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710.5753
Integrability and reduction of Poisson group actions
In this paper we study Poisson actions of complete Poisson groups, without any connectivity assumption or requiring the existence of a momentum map. For any complete Poisson group $G$ with dual $G^\star$ we obtain a suitably connected integrating symplectic double groupoid $\calS$. As a consequence, the cotangent lift of a Poisson action on an integrable Poisson manifold $P$ can be integrated to a Poisson action of the symplectic groupoid $\poidd{\calS}{G^\star}$ on the symplectic groupoid for $P$. Finally, we show that the quotient Poisson manifold $P/G$ is also integrable, giving an explicit construction of a symplectic groupoid for it, by a reduction procedure on an associated morphism of double Lie groupoids.
math.SG math.DG
in this paper we study poisson actions of complete poisson groups without any connectivity assumption or requiring the existence of a momentum map for any complete poisson group g with dual gstar we obtain a suitably connected integrating symplectic double groupoid cals as a consequence the cotangent lift of a poisson action on an integrable poisson manifold p can be integrated to a poisson action of the symplectic groupoid poiddcalsgstar on the symplectic groupoid for p finally we show that the quotient poisson manifold pg is also integrable giving an explicit construction of a symplectic groupoid for it by a reduction procedure on an associated morphism of double lie groupoids
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710.5754
Fine structures in the optical absorption spectra of photochemical silver in silver halides? A call for further research
A survey is presented of the work done so far to check earlier claims that a fine structure may be observed to occur under certain circumstances in the impurity spectral range of the optical absorption spectra of silver halides following photostimulation in the intrinsic range. This structure, associated with the photochemical formation of silver specks, has been questioned over the years. We now weigh carefully the experimental evidence on the silver halides against a background of similar data on the alkali halides, where competing processes run slower. We come to the conclusion that present day advances in experimental techniques may be quite adequate for providing a solid experimental basis to solve the problem unambiguously.
physics.chem-ph
a survey is presented of the work done so far to check earlier claims that a fine structure may be observed to occur under certain circumstances in the impurity spectral range of the optical absorption spectra of silver halides following photostimulation in the intrinsic range this structure associated with the photochemical formation of silver specks has been questioned over the years we now weigh carefully the experimental evidence on the silver halides against a background of similar data on the alkali halides where competing processes run slower we come to the conclusion that present day advances in experimental techniques may be quite adequate for providing a solid experimental basis to solve the problem unambiguously
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710.5755
On axiomatic aspects of N=2 vertex superalgebras with odd formal variables, and deformations of N=1 vertex superalgebras
The notion of "N = 2 vertex superalgebra with two odd formal variables" is presented, the main axiom being a Jacobi identity with odd formal variables in which an N=2 superconformal shift is incorporated into the usual Jacobi identity for a vertex superalgebra. It is shown that as a consequence of these axioms, the N=2 vertex superalgebra is naturally a representation of the Lie algebra isomorphic to the three-dimensional algebra of superderivations with basis consisting of the usual conformal operator and the two N=2 superconformal operators. The notion of N=2 Neveu-Schwarz vertex operator superalgebra with two odd formal variables is introduced, and consequences of this notion are derived. Various other formulations of the notion of N=2 (Neveu-Schwarz) vertex (operator) superalgebra appearing in the mathematics and physics literature are discussed, and several mistakes in the literature are noted and corrected. The notion of ``N=2 (Neveu-Schwarz) vertex (operator) superalgebra with one odd formal variable" is formulated. It is shown that this formulation naturally arises from alternate notions of N=1 superconformality and the continuous deformation of an N=1 (Neveu-Schwarz) vertex (operator) superalgebra with one odd formal variable. This notion is formulated to reflect the underlying N=1 superanalytic geometry, and it is shown that the equivalence of the notions of N=2 (Neveu-Schwarz) vertex (operator) superalgebra with one and with two odd formal variables reflects the equivalence of N=2 superconformal and N=1 superanalytic geometry. In particular we prove that the group of formal N=2 superconformal functions vanishing at zero and invertible in a neighborhood of zero is isomorphic to a certain subgroup of N=1 superanalytic functions vanishing at zero and invertible in a neighborhood of zero.
math.QA hep-th math-ph math.MP
the notion of n 2 vertex superalgebra with two odd formal variables is presented the main axiom being a jacobi identity with odd formal variables in which an n2 superconformal shift is incorporated into the usual jacobi identity for a vertex superalgebra it is shown that as a consequence of these axioms the n2 vertex superalgebra is naturally a representation of the lie algebra isomorphic to the threedimensional algebra of superderivations with basis consisting of the usual conformal operator and the two n2 superconformal operators the notion of n2 neveuschwarz vertex operator superalgebra with two odd formal variables is introduced and consequences of this notion are derived various other formulations of the notion of n2 neveuschwarz vertex operator superalgebra appearing in the mathematics and physics literature are discussed and several mistakes in the literature are noted and corrected the notion of n2 neveuschwarz vertex operator superalgebra with one odd formal variable is formulated it is shown that this formulation naturally arises from alternate notions of n1 superconformality and the continuous deformation of an n1 neveuschwarz vertex operator superalgebra with one odd formal variable this notion is formulated to reflect the underlying n1 superanalytic geometry and it is shown that the equivalence of the notions of n2 neveuschwarz vertex operator superalgebra with one and with two odd formal variables reflects the equivalence of n2 superconformal and n1 superanalytic geometry in particular we prove that the group of formal n2 superconformal functions vanishing at zero and invertible in a neighborhood of zero is isomorphic to a certain subgroup of n1 superanalytic functions vanishing at zero and invertible in a neighborhood of zero
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710.5756
Signals of the QGP phase transition - a view from microscopic transport models
In this contribution the results from various transport models on different observables - considered as possible signals of the phase transition from hadronic matter to the quark-gluon plasma (QGP) - are briefly reviewed.
nucl-th
in this contribution the results from various transport models on different observables considered as possible signals of the phase transition from hadronic matter to the quarkgluon plasma qgp are briefly reviewed
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710.5757
Remanence of Ni nanowire arrays: Influence of size and labyrinth magnetic structure
The influence of the macroscopic size of the Ni nanowire array system on their remanence state has been investigated. A simple magnetic phenomenological model has been developed to obtain the remanence as a function of the magnetostatic interactions in the array. We observe that, due to the long range of the dipolar interactions between the wires, the size of the sample strongly influence the remanence of the array. On the other hand, the magnetic state of nanowires has been studied by variable field magnetic force microscopy for different remanent states. The distribution of nanowires with the magnetization in up or down directions and the subsequent remanent magnetization has been deduced from the magnetic images. The existence of two short-range magnetic orderings with similar energies can explain the typical labyrinth pattern observed in magnetic force microscopy images of the nanowire arrays.
cond-mat.mtrl-sci
the influence of the macroscopic size of the ni nanowire array system on their remanence state has been investigated a simple magnetic phenomenological model has been developed to obtain the remanence as a function of the magnetostatic interactions in the array we observe that due to the long range of the dipolar interactions between the wires the size of the sample strongly influence the remanence of the array on the other hand the magnetic state of nanowires has been studied by variable field magnetic force microscopy for different remanent states the distribution of nanowires with the magnetization in up or down directions and the subsequent remanent magnetization has been deduced from the magnetic images the existence of two shortrange magnetic orderings with similar energies can explain the typical labyrinth pattern observed in magnetic force microscopy images of the nanowire arrays
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710.5758
Grassmannian Beamforming for MIMO Amplify-and-Forward Relaying
In this paper, we derive the optimal transmitter/ receiver beamforming vectors and relay weighting matrix for the multiple-input multiple-output amplify-and-forward relay channel. The analysis is accomplished in two steps. In the first step, the direct link between the transmitter (Tx) and receiver (Rx) is ignored and we show that the transmitter and the relay should map their signals to the strongest right singular vectors of the Tx-relay and relay-Rx channels. Based on the distributions of these vectors for independent identically distributed (i.i.d.) Rayleigh channels, the Grassmannian codebooks are used for quantizing and sending back the channel information to the transmitter and the relay. The simulation results show that even a few number of bits can considerably increase the link reliability in terms of bit error rate. For the second step, the direct link is considered in the problem model and we derive the optimization problem that identifies the optimal Tx beamforming vector. For the i.i.d Rayleigh channels, we show that the solution to this problem is uniformly distributed on the unit sphere and we justify the appropriateness of the Grassmannian codebook (for determining the optimal beamforming vector), both analytically and by simulation. Finally, a modified quantizing scheme is presented which introduces a negligible degradation in the system performance but significantly reduces the required number of feedback bits.
cs.IT math.IT
in this paper we derive the optimal transmitter receiver beamforming vectors and relay weighting matrix for the multipleinput multipleoutput amplifyandforward relay channel the analysis is accomplished in two steps in the first step the direct link between the transmitter tx and receiver rx is ignored and we show that the transmitter and the relay should map their signals to the strongest right singular vectors of the txrelay and relayrx channels based on the distributions of these vectors for independent identically distributed iid rayleigh channels the grassmannian codebooks are used for quantizing and sending back the channel information to the transmitter and the relay the simulation results show that even a few number of bits can considerably increase the link reliability in terms of bit error rate for the second step the direct link is considered in the problem model and we derive the optimization problem that identifies the optimal tx beamforming vector for the iid rayleigh channels we show that the solution to this problem is uniformly distributed on the unit sphere and we justify the appropriateness of the grassmannian codebook for determining the optimal beamforming vector both analytically and by simulation finally a modified quantizing scheme is presented which introduces a negligible degradation in the system performance but significantly reduces the required number of feedback bits
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710.5759
CN Bimodality at Low Metallicity: The Globular Cluster M53
We present low resolution UV-blue spectroscopic observations of red giant stars in the globular cluster M53 ([Fe/H]=-1.84), obtained to study primordial abundance variations and deep mixing via the CN and CH absorption bands. The metallicity of M53 makes it an attractive target: a bimodal distribution of 3883 angstrom CN bandstrength is common in moderate- and high-metallicity globular clusters ([Fe/H] > -1.6) but unusual in those of lower metallicity ([Fe/H] < -2.0). We find that M53 is an intermediate case, and has a broad but not strongly bimodal distribution of CN bandstrength, with CN and CH bandstrengths anticorrelated in the less-evolved stars. Like many other globular clusters, M53 also exhibits a general decline in CH bandstrength and [C/Fe] abundance with rising luminosity on the red giant branch.
astro-ph
we present low resolution uvblue spectroscopic observations of red giant stars in the globular cluster m53 feh184 obtained to study primordial abundance variations and deep mixing via the cn and ch absorption bands the metallicity of m53 makes it an attractive target a bimodal distribution of 3883 angstrom cn bandstrength is common in moderate and highmetallicity globular clusters feh 16 but unusual in those of lower metallicity feh 20 we find that m53 is an intermediate case and has a broad but not strongly bimodal distribution of cn bandstrength with cn and ch bandstrengths anticorrelated in the lessevolved stars like many other globular clusters m53 also exhibits a general decline in ch bandstrength and cfe abundance with rising luminosity on the red giant branch
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710.576
Discovery of Griffiths phase in itinerant magnetic semiconductor Fe_{1-x}Co_xS_2
Critical points that can be suppressed to zero temperature are interesting because quantum fluctuations have been shown to dramatically alter electron gas properties. Here, the metal formed by Co doping the paramagnetic insulator FeS$_2$, Fe$_{1-x}$Co$_x$S$_2$, is demonstrated to order ferromagnetically at $x>x_c=0.01\pm0.005$ where we observe unusual transport, magnetic, and thermodynamic properties. We show that this magnetic semiconductor undergoes a percolative magnetic transition with distinct similarities to the Griffiths phase, including singular behavior at $x_c$ and zero temperature.
