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707.243
A study of logarithmic corrections and universal amplitude ratios in the two-dimensional 4-state Potts model
Monte Carlo (MC) and series expansion (SE) data for the energy, specific heat, magnetization and susceptibility of the two-dimensional 4-state Potts model in the vicinity of the critical point are analysed. The role of logarithmic corrections is discussed and an approach is proposed in order to account numerically for these corrections in the determination of critical amplitudes. Accurate estimates of universal amplitude ratios $A_+/A_-$, $\Gamma_+/\Gamma_-$, $\Gamma_T/\Gamma_-$ and $R_C^\pm$ are given, which arouse new questions with respect to previous works.
cond-mat.stat-mech hep-lat hep-th
monte carlo mc and series expansion se data for the energy specific heat magnetization and susceptibility of the twodimensional 4state potts model in the vicinity of the critical point are analysed the role of logarithmic corrections is discussed and an approach is proposed in order to account numerically for these corrections in the determination of critical amplitudes accurate estimates of universal amplitude ratios a_a_ gamma_gamma_ gamma_tgamma_ and r_cpm are given which arouse new questions with respect to previous works
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707.2431
Quarkonium and hydrogen spectra with spin dependent relativistic wave equation
A non-linear non-perturbative relativistic atomic theory introduces spin in the dynamics of particle motion. The resulting energy levels of Hydrogen atom are exactly same as the Dirac theory. The theory accounts for the energy due to spin-orbit interaction and for the additional potential energy due to spin and spin-orbit coupling. Spin angular momentum operator is integrated into the equation of motion. This requires modification to classical Laplacian operator. Consequently the Dirac matrices and the k operator of Dirac's theory are dispensed with. The theory points out that the curvature of the orbit draws on certain amount of kinetic and potential energies affecting the momentum of electron and the spin-orbit interaction energy constitutes a part of this energy. The theory is developed for spin 1/2 bound state single electron in Coulomb potential and then further extended to quarkonium physics by introducing the linear confining potential. The unique feature of this quarkonium model is that the radial distance can be exactly determined and does not have a statistical interpretation. The established radial distance is then used to determine the wave function. The observed energy levels are used as the input parameters and the radial distance and the string tension are predicted. This ensures 100% conformance to all observed energy levels for the heavy quarkonium.
physics.gen-ph
a nonlinear nonperturbative relativistic atomic theory introduces spin in the dynamics of particle motion the resulting energy levels of hydrogen atom are exactly same as the dirac theory the theory accounts for the energy due to spinorbit interaction and for the additional potential energy due to spin and spinorbit coupling spin angular momentum operator is integrated into the equation of motion this requires modification to classical laplacian operator consequently the dirac matrices and the k operator of diracs theory are dispensed with the theory points out that the curvature of the orbit draws on certain amount of kinetic and potential energies affecting the momentum of electron and the spinorbit interaction energy constitutes a part of this energy the theory is developed for spin 12 bound state single electron in coulomb potential and then further extended to quarkonium physics by introducing the linear confining potential the unique feature of this quarkonium model is that the radial distance can be exactly determined and does not have a statistical interpretation the established radial distance is then used to determine the wave function the observed energy levels are used as the input parameters and the radial distance and the string tension are predicted this ensures 100 conformance to all observed energy levels for the heavy quarkonium
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707.2432
Pricing Asian Options for Jump Diffusions
We construct a sequence of functions that uniformly converge (on compact sets) to the price of Asian option, which is written on a stock whose dynamics follows a jump diffusion, exponentially fast. Each of the element in this sequence solves a parabolic partial differen- tial equation (not an integro-differential equation). As a result we obtain a fast numerical approximation scheme whose accuracy versus speed characteristics can be controlled. We analyze the performance of our numerical algorithm on several examples.
cs.CE
we construct a sequence of functions that uniformly converge on compact sets to the price of asian option which is written on a stock whose dynamics follows a jump diffusion exponentially fast each of the element in this sequence solves a parabolic partial differen tial equation not an integrodifferential equation as a result we obtain a fast numerical approximation scheme whose accuracy versus speed characteristics can be controlled we analyze the performance of our numerical algorithm on several examples
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707.2433
Kilohertz laser ablation for doping helium nanodroplets
A new setup for doping helium nanodroplets by means of laser ablation at kilohertz repetition rate is presented. The doping process is characterized and two distinct regimes of laser ablation are identified. The setup is shown to be efficient and stable enough to be used for spectroscopy, as demonstrated on beam-depletion spectra of lithium atoms attached to helium nanodroplets. For the first time, helium droplets are doped with high temperature refractory materials such as titanium and tantalum. Doping with the non-volatile DNA basis Guanine is found to be efficient and a number of oligomers are detected.
physics.atm-clus
a new setup for doping helium nanodroplets by means of laser ablation at kilohertz repetition rate is presented the doping process is characterized and two distinct regimes of laser ablation are identified the setup is shown to be efficient and stable enough to be used for spectroscopy as demonstrated on beamdepletion spectra of lithium atoms attached to helium nanodroplets for the first time helium droplets are doped with high temperature refractory materials such as titanium and tantalum doping with the nonvolatile dna basis guanine is found to be efficient and a number of oligomers are detected
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707.2434
3-point off-shell vertex in scalar QED in arbitrary gauge and dimension
We calculate the complete one-loop off-shell three-point scalar-photon vertex in arbitrary gauge and dimension for Scalar Quantum Electrodynamics. Explicit results are presented for the particular cases of dimensions 3 and 4 both for massive and massless scalars. We then propose non-perturbative forms of this vertex that coincide with the perturbative answer to order $e^2$.
hep-th
we calculate the complete oneloop offshell threepoint scalarphoton vertex in arbitrary gauge and dimension for scalar quantum electrodynamics explicit results are presented for the particular cases of dimensions 3 and 4 both for massive and massless scalars we then propose nonperturbative forms of this vertex that coincide with the perturbative answer to order e2
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707.2435
Effective mean-field equations for cigar-shaped and disk-shaped Bose-Einstein condensates
By applying the standard adiabatic approximation and using the accurate analytical expression for the corresponding local chemical potential obtained in our previous work [Phys. Rev. A \textbf{75}, 063610 (2007)] we derive an effective 1D equation that governs the axial dynamics of mean-field cigar-shaped condensates with repulsive interatomic interactions, accounting accurately for the contribution from the transverse degrees of freedom. This equation, which is more simple than previous proposals, is also more accurate. Moreover, it allows treating condensates containing an axisymmetric vortex with no additional cost. Our effective equation also has the correct limit in both the quasi-1D mean-field regime and the Thomas-Fermi regime and permits one to derive fully analytical expressions for ground-state properties such as the chemical potential, axial length, axial density profile, and local sound velocity. These analytical expressions remain valid and accurate in between the above two extreme regimes. Following the same procedure we also derive an effective 2D equation that governs the transverse dynamics of mean-field disk-shaped condensates. This equation, which also has the correct limit in both the quasi-2D and the Thomas-Fermi regime, is again more simple and accurate than previous proposals. We have checked the validity of our equations by numerically solving the full 3D Gross-Pitaevskii equation.
cond-mat.other
by applying the standard adiabatic approximation and using the accurate analytical expression for the corresponding local chemical potential obtained in our previous work phys rev a textbf75 063610 2007 we derive an effective 1d equation that governs the axial dynamics of meanfield cigarshaped condensates with repulsive interatomic interactions accounting accurately for the contribution from the transverse degrees of freedom this equation which is more simple than previous proposals is also more accurate moreover it allows treating condensates containing an axisymmetric vortex with no additional cost our effective equation also has the correct limit in both the quasi1d meanfield regime and the thomasfermi regime and permits one to derive fully analytical expressions for groundstate properties such as the chemical potential axial length axial density profile and local sound velocity these analytical expressions remain valid and accurate in between the above two extreme regimes following the same procedure we also derive an effective 2d equation that governs the transverse dynamics of meanfield diskshaped condensates this equation which also has the correct limit in both the quasi2d and the thomasfermi regime is again more simple and accurate than previous proposals we have checked the validity of our equations by numerically solving the full 3d grosspitaevskii equation
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707.2436
On the Polyphase Decomposition for Design of Generalized Comb Decimation Filters
Generalized comb filters (GCFs) are efficient anti-aliasing decimation filters with improved selectivity and quantization noise (QN) rejection performance around the so called folding bands with respect to classical comb filters. In this paper, we address the design of GCF filters by proposing an efficient partial polyphase architecture with the aim to reduce the data rate as much as possible after the Sigma-Delta A/D conversion. We propose a mathematical framework in order to completely characterize the dependence of the frequency response of GCFs on the quantization of the multipliers embedded in the proposed filter architecture. This analysis paves the way to the design of multiplier-less decimation architectures. We also derive the impulse response of a sample 3rd order GCF filter used as a reference scheme throughout the paper.
cs.OH
generalized comb filters gcfs are efficient antialiasing decimation filters with improved selectivity and quantization noise qn rejection performance around the so called folding bands with respect to classical comb filters in this paper we address the design of gcf filters by proposing an efficient partial polyphase architecture with the aim to reduce the data rate as much as possible after the sigmadelta ad conversion we propose a mathematical framework in order to completely characterize the dependence of the frequency response of gcfs on the quantization of the multipliers embedded in the proposed filter architecture this analysis paves the way to the design of multiplierless decimation architectures we also derive the impulse response of a sample 3rd order gcf filter used as a reference scheme throughout the paper
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707.2437
Investigation of a lattice Boltzmann model with a variable speed of sound
A lattice Boltzmann model is considered in which the speed of sound can be varied independently of the other parameters. The range over which the speed of sound can be varied is investigated and good agreement is found between simulations and theory. The onset of nonlinear effects due to variations in the speed of sound is also investigated and good agreement is again found with theory. It is also shown that the fluid viscosity is not altered by changing the speed of sound.
physics.flu-dyn physics.comp-ph
a lattice boltzmann model is considered in which the speed of sound can be varied independently of the other parameters the range over which the speed of sound can be varied is investigated and good agreement is found between simulations and theory the onset of nonlinear effects due to variations in the speed of sound is also investigated and good agreement is again found with theory it is also shown that the fluid viscosity is not altered by changing the speed of sound
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707.2438
LibCPIXE: a PIXE simulation open-source library for multilayered samples
Most particle induced X-ray emission (PIXE) data analysis codes are not focused on handling multilayered samples. We have developed an open-source library called "LibCPIXE", for PIXE data analysis. It is written in standard C and implements functions for simulating X-ray yields of PIXE spectra taken from arbitrary samples, including multilayered targets. The library is designed to be fast, portable, modular and scalable, as well as to facilitate its incorporation into any existing program. In order to demonstrate the capabilities of the library, a program called CPIXE was developed and used to analyze various real samples involving both bulk and layered samples. Just as the library, the CPIXE source code is freely available under the General Public License. We demonstrate that it runs both under GNU/Linux systems as well as under MS Windows. There is in principle no limitation to port it to other platforms.
cond-mat.mtrl-sci
most particle induced xray emission pixe data analysis codes are not focused on handling multilayered samples we have developed an opensource library called libcpixe for pixe data analysis it is written in standard c and implements functions for simulating xray yields of pixe spectra taken from arbitrary samples including multilayered targets the library is designed to be fast portable modular and scalable as well as to facilitate its incorporation into any existing program in order to demonstrate the capabilities of the library a program called cpixe was developed and used to analyze various real samples involving both bulk and layered samples just as the library the cpixe source code is freely available under the general public license we demonstrate that it runs both under gnulinux systems as well as under ms windows there is in principle no limitation to port it to other platforms
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707.2439
A Presentation for the Dual Symmetric Inverse Monoid
The dual symmetric inverse monoid $\mathscr{I}_n^*$ is the inverse monoid of all isomorphisms between quotients of an $n$-set. We give a monoid presentation of $\mathscr{I}_n^*$ and, along the way, establish criteria for a monoid to be inverse when it is generated by completely regular elements.
math.GR
the dual symmetric inverse monoid mathscri_n is the inverse monoid of all isomorphisms between quotients of an nset we give a monoid presentation of mathscri_n and along the way establish criteria for a monoid to be inverse when it is generated by completely regular elements
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707.244
Moduli spaces of quadratic complexes and their singular surfaces
We construct the coarse moduli space $\cM_{qc}(\sigma)$ of quadratic line complexes with a fixed Segre symbol $\sigma$ as well as the moduli space $\cM_{ss}(\sigma)$ of the corresponding singular surfaces. We show that the map associating to a quadratic line complex its singular surface induces a morphism $\pi: \cM_{qc}(\sigma) \ra \cM_{ss}(\sigma)$. Finally we deduce that the varieties of cosingular quadratic line complexes are almost always curves.
math.AG
we construct the coarse moduli space cm_qcsigma of quadratic line complexes with a fixed segre symbol sigma as well as the moduli space cm_sssigma of the corresponding singular surfaces we show that the map associating to a quadratic line complex its singular surface induces a morphism pi cm_qcsigma ra cm_sssigma finally we deduce that the varieties of cosingular quadratic line complexes are almost always curves
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707.2441
A Galois-theoretic approach to Kanev's correspondence
Let $G$ be a finite group, $\Lambda$ an absolutely irreducible $\Z[G]$-module and $w$ a weight of $\Lambda$. To any Galois covering with group $G$ we associate two correspondences, the Schur and the Kanev correspondence. We work out their relation and compute their invariants. Using this, we give some new examples of Prym-Tyurin varieties.
math.AG
let g be a finite group lambda an absolutely irreducible zgmodule and w a weight of lambda to any galois covering with group g we associate two correspondences the schur and the kanev correspondence we work out their relation and compute their invariants using this we give some new examples of prymtyurin varieties
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707.2442
Desynchronization of pulse-coupled oscillators with delayed excitatory coupling
Collective behavior of pulse-coupled oscillators has been investigated widely. As an example of pulse-coupled networks, fireflies display many kinds of flashing patterns. Mirollo and Strogatz (1990) proposed a pulse-coupled oscillator model to explain the synchronization of South East Asian fireflies ({\itshape Pteroptyx malaccae}). However, transmission delays were not considered in their model. In fact, the presence of transmission delays can lead to desychronization. In this paper, pulse-coupled oscillator networks with delayed excitatory coupling are studied. Our main result is that under reasonable assumptions, pulse-coupled oscillator networks with delayed excitatory coupling can not achieve complete synchronization, which can explain why another species of fireflies ({\itshape Photinus pyralis}) rarely synchronizes flashing. Finally, two numerical simulations are given. In the first simulation, we illustrate that even if all the initial phases are very close to each other, there could still be big variations in the times to process the pulses in the pipeline. It implies that asymptotical synchronization typically also cannot be achieved. In the second simulation, we exhibit a phenomenon of clustering synchronization.
math.DS
collective behavior of pulsecoupled oscillators has been investigated widely as an example of pulsecoupled networks fireflies display many kinds of flashing patterns mirollo and strogatz 1990 proposed a pulsecoupled oscillator model to explain the synchronization of south east asian fireflies itshape pteroptyx malaccae however transmission delays were not considered in their model in fact the presence of transmission delays can lead to desychronization in this paper pulsecoupled oscillator networks with delayed excitatory coupling are studied our main result is that under reasonable assumptions pulsecoupled oscillator networks with delayed excitatory coupling can not achieve complete synchronization which can explain why another species of fireflies itshape photinus pyralis rarely synchronizes flashing finally two numerical simulations are given in the first simulation we illustrate that even if all the initial phases are very close to each other there could still be big variations in the times to process the pulses in the pipeline it implies that asymptotical synchronization typically also cannot be achieved in the second simulation we exhibit a phenomenon of clustering synchronization
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707.2443
Correlated Anisotropies in the Cosmic Far-Infrared Background Detected by MIPS/Spitzer: Constraint on the Bias
We report the detection of correlated anisotropies in the Cosmic Far-Infrared Background at 160 microns. We measure the power spectrum in the Spitzer/SWIRE Lockman Hole field. It reveals unambiguously a strong excess above cirrus and Poisson contributions, at spatial scales between 5 and 30 arcminutes, interpreted as the signature of infrared galaxy clustering. Using our model of infrared galaxy evolution we derive a linear bias b=1.74 \pm 0.16. It is a factor 2 higher than the bias measured for the local IRAS galaxies. Our model indicates that galaxies dominating the 160 microns correlated anisotropies are at z~1. This implies that infrared galaxies at high redshifts are biased tracers of mass, unlike in the local Universe.
