phenomenological study for the case of a $U(1)_{(B-L)_3}$ flavoured $B-L$ symmetry. If perturbativity is required up to high-scales, we find an upper bound on the dark matter mass of $m_\chi\lesssim2$ TeV, significantly stronger than that obtained in simplified models. Furthermore, if the $U(1)_{(B-L)_3}$ breaking scalar has significant mixing with the SM Higgs, there are already strong constraints from direct detection. On the other hand, there remains significant viable parameter space in the case of small mixing, which may be probed in the future via LHC $Z^\prime$ searches and indirect detection. We also comment on more general anomaly-free symmetries consistent with a TeV-scale RH neutrino dark matter candidate, and show that if two heavy RH neutrinos for leptogenesis are also required, one is naturally led to a single-parameter class of $U(1)$ symmetries.
[ { "created": "Wed, 4 Oct 2017 13:07:40 GMT", "version": "v1" }, { "created": "Thu, 18 Jan 2018 01:37:02 GMT", "version": "v2" } ]
2018-01-19
[ [ "Cox", "Peter", "" ], [ "Han", "Chengcheng", "" ], [ "Yanagida", "Tsutomu T.", "" ] ]
We consider minimal $U(1)$ extensions of the Standard Model in which one of the right-handed neutrinos is charged under the new gauge symmetry and plays the role of dark matter. In particular, we perform a detailed phenomenological study for the case of a $U(1)_{(B-L)_3}$ flavoured $B-L$ symmetry. If perturbativity is required up to high-scales, we find an upper bound on the dark matter mass of $m_\chi\lesssim2$ TeV, significantly stronger than that obtained in simplified models. Furthermore, if the $U(1)_{(B-L)_3}$ breaking scalar has significant mixing with the SM Higgs, there are already strong constraints from direct detection. On the other hand, there remains significant viable parameter space in the case of small mixing, which may be probed in the future via LHC $Z^\prime$ searches and indirect detection. We also comment on more general anomaly-free symmetries consistent with a TeV-scale RH neutrino dark matter candidate, and show that if two heavy RH neutrinos for leptogenesis are also required, one is naturally led to a single-parameter class of $U(1)$ symmetries.
1106.3283
Damir Becirevic
Damir Becirevic and Elia Schneider
On transverse asymmetries in B --> K* l+l-
21 pages, 4 figures (png) - version published in NPB
null
10.1016/j.nuclphysb.2011.09.004
LPT 11-50
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We discuss the three independent asymmetries, AT(2)(q2), AT(im)(q2) and AT(re)(q2), that one can build from the amplitudes A_perp(q2) and A_par(q2). These quantities are expected to be accessible from the new B-physics experiments, they are sensitive to the presence of new physics, and they are not significantly sensitive to hadronic uncertainties. Studying their low q2-dependence can be helpful in discerning among various possible new physics scenarios. All three asymmetries can be extracted from the full angular analysis of B-->K* l+l-. Our formulas apply to both the massless and the massive lepton case.
[ { "created": "Thu, 16 Jun 2011 17:26:11 GMT", "version": "v1" }, { "created": "Mon, 4 Jul 2011 16:29:37 GMT", "version": "v2" }, { "created": "Mon, 19 Sep 2011 09:41:13 GMT", "version": "v3" }, { "created": "Thu, 2 Feb 2012 14:11:48 GMT", "version": "v4" } ]
2015-05-28
[ [ "Becirevic", "Damir", "" ], [ "Schneider", "Elia", "" ] ]
We discuss the three independent asymmetries, AT(2)(q2), AT(im)(q2) and AT(re)(q2), that one can build from the amplitudes A_perp(q2) and A_par(q2). These quantities are expected to be accessible from the new B-physics experiments, they are sensitive to the presence of new physics, and they are not significantly sensitive to hadronic uncertainties. Studying their low q2-dependence can be helpful in discerning among various possible new physics scenarios. All three asymmetries can be extracted from the full angular analysis of B-->K* l+l-. Our formulas apply to both the massless and the massive lepton case.