cond-mat.mtrl-sci cond-mat.str-el
critical points that can be suppressed to zero temperature are interesting because quantum fluctuations have been shown to dramatically alter electron gas properties here the metal formed by co doping the paramagnetic insulator fes_2 fe_1xco_xs_2 is demonstrated to order ferromagnetically at xx_c001pm0005 where we observe unusual transport magnetic and thermodynamic properties we show that this magnetic semiconductor undergoes a percolative magnetic transition with distinct similarities to the griffiths phase including singular behavior at x_c and zero temperature
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710.5761
On exotic modular tensor categories
It has been conjectured that every $(2+1)$-TQFT is a Chern-Simons-Witten (CSW) theory labelled by a pair $(G,\lambda)$, where $G$ is a compact Lie group, and $\lambda \in H^4(BG;Z)$ a cohomology class. We study two TQFTs constructed from Jones' subfactor theory which are believed to be counterexamples to this conjecture: one is the quantum double of the even sectors of the $E_6$ subfactor, and the other is the quantum double of the even sectors of the Haagerup subfactor. We cannot prove mathematically that the two TQFTs are indeed counterexamples because CSW TQFTs, while physically defined, are not yet mathematically constructed for every pair $(G,\lambda)$. The cases that are constructed mathematically include: 1. $G$ is a finite group--the Dijkgraaf-Witten TQFTs; 2. $G$ is torus $T^n$; 3. $G$ is a connected semi-simple Lie group--the Reshetikhin-Turaev TQFTs. We prove that the two TQFTs are not among those mathematically constructed TQFTs or their direct products. Both TQFTs are of the Turaev-Viro type: quantum doubles of spherical tensor categories. We further prove that neither TQFT is a quantum double of a braided fusion category, and give evidence that neither is an orbifold or coset of TQFTs above. Moreover, representation of the braid groups from the half $E_6$ TQFT can be used to build universal topological quantum computers, and the same is expected for the Haagerup case.
math.GT math.CT math.QA
it has been conjectured that every 21tqft is a chernsimonswitten csw theory labelled by a pair glambda where g is a compact lie group and lambda in h4bgz a cohomology class we study two tqfts constructed from jones subfactor theory which are believed to be counterexamples to this conjecture one is the quantum double of the even sectors of the e_6 subfactor and the other is the quantum double of the even sectors of the haagerup subfactor we cannot prove mathematically that the two tqfts are indeed counterexamples because csw tqfts while physically defined are not yet mathematically constructed for every pair glambda the cases that are constructed mathematically include 1 g is a finite groupthe dijkgraafwitten tqfts 2 g is torus tn 3 g is a connected semisimple lie groupthe reshetikhinturaev tqfts we prove that the two tqfts are not among those mathematically constructed tqfts or their direct products both tqfts are of the turaevviro type quantum doubles of spherical tensor categories we further prove that neither tqft is a quantum double of a braided fusion category and give evidence that neither is an orbifold or coset of tqfts above moreover representation of the braid groups from the half e_6 tqft can be used to build universal topological quantum computers and the same is expected for the haagerup case
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710.5762
Gluon self-interaction in the position space in Landau gauge
We propose a method to treat the three-gluon self-interaction vertex in the position space in D = 4 - 2e dimensions. As an example, we calculate a two-loop contribution to auxiliary Lcc vertex in the Landau gauge which contains the three-gluon vertex for SU(N) Yang-Mills theory. We represent the integral expression as a sum of separate contributions so that each of the contributions is a double finite integral or single integral (singular or finite) in the position space. In each double finite integral we use the freedom to shift exponents in powers in the denominator of integrands by some multiples of e, in order to perform at least one of the integrations by the uniqueness technique without corrupting the first term of the decomposition in e.
hep-th
we propose a method to treat the threegluon selfinteraction vertex in the position space in d 4 2e dimensions as an example we calculate a twoloop contribution to auxiliary lcc vertex in the landau gauge which contains the threegluon vertex for sun yangmills theory we represent the integral expression as a sum of separate contributions so that each of the contributions is a double finite integral or single integral singular or finite in the position space in each double finite integral we use the freedom to shift exponents in powers in the denominator of integrands by some multiples of e in order to perform at least one of the integrations by the uniqueness technique without corrupting the first term of the decomposition in e
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710.5763
A Study of Excited Charm-Strange Baryons with Evidence for new Baryons \Xi_c(3055)^+ and \Xi_c(3123)^+
We present a study of excited charm-strange baryon states produced in $e^+e^-$ annihilations at or near a center-of-mass energy of $10.58\mathrm{Ge\kern -0.1em V}$, in a data sample with an integrated luminosity of $384 fb^{-1}$ recorded with the BABAR detector at the PEP-II $e^+e^-$ storage rings at the Stanford Linear Accelerator Center. We study strong decays of charm-strange baryons to $\Lambda_c^+K^0_{\scriptscriptstyle S}$, $\Lambda_c^+K^-$, $\Lambda_c^+K^-\pi^+$, $\Lambda_c^+K^0_{\scriptscriptstyle S}\pi^-$, $\Lambda_c^+K^0_{\scriptscriptstyle S}\pi^-\pi^+$, and $\Lambda_c^+K^-\pi^+\pi^-$. This study confirms the existence of the states $\Xi_c(2980)^+$, $\Xi_c(3077)^+$, and $\Xi_c(3077)^0$, with a more accurate determination of the $\Xi_c(2980)^+$ mass and width. We also present evidence for two new states, $\Xi_c(3055)^+$ and $\Xi_c(3123)^+$, decaying through the intermediate resonant modes $\Sigma_c(2455)^{++}K^-$ and $\Sigma_c(2520)^{++}K^-$, respectively. For each of these baryons, we measure the yield in each final state, determine the statistical significance, and calculate the product of the production cross-section and branching fractions. We also measure the masses and widths of these excited charm-strange baryons.
hep-ex
we present a study of excited charmstrange baryon states produced in ee annihilations at or near a centerofmass energy of 1058mathrmgekern 01em v in a data sample with an integrated luminosity of 384 fb1 recorded with the babar detector at the pepii ee storage rings at the stanford linear accelerator center we study strong decays of charmstrange baryons to lambda_ck0_scriptscriptstyle s lambda_ck lambda_ckpi lambda_ck0_scriptscriptstyle spi lambda_ck0_scriptscriptstyle spipi and lambda_ckpipi this study confirms the existence of the states xi_c2980 xi_c3077 and xi_c30770 with a more accurate determination of the xi_c2980 mass and width we also present evidence for two new states xi_c3055 and xi_c3123 decaying through the intermediate resonant modes sigma_c2455k and sigma_c2520k respectively for each of these baryons we measure the yield in each final state determine the statistical significance and calculate the product of the production crosssection and branching fractions we also measure the masses and widths of these excited charmstrange baryons
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710.5764
Nonequilibrium dynamics of polymer translocation: a mean-field model
We analyse the dynamics of polymer translocation in the strong force regime by recasting the problem into solving a differential equation with a moving absorbing boundary. For the total translocation time, $\tau_{\rm tr}$, our simple mean-field model predicts that $\tau_{\rm tr}\sim$ (number of monomers)$^{1.5}$, which is in agreement with the exponent found in previous simulation results. Our model also predicts intricate dependencies of $\tau_{\rm tr}$ on the variations of the pulling force and of the temperature.
cond-mat.soft cond-mat.mtrl-sci
we analyse the dynamics of polymer translocation in the strong force regime by recasting the problem into solving a differential equation with a moving absorbing boundary for the total translocation time tau_rm tr our simple meanfield model predicts that tau_rm trsim number of monomers15 which is in agreement with the exponent found in previous simulation results our model also predicts intricate dependencies of tau_rm tr on the variations of the pulling force and of the temperature
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710.5765
Halo Gas Cross Sections And Covering Fractions of MgII Absorption Selected Galaxies
We examine halo gas cross sections and covering fractions, f_c, of intermediate redshift MgII absorption selected galaxies. We computed statistical absorber halo radii, R_x, using current values of dN/dz and Schechter luminosity function parameters, and have compared these values to the distribution of impact parameters and luminosities from a sample of 37 galaxies. For equivalent widths W_r(2796) > 0.3 Ang, we find 43 < R_x < 88 kpc, depending on the lower luminosity cutoff and the slope, beta, of the Holmberg-like luminosity scaling, R \propto L^beta. The observed distribution of impact parameters, D, are such that several absorbing galaxies lie at D > R_x and several non-absorbing galaxies lie at D < R_x. We deduced f_c must be less than unity and obtain a mean of <f_c> ~ 0.5 for our sample. Moreover, the data suggest halo radii of MgII absorbing galaxies do not follow a luminosity scaling with beta in the range of 0.2-0.28, if f_c= 1 as previously reported. However, provided f_c~0.5, we find that halo radii can remain consistent with a Holmberg-like luminosity relation with beta ~ 0.2 and R* = R_x/sqrt(f_c)= 110 kpc. No luminosity scaling (beta=0) is also consistent with the observed distribution of impact parameters if f_c < 0.37. The data support a scenario in which gaseous halos are patchy and likely have non-symmetric geometric distributions about the galaxies. We suggest halo gas distributions may not be govern primarily by galaxy mass/luminosity but also by stochastic processes local to the galaxy.
astro-ph
we examine halo gas cross sections and covering fractions f_c of intermediate redshift mgii absorption selected galaxies we computed statistical absorber halo radii r_x using current values of dndz and schechter luminosity function parameters and have compared these values to the distribution of impact parameters and luminosities from a sample of 37 galaxies for equivalent widths w_r2796 03 ang we find 43 r_x 88 kpc depending on the lower luminosity cutoff and the slope beta of the holmberglike luminosity scaling r propto lbeta the observed distribution of impact parameters d are such that several absorbing galaxies lie at d r_x and several nonabsorbing galaxies lie at d r_x we deduced f_c must be less than unity and obtain a mean of f_c 05 for our sample moreover the data suggest halo radii of mgii absorbing galaxies do not follow a luminosity scaling with beta in the range of 02028 if f_c 1 as previously reported however provided f_c05 we find that halo radii can remain consistent with a holmberglike luminosity relation with beta 02 and r r_xsqrtf_c 110 kpc no luminosity scaling beta0 is also consistent with the observed distribution of impact parameters if f_c 037 the data support a scenario in which gaseous halos are patchy and likely have nonsymmetric geometric distributions about the galaxies we suggest halo gas distributions may not be govern primarily by galaxy massluminosity but also by stochastic processes local to the galaxy
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710.5766
Dispersion and energy spectrum of spin excitations in an underdoped La_1.90Sr_0.10CuO_4
We performed inelastic neutron experiments on underdoped La_2-xSr_xCuO_4(x=0.10, T_c=28.6K) using a time-of-flight neutron scattering technique. Four incommensurate peaks on the two-dimensional reciprocal plane disperse inwards toward an antiferromagnetic zone center as the energy increases. These peaks merge into a single peak at an energy E_cross around w=40+-3meV. Beyond E_cross, the peak starts to broaden and ``hourglass-like'' excitations are observed. The E_cross in the underdoped sample is smaller than that reported for the optimally doped La_1.84Sr_0.16CuO_4. The reduction of the E_cross is explained by the doping-independent slope of the downward dispersion below the E_cross combined with the smaller incommensurability in the underdoped sample. In the energy spectrum of chi"(w), we observed a similar "peak-dip-hump" structure in the energy region of 10~45meV to that reported for the optimally doped sample. We discuss the relation between the hourglass-shaped dispersion and the peak-dip-hump energy spectrum.