astro-ph
we report the detection of correlated anisotropies in the cosmic farinfrared background at 160 microns we measure the power spectrum in the spitzerswire lockman hole field it reveals unambiguously a strong excess above cirrus and poisson contributions at spatial scales between 5 and 30 arcminutes interpreted as the signature of infrared galaxy clustering using our model of infrared galaxy evolution we derive a linear bias b174 pm 016 it is a factor 2 higher than the bias measured for the local iras galaxies our model indicates that galaxies dominating the 160 microns correlated anisotropies are at z1 this implies that infrared galaxies at high redshifts are biased tracers of mass unlike in the local universe
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707.2444
The equilibrium states for semigroups of rational maps
We consider the dynamics of skew product maps associated with finitely generated semigroups of rational maps on the Riemann sphere. We show that under some conditions on the dynamics and the potential function \psi, there exists a unique equilibrium state for \psi and a unique $\exp(\P(\psi)-\psi)$-conformal measure, where P(\psi) denotes the topological pressure of \psi.
math.DS math.CV math.PR
we consider the dynamics of skew product maps associated with finitely generated semigroups of rational maps on the riemann sphere we show that under some conditions on the dynamics and the potential function psi there exists a unique equilibrium state for psi and a unique expppsipsiconformal measure where ppsi denotes the topological pressure of psi
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707.2445
The Wigner-Fokker-Planck equation: Stationary states and large time behavior
This paper has been withdrawn by the authors due to a crucial error in the proof of the main result. In a new manuscript (with two new authors) available at arXiv:1010.2791v1 this problem has been resolved.
quant-ph cond-mat.stat-mech math-ph math.AP math.MP
this paper has been withdrawn by the authors due to a crucial error in the proof of the main result in a new manuscript with two new authors available at arxiv10102791v1 this problem has been resolved
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707.2446
Control of poultry chicken malaria by surface functionalized amorphous nanosilica
Surface modified amorphous nanoporous silica molecules with hydrophobic as well as hydrophilic character can be effectively used as therapeutic drug for combating chicken malaria in poultry industry. The amorphous nanosilica was developed by top-down approach using volcanic soil derived silica as source material. Amorphous silica has long been used as feed additive for poultry industry and considered to be safe for human consumption by WHO and USDA. The basic mechanism of action of these nanosilica molecules is mediated by the physical absorption of VLDL, serum triglycerides and other serum cholesterol components in the lipophilic nanopores of nanosilica. This reduces the supply of the host derived cholesterol, thus limiting the growth of the malarial parasite in vivo.
q-bio.BM q-bio.MN
surface modified amorphous nanoporous silica molecules with hydrophobic as well as hydrophilic character can be effectively used as therapeutic drug for combating chicken malaria in poultry industry the amorphous nanosilica was developed by topdown approach using volcanic soil derived silica as source material amorphous silica has long been used as feed additive for poultry industry and considered to be safe for human consumption by who and usda the basic mechanism of action of these nanosilica molecules is mediated by the physical absorption of vldl serum triglycerides and other serum cholesterol components in the lipophilic nanopores of nanosilica this reduces the supply of the host derived cholesterol thus limiting the growth of the malarial parasite in vivo
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707.2447
Real analyticity of Hausdorff dimension for expanding rational semigroups
We consider the dynamics of expanding semigroups generated by finitely many rational maps on the Riemann sphere. We show that for an analytic family of such semigroups, the Bowen parameter function is real-analytic and plurisubharmonic. Combining this with a result obtained by the first author, we show that if for each semigroup of such an analytic family of expanding semigroups satisfies the open set condition, then the function of the Hausdorff dimension of the Julia set is real-analytic and plurisubharmonic. Moreover, we provide an extensive collection of classes of examples of analytic families of semigroups satisfying all the above conditions and we analyze in detail the corresponding Bowen's parameters and Hausdorff dimension function.
math.DS math.CV math.PR
we consider the dynamics of expanding semigroups generated by finitely many rational maps on the riemann sphere we show that for an analytic family of such semigroups the bowen parameter function is realanalytic and plurisubharmonic combining this with a result obtained by the first author we show that if for each semigroup of such an analytic family of expanding semigroups satisfies the open set condition then the function of the hausdorff dimension of the julia set is realanalytic and plurisubharmonic moreover we provide an extensive collection of classes of examples of analytic families of semigroups satisfying all the above conditions and we analyze in detail the corresponding bowens parameters and hausdorff dimension function
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707.2448
Towards truly simultaneous PIXE and RBS analysis of layered objects in cultural heritage
For a long time, RBS and PIXE techniques have been used in the field of cultural heritage. Although the complementarity of both techniques has long been acknowledged, its full potential has not been yet developed due to the lack of general purpose software tools for analysing the data from both techniques in a coherent way. In this work we provide an example of how the recent addition of PIXE to the set of techniques supported by the DataFurnace code can significantly change this situation. We present a case in which a non homogeneous sample (an oxidized metal from a photographic plate -heliography- made by Niepce in 1827) is analysed using RBS and PIXE in a straightforward and powerful way that can only be performed with a code that treats both techniques simultaneously as a part of one single and coherent analysis. The optimization capabilities of DataFurnace, allowed us to obtain the composition profiles for these samples in a very simple way.
cond-mat.mtrl-sci
for a long time rbs and pixe techniques have been used in the field of cultural heritage although the complementarity of both techniques has long been acknowledged its full potential has not been yet developed due to the lack of general purpose software tools for analysing the data from both techniques in a coherent way in this work we provide an example of how the recent addition of pixe to the set of techniques supported by the datafurnace code can significantly change this situation we present a case in which a non homogeneous sample an oxidized metal from a photographic plate heliography made by niepce in 1827 is analysed using rbs and pixe in a straightforward and powerful way that can only be performed with a code that treats both techniques simultaneously as a part of one single and coherent analysis the optimization capabilities of datafurnace allowed us to obtain the composition profiles for these samples in a very simple way
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707.2449
Hawking Radiation and Covariant Anomalies
Generalising the method of Wilczek and collaborators we provide a derivation of Hawking radiation from charged black holes using only covariant gauge and gravitational anomalies. The reliability and universality of the anomaly cancellation approach to Hawking radiation is also discussed.
hep-th gr-qc
generalising the method of wilczek and collaborators we provide a derivation of hawking radiation from charged black holes using only covariant gauge and gravitational anomalies the reliability and universality of the anomaly cancellation approach to hawking radiation is also discussed
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707.245
"Black Star" or Astrophysical Black Hole?
Recently wide publicity has been given to a claim by T. Vachaspati that "black holes do not exist", that the objects known as black holes in astrophysics should rather be called "black stars" and they not only do not have event horizons but actually can be the source of spectacular gamma ray bursts. In this short essay (no flimsier than the original preprint where these extravagant claims appeared) I demonstrate that these ill-considered claims are clearly wrong. Yet they present a good occasion to reflect on some well known but little discussed conceptual difficulties which arise when applying relativistic terminology in an astrophysical context.
astro-ph
recently wide publicity has been given to a claim by t vachaspati that black holes do not exist that the objects known as black holes in astrophysics should rather be called black stars and they not only do not have event horizons but actually can be the source of spectacular gamma ray bursts in this short essay no flimsier than the original preprint where these extravagant claims appeared i demonstrate that these illconsidered claims are clearly wrong yet they present a good occasion to reflect on some well known but little discussed conceptual difficulties which arise when applying relativistic terminology in an astrophysical context
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707.2451
SUSY Unparticle and Conformal Sequestering
We investigate unparticle physics with supersymmetry (SUSY). The SUSY breaking effects due to the gravity mediation induce soft masses for the SUSY unparticles and hence break the conformal invariance. The unparticle physics observable in near future experiments is only consistent if the SUSY breaking effects from the hidden sector to the standard model sector are dominated by the gauge mediation, or if the SUSY breaking effects to the unparticle sector is sufficiently sequestered. We argue that the natural realization of the latter possibility is the conformal sequestering scenario.
hep-ph hep-th
we investigate unparticle physics with supersymmetry susy the susy breaking effects due to the gravity mediation induce soft masses for the susy unparticles and hence break the conformal invariance the unparticle physics observable in near future experiments is only consistent if the susy breaking effects from the hidden sector to the standard model sector are dominated by the gauge mediation or if the susy breaking effects to the unparticle sector is sufficiently sequestered we argue that the natural realization of the latter possibility is the conformal sequestering scenario
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707.2452
A new prescription for soft gluon resummation
We present a new prescription for the resummation of the divergent series of perturbative corrections, due to soft gluon emission, to hard processes near threshold in perturbative QCD (threshold resummation). This prescription is based on Borel resummation, and contrary to the commonly used minimal prescription, it does not introduce a dependence of resummed physical observables on the kinematically unaccessible x->0 region of parton distributions. We compare results for resummed deep-inelastic scattering obtained using the Borel prescription and the minimal prescription and exploit the comparison to discuss the ambiguities related to the resummation procedure.
hep-ph
we present a new prescription for the resummation of the divergent series of perturbative corrections due to soft gluon emission to hard processes near threshold in perturbative qcd threshold resummation this prescription is based on borel resummation and contrary to the commonly used minimal prescription it does not introduce a dependence of resummed physical observables on the kinematically unaccessible x0 region of parton distributions we compare results for resummed deepinelastic scattering obtained using the borel prescription and the minimal prescription and exploit the comparison to discuss the ambiguities related to the resummation procedure
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707.2453
Unfolding of differential energy spectra in the MAGIC experiment
The paper describes the different methods, used in the MAGIC experiment, to unfold experimental energy distributions of cosmic ray particles (gamma-rays). Questions and problems related to the unfolding are discussed. Various procedures are proposed which can help to make the unfolding robust and reliable. The different methods and procedures are implemented in the MAGIC software and are used in most of the analyses.
astro-ph
the paper describes the different methods used in the magic experiment to unfold experimental energy distributions of cosmic ray particles gammarays questions and problems related to the unfolding are discussed various procedures are proposed which can help to make the unfolding robust and reliable the different methods and procedures are implemented in the magic software and are used in most of the analyses
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707.2454
A semiregularity map annihilating obstructions to deforming holomorphic maps
We study deformations of holomorphic maps of compact, complex, K\"ahler manifolds. In particular, we describe a generalization of Bloch's semiregularity map that annihilates obstructions to deform holomorphic maps with fixed codomain.
math.AG math.QA
we study deformations of holomorphic maps of compact complex kahler manifolds in particular we describe a generalization of blochs semiregularity map that annihilates obstructions to deform holomorphic maps with fixed codomain
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707.2455
Chiral Asymmetry from a 5D Higgs Mechanism
An intriguing feature of the Standard Model is that the representations of the unbroken gauge symmetries are vector-like whereas those of the spontaneously broken gauge symmetries are chiral. Here we provide a toy model which shows that a natural explanation of this property could emerge in higher dimensional field theories and discuss the difficulties that arise in the attempt to construct a realistic theory. An interesting aspect of this type of models is that the 4D low energy effective theory is not generically gauge invariant. However, the non-invariant contributions to the observable quantities are very small, of the order of the square of the ratio between the light particle mass scale and the Kaluza-Klein mass scale. Remarkably, when we take the unbroken limit both the chiral asymmetry and the non-invariant terms disappear.
hep-th hep-ph
an intriguing feature of the standard model is that the representations of the unbroken gauge symmetries are vectorlike whereas those of the spontaneously broken gauge symmetries are chiral here we provide a toy model which shows that a natural explanation of this property could emerge in higher dimensional field theories and discuss the difficulties that arise in the attempt to construct a realistic theory an interesting aspect of this type of models is that the 4d low energy effective theory is not generically gauge invariant however the noninvariant contributions to the observable quantities are very small of the order of the square of the ratio between the light particle mass scale and the kaluzaklein mass scale remarkably when we take the unbroken limit both the chiral asymmetry and the noninvariant terms disappear
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707.2456
Effects of the low frequencies of noise on On-Off intermittency
A bifurcating system subject to multiplicative noise can exhibit on-off intermittency close to the instability threshold. For a canonical system, we discuss the dependence of this intermittency on the Power Spectrum Density (PSD) of the noise. Our study is based on the calculation of the Probability Density Function (PDF) of the unstable variable. We derive analytical results for some particular types of noises and interpret them in the framework of on-off intermittency. Besides, we perform a cumulant expansion for a random noise with arbitrary power spectrum density and show that the intermittent regime is controlled by the ratio between the departure from the threshold and the value of the PSD of the noise at zero frequency. Our results are in agreement with numerical simulations performed with two types of random perturbations: colored Gaussian noise and deterministic fluctuations of a chaotic variable. Extensions of this study to another, more complex, system are presented and the underlying mechanisms are discussed.
cond-mat.stat-mech nlin.CD
a bifurcating system subject to multiplicative noise can exhibit onoff intermittency close to the instability threshold for a canonical system we discuss the dependence of this intermittency on the power spectrum density psd of the noise our study is based on the calculation of the probability density function pdf of the unstable variable we derive analytical results for some particular types of noises and interpret them in the framework of onoff intermittency besides we perform a cumulant expansion for a random noise with arbitrary power spectrum density and show that the intermittent regime is controlled by the ratio between the departure from the threshold and the value of the psd of the noise at zero frequency our results are in agreement with numerical simulations performed with two types of random perturbations colored gaussian noise and deterministic fluctuations of a chaotic variable extensions of this study to another more complex system are presented and the underlying mechanisms are discussed
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707.2457
Glow Discharge AES: Methodological Peculiarities of Pulse Element Analysis and Flash Desorption
Different techniques of Glow Discharge AES are described in this paper. The most important parameters at such investigations are: the power of VHF-field, pressure of the inert gas and concentration of the easily ionizable additive, e.g. NaCl. The influences of these parameters were studied It is proposed a high sensitive flash desorption method, which enables investigation of the water desorption rate from humidified samples of biological origin, namely DNA and chromatin. The ways of minimizing of detection limit are considered as the most important characteristics of an analytical device. The concentration of any measured element is detectable if it correlates to the signal equal to tripled standard deviation of the results of background measurement. Electron temperature of the Helium has been evaluated by absorption rate at two lines of helium \lambda=353.828nm; \lambda'=344.759nm that was equal to T_c ~ 15000 K.