cond-mat.supr-con cond-mat.str-el
we performed inelastic neutron experiments on underdoped la_2xsr_xcuo_4x010 t_c286k using a timeofflight neutron scattering technique four incommensurate peaks on the twodimensional reciprocal plane disperse inwards toward an antiferromagnetic zone center as the energy increases these peaks merge into a single peak at an energy e_cross around w403mev beyond e_cross the peak starts to broaden and hourglasslike excitations are observed the e_cross in the underdoped sample is smaller than that reported for the optimally doped la_184sr_016cuo_4 the reduction of the e_cross is explained by the dopingindependent slope of the downward dispersion below the e_cross combined with the smaller incommensurability in the underdoped sample in the energy spectrum of chiw we observed a similar peakdiphump structure in the energy region of 1045mev to that reported for the optimally doped sample we discuss the relation between the hourglassshaped dispersion and the peakdiphump energy spectrum
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710.5767
Hunting Galaxies to (and for) Extinction
In studies of star-forming regions, near-infrared excess (NIRX) sources--objects with intrinsic colors redder than normal stars--constitute both signal (young stars) and noise (e.g. background galaxies). We hunt down (identify) galaxies using near-infrared observations in the Perseus star-forming region by combining structural information, colors, and number density estimates. Galaxies at moderate redshifts (z = 0.1 - 0.5) have colors similar to young stellar objects (YSOs) at both near- and mid-infrared (e.g. Spitzer) wavelengths, which limits our ability to identify YSOs from colors alone. Structural information from high-quality near-infrared observations allows us to better separate YSOs from galaxies, rejecting 2/5 of the YSO candidates identified from Spitzer observations of our regions and potentially extending the YSO luminosity function below K of 15 magnitudes where galaxy contamination dominates. Once they are identified we use galaxies as valuable extra signal for making extinction maps of molecular clouds. Our new iterative procedure: the Galaxies Near Infrared Color Excess method Revisited (GNICER), uses the mean colors of galaxies as a function of magnitude to include them in extinction maps in an unbiased way. GNICER increases the number of background sources used to probe the structure of a cloud, decreasing the noise and increasing the resolution of extinction maps made far from the galactic plane.
astro-ph
in studies of starforming regions nearinfrared excess nirx sourcesobjects with intrinsic colors redder than normal starsconstitute both signal young stars and noise eg background galaxies we hunt down identify galaxies using nearinfrared observations in the perseus starforming region by combining structural information colors and number density estimates galaxies at moderate redshifts z 01 05 have colors similar to young stellar objects ysos at both near and midinfrared eg spitzer wavelengths which limits our ability to identify ysos from colors alone structural information from highquality nearinfrared observations allows us to better separate ysos from galaxies rejecting 25 of the yso candidates identified from spitzer observations of our regions and potentially extending the yso luminosity function below k of 15 magnitudes where galaxy contamination dominates once they are identified we use galaxies as valuable extra signal for making extinction maps of molecular clouds our new iterative procedure the galaxies near infrared color excess method revisited gnicer uses the mean colors of galaxies as a function of magnitude to include them in extinction maps in an unbiased way gnicer increases the number of background sources used to probe the structure of a cloud decreasing the noise and increasing the resolution of extinction maps made far from the galactic plane
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710.5768
DVCS at HERMES: Recent Results
Hard exclusive reactions are the tool to learn about generalized parton distributions, which provide a more complete parametrization of the nucleon than the ordinary parton distribution functions. Recent measurements by the HERMES collaboration of the exclusive production of photons, i.e., Deeply-Virtual Compton Scattering, are summarized and compared to model calculations, focusing on the measurements and model comparisons relevant to the extraction of quark orbital angular momentum and on the measurements on heavy nuclei.
hep-ex
hard exclusive reactions are the tool to learn about generalized parton distributions which provide a more complete parametrization of the nucleon than the ordinary parton distribution functions recent measurements by the hermes collaboration of the exclusive production of photons ie deeplyvirtual compton scattering are summarized and compared to model calculations focusing on the measurements and model comparisons relevant to the extraction of quark orbital angular momentum and on the measurements on heavy nuclei
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710.5769
Searching for hexagonal analogues of the half-metallic half-Heusler XYZ compounds
The XYZ half-Heusler crystal structure can conveniently be described as a tetrahedral zinc blende YZ structure which is stuffed by a slightly ionic X species. This description is well suited to understand the electronic structure of semiconducting 8-electron compounds such as LiAlSi (formulated Li$^+$[AlSi]$^-$) or semiconducting 18-electron compounds such as TiCoSb (formulated Ti$^{4+}$[CoSb]$^{4-}$). The basis for this is that [AlSi]$^-$ (with the same electron count as Si$_2$) and [CoSb]$^{4-}$ (the same electron count as GaSb), are both structurally and electronically, zinc-blende semiconductors. The electronic structure of half-metallic ferromagnets in this structure type can then be described as semiconductors with stuffing magnetic ions which have a local moment: For example, 22 electron MnNiSb can be written Mn$^{3+}$[NiSb]$^{3-}$. The tendency in the 18 electron compound for a semiconducting gap -- believed to arise from strong covalency -- is carried over in MnNiSb to a tendency for a gap in one spin direction. Here we similarly propose the systematic examination of 18-electron hexagonal compounds for semiconducting gaps; these would be the "stuffed wurtzite" analogues of the "stuffed zinc blende" half-Heusler compounds. These semiconductors could then serve as the basis for possibly new families of half-metallic compounds, attained through appropriate replacement of non-magnetic ions by magnetic ones. These semiconductors and semimetals with tunable charge carrier concentrations could also be interesting in the context of magnetoresistive and thermoelectric materials.
cond-mat.mtrl-sci cond-mat.other
the xyz halfheusler crystal structure can conveniently be described as a tetrahedral zinc blende yz structure which is stuffed by a slightly ionic x species this description is well suited to understand the electronic structure of semiconducting 8electron compounds such as lialsi formulated lialsi or semiconducting 18electron compounds such as ticosb formulated ti4cosb4 the basis for this is that alsi with the same electron count as si_2 and cosb4 the same electron count as gasb are both structurally and electronically zincblende semiconductors the electronic structure of halfmetallic ferromagnets in this structure type can then be described as semiconductors with stuffing magnetic ions which have a local moment for example 22 electron mnnisb can be written mn3nisb3 the tendency in the 18 electron compound for a semiconducting gap believed to arise from strong covalency is carried over in mnnisb to a tendency for a gap in one spin direction here we similarly propose the systematic examination of 18electron hexagonal compounds for semiconducting gaps these would be the stuffed wurtzite analogues of the stuffed zinc blende halfheusler compounds these semiconductors could then serve as the basis for possibly new families of halfmetallic compounds attained through appropriate replacement of nonmagnetic ions by magnetic ones these semiconductors and semimetals with tunable charge carrier concentrations could also be interesting in the context of magnetoresistive and thermoelectric materials
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710.577
Compact massive objects in Virgo galaxies: the black hole population
We investigate the distribution of massive black holes (MBHs) in the Virgo cluster. Observations suggest that AGN activity is widespread in massive galaxies (M>1e10 solar masses), while at lower galaxy masses star clusters are more abundant, which might imply a limited presence of central black holes in these galaxy-mass regimes. We explore if this possible threshold in MBH hosting, is linked to nature, nurture, or a mixture of both. The nature scenario arises naturally in hierarchical cosmologies, as MBH formation mechanisms typically are efficient in biased systems, which would later evolve into massive galaxies. Nurture, in the guise of MBH ejections following MBH mergers, provides an additional mechanism that is more effective for low mass, satellite galaxies. The combination of inefficient formation, and lower retention of MBHs, leads to the natural explanation of the distribution of compact massive ob jects in Virgo galaxies. If MBHs arrive to the correlation with the host mass and velocity dispersion during merger-triggered accretion episodes, sustained tidal stripping of the host galaxies creates a population of MBHs which lie above the expected scaling between the holes and their host mass, suggesting a possible environmental dependence.
astro-ph
we investigate the distribution of massive black holes mbhs in the virgo cluster observations suggest that agn activity is widespread in massive galaxies m1e10 solar masses while at lower galaxy masses star clusters are more abundant which might imply a limited presence of central black holes in these galaxymass regimes we explore if this possible threshold in mbh hosting is linked to nature nurture or a mixture of both the nature scenario arises naturally in hierarchical cosmologies as mbh formation mechanisms typically are efficient in biased systems which would later evolve into massive galaxies nurture in the guise of mbh ejections following mbh mergers provides an additional mechanism that is more effective for low mass satellite galaxies the combination of inefficient formation and lower retention of mbhs leads to the natural explanation of the distribution of compact massive ob jects in virgo galaxies if mbhs arrive to the correlation with the host mass and velocity dispersion during mergertriggered accretion episodes sustained tidal stripping of the host galaxies creates a population of mbhs which lie above the expected scaling between the holes and their host mass suggesting a possible environmental dependence
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710.5771
Fisher's Zeros and Perturbative Series in Gluodynamics
We study the zeros of the partition function in the complex beta plane (Fisher's zeros) in SU(2) and SU(3) gluodynamics. We discuss their effects on the asymptotic behavior of the perturbative series for the average plaquette. We present new methods to infer the existence of these zeros in region of the complex beta plane where MC reweighting is not reliable. These methods are based on the assumption that the plaquette distribution can be approximated by a phi^4 type distribution. We give new estimates of the locations for a 4^4 lattice. For SU(2), we found zeros at beta =2.18(1) \pm i0.18(2) (which differs from previous estimates), and at beta =2.18(1) \pm i0.22(2). For SU(3), we confirm beta =5.54(2)\pm i0.10(2) and found additional zeros at beta =5.54(2)\pm i0.16(2). Some of the technical material can be found in recent preprints, in the following we emphasize the motivations (why it is important to know the locations of the zeros) and the challenges (why it is difficult to locate the zeros when the volume increases)
hep-lat
we study the zeros of the partition function in the complex beta plane fishers zeros in su2 and su3 gluodynamics we discuss their effects on the asymptotic behavior of the perturbative series for the average plaquette we present new methods to infer the existence of these zeros in region of the complex beta plane where mc reweighting is not reliable these methods are based on the assumption that the plaquette distribution can be approximated by a phi4 type distribution we give new estimates of the locations for a 44 lattice for su2 we found zeros at beta 2181 pm i0182 which differs from previous estimates and at beta 2181 pm i0222 for su3 we confirm beta 5542pm i0102 and found additional zeros at beta 5542pm i0162 some of the technical material can be found in recent preprints in the following we emphasize the motivations why it is important to know the locations of the zeros and the challenges why it is difficult to locate the zeros when the volume increases
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710.5772
Pre-Poisson submanifolds
This is an expository and introductory note on some results obtained in "Coisotropic embeddings in Poisson manifolds" (ArXiv math/0611480). Some original material is contained in the last two sections, where we consider linear Poisson structures.
math.SG math.DG
this is an expository and introductory note on some results obtained in coisotropic embeddings in poisson manifolds arxiv math0611480 some original material is contained in the last two sections where we consider linear poisson structures
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710.5773
Unparticle Searches Through Compton Scattering
We investigate the effects of unparticles on Compton scattering, e gamma -> e gamma based on a future e^+e^- linear collider such as the CLIC. For different polarization configurations, we calculate the lower limits of the unparticle energy scale Lambda_U for a discovery reach at the center of mass energies sqrt(s)=0.5 TeV- 3 TeV. It is shown that, especially, for smaller values of the mass dimension d, (1 <d <1.3), and for high energies and luminosities of the collider these bounds are very significant. As a stringent limit, we find Lambda_U>80 TeV for d<1.3 at sqrt(s)=3 TeV, and 1 ab^(-1) integrated luminosity per year, which is comparable with the limits calculated from other low and high energy physics implications.
hep-ph
we investigate the effects of unparticles on compton scattering e gamma e gamma based on a future ee linear collider such as the clic for different polarization configurations we calculate the lower limits of the unparticle energy scale lambda_u for a discovery reach at the center of mass energies sqrts05 tev 3 tev it is shown that especially for smaller values of the mass dimension d 1 d 13 and for high energies and luminosities of the collider these bounds are very significant as a stringent limit we find lambda_u80 tev for d13 at sqrts3 tev and 1 ab1 integrated luminosity per year which is comparable with the limits calculated from other low and high energy physics implications
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710.5774
Physical and Wind Properties of [WC] Stars
We review the properties of carbon-sequence ([WC]) Wolf-Rayet central stars of planetary nebulae (CSPNe). Differences between the subtype distribution of [WC] stars and their massive WC cousins are discussed. We conclude that [WO]-type differ from early-type [WC] stars as a result of weaker stellar winds due to high surface gravities, and that late- and early-type [WC] and [WO] stars generally span a similar range in abundances, X(He) ~ X(C) >> X(O), consistent with a late thermal pulse, and likely progenitors to PG1159 stars.