physics.bio-ph
different techniques of glow discharge aes are described in this paper the most important parameters at such investigations are the power of vhffield pressure of the inert gas and concentration of the easily ionizable additive eg nacl the influences of these parameters were studied it is proposed a high sensitive flash desorption method which enables investigation of the water desorption rate from humidified samples of biological origin namely dna and chromatin the ways of minimizing of detection limit are considered as the most important characteristics of an analytical device the concentration of any measured element is detectable if it correlates to the signal equal to tripled standard deviation of the results of background measurement electron temperature of the helium has been evaluated by absorption rate at two lines of helium lambda353828nm lambda344759nm that was equal to t_c 15000 k
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707.2458
Thermal imaginary part of a real-time static potential from classical lattice gauge theory simulations
Recently, a finite-temperature real-time static potential has been introduced via a Schr\"odinger-type equation satisfied by a certain heavy quarkonium Green's function. Furthermore, it has been pointed out that it possesses an imaginary part, which induces a finite width for the tip of the quarkonium peak in the thermal dilepton production rate. The imaginary part originates from Landau-damping of low-frequency gauge fields, which are essentially classical due to their high occupation number. Here we show how the imaginary part can be measured with classical lattice gauge theory simulations, accounting non-perturbatively for the infrared sector of finite-temperature field theory. We demonstrate that a non-vanishing imaginary part indeed exists non-perturbatively; and that its value agrees semi-quantitatively with that predicted by Hard Loop resummed perturbation theory.
hep-lat hep-ph
recently a finitetemperature realtime static potential has been introduced via a schrodingertype equation satisfied by a certain heavy quarkonium greens function furthermore it has been pointed out that it possesses an imaginary part which induces a finite width for the tip of the quarkonium peak in the thermal dilepton production rate the imaginary part originates from landaudamping of lowfrequency gauge fields which are essentially classical due to their high occupation number here we show how the imaginary part can be measured with classical lattice gauge theory simulations accounting nonperturbatively for the infrared sector of finitetemperature field theory we demonstrate that a nonvanishing imaginary part indeed exists nonperturbatively and that its value agrees semiquantitatively with that predicted by hard loop resummed perturbation theory
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707.2459
Using globular clusters to test gravity in the weak acceleration regime
We report on the results from an ongoing program aimed at testing Newton's law of gravity in the low acceleration regime using globular clusters. It is shown that all clusters studied so far do behave like galaxies, that is, their velocity dispersion profile flattens out at large radii where the acceleration of gravity goes below 1e-8 cm/s/s, instead of following the expected Keplerian fall off. In galaxies this behavior is ascribed to the existence of a dark matter halo. Globular clusters, however, do not contain dark matter, hence this result might indicate that our present understanding of gravity in the weak regime of accelerations is incomplete and somehow incorrect.
astro-ph
we report on the results from an ongoing program aimed at testing newtons law of gravity in the low acceleration regime using globular clusters it is shown that all clusters studied so far do behave like galaxies that is their velocity dispersion profile flattens out at large radii where the acceleration of gravity goes below 1e8 cmss instead of following the expected keplerian fall off in galaxies this behavior is ascribed to the existence of a dark matter halo globular clusters however do not contain dark matter hence this result might indicate that our present understanding of gravity in the weak regime of accelerations is incomplete and somehow incorrect
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707.246
Magnetic Interference Patterns and Vortices in Diffusive SNS junctions
We study theoretically the electronic and transport properties of a diffusive superconductor-normal metal-superconductor (SNS) junction in the presence of a perpendicular magnetic field. We show that the field dependence of the critical current crosses over from the well-known Fraunhofer pattern in wide junctions to a monotonous decay when the width of the normal wire is smaller than the magnetic length \xi_H = \sqrt{\Phi_0/H}, where H is the magnetic field and \Phi_0 the flux quantum. We demonstrate that this behavior is a direct consequence of the magnetic vortex structure appearing in the normal region and predict how such structure is manifested in the local density of states.
cond-mat.supr-con cond-mat.mes-hall
we study theoretically the electronic and transport properties of a diffusive superconductornormal metalsuperconductor sns junction in the presence of a perpendicular magnetic field we show that the field dependence of the critical current crosses over from the wellknown fraunhofer pattern in wide junctions to a monotonous decay when the width of the normal wire is smaller than the magnetic length xi_h sqrtphi_0h where h is the magnetic field and phi_0 the flux quantum we demonstrate that this behavior is a direct consequence of the magnetic vortex structure appearing in the normal region and predict how such structure is manifested in the local density of states
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707.2461
Bosons, Fermions and Branes
Starting from considerations of Bosons at the real life Compton scale we go on to a description of Fermions, specifically the Dirac equation in terms of an underlying noncommutative geometry described by the Dirac $\gamma$ matrices and generalize this to branes in an underlying C-space (with Clifford Algebra).
physics.gen-ph
starting from considerations of bosons at the real life compton scale we go on to a description of fermions specifically the dirac equation in terms of an underlying noncommutative geometry described by the dirac gamma matrices and generalize this to branes in an underlying cspace with clifford algebra
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707.2462
Search for B Meson Decays to omega K*0
We report a search for the charmless vector-vector decay B0->omega K*0 with 520x10^6 BBbar pairs collected with the Belle detector at the KEKB e+e- collider. We measure the branching fraction in units of 10^-6: Br = 1.2 +0.9-0.8 +-0.2 (<2.7), where the first error is statistical, the second systematic, and the upper limit is at the 90% confidence level.
hep-ex
we report a search for the charmless vectorvector decay b0omega k0 with 520x106 bbbar pairs collected with the belle detector at the kekb ee collider we measure the branching fraction in units of 106 br 12 0908 02 27 where the first error is statistical the second systematic and the upper limit is at the 90 confidence level
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707.2463
Composite Messenger Baryon as a Cold Dark Matter
Among various supersymmetric (SUSY) models, gauge-mediated SUSY breaking models with an ultra-light gravitino of mass m_{3/2} \lesssim O(10) eV are very attractive, since they are completely free from notorious gravitino problems. A drawback of such a scenario is the absence of the supersymmetric cold dark matter. In this letter, we propose that a baryonic bound state of strongly interacting messenger particles, with a mass of O(100) TeV, can naturally be the cold dark matter. We also exemplify a model which realizes such a scenario.
hep-ph
among various supersymmetric susy models gaugemediated susy breaking models with an ultralight gravitino of mass m_32 lesssim o10 ev are very attractive since they are completely free from notorious gravitino problems a drawback of such a scenario is the absence of the supersymmetric cold dark matter in this letter we propose that a baryonic bound state of strongly interacting messenger particles with a mass of o100 tev can naturally be the cold dark matter we also exemplify a model which realizes such a scenario
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707.2464
Nanometer-Resolved Collective Micromeniscus Oscillations through Optical Diffraction
We study the dynamics of periodic arrays of micrometer-sized liquid-gas menisci formed at superhydrophobic surfaces immersed into water. By measuring the intensity of optical diffraction peaks in real time we are able to resolve nanometer scale oscillations of the menisci with sub-microsecond time resolution. Upon driving the system with an ultrasound field at variable frequency we observe a pronounced resonance at a few hundred kHz, depending on the exact geometry. Modeling the system using the unsteady Stokes equation, we find that this low resonance frequency is caused by a collective mode of the acoustically coupled oscillating menisci.
cond-mat.soft
we study the dynamics of periodic arrays of micrometersized liquidgas menisci formed at superhydrophobic surfaces immersed into water by measuring the intensity of optical diffraction peaks in real time we are able to resolve nanometer scale oscillations of the menisci with submicrosecond time resolution upon driving the system with an ultrasound field at variable frequency we observe a pronounced resonance at a few hundred khz depending on the exact geometry modeling the system using the unsteady stokes equation we find that this low resonance frequency is caused by a collective mode of the acoustically coupled oscillating menisci
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707.2465
The XMM-Newton view of IRAS 09104+4109: evidence for a changing-look Type 2 quasar?
We analyzed the spectroscopic data from the PN and the MOS cameras in the 0.4-10 keV band. We also used an archival BeppoSAX 1-50 keV observation of IRAS 09104+4109 to investigate possible variations of the quasar emission. The X-ray emission in the EPIC band is dominated by the intra-cluster medium thermal emission. We found that the quasar contributes ~35% of the total flux in the 2-10 keV band. Both a transmission- (through a Compton-thin absorber with a Compton optical depth of \tau_C~0.3, i.e. Nh~5 x 10^{23} cm^-2) and a reflection-dominated (\tau_C>1) model provide an excellent fit to the quasar continuum emission. However, the value measured for the EW of Fe Kalpha emission line is only marginally consistent with the presence of a Compton-thick absorber in a reflection-dominated scenario, which had been suggested by a previous, marginal (i.e. 2.5\sigma) detection with the hard X-ray (15-50 keV), non-imaging BeppoSAX/PDS instrument. Moreover, the value of luminosity in the 2-10 keV band measured by the transmission-dominated model is fully consistent with that expected on the basis of the bolometric luminosity of IRAS 09104+4109. From the analysis of the XMM-Newton data we therefore suggest the possibility that the absorber along the line of sight to the nucleus of IRAS 09104+4109 is Compton-thin. Alternatively, the absorber column density could have changed from Compton-thick to -thin in the five years elapsed between the observations. If this is the case, then IRAS 09104+4109 is the first 'changing-look' quasar ever detected.
astro-ph
we analyzed the spectroscopic data from the pn and the mos cameras in the 0410 kev band we also used an archival bepposax 150 kev observation of iras 091044109 to investigate possible variations of the quasar emission the xray emission in the epic band is dominated by the intracluster medium thermal emission we found that the quasar contributes 35 of the total flux in the 210 kev band both a transmission through a comptonthin absorber with a compton optical depth of tau_c03 ie nh5 x 1023 cm2 and a reflectiondominated tau_c1 model provide an excellent fit to the quasar continuum emission however the value measured for the ew of fe kalpha emission line is only marginally consistent with the presence of a comptonthick absorber in a reflectiondominated scenario which had been suggested by a previous marginal ie 25sigma detection with the hard xray 1550 kev nonimaging bepposaxpds instrument moreover the value of luminosity in the 210 kev band measured by the transmissiondominated model is fully consistent with that expected on the basis of the bolometric luminosity of iras 091044109 from the analysis of the xmmnewton data we therefore suggest the possibility that the absorber along the line of sight to the nucleus of iras 091044109 is comptonthin alternatively the absorber column density could have changed from comptonthick to thin in the five years elapsed between the observations if this is the case then iras 091044109 is the first changinglook quasar ever detected
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707.2466
Initiation of granular surface flows in a narrow channel
We experimentally investigate how a long granular pile confined in a narrow channel destabilizes when it is inclined above the angle of repose. A uniform flow then develops, which is localized at the free surface. It first accelerates before reaching a steady uniform regime. During this process, an apparent erosion is observed and the thickness of the flowing layer increases. We precisely study the evolution of the vertical velocity profile in this transient regime. The measurements are compared with the prediction of a visco-plastic model [P. Jop, Y. Forterre and O. Pouliquen, Nature 441, 727 (2006)]
cond-mat.soft
we experimentally investigate how a long granular pile confined in a narrow channel destabilizes when it is inclined above the angle of repose a uniform flow then develops which is localized at the free surface it first accelerates before reaching a steady uniform regime during this process an apparent erosion is observed and the thickness of the flowing layer increases we precisely study the evolution of the vertical velocity profile in this transient regime the measurements are compared with the prediction of a viscoplastic model p jop y forterre and o pouliquen nature 441 727 2006
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707.2467
Cyclic coverings of the $p$-adic projective line by Mumford curves
Exact bounds for the positions of the branch points for cyclic coverings of the $p$-adic projective line by Mumford curves are calculated in two ways. Firstly, by using Fumiharu Kato's *-trees, and secondly by giving explicit matrix representations of the Schottky groups corresponding to the Mumford curves above the projective line through combinatorial group theory.
math.AG
exact bounds for the positions of the branch points for cyclic coverings of the padic projective line by mumford curves are calculated in two ways firstly by using fumiharu katos trees and secondly by giving explicit matrix representations of the schottky groups corresponding to the mumford curves above the projective line through combinatorial group theory
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707.2468
Radial Dependence of Extinction in Parent Galaxies of Supernovae
The problem of extinction is the most important issue to be dealt with in the process of obtaining true absolute magnitudes of core-collapse supernovae (SNe). The plane-parallel model which gives absorption dependent on galaxy inclination, widely used in the past, was shown not to describe extinction adequately. We try to apply an alternative model which introduces radial ependence of extinction. A certain trend of dimmer SNe with decreasing radius from the center of a galaxy was found, for a chosen sample of stripped-envelope SNe.
astro-ph
the problem of extinction is the most important issue to be dealt with in the process of obtaining true absolute magnitudes of corecollapse supernovae sne the planeparallel model which gives absorption dependent on galaxy inclination widely used in the past was shown not to describe extinction adequately we try to apply an alternative model which introduces radial ependence of extinction a certain trend of dimmer sne with decreasing radius from the center of a galaxy was found for a chosen sample of strippedenvelope sne
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707.2469
Pseudospectral versus finite-differences schemes in the numerical integration of stochastic models of surface growth
We present a comparison between finite differences schemes and a pseudospectral method applied to the numerical integration of stochastic partial differential equations that model surface growth. We have studied, in 1+1 dimensions, the Kardar, Parisi and Zhang model (KPZ) and the Lai, Das Sarma and Villain model (LDV). The pseudospectral method appears to be the most stable for a given time step for both models. This means that the time up to which we can follow the temporal evolution of a given system is larger for the pseudospectral method. Moreover, for the KPZ model, a pseudospectral scheme gives results closer to the predictions of the continuum model than those obtained through finite difference methods. On the other hand, some numerical instabilities appearing with finite difference methods for the LDV model are absent when a pseudospectral integration is performed. These numerical instabilities give rise to an approximate multiscaling observed in the numerical simulations. With the pseudospectral approach no multiscaling is seen in agreement with the continuum model.
cond-mat.stat-mech
we present a comparison between finite differences schemes and a pseudospectral method applied to the numerical integration of stochastic partial differential equations that model surface growth we have studied in 11 dimensions the kardar parisi and zhang model kpz and the lai das sarma and villain model ldv the pseudospectral method appears to be the most stable for a given time step for both models this means that the time up to which we can follow the temporal evolution of a given system is larger for the pseudospectral method moreover for the kpz model a pseudospectral scheme gives results closer to the predictions of the continuum model than those obtained through finite difference methods on the other hand some numerical instabilities appearing with finite difference methods for the ldv model are absent when a pseudospectral integration is performed these numerical instabilities give rise to an approximate multiscaling observed in the numerical simulations with the pseudospectral approach no multiscaling is seen in agreement with the continuum model
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707.247
Environmental Effects of Dark Matter Haloes: The Clustering-Substructure relation of Group-size Haloes
We estimate the two-point correlation function of dark matter haloes, with masses >10^{13} h^{-1} Mo, that have or not significant substructure. The haloes are identified with a friends of friends algorithm in a large LCDM simulation at two redshift snapshots (z=0 and 1), while halo substructure is determined using an observationally driven method. We find in both epochs a clear and significant signal by which haloes with substructure are more clustered than those with no-substructure. This is true for all the considered halo mass ranges, although for the highest halo masses the signal is noisy and present only out to ~20 h^{-1} Mpc. There is also a smooth increase of the halo correlation length with increasing amplitude of the halo substructure. We also find that substructured haloes are typically located in high-density large-scale environments, while the opposite is true for non-substructured haloes. If the haloes found in high-density regions have a relatively earlier formation time, as suggested by recent works, then they do indeed have more time to cluster than haloes, of a similar mass, which form later in the low-density regions. In such a case one would have naively expected that the former (earlier formed) haloes would typically be dynamically more relaxed than the latter (later formed). However, the higher merging and interaction rate,expected in high-density regions, could disrupt their relatively relaxed dynamical state and thus be the cause for the higher fraction of haloes with substructure found in such regions.