astro-ph
we review the properties of carbonsequence wc wolfrayet central stars of planetary nebulae cspne differences between the subtype distribution of wc stars and their massive wc cousins are discussed we conclude that wotype differ from earlytype wc stars as a result of weaker stellar winds due to high surface gravities and that late and earlytype wc and wo stars generally span a similar range in abundances xhe xc xo consistent with a late thermal pulse and likely progenitors to pg1159 stars
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710.5775
A study of Bbar -> Xi_c Lambda_c^- and Bbar -> Lambda_c^+ Lambda_c^- Kbar decays at BABAR
We report measurements of B-meson decays into two- and three-body final states containing two charmed baryons using a sample of 230 million Y(4S) -> B Bbar decays. We find significant signals in two modes, measuring branching fractions BF(B^- -> \Lambda_c^+ \Lambda_c^- K^-) = (1.14 +- 0.15 +- 0.17 +- 0.60) x 10^{-3} and BF(B^- -> \Xi_c^0 \Lambda_c^-) x BF(\Xi_c^0 -> \Xi^- \pi^+) = (2.08 +- 0.65 +- 0.29 +- 0.54) x 10^{-5}, where the uncertainties are statistical, systematic, and from the branching fraction BF(\Lambda_c^+ -> p K^- \pi^+), respectively. We also set upper limits at the 90% confidence level on two other modes: BF(B0bar -> \Xi_c^+ \Lambda_c^-) x BF(\Xi_c^+ -> \Xi^- \pi^+ \pi^+) < 5.6 x 10^{-5} and BF(B0bar -> \Lambda_c^+ \Lambda_c^- K0bar) < 1.5 x 10^{-3}. We observe structure centered at an invariant mass of 2.93 GeV/c^2 in the \Lambda_c^+ K^- mass distribution of the decay B^- -> \Lambda_c^+ \Lambda_c^- K^-.
hep-ex
we report measurements of bmeson decays into two and threebody final states containing two charmed baryons using a sample of 230 million y4s b bbar decays we find significant signals in two modes measuring branching fractions bfb lambda_c lambda_c k 114 015 017 060 x 103 and bfb xi_c0 lambda_c x bfxi_c0 xi pi 208 065 029 054 x 105 where the uncertainties are statistical systematic and from the branching fraction bflambda_c p k pi respectively we also set upper limits at the 90 confidence level on two other modes bfb0bar xi_c lambda_c x bfxi_c xi pi pi 56 x 105 and bfb0bar lambda_c lambda_c k0bar 15 x 103 we observe structure centered at an invariant mass of 293 gevc2 in the lambda_c k mass distribution of the decay b lambda_c lambda_c k
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710.5776
Entanglement Generation in the Scattering of One-Dimensional Particles
This article provides a convenient framework for quantitative evaluation of the entanglement generated when two structureless, distinguishable particles scatter non-relativistically in one dimension. It explores how three factors determine the amount of entanglement generated: the momentum distributions of the incoming particles, their masses, and the interaction potential. Two important scales emerge, one set by the kinematics and one set by the dynamics. This method also provides two approximate analytic formulas useful for numerical evaluation of entanglement and reveals an interesting connection between purity, linear coordinate transformations, and momentum uncertainties.
quant-ph
this article provides a convenient framework for quantitative evaluation of the entanglement generated when two structureless distinguishable particles scatter nonrelativistically in one dimension it explores how three factors determine the amount of entanglement generated the momentum distributions of the incoming particles their masses and the interaction potential two important scales emerge one set by the kinematics and one set by the dynamics this method also provides two approximate analytic formulas useful for numerical evaluation of entanglement and reveals an interesting connection between purity linear coordinate transformations and momentum uncertainties
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710.5777
On metallic gratings coated conformally with isotropic negative-phase-velocity materials
Application of the differential method (also called the C method) to plane-wave diffraction by a perfectly conducting, sinusoidally corrugated metallic grating coated with a linear, homogeneous, isotropic, lossless dielectric-magnetic material shows that coating materials with negative index of refraction may deliver enhanced maximum nonspecular reflection efficiencies in comparison to coating materials with positive index of refraction.
physics.optics physics.class-ph
application of the differential method also called the c method to planewave diffraction by a perfectly conducting sinusoidally corrugated metallic grating coated with a linear homogeneous isotropic lossless dielectricmagnetic material shows that coating materials with negative index of refraction may deliver enhanced maximum nonspecular reflection efficiencies in comparison to coating materials with positive index of refraction
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710.5778
The SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular and Open Clusters
We validate the performance and accuracy of the current SEGUE (Sloan Extension for Galactic Understanding and Exploration) Stellar Parameter Pipeline (SSPP), which determines stellar atmospheric parameters (effective temperature, surface gravity, and metallicity) by comparing derived overall metallicities and radial velocities from selected likely members of three globular clusters (M 13, M 15, and M 2) and two open clusters (NGC 2420 and M 67) to the literature values. Spectroscopic and photometric data obtained during the course of the original Sloan Digital Sky Survey (SDSS-I) and its first extension (SDSS-II/SEGUE) are used to determine stellar radial velocities and atmospheric parameter estimates for stars in these clusters. Based on the scatter in the metallicities derived for the members of each cluster, we quantify the typical uncertainty of the SSPP values, sigma([Fe/H]) = 0.13 dex for stars in the range of 4500 K < Teff < 7500 K and 2.0 < log g < 5.0, at least over the metallicity interval spanned by the clusters studied (-2.3 < [Fe/H] < 0). The surface gravities and effective temperatures derived by the SSPP are also compared with those estimated from the comparison of the color-magnitude diagrams with stellar evolution models; we find satisfactory agreement. At present, the SSPP underestimates [Fe/H] for near-solar-metallicity stars, represented by members of M 67 in this study, by about 0.3 dex.
astro-ph
we validate the performance and accuracy of the current segue sloan extension for galactic understanding and exploration stellar parameter pipeline sspp which determines stellar atmospheric parameters effective temperature surface gravity and metallicity by comparing derived overall metallicities and radial velocities from selected likely members of three globular clusters m 13 m 15 and m 2 and two open clusters ngc 2420 and m 67 to the literature values spectroscopic and photometric data obtained during the course of the original sloan digital sky survey sdssi and its first extension sdssiisegue are used to determine stellar radial velocities and atmospheric parameter estimates for stars in these clusters based on the scatter in the metallicities derived for the members of each cluster we quantify the typical uncertainty of the sspp values sigmafeh 013 dex for stars in the range of 4500 k teff 7500 k and 20 log g 50 at least over the metallicity interval spanned by the clusters studied 23 feh 0 the surface gravities and effective temperatures derived by the sspp are also compared with those estimated from the comparison of the colormagnitude diagrams with stellar evolution models we find satisfactory agreement at present the sspp underestimates feh for nearsolarmetallicity stars represented by members of m 67 in this study by about 03 dex
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710.5779
Geometric approach towards stable homotopy groups of spheres. The Hopf invariant
We develop a geometric approach to stable homotopy groups of spheres in the spirit of the work of Pontrjagin and Rokhlin. A new proof of the Hopf Invariant One Theorem by J.F.Adams is obtained in all dimensions except 15 and 31. To prove that the stable Hopf invariant H: \Pi_n \to Z/2 vanishes for n>31, we apply methods of geometric topology. The Pontrjagin-Thom construction along with Hirsch's compression lemma identify every \alpha \in \Pi_n with the framed bordism class of a framed immersion of a closed n-manifold into R^{n+k}, for any given k>0. Its self-intersection M projects to an immersion f: M \to R^n which is framed by k copies of a line bundle \kappa. It is well-known that H(\alpha) = <w_1(\kappa)^{n-k}, [M]>. The self-intersection N of f is framed by k copies of a plane bundle with structure group D_4. We observe that H(\alpha) = <w_1(i^*\kappa)^{n-2k}, [\bar N]>, where i immerses the double cover \bar N of N into M. The hardest part of the proof is to show that, after modifying f in its skew-framed bordism class, the classifying map g: N \to K(D_4,1) factors through K(Z/4,1), provided that n=2^l-1, l>5 and n-2k=15. This is achieved by analyzing immersions in the regular homotopy class of f that approximate the composition of the classifying map M \to RP^{n-k}, the projection of RP^{n-k} onto the join of copies of S^1/(Z/4) (the standard sphere), and an embedding of this join in R^n. The last step is proved with the quaternions.
math.AT math.GT
we develop a geometric approach to stable homotopy groups of spheres in the spirit of the work of pontrjagin and rokhlin a new proof of the hopf invariant one theorem by jfadams is obtained in all dimensions except 15 and 31 to prove that the stable hopf invariant h pi_n to z2 vanishes for n31 we apply methods of geometric topology the pontrjaginthom construction along with hirschs compression lemma identify every alpha in pi_n with the framed bordism class of a framed immersion of a closed nmanifold into rnk for any given k0 its selfintersection m projects to an immersion f m to rn which is framed by k copies of a line bundle kappa it is wellknown that halpha w_1kappank m the selfintersection n of f is framed by k copies of a plane bundle with structure group d_4 we observe that halpha w_1ikappan2k bar n where i immerses the double cover bar n of n into m the hardest part of the proof is to show that after modifying f in its skewframed bordism class the classifying map g n to kd_41 factors through kz41 provided that n2l1 l5 and n2k15 this is achieved by analyzing immersions in the regular homotopy class of f that approximate the composition of the classifying map m to rpnk the projection of rpnk onto the join of copies of s1z4 the standard sphere and an embedding of this join in rn the last step is proved with the quaternions
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710.578
The SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution Spectroscopy of SDSS/SEGUE Field Stars
We report high-resolution spectroscopy of 125 field stars previously observed as part of the Sloan Digital Sky Survey and its program for Galactic studies, the Sloan Extension for Galactic Understanding and Exploration (SEGUE). These spectra are used to measure radial velocities and to derive atmospheric parameters, which we compare with those reported by the SEGUE Stellar Parameter Pipeline (SSPP). The SSPP obtains estimates of these quantities based on SDSS ugriz photometry and low-resolution (R = 2000) spectroscopy. For F- and G-type stars observed with high signal-to-noise ratios (S/N), we empirically determine the typical random uncertainties in the radial velocities, effective temperatures, surface gravities, and metallicities delivered by the SSPP to be 2.4 km/s, 130 K (2.2%), 0.21 dex, and 0.11 dex, respectively, with systematic uncertainties of a similar magnitude in the effective temperatures and metallicities. We estimate random errors for lower S/N spectra based on numerical simulations.
astro-ph
we report highresolution spectroscopy of 125 field stars previously observed as part of the sloan digital sky survey and its program for galactic studies the sloan extension for galactic understanding and exploration segue these spectra are used to measure radial velocities and to derive atmospheric parameters which we compare with those reported by the segue stellar parameter pipeline sspp the sspp obtains estimates of these quantities based on sdss ugriz photometry and lowresolution r 2000 spectroscopy for f and gtype stars observed with high signaltonoise ratios sn we empirically determine the typical random uncertainties in the radial velocities effective temperatures surface gravities and metallicities delivered by the sspp to be 24 kms 130 k 22 021 dex and 011 dex respectively with systematic uncertainties of a similar magnitude in the effective temperatures and metallicities we estimate random errors for lower sn spectra based on numerical simulations
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710.5781
Vortex Redistribution below the First-Order Transition Temperature in the \beta-Pyrochlore Superconductor KOs_2O_6
A miniature Hall sensor array was used to detect magnetic induction locally in the vortex states of the $\beta$-pyrochlore superconductor KOs$_2$O$_6$. Below the first-order transition at $T_{\rm p}\sim 8$ K, which is associated with a change in the rattling motion of K ions, the lower critical field and the remanent magnetization both show a distinct decrease, suggesting that the electron-phonon coupling is weakened below the transition. At high magnetic fields, the local induction shows an unexpectedly large jump at $T_{\rm p}$ whose sign changes with position inside the sample. Our results demonstrate a novel redistribution of vortices whose energy is reduced abruptly below the first-order transition at $T_{\rm p}$.