astro-ph
we estimate the twopoint correlation function of dark matter haloes with masses 1013 h1 mo that have or not significant substructure the haloes are identified with a friends of friends algorithm in a large lcdm simulation at two redshift snapshots z0 and 1 while halo substructure is determined using an observationally driven method we find in both epochs a clear and significant signal by which haloes with substructure are more clustered than those with nosubstructure this is true for all the considered halo mass ranges although for the highest halo masses the signal is noisy and present only out to 20 h1 mpc there is also a smooth increase of the halo correlation length with increasing amplitude of the halo substructure we also find that substructured haloes are typically located in highdensity largescale environments while the opposite is true for nonsubstructured haloes if the haloes found in highdensity regions have a relatively earlier formation time as suggested by recent works then they do indeed have more time to cluster than haloes of a similar mass which form later in the lowdensity regions in such a case one would have naively expected that the former earlier formed haloes would typically be dynamically more relaxed than the latter later formed however the higher merging and interaction rateexpected in highdensity regions could disrupt their relatively relaxed dynamical state and thus be the cause for the higher fraction of haloes with substructure found in such regions
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707.2471
On the number of independent adiabatic invariants for gyrating particles
It is pointed out that the three established adiabatic invariants are separating invariants in the sense of Liouville. It is widely claimed that no more than three adiabatic invariants can exist for the motion of a point charge. However, additional independent (not separating) adiabatic invariants do exist. For a force free motion, the components of angular momentum provide two additional constants of motion. This result can be generalized to the Hamilton Jacobi equation. The number of independent constants of motion is reduced if there is a global symmetry. For a gyrating particle, neglecting a gyro helix type of invariant, four 'useful' invariants could exist. A radial drift invariant, corresponding to the average of the radial coordinate of the particle, is a constant of motion for a confined gyrating particle. For the special case of a screw pinch where each gyro center moves on a magnetic flux surface without mirror trapping, the radial drift invariant is the radial coordinate of the gyro center. For a screw pinch, the set of constants of motion consising of the energy, parallel velocity and radial drift invariant is convenient to model the equilibrium. Local Maxwellian distribution functions expressed in this set of invariants are demonstrated to provide MHD-type of equilibria, for which it is straightforward to model the radial profiles of the particle and field components.
physics.plasm-ph
it is pointed out that the three established adiabatic invariants are separating invariants in the sense of liouville it is widely claimed that no more than three adiabatic invariants can exist for the motion of a point charge however additional independent not separating adiabatic invariants do exist for a force free motion the components of angular momentum provide two additional constants of motion this result can be generalized to the hamilton jacobi equation the number of independent constants of motion is reduced if there is a global symmetry for a gyrating particle neglecting a gyro helix type of invariant four useful invariants could exist a radial drift invariant corresponding to the average of the radial coordinate of the particle is a constant of motion for a confined gyrating particle for the special case of a screw pinch where each gyro center moves on a magnetic flux surface without mirror trapping the radial drift invariant is the radial coordinate of the gyro center for a screw pinch the set of constants of motion consising of the energy parallel velocity and radial drift invariant is convenient to model the equilibrium local maxwellian distribution functions expressed in this set of invariants are demonstrated to provide mhdtype of equilibria for which it is straightforward to model the radial profiles of the particle and field components
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707.2472
Applications of the q-Fourier Analysis to the Symmetric Moment Problem
Sufficient condition for the symmetric moment problem to be determinate is given using standards methods of $q$-Fourier analysis. This condition it cannot be a particular case of Carleman's criterion.
math.CA
sufficient condition for the symmetric moment problem to be determinate is given using standards methods of qfourier analysis this condition it cannot be a particular case of carlemans criterion
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707.2473
Coulomb analogy for nonhermitian degeneracies near quantum phase transitions
Degeneracies near the real axis in a complex-extended parameter space of a hermitian Hamiltonian are studied. We present a method to measure distributions of such degeneracies on the Riemann sheet of a selected level and apply it in classification of quantum phase transitions. The degeneracies are shown to behave similarly as complex zeros of a partition function.
quant-ph math-ph math.MP nucl-th
degeneracies near the real axis in a complexextended parameter space of a hermitian hamiltonian are studied we present a method to measure distributions of such degeneracies on the riemann sheet of a selected level and apply it in classification of quantum phase transitions the degeneracies are shown to behave similarly as complex zeros of a partition function
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707.2474
Visualization, Exploration and Data Analysis of Complex Astrophysical Data
In this paper we show how advanced visualization tools can help the researcher in investigating and extracting information from data. The focus is on VisIVO, a novel open source graphics application, which blends high performance multidimensional visualization techniques and up-to-date technologies to cooperate with other applications and to access remote, distributed data archives. VisIVO supports the standards defined by the International Virtual Observatory Alliance in order to make it interoperable with VO data repositories. The paper describes the basic technical details and features of the software and it dedicates a large section to show how VisIVO can be used in several scientific cases.
astro-ph
in this paper we show how advanced visualization tools can help the researcher in investigating and extracting information from data the focus is on visivo a novel open source graphics application which blends high performance multidimensional visualization techniques and uptodate technologies to cooperate with other applications and to access remote distributed data archives visivo supports the standards defined by the international virtual observatory alliance in order to make it interoperable with vo data repositories the paper describes the basic technical details and features of the software and it dedicates a large section to show how visivo can be used in several scientific cases
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707.2475
Effect of General Relativity and rotation on the energy deposition rate for $\nu + \bar{\nu} \to e^+ + e^- $ inside a compact star
We have studied the $\nu + \bar{\nu} \to e^+ + e^- $ energy deposition rate in a rotating compact star. This reaction is important for the study of gamma ray bursts. The General Relativistic (GR) effects on the energy deposition rate have been incorporated. We find that the efficiency of the process is larger for a rotating star. The total energy deposition rate increases by more than an order of magnitude due to rotation. The dependence of this energy deposition rate on the deformation parameter of the star has also been discussed.
astro-ph hep-ph
we have studied the nu barnu to e e energy deposition rate in a rotating compact star this reaction is important for the study of gamma ray bursts the general relativistic gr effects on the energy deposition rate have been incorporated we find that the efficiency of the process is larger for a rotating star the total energy deposition rate increases by more than an order of magnitude due to rotation the dependence of this energy deposition rate on the deformation parameter of the star has also been discussed
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707.2476
Shock waves in tidally compressed stars by massive black holes
We interest in the case of a main-sequence star deeply penetrating within the tidal radius of a massive black hole. We focus on the compression phase leading to a so-called pancake configuration of the star at the instant of maximal compression. The aim is to study the tidal compression process paying particular attention to the development of shock waves;to deduce reliable estimates of the thermodynamical quantities involved in the pancake star; and to solve a controversy about whether or not thermonuclear reactions can be triggered in the core of a tidally compressed star. We have set up a one-dimensional hydrodynamical model well-adapted to the geometry of the problem. Based on the high-resolution shock-capturing Godunov-type approach, it allows to study the compression phase undergone by the star in the direction orthogonal to its orbital plane. We show the existence of two regimes depending on whether shock waves develop before or after the instant of maximal core compression. In both cases we confirm high compression and heating factors in the stellar core able to trigger a thermonuclear explosion. Moreover, we show that the shock waves carry outwards a brief but very high peak of temperature from the centre to the surface of the star. We tentatively conclude that the phenomenon could give rise to hard electromagnetic radiation, to be compared to some X-ray flares already observed in some galactic nuclei harbouring massive black holes. Finally, we estimate that the rate of pancake stars should be about $10^{-5}$ per galaxy per year. If generated in hard X- or $\gamma$-ray band, several events of this kind per year should be detectable within the full observable universe.
astro-ph
we interest in the case of a mainsequence star deeply penetrating within the tidal radius of a massive black hole we focus on the compression phase leading to a socalled pancake configuration of the star at the instant of maximal compression the aim is to study the tidal compression process paying particular attention to the development of shock wavesto deduce reliable estimates of the thermodynamical quantities involved in the pancake star and to solve a controversy about whether or not thermonuclear reactions can be triggered in the core of a tidally compressed star we have set up a onedimensional hydrodynamical model welladapted to the geometry of the problem based on the highresolution shockcapturing godunovtype approach it allows to study the compression phase undergone by the star in the direction orthogonal to its orbital plane we show the existence of two regimes depending on whether shock waves develop before or after the instant of maximal core compression in both cases we confirm high compression and heating factors in the stellar core able to trigger a thermonuclear explosion moreover we show that the shock waves carry outwards a brief but very high peak of temperature from the centre to the surface of the star we tentatively conclude that the phenomenon could give rise to hard electromagnetic radiation to be compared to some xray flares already observed in some galactic nuclei harbouring massive black holes finally we estimate that the rate of pancake stars should be about 105 per galaxy per year if generated in hard x or gammaray band several events of this kind per year should be detectable within the full observable universe
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707.2477
$L^p$-Spectral theory of locally symmetric spaces with $Q$-rank one
We study the $L^p$-spectrum of the Laplace-Beltrami operator on certain complete locally symmetric spaces $M=\Gamma\backslash X$ with finite volume and arithmetic fundamental group $\Gamma$ whose universal covering $X$ is a symmetric space of non-compact type. We also show, how the obtained results for locally symmetric spaces can be generalized to manifolds with cusps of rank one.
math.SP math.DG
we study the lpspectrum of the laplacebeltrami operator on certain complete locally symmetric spaces mgammabackslash x with finite volume and arithmetic fundamental group gamma whose universal covering x is a symmetric space of noncompact type we also show how the obtained results for locally symmetric spaces can be generalized to manifolds with cusps of rank one
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707.2478
Zeeman ratchets: pure spin current generation in mesoscopic conductors with non-uniform magnetic fields
We consider the possibility to employ a quantum wire realized in a two-dimensional electron gas (2DEG) as a spin ratchet. We show that a net spin current without accompanying net charge transport can be induced in the nonlinear regime by an unbiased external driving via an ac voltage applied between the contacts at the ends of the quantum wire. To achieve this we make use of the coupling of the electron spin to inhomogenous magnetic fields created by ferromagnetic stripes patterned on the semiconductor heterostructure that harbours the 2DEG. Using recursive Green function techniques we numerically study two different setups, consisting of one and two ferromagnetic stripes, respectively.
cond-mat.mes-hall
we consider the possibility to employ a quantum wire realized in a twodimensional electron gas 2deg as a spin ratchet we show that a net spin current without accompanying net charge transport can be induced in the nonlinear regime by an unbiased external driving via an ac voltage applied between the contacts at the ends of the quantum wire to achieve this we make use of the coupling of the electron spin to inhomogenous magnetic fields created by ferromagnetic stripes patterned on the semiconductor heterostructure that harbours the 2deg using recursive green function techniques we numerically study two different setups consisting of one and two ferromagnetic stripes respectively
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707.2479
Detecting synchronization clusters in multivariate time series via coarse-graining of Markov chains
Synchronization cluster analysis is an approach to the detection of underlying structures in data sets of multivariate time series, starting from a matrix R of bivariate synchronization indices. A previous method utilized the eigenvectors of R for cluster identification, analogous to several recent attempts at group identification using eigenvectors of the correlation matrix. All of these approaches assumed a one-to-one correspondence of dominant eigenvectors and clusters, which has however been shown to be wrong in important cases. We clarify the usefulness of eigenvalue decomposition for synchronization cluster analysis by translating the problem into the language of stochastic processes, and derive an enhanced clustering method harnessing recent insights from the coarse-graining of finite-state Markov processes. We illustrate the operation of our method using a simulated system of coupled Lorenz oscillators, and we demonstrate its superior performance over the previous approach. Finally we investigate the question of robustness of the algorithm against small sample size, which is important with regard to field applications.
physics.data-an
synchronization cluster analysis is an approach to the detection of underlying structures in data sets of multivariate time series starting from a matrix r of bivariate synchronization indices a previous method utilized the eigenvectors of r for cluster identification analogous to several recent attempts at group identification using eigenvectors of the correlation matrix all of these approaches assumed a onetoone correspondence of dominant eigenvectors and clusters which has however been shown to be wrong in important cases we clarify the usefulness of eigenvalue decomposition for synchronization cluster analysis by translating the problem into the language of stochastic processes and derive an enhanced clustering method harnessing recent insights from the coarsegraining of finitestate markov processes we illustrate the operation of our method using a simulated system of coupled lorenz oscillators and we demonstrate its superior performance over the previous approach finally we investigate the question of robustness of the algorithm against small sample size which is important with regard to field applications
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707.248
Renormalization of Lorentz violating theories
We classify the unitary, renormalizable, Lorentz violating quantum field theories of interacting scalars and fermions, obtained improving the behavior of Feynman diagrams by means of higher space derivatives. Higher time derivatives are not generated by renormalization. Renormalizability is ensured by a "weighted power counting" criterion. The theories contain a dimensionful parameter, yet a set of models are classically invariant under a weighted scale transformation, which is anomalous at the quantum level. Formulas for the weighted trace anomaly are derived. The renormalization-group properties are studied.
hep-th
we classify the unitary renormalizable lorentz violating quantum field theories of interacting scalars and fermions obtained improving the behavior of feynman diagrams by means of higher space derivatives higher time derivatives are not generated by renormalization renormalizability is ensured by a weighted power counting criterion the theories contain a dimensionful parameter yet a set of models are classically invariant under a weighted scale transformation which is anomalous at the quantum level formulas for the weighted trace anomaly are derived the renormalizationgroup properties are studied
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707.2481
The (3+2) Neutrino Mass Spectrum and Double Chooz
The implications of extra sterile neutrinos for the Double Chooz experiment is expounded. The so-called ``3+2'' mass spectrum with 2 sterile neutrinos mixed with the active ones, is still allowed by the global neutrino data including MiniBooNE. We probe its impact on the resultant reactor antineutrino signal at the near and far detector of the Double Chooz experiment. The oscillations driven by the additional mass squared difference due to the sterile states bring an energy independent constant suppression at both the near and far detectors. We study to what extent the measurement of $\theta_{13}$ would get affected due to the presence of sterile mixing. We also give the projected sensitivity that Double Chooz will have to constrain the extra mixing angles associated with the sterile states.
hep-ph astro-ph hep-ex
the implications of extra sterile neutrinos for the double chooz experiment is expounded the socalled 32 mass spectrum with 2 sterile neutrinos mixed with the active ones is still allowed by the global neutrino data including miniboone we probe its impact on the resultant reactor antineutrino signal at the near and far detector of the double chooz experiment the oscillations driven by the additional mass squared difference due to the sterile states bring an energy independent constant suppression at both the near and far detectors we study to what extent the measurement of theta_13 would get affected due to the presence of sterile mixing we also give the projected sensitivity that double chooz will have to constrain the extra mixing angles associated with the sterile states
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707.2482
Multiple-Description Lattice Vector Quantization
In this thesis, we construct and analyze multiple-description codes based on lattice vector quantization.
cs.IT math.IT
in this thesis we construct and analyze multipledescription codes based on lattice vector quantization
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707.2483
Lyman-alpha radiative transfer during the Epoch of Reionization: contribution to 21-cm signal fluctuations
During the epoch of reionization, Ly-alpha photons emitted by the first stars can couple the neutral hydrogen spin temperature to the kinetic gas temperature, providing the opportunity to observe the gas in emission or absorption in the 21-cm line. Given the bright foregrounds, it is of prime importance to determine precisely the fluctuations signature of the signal, to be able to extract it by its correlation power. LICORICE is a Monte-Carlo radiative transfer code, coupled to the dynamics via an adaptative Tree-SPH code. We present here the Ly-alpha part of the implementation, and validate it through three classical tests. Contrary to previous works, we do not assume that P_alpha, the number of scatterings of Ly-alpha photons per atom per second, is proportional to the Ly-alpha background flux, but take into account the scatterings in the Ly-alpha line wings. The latter have the effect to steepen the radial profile of P_alpha around each source, and re-inforce the contrast of the fluctuations. In the particular geometry of cosmic filaments of baryonic matter, Ly-alpha photons are scattered out of the filament, and the large scale structure of P_alpha is significantly anisotropic. This could have strong implications for the possible detection of the 21-cm signal.
astro-ph
during the epoch of reionization lyalpha photons emitted by the first stars can couple the neutral hydrogen spin temperature to the kinetic gas temperature providing the opportunity to observe the gas in emission or absorption in the 21cm line given the bright foregrounds it is of prime importance to determine precisely the fluctuations signature of the signal to be able to extract it by its correlation power licorice is a montecarlo radiative transfer code coupled to the dynamics via an adaptative treesph code we present here the lyalpha part of the implementation and validate it through three classical tests contrary to previous works we do not assume that p_alpha the number of scatterings of lyalpha photons per atom per second is proportional to the lyalpha background flux but take into account the scatterings in the lyalpha line wings the latter have the effect to steepen the radial profile of p_alpha around each source and reinforce the contrast of the fluctuations in the particular geometry of cosmic filaments of baryonic matter lyalpha photons are scattered out of the filament and the large scale structure of p_alpha is significantly anisotropic this could have strong implications for the possible detection of the 21cm signal
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707.2484
Quantum vortex tunneling in $YBa_2Cu_3O_{7-\delta}$ thin films
Cuprate films offer a unique opportunity to observe vortex tunneling effects, due to their unusually low superfluid density and short coherence length. Here, we measure the magnetoresistance (\textit{MR}) due to vortex motion of a long meander line of a superconducting film made of underdoped $YBa_2Cu_3O_{7-\delta}$. At low temperatures (\textit{T}), the \textit{MR} shows a significant deviation from Arrhenius activation. The data is consistent with two dimensional Variable Range Hopping (VRH) of single vortices, i.e. $MR\propto exp[-(T_0/T)^{1/3}]$. The VRH temperature scale $T_0$ depends on the vortex tunneling rates between pinning sites. We discuss its magnitude with respect to estimated parameters of the meander thin film.
cond-mat.supr-con cond-mat.str-el
cuprate films offer a unique opportunity to observe vortex tunneling effects due to their unusually low superfluid density and short coherence length here we measure the magnetoresistance textitmr due to vortex motion of a long meander line of a superconducting film made of underdoped yba_2cu_3o_7delta at low temperatures textitt the textitmr shows a significant deviation from arrhenius activation the data is consistent with two dimensional variable range hopping vrh of single vortices ie mrpropto expt_0t13 the vrh temperature scale t_0 depends on the vortex tunneling rates between pinning sites we discuss its magnitude with respect to estimated parameters of the meander thin film
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707.2485
Spectral analysis of boundary layers in Rayleigh-Benard convection
A combined experimental and numerical study of the boundary layer in a 4:1 aspect-ratio Rayleigh-B\'{e}nard cell over a four-decade range of Rayleigh numbers has been undertaken aimed at gaining a better insight into the character of the boundary layers. The experiments involved the simultaneous Laser Doppler Anemometry (LDA) measurements of fluid velocity at two locations, i.e. in the boundary layer and far away from it in the bulk, for Rayleigh numbers varying between $1.6 \times 10^7$ and $2.4 \times 10^9$. In parallel, direct numerical simulations (DNS) have been performed for the same configuration for Rayleigh numbers between $7.0 \times 10^4$ and $7.7 \times 10^7$. The temperature and velocity probability density functions and the power spectra of the horizontal velocity fluctuations measured in the boundary layer and in the bulk flow are found to be practically identical. Except for the smallest Rayleigh numbers, the spectra in the boundary layer and in the bulk central region are continuous and have a wide range of active scales. This indicates that both the bulk and the boundary layers are turbulent in the $\textrm{Ra}$ number range considered. However, molecular effects can still be observed and the boundary layer does not behave like a classical shear-driven turbulent boundary layer.
physics.flu-dyn
a combined experimental and numerical study of the boundary layer in a 41 aspectratio rayleighbenard cell over a fourdecade range of rayleigh numbers has been undertaken aimed at gaining a better insight into the character of the boundary layers the experiments involved the simultaneous laser doppler anemometry lda measurements of fluid velocity at two locations ie in the boundary layer and far away from it in the bulk for rayleigh numbers varying between 16 times 107 and 24 times 109 in parallel direct numerical simulations dns have been performed for the same configuration for rayleigh numbers between 70 times 104 and 77 times 107 the temperature and velocity probability density functions and the power spectra of the horizontal velocity fluctuations measured in the boundary layer and in the bulk flow are found to be practically identical except for the smallest rayleigh numbers the spectra in the boundary layer and in the bulk central region are continuous and have a wide range of active scales this indicates that both the bulk and the boundary layers are turbulent in the textrmra number range considered however molecular effects can still be observed and the boundary layer does not behave like a classical sheardriven turbulent boundary layer
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707.2486
Transverse Target-Spin Asymmetry of Exclusive $\rho^0$ Meson Production on Proton at HERMES
Preliminary measurements are reported on the azimuthal single-spin asymmetry of exclusive rho0 mesons for a transversely polarized hydrogen target at HERMES using the 27.6 GeV HERA positron beam. Within the generalized parton distribution (GPD) formalism, this asymmetry is sensitive to the total angular momentum of quarks and gluons in the nucleon. Since the GPD formalism is only valid for mesons produced by longitudinal photons, the transverse target-spin asymmetry of longitudinal rho0 mesons is extracted assuming s-channel helicity conservation and compared to theoretical calculations.
hep-ex
preliminary measurements are reported on the azimuthal singlespin asymmetry of exclusive rho0 mesons for a transversely polarized hydrogen target at hermes using the 276 gev hera positron beam within the generalized parton distribution gpd formalism this asymmetry is sensitive to the total angular momentum of quarks and gluons in the nucleon since the gpd formalism is only valid for mesons produced by longitudinal photons the transverse targetspin asymmetry of longitudinal rho0 mesons is extracted assuming schannel helicity conservation and compared to theoretical calculations
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707.2487
Gate-induced insulating state in bilayer graphene devices
The potential of graphene-based materials consisting of one or a few layers of graphite for integrated electronics originates from the large room-temperature carrier mobility in these systems (approx. 10,000 cm2/Vs). However, the realization of electronic devices such as field-effect transistors will require controlling and even switching off the electrical conductivity by means of gate electrodes, which is made difficult by the absence of a bandgap in the intrinsic material. Here, we demonstrate the controlled induction of an insulating state - with large suppression of the conductivity - in bilayer graphene, by using a double-gate device configuration that allows an electric field to be applied perpendicular to the plane. The dependence of the resistance on temperature and electric field, and the absence of any effect in a single-layer device, strongly suggest that the gate-induced insulating state originates from the recently predicted opening of a bandgap between valence and conduction bands.
cond-mat.mes-hall cond-mat.mtrl-sci
the potential of graphenebased materials consisting of one or a few layers of graphite for integrated electronics originates from the large roomtemperature carrier mobility in these systems approx 10000 cm2vs however the realization of electronic devices such as fieldeffect transistors will require controlling and even switching off the electrical conductivity by means of gate electrodes which is made difficult by the absence of a bandgap in the intrinsic material here we demonstrate the controlled induction of an insulating state with large suppression of the conductivity in bilayer graphene by using a doublegate device configuration that allows an electric field to be applied perpendicular to the plane the dependence of the resistance on temperature and electric field and the absence of any effect in a singlelayer device strongly suggest that the gateinduced insulating state originates from the recently predicted opening of a bandgap between valence and conduction bands
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707.2488
Primitive contractions of Calabi-Yau threefolds II
We construct 16 new examples of Calabi--Yau threefolds with Picard group of rank 1. Each of these examples is obtained by smoothing the image of a primitive contraction with exceptional divisor being a del Pezzo surface of degree 6, 7 or $\mathbb{P}^1\times \mathbb{P}^1$.
math.AG
we construct 16 new examples of calabiyau threefolds with picard group of rank 1 each of these examples is obtained by smoothing the image of a primitive contraction with exceptional divisor being a del pezzo surface of degree 6 7 or mathbbp1times mathbbp1
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707.2489
A Little About Folklore
Comment on paper by P.W. Anderson is presented. This Anderson's work is shown to contain a number of inaccurate and ungrounded statements. We point out, in particular, that the total static dielectric function not only can be negative, but inevitably has a minus sign in many stable systems. We also demonstrate that in many metals, the effective electron-phonon interaction is stronger than the direct Coulomb repulsion, without taking into account the ladder-sum renormalization or pseudization of the Coulomb repulsion. Other issues touched in Anderson's paper are also discussed.
cond-mat.supr-con
comment on paper by pw anderson is presented this andersons work is shown to contain a number of inaccurate and ungrounded statements we point out in particular that the total static dielectric function not only can be negative but inevitably has a minus sign in many stable systems we also demonstrate that in many metals the effective electronphonon interaction is stronger than the direct coulomb repulsion without taking into account the laddersum renormalization or pseudization of the coulomb repulsion other issues touched in andersons paper are also discussed
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707.249
Influence of a carbon over-coat on the X-ray reflectance of XEUS mirrors
We describe measurements of the X-ray reflectance in the range 2 to 10 keV of samples representative of coated silicon wafers that are proposed for the fabrication of the XEUS (X-ray Evolving Universe Spectrometer) mission. We compare the reflectance of silicon samples coated with bare Pt, with that for samples with an additional 10nm thick carbon over-coating. We demonstrate a significant improvement in reflectance in the energy range ~1 to 4 keV, and at a grazing incidence angle of 10 mrad (0.57 degrees). We consider the resulting effective area that could be attained with an optimized design of the XEUS telescope. Typically an improvement of 10 to 60 % in effective area, depending on photon energy, can be achieved using the carbon overcoat.
astro-ph
we describe measurements of the xray reflectance in the range 2 to 10 kev of samples representative of coated silicon wafers that are proposed for the fabrication of the xeus xray evolving universe spectrometer mission we compare the reflectance of silicon samples coated with bare pt with that for samples with an additional 10nm thick carbon overcoating we demonstrate a significant improvement in reflectance in the energy range 1 to 4 kev and at a grazing incidence angle of 10 mrad 057 degrees we consider the resulting effective area that could be attained with an optimized design of the xeus telescope typically an improvement of 10 to 60 in effective area depending on photon energy can be achieved using the carbon overcoat
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707.2491
Instability of bound states of a nonlinear Schr\"odinger equation with a Dirac potential
We study analytically and numerically the stability of the standing waves for a nonlinear Schr\"odinger equation with a point defect and a power type nonlinearity. A main difficulty is to compute the number of negative eigenvalues of the linearized operator around the standing waves, and it is overcome by a perturbation method and continuation arguments. Among others, in the case of a repulsive defect, we show that the standing wave solution is stable in $\hurad$ and unstable in $\hu$ under subcritical nonlinearity. Further we investigate the nature of instability: under critical or supercritical nonlinear interaction, we prove the instability by blowup in the repulsive case by showing a virial theorem and using a minimization method involving two constraints. In the subcritical radial case, unstable bound states cannot collapse, but rather narrow down until they reach the stable regime (a {\em finite-width instability}). In the non-radial repulsive case, all bound states are unstable, and the instability is manifested by a lateral drift away from the defect, sometimes in combination with a finite-width instability or a blowup instability.
nlin.PS nlin.SI
we study analytically and numerically the stability of the standing waves for a nonlinear schrodinger equation with a point defect and a power type nonlinearity a main difficulty is to compute the number of negative eigenvalues of the linearized operator around the standing waves and it is overcome by a perturbation method and continuation arguments among others in the case of a repulsive defect we show that the standing wave solution is stable in hurad and unstable in hu under subcritical nonlinearity further we investigate the nature of instability under critical or supercritical nonlinear interaction we prove the instability by blowup in the repulsive case by showing a virial theorem and using a minimization method involving two constraints in the subcritical radial case unstable bound states cannot collapse but rather narrow down until they reach the stable regime a em finitewidth instability in the nonradial repulsive case all bound states are unstable and the instability is manifested by a lateral drift away from the defect sometimes in combination with a finitewidth instability or a blowup instability
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707.2492
Structural transformations of double-walled carbon nanotube bundle under hydrostatic pressure
Three kinds of the response mechanisms to the external pressure have been found for double-walled carbon nanotube (DWNT) bundle, depending strongly on their average radius and symmetry. The small-diameter DWNT bundle undergoes a small discontinuous volume change, and then deform continuously. The intermediate-diameter DWNT bundle collapses completely after a structure phase transition (SPT). Significantly, two SPTs exist for the larger-diameter DWNT bundle if the outer tube has no $C_{6}$ or $C_{3}$ symmetry. It would be interesting to search for signatures of these different structural transformations by experimentally investigating mechanical, optical and thermal response functions of DWNT bundle.
cond-mat.mtrl-sci
three kinds of the response mechanisms to the external pressure have been found for doublewalled carbon nanotube dwnt bundle depending strongly on their average radius and symmetry the smalldiameter dwnt bundle undergoes a small discontinuous volume change and then deform continuously the intermediatediameter dwnt bundle collapses completely after a structure phase transition spt significantly two spts exist for the largerdiameter dwnt bundle if the outer tube has no c_6 or c_3 symmetry it would be interesting to search for signatures of these different structural transformations by experimentally investigating mechanical optical and thermal response functions of dwnt bundle
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707.2493
Inclusive semileptonic B decays and the determination of |V_ub|
We study the triple differential distribution of B-> Xu l nu, consistently including all perturbative and non-perturbative effects through O(alphas^2 beta_0) and O(1/mb^3). The Fermi motion is parameterized in terms of a single light-cone function for each structure function and for any value of q^2, accounting for all subleading effects. We discuss the problems and uncertainties related to the high-q^2 tail and to Weak Annihilation effects. We work in the kinetic scheme, a framework characterized by a Wilsonian treatment with a hard cutoff mu ~ 1GeV. Our method is illustrated with the extraction of |V_ub| from some of the latest experimental data, providing a detailed estimate of the theoretical uncertainty.
hep-ph
we study the triple differential distribution of b xu l nu consistently including all perturbative and nonperturbative effects through oalphas2 beta_0 and o1mb3 the fermi motion is parameterized in terms of a single lightcone function for each structure function and for any value of q2 accounting for all subleading effects we discuss the problems and uncertainties related to the highq2 tail and to weak annihilation effects we work in the kinetic scheme a framework characterized by a wilsonian treatment with a hard cutoff mu 1gev our method is illustrated with the extraction of v_ub from some of the latest experimental data providing a detailed estimate of the theoretical uncertainty
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707.2494
The Achromatic Interfero Coronagraph
We report on the Achromatic Interfero Coronagraph, a focal imaging device which aims at rejecting the energy contribution of a point-like source set on-axis, so as to make detectable its angularly-close environment (applicable to stellar environment: circumstellar matter, faint companions, planetary systems, but also conceivably to Active Galatic Nucleii and multiple asteroids). With AIC, starlight rejection is based on destructive interference, which allows exploration of the star's neighbouring at angular resolution better than the diffraction limit of the hosting telescope. Thanks to the focus crossing property of light, rejection is achromatic thus yielding a large spectral bandwidth of work. Descriptions and comments are given regarding the principle, the device itself, the constraints and limitations, and the theoretical performance. Results are presented which demonstrate the close-sensing capability and which show images of a companion obtained in laboratory and 'on the sky' as well. A short pictorial description of alternative AIC concepts, CIAXE and Open-Air CIAXE, currently under study, is given.