cond-mat.supr-con
a miniature hall sensor array was used to detect magnetic induction locally in the vortex states of the betapyrochlore superconductor kos_2o_6 below the firstorder transition at t_rm psim 8 k which is associated with a change in the rattling motion of k ions the lower critical field and the remanent magnetization both show a distinct decrease suggesting that the electronphonon coupling is weakened below the transition at high magnetic fields the local induction shows an unexpectedly large jump at t_rm p whose sign changes with position inside the sample our results demonstrate a novel redistribution of vortices whose energy is reduced abruptly below the firstorder transition at t_rm p
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710.5782
Evolution of the Intracluster Medium Between 0.2 < z < 1.3 in a Chandra Sample of 70 Galaxy Clusters
We study the evolution of the ICM with a sample of 70 galaxy clusters spanning 0.18 < z < 1.24. We find that X-ray luminosity and ICM mass at a fixed temperature evolve with redshift in a manner inconsistent with the standard self-similar model of cluster formation. Both luminosity and ICM mass evolve more slowly toward high redshift than the self-similar prediction. We find that evolution in these two observables can be modeled by a simple evolution in the cluster gas mass fraction. Excluding cluster cores from measurements results in evolution more consistent with the self-similar model than when the entire cluster is used, indicating that the fraction of clusters with cool cores increases with time, or that cool cores become more developed over time in those clusters that have them; this is supported by direct study of the redshift dependence of central surface brightness, which increases in scatter and magnitude at low redshift. We find that isophotal size-temperature relations evolve differently according to which isophote is used, indicating that the central and outer regions of cluster ICM evolve differently. We show that constraints on the evolution of the gas fraction and isophotal size-temperature relations constraints can be combined to measure cluster distances, and thus to constrain cosmological parameters. There are indications that scaling relation scatter decreases at higher redshift, suggesting that merging is not the dominant source of cluster structural variation. Our results provide constraints for simulations attempting to model cluster physics, indicate some difficulties for cosmological studies that assume constant cluster gas fractions, and point toward other potentially more robust uses of clusters for cosmological applications. (Abridged)
astro-ph
we study the evolution of the icm with a sample of 70 galaxy clusters spanning 018 z 124 we find that xray luminosity and icm mass at a fixed temperature evolve with redshift in a manner inconsistent with the standard selfsimilar model of cluster formation both luminosity and icm mass evolve more slowly toward high redshift than the selfsimilar prediction we find that evolution in these two observables can be modeled by a simple evolution in the cluster gas mass fraction excluding cluster cores from measurements results in evolution more consistent with the selfsimilar model than when the entire cluster is used indicating that the fraction of clusters with cool cores increases with time or that cool cores become more developed over time in those clusters that have them this is supported by direct study of the redshift dependence of central surface brightness which increases in scatter and magnitude at low redshift we find that isophotal sizetemperature relations evolve differently according to which isophote is used indicating that the central and outer regions of cluster icm evolve differently we show that constraints on the evolution of the gas fraction and isophotal sizetemperature relations constraints can be combined to measure cluster distances and thus to constrain cosmological parameters there are indications that scaling relation scatter decreases at higher redshift suggesting that merging is not the dominant source of cluster structural variation our results provide constraints for simulations attempting to model cluster physics indicate some difficulties for cosmological studies that assume constant cluster gas fractions and point toward other potentially more robust uses of clusters for cosmological applications abridged
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710.5783
Logarithmic singularities of Schwartz kernels and local invariants of conformal and CR structures
This paper consists of two parts. In the first part we show that in odd dimension, as well as in even dimension below the critical weight (i.e. half the dimension), the logarithmic singularities of Schwartz kernels and Green kernels of conformal invariant pseudodifferential operators are linear combinations of Weyl conformal invariants, i.e., of local conformal invariants arising from complete tensorial contractions of the covariant derivatives of the Lorentz ambient metric of Fefferman-Graham. In even dimension and above the critical weight exceptional local conformal invariants may further come into play. As a consequence, this allows us to get invariant expressions for the logarithmic singularities of the Green kernels of the GJMS operators (including the Yamabe and Paneitz operators). In the second part, we prove analogues of these results in CR geometry. Namely, we prove that the logarithmic singularities of Schwartz kernels and Green kernels of CR invariant Heisenberg pseudodifferential operators give rise to local CR invariants, and below the critical weight are linear combinations of complete tensorial contractions of the covariant derivatives of Fefferman's K\"alher-Lorentz ambient metric. As a consequence, we can obtain invariant descriptions of the logarithmic singularities of the Green kernels of the CR GJMS operators of Gover-Graham (including the CR Yamabe operator of Jerison-Lee).
math.DG math.AP
this paper consists of two parts in the first part we show that in odd dimension as well as in even dimension below the critical weight ie half the dimension the logarithmic singularities of schwartz kernels and green kernels of conformal invariant pseudodifferential operators are linear combinations of weyl conformal invariants ie of local conformal invariants arising from complete tensorial contractions of the covariant derivatives of the lorentz ambient metric of feffermangraham in even dimension and above the critical weight exceptional local conformal invariants may further come into play as a consequence this allows us to get invariant expressions for the logarithmic singularities of the green kernels of the gjms operators including the yamabe and paneitz operators in the second part we prove analogues of these results in cr geometry namely we prove that the logarithmic singularities of schwartz kernels and green kernels of cr invariant heisenberg pseudodifferential operators give rise to local cr invariants and below the critical weight are linear combinations of complete tensorial contractions of the covariant derivatives of feffermans kalherlorentz ambient metric as a consequence we can obtain invariant descriptions of the logarithmic singularities of the green kernels of the cr gjms operators of govergraham including the cr yamabe operator of jerisonlee
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710.5784
Density profiles of Ar adsorbed in slits of CO_2: spontaneous symmetry breaking
A recently reported symmetry breaking of density profiles of fluid argon confined by two parallel solid walls of carbon dioxide is studied. The calculations are performed in the framework of a nonlocal density functional theory. It is shown that the existence of such asymmetrical solutions is restricted to a special choice for the adsorption potential, where the attraction of the solid-fluid interaction is reduced by the introduction of a hard-wall repulsion. The behavior as a function of the slit's width is also discussed. All the results are placed in the context of the current knowledge on this matter.
cond-mat.soft
a recently reported symmetry breaking of density profiles of fluid argon confined by two parallel solid walls of carbon dioxide is studied the calculations are performed in the framework of a nonlocal density functional theory it is shown that the existence of such asymmetrical solutions is restricted to a special choice for the adsorption potential where the attraction of the solidfluid interaction is reduced by the introduction of a hardwall repulsion the behavior as a function of the slits width is also discussed all the results are placed in the context of the current knowledge on this matter
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710.5785
On extremely amenable groups of homeomorphisms
A topological group $G$ is {\em extremely amenable} if every compact $G$-space has a $G$-fixed point. Let $X$ be compact and $G\subset{\mathrm{Homeo}} (X)$. We prove that the following are equivalent: (1) $G$ is extremely amenable; (2) every minimal closed $G$-invariant subset of $\exp R$ is a singleton, where $R$ is the closure of the set of all graphs of $g\in G$ in the space $\exp (X^2)$ ($\exp$ stands for the space of closed subsets); (3) for each $n=1,2,...$ there is a closed $G$-invariant subset $Y_n$ of $(\exp X)^n$ such that $\cup_{n=1}^\infty Y_n$ contains arbitrarily fine covers of $X$ and for every $n\ge 1$ every minimal closed $G$-invariant subset of $\exp Y_n$ is a singleton. This yields an alternative proof of Pestov's theorem that the group of all order-preserving self-homeomorphisms of the Cantor middle-third set (or of the interval $[0,1]$) is extremely amenable.
math.DS math.GN
a topological group g is em extremely amenable if every compact gspace has a gfixed point let x be compact and gsubsetmathrmhomeo x we prove that the following are equivalent 1 g is extremely amenable 2 every minimal closed ginvariant subset of exp r is a singleton where r is the closure of the set of all graphs of gin g in the space exp x2 exp stands for the space of closed subsets 3 for each n12 there is a closed ginvariant subset y_n of exp xn such that cup_n1infty y_n contains arbitrarily fine covers of x and for every nge 1 every minimal closed ginvariant subset of exp y_n is a singleton this yields an alternative proof of pestovs theorem that the group of all orderpreserving selfhomeomorphisms of the cantor middlethird set or of the interval 01 is extremely amenable
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710.5786
Electron polarizability of crystalline solids in quantizing magnetic fields and topological gap numbers
A theory of the static electron polarizability of crystals whose energy spectrum is modified by quantizing magnetic fields is presented. It is argued that The polarizability is strongly affected by non-dissipative Hall currents induced by the presence of crossed electric and magnetic fields: these can even change its sign. Results are illustrated in detail for a two dimensional square lattice. The polarizability and the Hall conductivity are respectively linked to the two topological quantum numbers entering the so--called Diophantine equation. These numbers could in principle be detected in actual experiments.
cond-mat.mes-hall
a theory of the static electron polarizability of crystals whose energy spectrum is modified by quantizing magnetic fields is presented it is argued that the polarizability is strongly affected by nondissipative hall currents induced by the presence of crossed electric and magnetic fields these can even change its sign results are illustrated in detail for a two dimensional square lattice the polarizability and the hall conductivity are respectively linked to the two topological quantum numbers entering the socalled diophantine equation these numbers could in principle be detected in actual experiments
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710.5787
The Selberg Trace Formula for Hecke operators on cocompact Kleinian groups
We compute the Selberg trace formula for Hecke operators (also called the trace formula for modular correspondences) in the context of cocompact Kleinian groups with finite-dimentional unitary representations. We give some applications to the distribution of Hecke eigenvalues, and give an analogue of Huber's theorem.
math.NT math.SP
we compute the selberg trace formula for hecke operators also called the trace formula for modular correspondences in the context of cocompact kleinian groups with finitedimentional unitary representations we give some applications to the distribution of hecke eigenvalues and give an analogue of hubers theorem
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710.5788
Variations in Stellar Clustering with Environment: Dispersed Star Formation and the Origin of Faint Fuzzies
The observed increase in star formation efficiency with average cloud density, from several percent in whole giant molecular clouds to ~30 or more in cluster-forming cores, can be understood as the result of hierarchical cloud structure if there is a characteristic density as which individual stars become well defined. Also in this case, the efficiency of star formation increases with the dispersion of the density probability distribution function (pdf). Models with log-normal pdf's illustrate these effects. The difference between star formation in bound clusters and star formation in loose groupings is attributed to a difference in cloud pressure, with higher pressures forming more tightly bound clusters. This correlation accounts for the observed increase in clustering fraction with star formation rate and with the observation of Scaled OB Associations in low pressure environments. ``Faint fuzzie'' star clusters, which are bound but have low densities, can form in regions with high Mach numbers and low background tidal forces. The proposal by Burkert, Brodie & Larsen (2005) that faint fuzzies form at large radii in galactic collisional rings, satisfies these constraints.
astro-ph
the observed increase in star formation efficiency with average cloud density from several percent in whole giant molecular clouds to 30 or more in clusterforming cores can be understood as the result of hierarchical cloud structure if there is a characteristic density as which individual stars become well defined also in this case the efficiency of star formation increases with the dispersion of the density probability distribution function pdf models with lognormal pdfs illustrate these effects the difference between star formation in bound clusters and star formation in loose groupings is attributed to a difference in cloud pressure with higher pressures forming more tightly bound clusters this correlation accounts for the observed increase in clustering fraction with star formation rate and with the observation of scaled ob associations in low pressure environments faint fuzzie star clusters which are bound but have low densities can form in regions with high mach numbers and low background tidal forces the proposal by burkert brodie larsen 2005 that faint fuzzies form at large radii in galactic collisional rings satisfies these constraints
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710.5789
The Proto-neutron Star Phase of the Collapsar Model and the Route to Long-soft Gamma-ray Bursts and Hypernovae
Recent stellar evolutionary calculations of low-metallicity massive fast-rotating main-sequence stars yield iron cores at collapse endowed with high angular momentum. It is thought that high angular momentum and black hole formation are critical ingredients of the collapsar model of long-soft gamma-ray bursts (GRBs). Here, we present 2D multi-group, flux-limited-diffusion MHD simulations of the collapse, bounce, and immediate post-bounce phases of a 35-Msun collapsar-candidate model of Woosley & Heger. We find that, provided the magneto-rotational instability (MRI) operates in the differentially-rotating surface layers of the millisecond-period neutron star, a magnetically-driven explosion ensues during the proto-neutron star phase, in the form of a baryon-loaded non-relativistic jet, and that a black hole, central to the collapsar model, does not form. Paradoxically, and although much uncertainty surrounds stellar mass loss, angular momentum transport, magnetic fields, and the MRI, current models of chemically homogeneous evolution at low metallicity yield massive stars with iron cores that may have too much angular momentum to avoid a magnetically-driven, hypernova-like, explosion in the immediate post-bounce phase. We surmise that fast rotation in the iron core may inhibit, rather than enable, collapsar formation, which requires a large angular momentum not in the core but above it. Variations in the angular momentum distribution of massive stars at core collapse might explain both the diversity of Type Ic supernovae/hypernovae and their possible association with a GRB. A corollary might be that, rather than the progenitor mass, the angular momentum distribution, through its effect on magnetic field amplification, distinguishes these outcomes.