astro-ph
we report on the achromatic interfero coronagraph a focal imaging device which aims at rejecting the energy contribution of a pointlike source set onaxis so as to make detectable its angularlyclose environment applicable to stellar environment circumstellar matter faint companions planetary systems but also conceivably to active galatic nucleii and multiple asteroids with aic starlight rejection is based on destructive interference which allows exploration of the stars neighbouring at angular resolution better than the diffraction limit of the hosting telescope thanks to the focus crossing property of light rejection is achromatic thus yielding a large spectral bandwidth of work descriptions and comments are given regarding the principle the device itself the constraints and limitations and the theoretical performance results are presented which demonstrate the closesensing capability and which show images of a companion obtained in laboratory and on the sky as well a short pictorial description of alternative aic concepts ciaxe and openair ciaxe currently under study is given
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707.2495
Geometrical and electronic structures of the (5, 3) single-walled gold nanotube from first-principles calculations
The geometrical and electronic structures of the 4 {\AA} diameter perfect and deformed (5, 3) single-walled gold nanotube (SWGT) have been studied based upon the density-functional theory in the local-density approximation (LDA). The calculated relaxed geometries show clearly significant deviations from those of the ideally rolled triangular gold sheet. It is found that the different strains have different effects on the electronic structures and density of states of the SWGTs. And the small shear strain can reduce the binding energy per gold atom of the deformed SWGT, which is consistent with the experimentally observed result. Finally, we found the finite SWGT can show the metal-semiconductor transition.
cond-mat.mtrl-sci
the geometrical and electronic structures of the 4 aa diameter perfect and deformed 5 3 singlewalled gold nanotube swgt have been studied based upon the densityfunctional theory in the localdensity approximation lda the calculated relaxed geometries show clearly significant deviations from those of the ideally rolled triangular gold sheet it is found that the different strains have different effects on the electronic structures and density of states of the swgts and the small shear strain can reduce the binding energy per gold atom of the deformed swgt which is consistent with the experimentally observed result finally we found the finite swgt can show the metalsemiconductor transition
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707.2496
Tau anomalous magnetic moment form factor at Super B/Flavor factories
The proposed high-luminosity B/Flavor factories offer new opportunities for the improved determination of the fundamental physical parameters of standard heavy leptons. Compared to the electron or the muon case, the magnetic properties of the $\tau$ lepton are largely unexplored. We show that the electromagnetic properties of the $\tau$, and in particular its magnetic form factor, may be measured competitively in these facilities, using unpolarized or polarized electron beams. Various observables of the $\tau$'s produced on top of the $\Upsilon$ resonances, such as cross-section and normal polarization for unpolarized electrons or longitudinal and transverse asymmetries for polarized beams, can be combined in order to increase the sensitivity on the magnetic moment form factor. In the case of polarized electrons, we identify a special combination of transverse and longitudinal $\tau$ polarizations able to disentangle this anomalous magnetic form factor from both the charge form factor and the interference with the Z-mediating amplitude. For an integrated luminosity of $15 \times 10^{18} b^{-1}$ one could achieve a sensitivity of about $10^{-6}$, which is several orders of magnitude below any other existing high- or low-energy bound on the magnetic moment. Thus one may obtain a QED test of this fundamental quantity to a few % precision.
hep-ph
the proposed highluminosity bflavor factories offer new opportunities for the improved determination of the fundamental physical parameters of standard heavy leptons compared to the electron or the muon case the magnetic properties of the tau lepton are largely unexplored we show that the electromagnetic properties of the tau and in particular its magnetic form factor may be measured competitively in these facilities using unpolarized or polarized electron beams various observables of the taus produced on top of the upsilon resonances such as crosssection and normal polarization for unpolarized electrons or longitudinal and transverse asymmetries for polarized beams can be combined in order to increase the sensitivity on the magnetic moment form factor in the case of polarized electrons we identify a special combination of transverse and longitudinal tau polarizations able to disentangle this anomalous magnetic form factor from both the charge form factor and the interference with the zmediating amplitude for an integrated luminosity of 15 times 1018 b1 one could achieve a sensitivity of about 106 which is several orders of magnitude below any other existing high or lowenergy bound on the magnetic moment thus one may obtain a qed test of this fundamental quantity to a few precision
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707.2497
A study of the ferromagnetic transition of $SrRuO_3$ in nanometer thick bilayers with $YBa_2Cu_3O_y$, $La_{1.88}Sr_{0.12}CuO_{4-y}$, Au and Cr: Signature of injected carriers in the pseudogap regime
The hypothesis regarding the existence of uncorrelated pre-formed pairs in the pseudogap regime of superconducting $YBa_2Cu_3O_y$ is tested experimentally using bilayers of $YBa_2Cu_3O_y$ and the itinerant ferromagnet $SrRuO_3$. In our study, we monitor the influence of $YBa_2Cu_3O_y$ on $T_p$, the ferromagnetic ordering temperature of $SrRuO_3$. Here, $T_p$ is the temperature of maximum dM/dT or dR/dT where M and R are the magnetization and resistance of $SrRuO_3$, respectively. We compare the results with similar measurements carried out on bilayers of $La_{1.88}Sr_{0.12}CuO_{4-y}$, $Au$ and $Cr$ with $SrRuO_3$. We find that in bilayers made of underdoped 10 nm $YBa_2Cu_3O_y$/5 nm $SrRuO_3$, the $T_p$ values are shifted to lower temperatures by up to 6-8 K as compared to $T_p\approx 140$ K of the 5 nm thick reference $SrRuO_3$ film. In contrast, in the other type of bilayers, which are not in the pseudogap regime near $T_p$, only a smaller shift of up to $\pm$2 K is observed. These differences are discussed in terms of a proximity effect, where carriers from the $YBa_2Cu_3O_y$ layer are injected into the $SrRuO_3$ layer and vice versa. We suggest that correlated electrons in the pseudogap regime of $YBa_2Cu_3O_y$ are responsible for the observed large $T_p$ shifts.
cond-mat.supr-con cond-mat.str-el
the hypothesis regarding the existence of uncorrelated preformed pairs in the pseudogap regime of superconducting yba_2cu_3o_y is tested experimentally using bilayers of yba_2cu_3o_y and the itinerant ferromagnet srruo_3 in our study we monitor the influence of yba_2cu_3o_y on t_p the ferromagnetic ordering temperature of srruo_3 here t_p is the temperature of maximum dmdt or drdt where m and r are the magnetization and resistance of srruo_3 respectively we compare the results with similar measurements carried out on bilayers of la_188sr_012cuo_4y au and cr with srruo_3 we find that in bilayers made of underdoped 10 nm yba_2cu_3o_y5 nm srruo_3 the t_p values are shifted to lower temperatures by up to 68 k as compared to t_papprox 140 k of the 5 nm thick reference srruo_3 film in contrast in the other type of bilayers which are not in the pseudogap regime near t_p only a smaller shift of up to pm2 k is observed these differences are discussed in terms of a proximity effect where carriers from the yba_2cu_3o_y layer are injected into the srruo_3 layer and vice versa we suggest that correlated electrons in the pseudogap regime of yba_2cu_3o_y are responsible for the observed large t_p shifts
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707.2498
Subcritical dynamo bifurcation in the Taylor Green flow
We report direct numerical simulations of dynamo generation for flow generated using a Taylor-Green forcing. We find that the bifurcation is subcritical, and show its bifurcation diagram. We connect the associated hysteretic behavior with hydrodynamics changes induced by the action of the Lorentz force. We show the geometry of the dynamo magnetic field and discuss how the dynamo transition can be induced when an external field is applied to the flow.
physics.flu-dyn astro-ph
we report direct numerical simulations of dynamo generation for flow generated using a taylorgreen forcing we find that the bifurcation is subcritical and show its bifurcation diagram we connect the associated hysteretic behavior with hydrodynamics changes induced by the action of the lorentz force we show the geometry of the dynamo magnetic field and discuss how the dynamo transition can be induced when an external field is applied to the flow
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707.2499
Invariance of the relativistic one-particle distribution function
The one-particle distribution function is of importance both in non-relativistic and relativistic statistical physics. In the relativistic framework, Lorentz invariance is possibly its most fundamental property. The present article on the subject is a contrastive one: we review, discuss critically, and, when necessary, complete, the treatments found in the standard literature.
astro-ph
the oneparticle distribution function is of importance both in nonrelativistic and relativistic statistical physics in the relativistic framework lorentz invariance is possibly its most fundamental property the present article on the subject is a contrastive one we review discuss critically and when necessary complete the treatments found in the standard literature
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707.25
Landen survey
Landen transformations are maps on the coefficients of an integral that preserve its value. We present a brief survey of their appearnce in the literature.
math.CA
landen transformations are maps on the coefficients of an integral that preserve its value we present a brief survey of their appearnce in the literature
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707.2501
Single-walled carbon nanotube bundle under hydrostatic pressure studied by the first-principles calculations
The structural, electronic, optical and vibrational properties of the collapsed (10,10) single-walled carbon nanotube bundle under hydrostatic pressure have been studied by the first-principles calculations. Some features are observed in the present study: First, a collapsed structure is found, which is distinct from both of the herringbone and parallel structures obtained previously. Secondly, a pseudo-gap induced by the collapse appears along the symmetry axis \textit{$\Gamma $X}. Thirdly, the relative orientation between the collapsed tubes has an important effect on their electronic, optical and vibrational properties, which provides an efficient experimental method to distinguish unambiguously three different collapsed structures.
cond-mat.mtrl-sci
the structural electronic optical and vibrational properties of the collapsed 1010 singlewalled carbon nanotube bundle under hydrostatic pressure have been studied by the firstprinciples calculations some features are observed in the present study first a collapsed structure is found which is distinct from both of the herringbone and parallel structures obtained previously secondly a pseudogap induced by the collapse appears along the symmetry axis textitgamma x thirdly the relative orientation between the collapsed tubes has an important effect on their electronic optical and vibrational properties which provides an efficient experimental method to distinguish unambiguously three different collapsed structures
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707.2502
Electronic and Transport Properties of Radially Deformed Double-walled Carbon Nanotube Intramolecular Junction
The electronic and transport property of a radially deformed double-walled carbon nanotube (DWNT) intramolecular junction (IMJ) has been studied by the tight-binding (TB) model combined with the first-principle calculations. The geometrical structures of the DWNT IMJ have been first optimized in energy by the universal force field (UFF) method. It is found that when heavily squashed, the DWNT will become an insulator-coated metallic wire, and the conductance near the Fermi level has been significantly changed by the radial squash. Specially, several resonance conductance peaks appear at some energies in the conduction band of the squashed DWNT IMJ. Finally, we have also investigated the conductance variation due to change of the length of the central semiconductor in the squashed DWNT IMJ. Furthermore, a promising pure carbon nanoscale electronic device is proposed based on the DWNT IMJ.
cond-mat.mtrl-sci
the electronic and transport property of a radially deformed doublewalled carbon nanotube dwnt intramolecular junction imj has been studied by the tightbinding tb model combined with the firstprinciple calculations the geometrical structures of the dwnt imj have been first optimized in energy by the universal force field uff method it is found that when heavily squashed the dwnt will become an insulatorcoated metallic wire and the conductance near the fermi level has been significantly changed by the radial squash specially several resonance conductance peaks appear at some energies in the conduction band of the squashed dwnt imj finally we have also investigated the conductance variation due to change of the length of the central semiconductor in the squashed dwnt imj furthermore a promising pure carbon nanoscale electronic device is proposed based on the dwnt imj
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707.2503
Intergrowth and thermoelectric properties in the Bi-Ca-Co-O system
Single crystals of the Bi-Ca-Co-O system have been grown using the flux method with cooling from 900$\celsius$ and 950$\celsius$, respectively. The single crystals are characterized by transmission electron microscopy and X-ray diffraction. The misfit cobaltite [Ca$_2$Bi$_{1.4}$Co$_{0.6}$O$_4$]$^{RS}$[CoO$_2$]$_{1.69}$ single crystals with quadruple ($n$=4) rocksalt (RS) layer are achieved with cooling from 900$\celsius$. Such crystal exhibits room-temperature thermoelectric power (TEP) of 180$\mu$V/K, much larger than that in Sr-based misfit cobaltites with quadruple RS layer. However, intergrowth of single crystals of quadruple ($n$=4) and triple ($n$=3) RS-type layer-based misfit cobaltites is observed with cooling from 950$\celsius$. Both of TEP and resistivity were obviously enhanced by the intergrowth compared to [Ca$_2$Bi$_{1.4}$Co$_{0.6}$O$_4$]$^{RS}$[CoO$_2$]$_{1.69}$ single crystal, while the power factor at room temperature remains unchanged.
cond-mat.mtrl-sci cond-mat.str-el
single crystals of the bicacoo system have been grown using the flux method with cooling from 900celsius and 950celsius respectively the single crystals are characterized by transmission electron microscopy and xray diffraction the misfit cobaltite ca_2bi_14co_06o_4rscoo_2_169 single crystals with quadruple n4 rocksalt rs layer are achieved with cooling from 900celsius such crystal exhibits roomtemperature thermoelectric power tep of 180muvk much larger than that in srbased misfit cobaltites with quadruple rs layer however intergrowth of single crystals of quadruple n4 and triple n3 rstype layerbased misfit cobaltites is observed with cooling from 950celsius both of tep and resistivity were obviously enhanced by the intergrowth compared to ca_2bi_14co_06o_4rscoo_2_169 single crystal while the power factor at room temperature remains unchanged
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707.2504
$B\to K$ Transition Form Factor up to ${\cal O}(1/m^2_b)$ within the $k_T$ Factorization Approach
In the paper, we apply the $k_T$ factorization approach to deal with the $B\to K$ transition form factor $F^{B\to K}_{+,0}(q^2)$ in the large recoil regions. The B-meson wave functions $\Psi_B$ and $\bar\Psi_B$ that include the three-particle Fock states' contributions are adopted to give a consistent PQCD analysis of the form factor up to ${\cal O} (1/m^2_b)$. It has been found that both the wave functions $\Psi_B$ and $\bar\Psi_B$ can give sizable contributions to the form factor and should be kept for a better understanding of the $B$ meson decays. Then the contributions from different twist structures of the kaon wavefunction are discussed, including the $SU_f(3)$-breaking effects. A sizable contribution from the twist-3 wave function $\Psi_p$ is found, whose model dependence is discussed by taking two group of parameters that are determined by different distribution amplitude moments obtained in the literature. It is also shown that $F^{B\to K}_{+,0}(0)=0.30\pm0.04$ and $[F^{B\to K}_{+,0}(0)/F^{B\to \pi}_{+,0}(0)]=1.13\pm0.02$, which are more reasonable and consistent with the light-cone sum rule results in the large recoil regions.
hep-ph
in the paper we apply the k_t factorization approach to deal with the bto k transition form factor fbto k_0q2 in the large recoil regions the bmeson wave functions psi_b and barpsi_b that include the threeparticle fock states contributions are adopted to give a consistent pqcd analysis of the form factor up to cal o 1m2_b it has been found that both the wave functions psi_b and barpsi_b can give sizable contributions to the form factor and should be kept for a better understanding of the b meson decays then the contributions from different twist structures of the kaon wavefunction are discussed including the su_f3breaking effects a sizable contribution from the twist3 wave function psi_p is found whose model dependence is discussed by taking two group of parameters that are determined by different distribution amplitude moments obtained in the literature it is also shown that fbto k_00030pm004 and fbto k_00fbto pi_00113pm002 which are more reasonable and consistent with the lightcone sum rule results in the large recoil regions
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707.2505
Primitive Divisors in Arithmetic Dynamics
Let F(z) be a rational function in Q(z) of degree at least 2 with F(0) = 0 and such that F does not vanish to order d at 0. Let b be a rational number having infinite orbit under iteration of F, and write F^n(b) = A_n/B_n as a fraction in lowest terms. We prove that for all but finitely many n > 0, the numerator A_n has a primitive divisor, i.e., there is a prime p such that p divides A_n and p does not divide A_i for all i < n. More generally, we prove an analogous result when F is defined over a number field and 0 is a periodic point for F.
math.NT math.DS
let fz be a rational function in qz of degree at least 2 with f0 0 and such that f does not vanish to order d at 0 let b be a rational number having infinite orbit under iteration of f and write fnb a_nb_n as a fraction in lowest terms we prove that for all but finitely many n 0 the numerator a_n has a primitive divisor ie there is a prime p such that p divides a_n and p does not divide a_i for all i n more generally we prove an analogous result when f is defined over a number field and 0 is a periodic point for f
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707.2506
Mixed Integer Linear Programming For Exact Finite-Horizon Planning In Decentralized Pomdps
We consider the problem of finding an n-agent joint-policy for the optimal finite-horizon control of a decentralized Pomdp (Dec-Pomdp). This is a problem of very high complexity (NEXP-hard in n >= 2). In this paper, we propose a new mathematical programming approach for the problem. Our approach is based on two ideas: First, we represent each agent's policy in the sequence-form and not in the tree-form, thereby obtaining a very compact representation of the set of joint-policies. Second, using this compact representation, we solve this problem as an instance of combinatorial optimization for which we formulate a mixed integer linear program (MILP). The optimal solution of the MILP directly yields an optimal joint-policy for the Dec-Pomdp. Computational experience shows that formulating and solving the MILP requires significantly less time to solve benchmark Dec-Pomdp problems than existing algorithms. For example, the multi-agent tiger problem for horizon 4 is solved in 72 secs with the MILP whereas existing algorithms require several hours to solve it.
cs.AI
we consider the problem of finding an nagent jointpolicy for the optimal finitehorizon control of a decentralized pomdp decpomdp this is a problem of very high complexity nexphard in n 2 in this paper we propose a new mathematical programming approach for the problem our approach is based on two ideas first we represent each agents policy in the sequenceform and not in the treeform thereby obtaining a very compact representation of the set of jointpolicies second using this compact representation we solve this problem as an instance of combinatorial optimization for which we formulate a mixed integer linear program milp the optimal solution of the milp directly yields an optimal jointpolicy for the decpomdp computational experience shows that formulating and solving the milp requires significantly less time to solve benchmark decpomdp problems than existing algorithms for example the multiagent tiger problem for horizon 4 is solved in 72 secs with the milp whereas existing algorithms require several hours to solve it
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707.2507
Surface oscillations in channeled snow flows
An experimental device has been built to measure velocity profiles and friction laws in channeled snow flows. The measurements show that the velocity depends linearly on the vertical position in the flow and that the friction coefficient is a first-order polynomial in velocity (u) and thickness (h) of the flow. In all flows, oscillations on the surface of the flow were observed throughout the channel and measured at the location of the probes. The experimental results are confronted with a shallow water approach. Using a Saint-Venant modeling, we show that the flow is effectively uniform in the streamwise direction at the measurement location. We show that the surface oscillations produced by the Archimedes's screw at the top of the channel persist throughout the whole length of the channel and are the source of the measured oscillations. This last result provides good validation of the description of such channeled snow flows by a Saint-Venant modeling.
physics.class-ph
an experimental device has been built to measure velocity profiles and friction laws in channeled snow flows the measurements show that the velocity depends linearly on the vertical position in the flow and that the friction coefficient is a firstorder polynomial in velocity u and thickness h of the flow in all flows oscillations on the surface of the flow were observed throughout the channel and measured at the location of the probes the experimental results are confronted with a shallow water approach using a saintvenant modeling we show that the flow is effectively uniform in the streamwise direction at the measurement location we show that the surface oscillations produced by the archimedess screw at the top of the channel persist throughout the whole length of the channel and are the source of the measured oscillations this last result provides good validation of the description of such channeled snow flows by a saintvenant modeling
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707.2508
Analysis of the SN1987A two-stage explosion hypothesis with account for the MSW neutrino flavour conversion
Detection of 5 events by the Liquid Scintillation Detector (LSD) on February, 23, 1987 was interpreted in the literature as the detection of neutrinos from the first stage of the two-stage supernova collapse. We pose rigid constraints on the properties of the first stage of the collapse, taking into account neutrino flavour conversion due to the MSW-effect and general properties of supernova neutrino emission. The constraints depend on the unknown neutrino mass hierarchy and mixing angle \theta_{13}.
astro-ph
detection of 5 events by the liquid scintillation detector lsd on february 23 1987 was interpreted in the literature as the detection of neutrinos from the first stage of the twostage supernova collapse we pose rigid constraints on the properties of the first stage of the collapse taking into account neutrino flavour conversion due to the msweffect and general properties of supernova neutrino emission the constraints depend on the unknown neutrino mass hierarchy and mixing angle theta_13
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707.2509
Tomography for amplitudes of hard exclusive processes
We discuss which part of information about hadron structure encoded in the Generalized Parton Distributions (GPDs) [part of total GPD image] can be restored from the known amplitude of a hard exclusive process. The physics content of this partial image is analyzed. Among other things, we show that this partial image contains direct information about how the target hadron responses to the (string) quark-antiquark operator of {\it arbitrary} spin J. Explicit equations relating physics content of the partial image of GPDs directly to the data are derived. Also some new results concerning the dual parametrization of GPDs are presented.
hep-ph hep-ex nucl-ex
we discuss which part of information about hadron structure encoded in the generalized parton distributions gpds part of total gpd image can be restored from the known amplitude of a hard exclusive process the physics content of this partial image is analyzed among other things we show that this partial image contains direct information about how the target hadron responses to the string quarkantiquark operator of it arbitrary spin j explicit equations relating physics content of the partial image of gpds directly to the data are derived also some new results concerning the dual parametrization of gpds are presented
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707.251
Radiative gravitino decays from R-parity violation
We study radiative gravitino decay within the framework of R-violating supersymmetry. For trilinear R-violating couplings that involve the third generation of fermions, or for light gravitinos, we find that the radiative loop-decay $\tilde{G} \to \gamma \nu$ dominates over the tree-level ones for a wide set of parameters. We calculate the gravitino decay width and study its implications for cosmology and collider physics. Slow-decaying gravitinos are good dark matter candidates, for a range of parameters that would also predict observable R-violating signatures in colliders. In general the branching ratios are very dependent on the relative hierarchies of R-violating operators, and may provide relevant information on the flavour structure of the underlying fundamental theory.
hep-ph
we study radiative gravitino decay within the framework of rviolating supersymmetry for trilinear rviolating couplings that involve the third generation of fermions or for light gravitinos we find that the radiative loopdecay tildeg to gamma nu dominates over the treelevel ones for a wide set of parameters we calculate the gravitino decay width and study its implications for cosmology and collider physics slowdecaying gravitinos are good dark matter candidates for a range of parameters that would also predict observable rviolating signatures in colliders in general the branching ratios are very dependent on the relative hierarchies of rviolating operators and may provide relevant information on the flavour structure of the underlying fundamental theory
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707.2511
Symmetries of perturbed conformal field theories
The symmetries of perturbed conformal field theories are analysed. We explain which generators of the chiral algebras of a bulk theory survive a perturbation by an exactly marginal bulk field. We also study the behaviour of D-branes under current-current bulk deformations. We find that the branes always continue to preserve as much symmetry as they possibly can, i.e. as much as is preserved in the bulk. We illustrate these findings with several examples, including permutation branes in WZW models and B-type D-branes in Gepner models.
hep-th
the symmetries of perturbed conformal field theories are analysed we explain which generators of the chiral algebras of a bulk theory survive a perturbation by an exactly marginal bulk field we also study the behaviour of dbranes under currentcurrent bulk deformations we find that the branes always continue to preserve as much symmetry as they possibly can ie as much as is preserved in the bulk we illustrate these findings with several examples including permutation branes in wzw models and btype dbranes in gepner models
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707.2512
Generalized Neighbor-Interaction Models Induced by Nonlinear Lattices
It is shown that the tight-binding approximation of the nonlinear Schr\"odinger equation with a periodic linear potential and periodic in space nonlinearity coefficient gives rise to a number of nonlinear lattices with complex, both linear and nonlinear, neighbor interactions. The obtained lattices present non-standard possibilities, among which we mention a quasi-linear regime, where the pulse dynamics obeys essentially the linear Schr{\"o}dinger equation. We analyze the properties of such models both in connection with their modulational stability, as well as in regard to the existence and stability of their localized solitary wave solutions.
cond-mat.other nlin.PS
it is shown that the tightbinding approximation of the nonlinear schrodinger equation with a periodic linear potential and periodic in space nonlinearity coefficient gives rise to a number of nonlinear lattices with complex both linear and nonlinear neighbor interactions the obtained lattices present nonstandard possibilities among which we mention a quasilinear regime where the pulse dynamics obeys essentially the linear schrodinger equation we analyze the properties of such models both in connection with their modulational stability as well as in regard to the existence and stability of their localized solitary wave solutions
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707.2513
Time for pulse traversal through slabs of dispersive and negative ($\epsilon$, $\mu$) materials
The traversal times for an electromagnetic pulse traversing a slab of dispersive and dissipative material with negative dielectric permittivity ($\epsilon$) and magnetic permeability ($\mu$) have been calculated by using the average flow of electromagnetic energy in the medium. The effects of bandwidth of the pulse and dissipation in the medium have been investigated. While both large bandwidth and large dissipation have similar effects in smoothening out the resonant features that appear due to Fabry-P\'{e}rot resonances, large dissipation can result in very small or even negative traversal times near the resonant frequencies. We have also investigated the traversal times and Wigner delay times for obliquely incident pulses and evanescent pulses. The coupling to slab plasmon polariton modes in frequency ranges with negative $\epsilon$ or $\mu$ is shown to result in large traversal times at the resonant conditions. We also find that the group velocity mainly contributes to the delay times for pulse propagating across a slab with n=-1. We have checked that the traversal times are positive and subluminal for pulses with sufficiently large bandwidths.
cond-mat.mtrl-sci cond-mat.other physics.optics
the traversal times for an electromagnetic pulse traversing a slab of dispersive and dissipative material with negative dielectric permittivity epsilon and magnetic permeability mu have been calculated by using the average flow of electromagnetic energy in the medium the effects of bandwidth of the pulse and dissipation in the medium have been investigated while both large bandwidth and large dissipation have similar effects in smoothening out the resonant features that appear due to fabryperot resonances large dissipation can result in very small or even negative traversal times near the resonant frequencies we have also investigated the traversal times and wigner delay times for obliquely incident pulses and evanescent pulses the coupling to slab plasmon polariton modes in frequency ranges with negative epsilon or mu is shown to result in large traversal times at the resonant conditions we also find that the group velocity mainly contributes to the delay times for pulse propagating across a slab with n1 we have checked that the traversal times are positive and subluminal for pulses with sufficiently large bandwidths
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707.2514
Radiation-cooled Dew Water Condensers Studied by Computational Fluid Dynamic (CFD)
Harvesting condensed atmospheric vapour as dew water can be an alternative or complementary potable water resource in specific arid or insular areas. Such radiation-cooled condensing devices use already existing flat surfaces (roofs) or innovative structures with more complex shapes to enhance the dew yield. The Computational Fluid Dynamic - CFD - software PHOENICS has been programmed and applied to such radiation cooled condensers. For this purpose, the sky radiation is previously integrated and averaged for each structure. The radiative balance is then included in the CFD simulation tool to compare the efficiency of the different structures under various meteorological parameters, for complex or simple shapes and at various scales. It has been used to precise different structures before construction. (1) a 7.32 m^2 funnel shape was studied; a 30 degree tilted angle (60 degree cone half-angle) was computed to be the best compromise for funnel cooling. Compared to a 1 m^2 flat condenser, the cooling efficiency was expected to be improved by 40%. Seventeen months measurements in outdoor tests presented a 138 % increased dew yield as compared to the 1 m^2 flat condenser. (2) The simulation results for 5 various condenser shapes were also compared with experimental measurement on corresponding pilots systems: 0.16 m^2 flat planar condenser, 1 m^2 and 30 degree tilted planar condenser, 30 m^2 and 30 degree tilted planar condenser, 255 m^2 multi ridges, a preliminary construction of a large scale dew plant being implemented in the Kutch area (Gujarat, India).
physics.flu-dyn
harvesting condensed atmospheric vapour as dew water can be an alternative or complementary potable water resource in specific arid or insular areas such radiationcooled condensing devices use already existing flat surfaces roofs or innovative structures with more complex shapes to enhance the dew yield the computational fluid dynamic cfd software phoenics has been programmed and applied to such radiation cooled condensers for this purpose the sky radiation is previously integrated and averaged for each structure the radiative balance is then included in the cfd simulation tool to compare the efficiency of the different structures under various meteorological parameters for complex or simple shapes and at various scales it has been used to precise different structures before construction 1 a 732 m2 funnel shape was studied a 30 degree tilted angle 60 degree cone halfangle was computed to be the best compromise for funnel cooling compared to a 1 m2 flat condenser the cooling efficiency was expected to be improved by 40 seventeen months measurements in outdoor tests presented a 138 increased dew yield as compared to the 1 m2 flat condenser 2 the simulation results for 5 various condenser shapes were also compared with experimental measurement on corresponding pilots systems 016 m2 flat planar condenser 1 m2 and 30 degree tilted planar condenser 30 m2 and 30 degree tilted planar condenser 255 m2 multi ridges a preliminary construction of a large scale dew plant being implemented in the kutch area gujarat india
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707.2515
Generic measures for hyperbolic flows on non compact spaces
We consider the geodesic flow on a complete connected negatively curved manifold. We show that the set of invariant borel probability measures contains a dense $G_\delta$-subset consisting of ergodic measures fully supported on the non-wandering set. We also trat the case of non-positively curved manifolds and provide general tools to deal with hyperbolic systems defined on non-compact spaces.
math.DS
we consider the geodesic flow on a complete connected negatively curved manifold we show that the set of invariant borel probability measures contains a dense g_deltasubset consisting of ergodic measures fully supported on the nonwandering set we also trat the case of nonpositively curved manifolds and provide general tools to deal with hyperbolic systems defined on noncompact spaces
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707.2516
Evolution of Massive Haloes in non-Gaussian Scenarios
We have performed high-resolution cosmological N-body simulations of a concordance LCDM model to study the evolution of virialized, dark matter haloes in the presence of primordial non-Gaussianity. Following a standard procedure, departures from Gaussianity are modeled through a quadratic Gaussian term in the primordial gravitational potential, characterized by a dimensionless non-linearity strength parameter f_NL. We find that the halo mass function and its redshift evolution closely follow the analytic predictions of Matarrese et al.(2000). The existence of precise analytic predictions makes the observation of rare, massive objects at large redshift an even more attractive test to detect primordial non-Gaussian features in the large scale structure of the universe.