astro-ph
recent stellar evolutionary calculations of lowmetallicity massive fastrotating mainsequence stars yield iron cores at collapse endowed with high angular momentum it is thought that high angular momentum and black hole formation are critical ingredients of the collapsar model of longsoft gammaray bursts grbs here we present 2d multigroup fluxlimiteddiffusion mhd simulations of the collapse bounce and immediate postbounce phases of a 35msun collapsarcandidate model of woosley heger we find that provided the magnetorotational instability mri operates in the differentiallyrotating surface layers of the millisecondperiod neutron star a magneticallydriven explosion ensues during the protoneutron star phase in the form of a baryonloaded nonrelativistic jet and that a black hole central to the collapsar model does not form paradoxically and although much uncertainty surrounds stellar mass loss angular momentum transport magnetic fields and the mri current models of chemically homogeneous evolution at low metallicity yield massive stars with iron cores that may have too much angular momentum to avoid a magneticallydriven hypernovalike explosion in the immediate postbounce phase we surmise that fast rotation in the iron core may inhibit rather than enable collapsar formation which requires a large angular momentum not in the core but above it variations in the angular momentum distribution of massive stars at core collapse might explain both the diversity of type ic supernovaehypernovae and their possible association with a grb a corollary might be that rather than the progenitor mass the angular momentum distribution through its effect on magnetic field amplification distinguishes these outcomes
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710.579
On uniform continuity of Cauchy's function and uniform convergence of Cauchy's integral formula with applications
This study is on Cauchy's function $f(z)$ and its integral, $J[f(z)]\equiv (2\pi i)^{-1}\oint_C f(t)dt/(t-z)$ taken along a closed simple contour $C$, in regard to their comprehensive properties over the entire $z=x+iy$ plane consisted of the open domain ${\cal D}^+$ bounded by $C$ and the open domain ${\cal D}^-$ outside $C$. (i) With $f(z)$ assumed to be $C^n$ ($n$ times continuously differentiable) $\forall z\in {\cal D}^+$ and in a neighborhood of $C$, $f(z)$ and its derivatives $f^{(n)}(z)$ are proved uniformly continuous in the closed domain $\bar{{\cal D}^+}=[\cal D^++C]$. (ii) Under this new assumption, integral $J[f(z)]$ and its derivatives $J_n[f(z)]=d^n J[f(z)]/dz^n$ are proved to converge uniformly in $\bar{{\cal D}^+}$, thereby rendering the integral formula valid over the entire $z$-plane. (iii) The same claims (as for $f(z)$ and $J[f(z)]$) are shown extended to hold for the complement function $F(z)$, defined to be $C^n \forall z\in \bar{{\cal D}^-}=[\cal D^-+C]$, in $\bar{{\cal D}^-}$. (iv) Further, the singularity distribution of $f(z)$ in ${\cal D}^-$ (existing unless $f(z)\equiv$ const.in the $z$-plane) is elucidated by considering the direct problem exemplified with several typical singularities prescribed in ${\cal D}^-$. (v) The uniform convergence theorems for $f(z)$ and $F(z)$ shown for contour $C$ of arbitrary shape are adapted to apply to special domains in the upper or lower half $z$-planes and those inside and outside the unit circle $|z|=1$ to achieve the generalized Hilbert transforms for these cases. (vi) Finally, an unsolved inverse problem to determine all the singularities of Cauchy function $f(z)$ in domain ${\cal D}^-$ is presented for resolution as a conjecture.
math.CV math-ph math.MP
this study is on cauchys function fz and its integral jfzequiv 2pi i1oint_c ftdttz taken along a closed simple contour c in regard to their comprehensive properties over the entire zxiy plane consisted of the open domain cal d bounded by c and the open domain cal d outside c i with fz assumed to be cn n times continuously differentiable forall zin cal d and in a neighborhood of c fz and its derivatives fnz are proved uniformly continuous in the closed domain barcal dcal dc ii under this new assumption integral jfz and its derivatives j_nfzdn jfzdzn are proved to converge uniformly in barcal d thereby rendering the integral formula valid over the entire zplane iii the same claims as for fz and jfz are shown extended to hold for the complement function fz defined to be cn forall zin barcal dcal dc in barcal d iv further the singularity distribution of fz in cal d existing unless fzequiv constin the zplane is elucidated by considering the direct problem exemplified with several typical singularities prescribed in cal d v the uniform convergence theorems for fz and fz shown for contour c of arbitrary shape are adapted to apply to special domains in the upper or lower half zplanes and those inside and outside the unit circle z1 to achieve the generalized hilbert transforms for these cases vi finally an unsolved inverse problem to determine all the singularities of cauchy function fz in domain cal d is presented for resolution as a conjecture
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710.5791
Topological physics in the standard model and beyond
Topological interactions are an essential ingredient for building consistent low-energy theories of fermions, gauge fields and Nambu-Goldstone bosons in the absence of explicit UV completions, such as in Little Higgs models. These interactions are also a probe of UV completion physics that may be out of direct experimental reach. The technology of topological, or Wess-Zumino-Witten interactions is described, using explicit examples in the standard model and in Little Higgs models. The construction of a simple topological action on SU(3)/SU(2) is described. Inconsistencies in some popular Little Higgs models are pointed out.
hep-ph
topological interactions are an essential ingredient for building consistent lowenergy theories of fermions gauge fields and nambugoldstone bosons in the absence of explicit uv completions such as in little higgs models these interactions are also a probe of uv completion physics that may be out of direct experimental reach the technology of topological or wesszuminowitten interactions is described using explicit examples in the standard model and in little higgs models the construction of a simple topological action on su3su2 is described inconsistencies in some popular little higgs models are pointed out
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710.5792
Light-Cone Coordinate System in General Relativity
If there is a null gradient field in 1+3 dimensional space-time, we can set up a kind of light-cone coordinate system in the space-time. In such coordinate system, the metric takes a simple form, which is much helpful for simplifying and solving the Einstein's field equation. This light-cone coordinate system has wonderful properties and has been widely used in astrophysics to calculate parameters. In this paper, we give a detailed discussion for the structure of space-time with light-cone coordinate system. We derive the conditions for existence of such coordinate system, and show how to construct the light-cone coordinate system from usual ones, then explain their geometrical and physical meanings by examples.
physics.gen-ph
if there is a null gradient field in 13 dimensional spacetime we can set up a kind of lightcone coordinate system in the spacetime in such coordinate system the metric takes a simple form which is much helpful for simplifying and solving the einsteins field equation this lightcone coordinate system has wonderful properties and has been widely used in astrophysics to calculate parameters in this paper we give a detailed discussion for the structure of spacetime with lightcone coordinate system we derive the conditions for existence of such coordinate system and show how to construct the lightcone coordinate system from usual ones then explain their geometrical and physical meanings by examples
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710.5793
Congruences for Andrews' Smallest Parts Partition Function and New Congruences for Dyson's Rank
Let spt(n) denote the total number of appearances of smallest parts in the partitions of n. Recently, Andrews showed how spt(n) is related to the second rank moment, and proved some surprising Ramanujan-type congruences mod 5, 7 and 13. We prove a generalization of these congruences using known relations between rank and crank moments. We obtain explicit Ramanujan-type congruences for spt(n) mod p for p = 11, 17, 19, 29, 31 and 37. Recently, Bringmann and Ono proved that Dyson's rank function has infinitely many Ramanujan-type congruences. Their proof is non-constructive and utilizes the theory of weak Maass forms. We construct two explicit nontrivial examples mod 11 using elementary congruences between rank moments and half-integer weight Hecke eigenforms.
math.NT math.CO
let sptn denote the total number of appearances of smallest parts in the partitions of n recently andrews showed how sptn is related to the second rank moment and proved some surprising ramanujantype congruences mod 5 7 and 13 we prove a generalization of these congruences using known relations between rank and crank moments we obtain explicit ramanujantype congruences for sptn mod p for p 11 17 19 29 31 and 37 recently bringmann and ono proved that dysons rank function has infinitely many ramanujantype congruences their proof is nonconstructive and utilizes the theory of weak maass forms we construct two explicit nontrivial examples mod 11 using elementary congruences between rank moments and halfinteger weight hecke eigenforms
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710.5794
Quantum Algorithms for Evaluating MIN-MAX Trees
We present a bounded-error quantum algorithm for evaluating Min-Max trees. For a tree of size N our algorithm makes N^{1/2+o(1)} comparison queries, which is close to the optimal complexity for this problem.
quant-ph
we present a boundederror quantum algorithm for evaluating minmax trees for a tree of size n our algorithm makes n12o1 comparison queries which is close to the optimal complexity for this problem
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710.5795
Mass ordering of differential elliptic flow and its violation for phi mesons
We simulate the dynamics of Au+Au collisions at the Relativistic Heavy Ion Collider (RHIC) with a hybrid model that treats the dense early quark-gluon plasma (QGP) stage macroscopically as an ideal fluid, but models the dilute late hadron resonance gas (HG) microscopically using a hadronic cascade. By comparing with a pure hydrodynamic approach we identify effects of hadronic viscosity on the transverse momentum spectra and differential elliptic flow v_2(p_T). We investigate the dynamical origins of the observed mass-ordering of v_2(p_T) for identified hadrons, focusing on dissipative effects during the late hadronic stage. We find that, at RHIC energies, much of the finally observed mass-splitting is generated during the hadronic stage, due to build-up of additional radial flow. The phi meson, having a small interaction cross section, does not fully participate in this additional flow. As a result, it violates the mass-ordering pattern for v_2(p_T) that is observed for other hadron species. We also show that the early decoupling of the phi meson from the hadronic rescattering dynamics leads to interesting and unambiguous features in the p_T-dependence of the nuclear suppression factor R_AA and of the phi/p ratio.
nucl-th hep-ph nucl-ex
we simulate the dynamics of auau collisions at the relativistic heavy ion collider rhic with a hybrid model that treats the dense early quarkgluon plasma qgp stage macroscopically as an ideal fluid but models the dilute late hadron resonance gas hg microscopically using a hadronic cascade by comparing with a pure hydrodynamic approach we identify effects of hadronic viscosity on the transverse momentum spectra and differential elliptic flow v_2p_t we investigate the dynamical origins of the observed massordering of v_2p_t for identified hadrons focusing on dissipative effects during the late hadronic stage we find that at rhic energies much of the finally observed masssplitting is generated during the hadronic stage due to buildup of additional radial flow the phi meson having a small interaction cross section does not fully participate in this additional flow as a result it violates the massordering pattern for v_2p_t that is observed for other hadron species we also show that the early decoupling of the phi meson from the hadronic rescattering dynamics leads to interesting and unambiguous features in the p_tdependence of the nuclear suppression factor r_aa and of the phip ratio
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710.5796
Gauging Spacetime Symmetries on the Worldsheet and the Geometric Langlands Program
We study the two-dimensional twisted (0,2) sigma-model on various smooth complex flag manifolds G/B, and explore its relevance to the geometric Langlands program. We find that an equivalence - at the level of the holomorphic chiral algebra - between a bosonic string on G/B and a B-gauged version of itself on G, will imply an isomorphism of classical W-algebras and a level relation which underlie a geometric Langlands correspondence for G=SL(N,C). This furnishes an alternative physical interpretation of the geometric Langlands correspondence for G=SL(N,C), to that demonstrated earlier by Kapustin and Witten via an electric-magnetic duality of four-dimensional gauge theory. Likewise, the Hecke operators and Hecke eigensheaves will have an alternative physical interpretation in terms of the correlation functions of local operators in the holomorphic chiral algebra of a quasi-topological sigma-model without boundaries. A forthcoming paper will investigate the interpretation of a ``quantum'' geometric Langlands correspondence for G=SL(N,C) in a similar setting, albeit with fluxes of the sigma-model moduli which induce a ``quantum'' deformation of the relevant classical algebras turned on.
hep-th math.AG math.QA
we study the twodimensional twisted 02 sigmamodel on various smooth complex flag manifolds gb and explore its relevance to the geometric langlands program we find that an equivalence at the level of the holomorphic chiral algebra between a bosonic string on gb and a bgauged version of itself on g will imply an isomorphism of classical walgebras and a level relation which underlie a geometric langlands correspondence for gslnc this furnishes an alternative physical interpretation of the geometric langlands correspondence for gslnc to that demonstrated earlier by kapustin and witten via an electricmagnetic duality of fourdimensional gauge theory likewise the hecke operators and hecke eigensheaves will have an alternative physical interpretation in terms of the correlation functions of local operators in the holomorphic chiral algebra of a quasitopological sigmamodel without boundaries a forthcoming paper will investigate the interpretation of a quantum geometric langlands correspondence for gslnc in a similar setting albeit with fluxes of the sigmamodel moduli which induce a quantum deformation of the relevant classical algebras turned on
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710.5797
The distribution of maxima of approximately Gaussian random fields
Motivated by the problem of testing for the existence of a signal of known parametric structure and unknown ``location'' (as explained below) against a noisy background, we obtain for the maximum of a centered, smooth random field an approximation for the tail of the distribution. For the motivating class of problems this gives approximately the significance level of the maximum score test. The method is based on an application of a likelihood-ratio-identity followed by approximations of local fields. Numerical examples illustrate the accuracy of the approximations.
math.ST stat.TH
motivated by the problem of testing for the existence of a signal of known parametric structure and unknown location as explained below against a noisy background we obtain for the maximum of a centered smooth random field an approximation for the tail of the distribution for the motivating class of problems this gives approximately the significance level of the maximum score test the method is based on an application of a likelihoodratioidentity followed by approximations of local fields numerical examples illustrate the accuracy of the approximations
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710.5798
Two point correlations of a trapped interacting Bose gas at finite temperature
We develop a computationally tractable method for calculating correlation functions of the finite temperature trapped Bose gas that includes the effects of s-wave interactions. Our approach uses a classical field method to model the low energy modes and treats the high energy modes using a Hartree-Fock description. We present results of first and second order correlation functions, in position and momentum space, for an experimentally realistic system in the temperature range of $0.6T_c$ to $1.0T_c$. We also characterize the spatial coherence length of the system. Our theory should be applicable in the critical region where experiments are now able to measure first and second order correlations.
cond-mat.other
we develop a computationally tractable method for calculating correlation functions of the finite temperature trapped bose gas that includes the effects of swave interactions our approach uses a classical field method to model the low energy modes and treats the high energy modes using a hartreefock description we present results of first and second order correlation functions in position and momentum space for an experimentally realistic system in the temperature range of 06t_c to 10t_c we also characterize the spatial coherence length of the system our theory should be applicable in the critical region where experiments are now able to measure first and second order correlations
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710.5799
Configurations of Rank-40r Extremal Even Unimodular Lattices (r=1,2,3)
We show that if L is an extremal even unimodular lattice of rank 40r with r=1,2,3 then L is generated by its vectors of norms 4r and 4r+2. Our result is an extension of Ozeki's result for the case r=1.
math.NT
we show that if l is an extremal even unimodular lattice of rank 40r with r123 then l is generated by its vectors of norms 4r and 4r2 our result is an extension of ozekis result for the case r1
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710.58
Cuntz semigroups of ideals and quotients and a generalized Kasparov Stabilization Theorem
Let A be a C*-algebra and I a closed two-sided ideal of A. We use the Hilbert C*-modules picture of the Cuntz semigroup to investigate the relations between the Cuntz semigroups of I, A and A/I. We obtain a relation on two elements of the Cuntz semigroup of A that characterizes when they are equal in the Cuntz semigroup of A/I. As a corollary, we show that the Cuntz semigroup functor is exact. Replacing the Cuntz equivalence relation of Hilbert modules by their isomorphism, we obtain a generalization of Kasparov's Stabilization theorem.
math.OA
let a be a calgebra and i a closed twosided ideal of a we use the hilbert cmodules picture of the cuntz semigroup to investigate the relations between the cuntz semigroups of i a and ai we obtain a relation on two elements of the cuntz semigroup of a that characterizes when they are equal in the cuntz semigroup of ai as a corollary we show that the cuntz semigroup functor is exact replacing the cuntz equivalence relation of hilbert modules by their isomorphism we obtain a generalization of kasparovs stabilization theorem
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710.5801
Setting UBVRI Photometric Zero-Points Using Sloan Digital Sky Survey ugriz Magnitudes
We discuss the use of Sloan Digital Sky Survey (SDSS) ugriz point-spread function (PSF) photometry for setting the zero points of UBVRI CCD images. From a comparison with the Landolt (1992) standards and our own photometry we find that there is a fairly abrupt change in B, V, R, & I zero points around g, r, i ~ 14.5, and in the U zero point at u ~ 16. These changes correspond to where there is significant interpolation due to saturation in the SDSS PSF fluxes. There also seems to be another, much smaller systematic effect for stars with g, r > 19.5. The latter effect is consistent with a small Malmquist bias. Because of the difficulties with PSF fluxes of brighter stars, we recommend that comparisons of ugriz and UBVRI photometry should only be made for unsaturated stars with g, r and i in the range 14.5 - 19.5, and u in the range 16 - 19.5. We give a prescription for setting the UBVRI zero points for CCD images, and general equations for transforming from ugriz to UBVRI.
astro-ph
we discuss the use of sloan digital sky survey sdss ugriz pointspread function psf photometry for setting the zero points of ubvri ccd images from a comparison with the landolt 1992 standards and our own photometry we find that there is a fairly abrupt change in b v r i zero points around g r i 145 and in the u zero point at u 16 these changes correspond to where there is significant interpolation due to saturation in the sdss psf fluxes there also seems to be another much smaller systematic effect for stars with g r 195 the latter effect is consistent with a small malmquist bias because of the difficulties with psf fluxes of brighter stars we recommend that comparisons of ugriz and ubvri photometry should only be made for unsaturated stars with g r and i in the range 145 195 and u in the range 16 195 we give a prescription for setting the ubvri zero points for ccd images and general equations for transforming from ugriz to ubvri
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710.5802
Leptogenesis in SO(10) models with a left-right symmetric seesaw mechanism
We study leptogenesis in supersymmetric SO(10) models with a left-right symmetric seesaw mechanism, including flavour effects and the contribution of the next-to-lightest right-handed neutrino. Assuming M_D = M_u and hierarchical light neutrino masses, we find that successful leptogenesis is possible for 4 out of the 8 right-handed neutrino mass spectra that are compatible with the observed neutrino data. An accurate description of charged fermion masses appears to be an important ingredient in the analysis.
hep-ph
we study leptogenesis in supersymmetric so10 models with a leftright symmetric seesaw mechanism including flavour effects and the contribution of the nexttolightest righthanded neutrino assuming m_d m_u and hierarchical light neutrino masses we find that successful leptogenesis is possible for 4 out of the 8 righthanded neutrino mass spectra that are compatible with the observed neutrino data an accurate description of charged fermion masses appears to be an important ingredient in the analysis
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710.5803
Covariant Theory of Gravitation in the Spacetime with Finsler Structure
The theory of gravitation in the spacetime with Finsler structure is constructed. It is shown that the theory keeps general covariance. Such theory reduces to Einstein's general relativity when the Finsler structure is Riemannian. Therefore, this covariant theory of gravitation is an elegant realization of Einstein's thoughts on gravitation in the spacetime with Finsler structure.
gr-qc
the theory of gravitation in the spacetime with finsler structure is constructed it is shown that the theory keeps general covariance such theory reduces to einsteins general relativity when the finsler structure is riemannian therefore this covariant theory of gravitation is an elegant realization of einsteins thoughts on gravitation in the spacetime with finsler structure
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710.5804
Experimental Demonstration of the Unified Framework for the Mixed State Geometric Phase
Geometrical phases have been applied in virtually every major branch of physics and they play an important role in topology and knot theory in mathematics and quantum computation. However, most of the early works focus on pure quantum states which are very unrealistic and almost never occur in practice. The two existed definitions -Uhlmann's and Sj\"{o}qvist's- would result in different values for the geometric phase in general. The definition of geometric phase in mixed state scenario is still an open question. Here we present a unified framework for both approaches within one and the same formalism based on simple interferometry. We then present experimental results which confirm both approaches to mixed state geometric phase and clearly demonstrate that their unification is possible. Our experiments are furthermore the first such to measure Uhlmann's mixed state geometric phase and show in addition that it is different to the Sj\"{o}qvist's phase.
quant-ph
geometrical phases have been applied in virtually every major branch of physics and they play an important role in topology and knot theory in mathematics and quantum computation however most of the early works focus on pure quantum states which are very unrealistic and almost never occur in practice the two existed definitions uhlmanns and sjoqvists would result in different values for the geometric phase in general the definition of geometric phase in mixed state scenario is still an open question here we present a unified framework for both approaches within one and the same formalism based on simple interferometry we then present experimental results which confirm both approaches to mixed state geometric phase and clearly demonstrate that their unification is possible our experiments are furthermore the first such to measure uhlmanns mixed state geometric phase and show in addition that it is different to the sjoqvists phase
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710.5805
Estimating exposure response functions using ambient pollution concentrations
This paper presents an approach to estimating the health effects of an environmental hazard. The approach is general in nature, but is applied here to the case of air pollution. It uses a computer model involving ambient pollution and temperature inputs, to simulate the exposures experienced by individuals in an urban area, whilst incorporating the mechanisms that determine exposures. The output from the model comprises a set of daily exposures for a sample of individuals from the population of interest. These daily exposures are approximated by parametric distributions, so that the predictive exposure distribution of a randomly selected individual can be generated. These distributions are then incorporated into a hierarchical Bayesian framework (with inference using Markov Chain Monte Carlo simulation) in order to examine the relationship between short-term changes in exposures and health outcomes, whilst making allowance for long-term trends, seasonality, the effect of potential confounders and the possibility of ecological bias. The paper applies this approach to particulate pollution (PM$_{10}$) and respiratory mortality counts for seniors in greater London ($\geq$65 years) during 1997. Within this substantive epidemiological study, the effects on health of ambient concentrations and (estimated) personal exposures are compared.
stat.AP
this paper presents an approach to estimating the health effects of an environmental hazard the approach is general in nature but is applied here to the case of air pollution it uses a computer model involving ambient pollution and temperature inputs to simulate the exposures experienced by individuals in an urban area whilst incorporating the mechanisms that determine exposures the output from the model comprises a set of daily exposures for a sample of individuals from the population of interest these daily exposures are approximated by parametric distributions so that the predictive exposure distribution of a randomly selected individual can be generated these distributions are then incorporated into a hierarchical bayesian framework with inference using markov chain monte carlo simulation in order to examine the relationship between shortterm changes in exposures and health outcomes whilst making allowance for longterm trends seasonality the effect of potential confounders and the possibility of ecological bias the paper applies this approach to particulate pollution pm_10 and respiratory mortality counts for seniors in greater london geq65 years during 1997 within this substantive epidemiological study the effects on health of ambient concentrations and estimated personal exposures are compared
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710.5806
Bernoulli-Taylor formula in the case of Q-umbral Calculus
In this note we derive the Q-difference Bernoulli-Taylor formula with the rest term of the Cauchy form by the Viskov's method. This is an extension of technique by the use of Q-extented Kwasniewski's *-product . The main theorems of Q-umbral calculus were given by G. Markowsky in 1968 and extented by A.K.Kwasniewski.