astro-ph
we have performed highresolution cosmological nbody simulations of a concordance lcdm model to study the evolution of virialized dark matter haloes in the presence of primordial nongaussianity following a standard procedure departures from gaussianity are modeled through a quadratic gaussian term in the primordial gravitational potential characterized by a dimensionless nonlinearity strength parameter f_nl we find that the halo mass function and its redshift evolution closely follow the analytic predictions of matarrese et al2000 the existence of precise analytic predictions makes the observation of rare massive objects at large redshift an even more attractive test to detect primordial nongaussian features in the large scale structure of the universe
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707.2517
Sound velocity and absorption measurements under high pressure using picosecond ultrasonics in diamond anvil cell. Application to the stability study of AlPdMn
We report an innovative high pressure method combining the diamond anvil cell device with the technique of picosecond ultrasonics. Such an approach allows to accurately measure sound velocity and attenuation of solids and liquids under pressure of tens of GPa, overcoming all the drawbacks of traditional techniques. The power of this new experimental technique is demonstrated in studies of lattice dynamics, stability domain and relaxation process in a metallic sample, a perfect single-grain AlPdMn quasicrystal, and rare gas, neon and argon. Application to the study of defect-induced lattice stability in AlPdMn up to 30 GPa is proposed. The present work has potential for application in areas ranging from fundamental problems in physics of solid and liquid state, which in turn could be beneficial for various other scientific fields as Earth and planetary science or material research.
cond-mat.mtrl-sci
we report an innovative high pressure method combining the diamond anvil cell device with the technique of picosecond ultrasonics such an approach allows to accurately measure sound velocity and attenuation of solids and liquids under pressure of tens of gpa overcoming all the drawbacks of traditional techniques the power of this new experimental technique is demonstrated in studies of lattice dynamics stability domain and relaxation process in a metallic sample a perfect singlegrain alpdmn quasicrystal and rare gas neon and argon application to the study of defectinduced lattice stability in alpdmn up to 30 gpa is proposed the present work has potential for application in areas ranging from fundamental problems in physics of solid and liquid state which in turn could be beneficial for various other scientific fields as earth and planetary science or material research
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707.2518
Positive and negative pressure effects on the magnetic ordering and the Kondo effect in the compound Ce2RhSi3
The competition between magnetic ordering and the Kondo effect in Ce2RhSi3, ordering antiferromagnetically at 7 K, is investigated by the measurements of magnetization, heat capacity and electrical resistivity on the solid solutions, Ce(2-x)La(x)RhSi3, Ce(2-y)Y(y)RhSi3, and Ce2RhSi(3-z)Ge(z), as well as by high pressure studies on this compound. The trends in the Kondo and Neel temperature variations among these alloys are compared to infer the roles of unit-cell volume and electronic structure changes. On the basis of the results, we infer that this compound lies at the peak of Doniach-magnetic-phase-diagram. The high pressure electrical resistivity data indicate that the quantum critical point for this compound is in the vicinity of 4 GPa.
cond-mat.str-el cond-mat.mtrl-sci
the competition between magnetic ordering and the kondo effect in ce2rhsi3 ordering antiferromagnetically at 7 k is investigated by the measurements of magnetization heat capacity and electrical resistivity on the solid solutions ce2xlaxrhsi3 ce2yyyrhsi3 and ce2rhsi3zgez as well as by high pressure studies on this compound the trends in the kondo and neel temperature variations among these alloys are compared to infer the roles of unitcell volume and electronic structure changes on the basis of the results we infer that this compound lies at the peak of doniachmagneticphasediagram the high pressure electrical resistivity data indicate that the quantum critical point for this compound is in the vicinity of 4 gpa
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707.2519
Gravitational Collapse to Toroidal and Higher Genus asymptotically AdS Black Holes
We match collapsing inhomogeneous as well as spatially homogeneous but anisotropic spacetimes to vacuum static exteriors with a negative cosmological constant and planar or hyperbolic symmetry. The collapsing interiors include the inhomogeneous solutions of Szekeres and of Barnes, which in turn include the Lemaitre-Tolman and the McVittie solutions. The collapse can result in toroidal or higher genus asymptotically AdS black holes.
gr-qc astro-ph hep-th
we match collapsing inhomogeneous as well as spatially homogeneous but anisotropic spacetimes to vacuum static exteriors with a negative cosmological constant and planar or hyperbolic symmetry the collapsing interiors include the inhomogeneous solutions of szekeres and of barnes which in turn include the lemaitretolman and the mcvittie solutions the collapse can result in toroidal or higher genus asymptotically ads black holes
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707.252
Schwinger's Magnetic Model of Matter: Can It Help Us With Grand Unification?
Many have argued that research on grand unification or local realistic physics will not be truly relevant until it makes predictions verified by experiment, different from the prediction of prior theory (the standard model). This paper proposes a new strategy (and candidate Lagrangians) for such models; that strategy in turn calls for reconsideration of Schwinger's magnetic model of matter. High priority should be given to experiments which fully confirm or deny recent scattering calculations which suggest the presence of van der Waals effects in low energy p-p and pi-pi scattering, consistent with Schwinger's model and inconsistent with QCD as we know it (with a mass gap). I briefly discuss other evidence, which does not yet rule out Schwinger's theory. A recent analysis of hadron masses also seems more consistent with the Schwinger model than with QCD.
physics.gen-ph physics.class-ph
many have argued that research on grand unification or local realistic physics will not be truly relevant until it makes predictions verified by experiment different from the prediction of prior theory the standard model this paper proposes a new strategy and candidate lagrangians for such models that strategy in turn calls for reconsideration of schwingers magnetic model of matter high priority should be given to experiments which fully confirm or deny recent scattering calculations which suggest the presence of van der waals effects in low energy pp and pipi scattering consistent with schwingers model and inconsistent with qcd as we know it with a mass gap i briefly discuss other evidence which does not yet rule out schwingers theory a recent analysis of hadron masses also seems more consistent with the schwinger model than with qcd
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707.2521
Nonlinear viscoelastic dynamics of nano-confined water
The viscoelastic dynamics of nano-confined water is studied by means of atomic force microscopy (AFM). We observe a nonlinear viscoelastic behavior remarkably similar to that widely observed in metastable complex fluids. We show that the origin of the measured nonlinear viscoelasticity in nano-confined water is a strain rate dependent relaxation time and slow dynamics. By measuring the viscoelastic modulus at different frequencies and strains, we find that the intrinsic relaxation time of nano-confined water is in the range 0.1-0.0001 s, orders of magnitude longer than that of bulk water, and comparable to the dielectric relaxation time measured in supercooled water at 170-210 K.
cond-mat.soft
the viscoelastic dynamics of nanoconfined water is studied by means of atomic force microscopy afm we observe a nonlinear viscoelastic behavior remarkably similar to that widely observed in metastable complex fluids we show that the origin of the measured nonlinear viscoelasticity in nanoconfined water is a strain rate dependent relaxation time and slow dynamics by measuring the viscoelastic modulus at different frequencies and strains we find that the intrinsic relaxation time of nanoconfined water is in the range 0100001 s orders of magnitude longer than that of bulk water and comparable to the dielectric relaxation time measured in supercooled water at 170210 k
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707.2522
On embedding well-separable graphs
Call a simple graph $H$ of order $n$ well-separable, if by deleting a separator set of size $o(n)$ the leftover will have components of size at most $o(n)$. We prove, that bounded degree well-separable spanning subgraphs are easy to embed: for every $\gamma >0$ and positive integer $\Delta$ there exists an $n_0$ such that if $n>n_0$, $\Delta(H) \le \Delta$ for a well-separable graph $H$ of order $n$ and $\delta(G) \ge (1-{1 \over 2(\chi(H)-1)} + \gamma)n$ for a simple graph $G$ of order $n$, then $H \subset G$. We extend our result to graphs with small band-width, too.
math.CO
call a simple graph h of order n wellseparable if by deleting a separator set of size on the leftover will have components of size at most on we prove that bounded degree wellseparable spanning subgraphs are easy to embed for every gamma 0 and positive integer delta there exists an n_0 such that if nn_0 deltah le delta for a wellseparable graph h of order n and deltag ge 11 over 2chih1 gamman for a simple graph g of order n then h subset g we extend our result to graphs with small bandwidth too
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707.2523
Quarkonium production in coherent hadron-hadron interactions at the LHC
The photoproduction of quarkonium in coherent hadron-hadron (pp/pA/AA$) interactions for LHC energies is an important tool to investigate the QCD dynamics at high energies. In this paper we estimate the integrated cross section and rapidity distribution for J/Psi and Upsilon production using the Color Glass Condensate (CGC) formalism. We predict large rates, implying that the experimental identification could be feasible at the LHC.
hep-ph
the photoproduction of quarkonium in coherent hadronhadron pppaaa interactions for lhc energies is an important tool to investigate the qcd dynamics at high energies in this paper we estimate the integrated cross section and rapidity distribution for jpsi and upsilon production using the color glass condensate cgc formalism we predict large rates implying that the experimental identification could be feasible at the lhc
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707.2524
Search for New Physics in High Mass Electron-Positron Events in ppbar Collisions at sqrt(s) = 1.96 TeV
We report the results of a search for a narrow resonance in electron-positron events in the invariant mass range of 150-950 GeV/c^2 using 1.3 fb^-1 of ppbar collision data at sqrt(s) = 1.96 TeV collected by the CDF II detector at Fermilab. No significant evidence of such a resonance is observed and we interpret the results to exclude the standard model-like Z' with a mass below 923 GeV/c^2 and the Randall-Sundrum graviton with a mass below 807 GeV/c^2 for k/M_pl=0.1, both at the 95% confidence level. Combining with di-photon data excludes the Randall-Sundrum graviton for masses below 889 GeV/c^2 for k/M_pl=0.1.
hep-ex
we report the results of a search for a narrow resonance in electronpositron events in the invariant mass range of 150950 gevc2 using 13 fb1 of ppbar collision data at sqrts 196 tev collected by the cdf ii detector at fermilab no significant evidence of such a resonance is observed and we interpret the results to exclude the standard modellike z with a mass below 923 gevc2 and the randallsundrum graviton with a mass below 807 gevc2 for km_pl01 both at the 95 confidence level combining with diphoton data excludes the randallsundrum graviton for masses below 889 gevc2 for km_pl01
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707.2525
Tilings With Very Elastic Tiles
We consider tiles of some fixed size, with an associated weighting on the shapes of tile, of total mass 1. We study the pressure, $p$, of tilings with those tiles; the pressure, one over the volume times the logarithm of the partition function. (The quantity we define as "pressure" could, perhaps equally harmoniously with physics notation, be called "entropy per volume", neither nomenclature is "correct".) We let $\hat p^0$ (easy to compute) be the pressure in the limit of absolute smoothness (the weighting function is constant). Then as smoothness, suitably defined, increases, $p$ converges to $\hat p^0$, uniformly in the volume. It is the uniformity requirement that makes the result non-trivial. This seems like a very basic result in the theory of pressure of tilings. Though at the same time, perhaps non-glamorous, being bereft of geometry and not very difficult. The problem arose for us out of study of a problem in mathematical physics, associated to a model of ferromagnetism.
math-ph math.MP
we consider tiles of some fixed size with an associated weighting on the shapes of tile of total mass 1 we study the pressure p of tilings with those tiles the pressure one over the volume times the logarithm of the partition function the quantity we define as pressure could perhaps equally harmoniously with physics notation be called entropy per volume neither nomenclature is correct we let hat p0 easy to compute be the pressure in the limit of absolute smoothness the weighting function is constant then as smoothness suitably defined increases p converges to hat p0 uniformly in the volume it is the uniformity requirement that makes the result nontrivial this seems like a very basic result in the theory of pressure of tilings though at the same time perhaps nonglamorous being bereft of geometry and not very difficult the problem arose for us out of study of a problem in mathematical physics associated to a model of ferromagnetism
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707.2526
Heavy flavour production in ALICE
We review the most recent studies on the performance of ALICE in heavy flavour production measurements in both hadronic and semileptonic decay channels.
hep-ex
we review the most recent studies on the performance of alice in heavy flavour production measurements in both hadronic and semileptonic decay channels
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707.2527
Rate and Power Allocation for Discrete-Rate Link Adaptation
Link adaptation, in particular adaptive coded modulation (ACM), is a promising tool for bandwidth-efficient transmission in a fading environment. The main motivation behind employing ACM schemes is to improve the spectral efficiency of wireless communication systems. In this paper, using a finite number of capacity achieving component codes, we propose new transmission schemes employing constant power transmission, as well as discrete and continuous power adaptation, for slowly varying flat-fading channels. We show that the proposed transmission schemes can achieve throughputs close to the Shannon limits of flat-fading channels using only a small number of codes. Specifically, using a fully discrete scheme with just four codes, each associated with four power levels, we achieve a spectral efficiency within 1 dB of the continuous-rate continuous-power Shannon capacity. Furthermore, when restricted to a fixed number of codes, the introduction of power adaptation has significant gains with respect to ASE and probability of no transmission compared to a constant power scheme.
cs.IT math.IT
link adaptation in particular adaptive coded modulation acm is a promising tool for bandwidthefficient transmission in a fading environment the main motivation behind employing acm schemes is to improve the spectral efficiency of wireless communication systems in this paper using a finite number of capacity achieving component codes we propose new transmission schemes employing constant power transmission as well as discrete and continuous power adaptation for slowly varying flatfading channels we show that the proposed transmission schemes can achieve throughputs close to the shannon limits of flatfading channels using only a small number of codes specifically using a fully discrete scheme with just four codes each associated with four power levels we achieve a spectral efficiency within 1 db of the continuousrate continuouspower shannon capacity furthermore when restricted to a fixed number of codes the introduction of power adaptation has significant gains with respect to ase and probability of no transmission compared to a constant power scheme
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707.2528
On the Feigel Effect: Extraction of Momentum from Vacuum?
The Green-function formalism for the electromagnetic field in a magnetoelectric (ME) medium is constructed, as a generalization of conventional Casimir theory. Zero temperature is assumed. It is shown how the formalism predicts electromagnetic momentum to be extracted from the vacuum field, just analogous to how energy is extracted in the Casimir case. The possibility of extracting momentum from vacuum was discussed recently by Feigel [Phys. Rev. Lett. 92, 020404 (2004)]. By contrast to Feigel's approach, we assume that the ME coupling occurs naturally, and is not produced by external strong fields. We also find the same effect qualitatively via another route, by considering one single electromagnetic mode.
quant-ph hep-th
the greenfunction formalism for the electromagnetic field in a magnetoelectric me medium is constructed as a generalization of conventional casimir theory zero temperature is assumed it is shown how the formalism predicts electromagnetic momentum to be extracted from the vacuum field just analogous to how energy is extracted in the casimir case the possibility of extracting momentum from vacuum was discussed recently by feigel phys rev lett 92 020404 2004 by contrast to feigels approach we assume that the me coupling occurs naturally and is not produced by external strong fields we also find the same effect qualitatively via another route by considering one single electromagnetic mode
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707.2529
Decoherence of coupled electron spins via nuclear spin dynamics in quantum dots
In double quantum dots, the exchange interaction between two electron spins renormalizes the excitation energy of pair-flips in the nuclear spin bath, which in turn modifies the non-Markovian bath dynamics. As the energy renormalization varies with the Overhauser field mismatch between the quantum dots, the electron singlet-triplet decoherence resulting from the bath dynamics depends on sampling of nuclear spin states from an ensemble, leading to the transition from exponential decoherence in single-sample dynamics to power-law decay under ensemble averaging. In contrast, the decoherence of a single electron spin in one dot is essentially the same for different choices of the nuclear spin configuration.
cond-mat.mes-hall
in double quantum dots the exchange interaction between two electron spins renormalizes the excitation energy of pairflips in the nuclear spin bath which in turn modifies the nonmarkovian bath dynamics as the energy renormalization varies with the overhauser field mismatch between the quantum dots the electron singlettriplet decoherence resulting from the bath dynamics depends on sampling of nuclear spin states from an ensemble leading to the transition from exponential decoherence in singlesample dynamics to powerlaw decay under ensemble averaging in contrast the decoherence of a single electron spin in one dot is essentially the same for different choices of the nuclear spin configuration
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