math.GM
in this note we derive the qdifference bernoullitaylor formula with the rest term of the cauchy form by the viskovs method this is an extension of technique by the use of qextented kwasniewskis product the main theorems of qumbral calculus were given by g markowsky in 1968 and extented by akkwasniewski
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710.5807
Clustering of point vortices in a periodic box
The Monte Carlo simulation of $N$ point vortices with square periodic boundary conditions is performed where $N$ is order of 100. The clustering property is examined by computing the $L$ function familiar in the field of spatial ecology. The case of a positive value of $L$ corresponds to the state of clustering and the Onsager's negative temperature.
physics.flu-dyn
the monte carlo simulation of n point vortices with square periodic boundary conditions is performed where n is order of 100 the clustering property is examined by computing the l function familiar in the field of spatial ecology the case of a positive value of l corresponds to the state of clustering and the onsagers negative temperature
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710.5808
Optimal approach to quantum communication using dynamic programming
Reliable preparation of entanglement between distant systems is an outstanding problem in quantum information science and quantum communication. In practice, this has to be accomplished via noisy channels (such as optical fibers) that generally result in exponential attenuation of quantum signals at large distances. A special class of quantum error correction protocols--quantum repeater protocols--can be used to overcome such losses. In this work, we introduce a method for systematically optimizing existing protocols and developing new, more efficient protocols. Our approach makes use of a dynamic programming-based searching algorithm, the complexity of which scales only polynomially with the communication distance, letting us efficiently determine near-optimal solutions. We find significant improvements in both the speed and the final state fidelity for preparing long distance entangled states.
quant-ph
reliable preparation of entanglement between distant systems is an outstanding problem in quantum information science and quantum communication in practice this has to be accomplished via noisy channels such as optical fibers that generally result in exponential attenuation of quantum signals at large distances a special class of quantum error correction protocolsquantum repeater protocolscan be used to overcome such losses in this work we introduce a method for systematically optimizing existing protocols and developing new more efficient protocols our approach makes use of a dynamic programmingbased searching algorithm the complexity of which scales only polynomially with the communication distance letting us efficiently determine nearoptimal solutions we find significant improvements in both the speed and the final state fidelity for preparing long distance entangled states
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710.5809
Spectral properties of massless and massive quarks coupled with massive boson at finite temperature
We study the properties of massless and massive quarks coupled with a scalar and pseudoscalar boson at finite temperature in Yukawa models at the one-loop order. The behavior of the spectral function and the pole structure of the propagator are analyzed as functions of temperature $T$ and the quark mass $m_f$. It is shown that the three-peak structure of the spectral function found in a previous work for massless quarks is formed at temperatures comparable to the boson mass even for finite $m_f$, but gradually ceases to exist as $m_f$ becomes larger. We identify the three poles of the quark propagator corresponding to the collective excitations of the quark in the complex energy plane. It is shown that the three trajectories made by the poles along with a variation of $T$ undergo a structural rearrangement at a critical quark mass when $m_f$ is increased. This suggests that the physics content of the collective quark excitations is changed in a drastic way at this point. The results are nicely accounted for with the notion of the level mixing induced by a resonant scattering of the massive boson with quarks and holes of thermally excited anti-quarks.
hep-ph cond-mat.str-el nucl-th
we study the properties of massless and massive quarks coupled with a scalar and pseudoscalar boson at finite temperature in yukawa models at the oneloop order the behavior of the spectral function and the pole structure of the propagator are analyzed as functions of temperature t and the quark mass m_f it is shown that the threepeak structure of the spectral function found in a previous work for massless quarks is formed at temperatures comparable to the boson mass even for finite m_f but gradually ceases to exist as m_f becomes larger we identify the three poles of the quark propagator corresponding to the collective excitations of the quark in the complex energy plane it is shown that the three trajectories made by the poles along with a variation of t undergo a structural rearrangement at a critical quark mass when m_f is increased this suggests that the physics content of the collective quark excitations is changed in a drastic way at this point the results are nicely accounted for with the notion of the level mixing induced by a resonant scattering of the massive boson with quarks and holes of thermally excited antiquarks
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710.581
Note on q-extensions of Euler numbers and polynomials of higher order
In [14] Ozden-Simsek-Cangul constructed generating functions of higher-order twisted $(h,q)$-extension of Euler polynomials and numbers, by using $p$-adic q-deformed fermionic integral on $\Bbb Z_p$. By applying their generating functions, they derived the complete sums of products of the twisted $(h,q)$-extension of Euler polynomials and numbers, see[13, 14]. In this paper we cosider the new $q$-extension of Euler numbers and polynomials to be different which is treated by Ozden-Simsek-Cangul. From our $q$-Euler numbers and polynomials we derive some interesting identities and we construct $q$-Euler zeta functions which interpolate the new $q$-Euler numbers and polynomials at a negative integer. Furthermore we study Barnes' type $q$-Euler zeta functions. Finally we will derive the new formula for " sums products of $q$-Euler numbers and polynomials" by using fermionic $p$-adic $q$-integral on $\Bbb Z_p$.
math.NT
in 14 ozdensimsekcangul constructed generating functions of higherorder twisted hqextension of euler polynomials and numbers by using padic qdeformed fermionic integral on bbb z_p by applying their generating functions they derived the complete sums of products of the twisted hqextension of euler polynomials and numbers see13 14 in this paper we cosider the new qextension of euler numbers and polynomials to be different which is treated by ozdensimsekcangul from our qeuler numbers and polynomials we derive some interesting identities and we construct qeuler zeta functions which interpolate the new qeuler numbers and polynomials at a negative integer furthermore we study barnes type qeuler zeta functions finally we will derive the new formula for sums products of qeuler numbers and polynomials by using fermionic padic qintegral on bbb z_p
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710.5811
Void-induced cross slip of screw dislocations in fcc copper
Pinning interaction between a screw dislocation and a void in fcc copper is investigated by means of molecular dynamics simulation. A screw dislocation bows out to undergo depinning on the original glide plane at low temperatures, where the behavior of the depinning stress is consistent with that obtained by a continuum model. If the temperature is higher than 300 K, the motion of a screw dislocation is no longer restricted to a single glide plane due to cross slip on the void surface. Several depinning mechanisms that involve multiple glide planes are found. In particular, a depinning mechanism that produces an intrinsic prismatic loop is found. We show that these complex depinning mechanisms significantly increase the depinning stress.
cond-mat.mtrl-sci cond-mat.soft
pinning interaction between a screw dislocation and a void in fcc copper is investigated by means of molecular dynamics simulation a screw dislocation bows out to undergo depinning on the original glide plane at low temperatures where the behavior of the depinning stress is consistent with that obtained by a continuum model if the temperature is higher than 300 k the motion of a screw dislocation is no longer restricted to a single glide plane due to cross slip on the void surface several depinning mechanisms that involve multiple glide planes are found in particular a depinning mechanism that produces an intrinsic prismatic loop is found we show that these complex depinning mechanisms significantly increase the depinning stress
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710.5812
Spatial nonlocal pair correlations in a repulsive 1D Bose gas
We analytically calculate the spatial nonlocal pair correlation function for an interacting uniform 1D Bose gas at finite temperature and propose an experimental method to measure nonlocal correlations. Our results span six different physical realms, including the weakly and strongly interacting regimes. We show explicitly that the characteristic correlation lengths are given by one of four length scales: the thermal de Broglie wavelength, the mean interparticle separation, the healing length, or the phase coherence length. In all regimes, we identify the profound role of interactions and find that under certain conditions the pair correlation may develop a global maximum at a finite interparticle separation due to the competition between repulsive interactions and thermal effects.
cond-mat.other cond-mat.stat-mech
we analytically calculate the spatial nonlocal pair correlation function for an interacting uniform 1d bose gas at finite temperature and propose an experimental method to measure nonlocal correlations our results span six different physical realms including the weakly and strongly interacting regimes we show explicitly that the characteristic correlation lengths are given by one of four length scales the thermal de broglie wavelength the mean interparticle separation the healing length or the phase coherence length in all regimes we identify the profound role of interactions and find that under certain conditions the pair correlation may develop a global maximum at a finite interparticle separation due to the competition between repulsive interactions and thermal effects
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710.5813
Study of continuous-time quantum walks on quotient graphs via quantum probability theory
In the present paper, we study the continuous-time quantum walk on quotient graphs. On such graphs, there is a straightforward reduction of problem to a subspace that can be considerably smaller than the original one. Along the lines of reductions, by using the idea of calculation of the probability amplitudes for continuous-time quantum walk in terms of the spectral distribution associated with the adjacency matrix of graphs [Jafarizadeh and Salimi (Ann. Phys 322(2007))], we show the continuous-time quantum walk on original graph $\Gamma$ induces a continuous-time quantum walk on quotient graph $\Gamma_H$. Finally, for example we investigate continuous-time quantum walk on some quotient Cayley graphs.
quant-ph
in the present paper we study the continuoustime quantum walk on quotient graphs on such graphs there is a straightforward reduction of problem to a subspace that can be considerably smaller than the original one along the lines of reductions by using the idea of calculation of the probability amplitudes for continuoustime quantum walk in terms of the spectral distribution associated with the adjacency matrix of graphs jafarizadeh and salimi ann phys 3222007 we show the continuoustime quantum walk on original graph gamma induces a continuoustime quantum walk on quotient graph gamma_h finally for example we investigate continuoustime quantum walk on some quotient cayley graphs
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710.5814
A class of spherically-separable non-Hermitian PphiTphi-symmetric Hamiltonians
A family of spherical non-Hermitian potentials is studied. It is shown that the corresponding non-Hermitian Hamiltonians admit some "new" P$phi$T$phi$-symmetry. It is observed that whilst such P$phi$T$phi$-symmetric Hamiltonians just copy the eigenvalues of V(r), the corresponding wavefunctions would rather indulge some new probabilistic interpretations due to the change in the azimuthal part.
quant-ph
a family of spherical nonhermitian potentials is studied it is shown that the corresponding nonhermitian hamiltonians admit some new pphitphisymmetry it is observed that whilst such pphitphisymmetric hamiltonians just copy the eigenvalues of vr the corresponding wavefunctions would rather indulge some new probabilistic interpretations due to the change in the azimuthal part
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710.5815
Periodic cyclic homology of reductive p-adic groups
Let G be a reductive p-adic group, H(G) its Hecke algebra and S(G) its Schwartz algebra. We will show that these algebras have the same periodic cyclic homology. This might be used to provide an alternative proof of the Baum-Connes conjecture for G, modulo torsion. As preparation for our main theorem we prove two results that have independent interest. Firstly a general comparison theorem for the periodic cyclic homology of finite type algebras and certain Fr\'echet completions thereof. Secondly a refined form of the Langlands classification for G, which clarifies the relation between the smooth spectrum and the tempered spectrum.
math.KT math.RT
let g be a reductive padic group hg its hecke algebra and sg its schwartz algebra we will show that these algebras have the same periodic cyclic homology this might be used to provide an alternative proof of the baumconnes conjecture for g modulo torsion as preparation for our main theorem we prove two results that have independent interest firstly a general comparison theorem for the periodic cyclic homology of finite type algebras and certain frechet completions thereof secondly a refined form of the langlands classification for g which clarifies the relation between the smooth spectrum and the tempered spectrum
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710.5816
Localization problem of the quasiperiodic system with the spin orbit interaction
We study one dimensional quasiperiodic system obtained from the tight-binding model on the square lattice in a uniform magnetic field with the spin orbit interaction. The phase diagram with respect to the Harper coupling and the Rashba coupling are proposed from a number of numerical studies including a multifractal analysis. There are four phases, I, II, III, and IV in this order from weak to strong Harper coupling. In the weak coupling phase I all the wave functions are extended, in the intermediate coupling phases II and III mobility edges exist, and accordingly both localized and extended wave functions exist, and in the strong Harper coupling phase IV all the wave functions are localized. Phase I and Phase IV are related by the duality, and phases II and III are related by the duality, as well. A localized wave function is related to an extended wave function by the duality, and vice versa. The boundary between phases II and III is the self-dual line on which all the wave functions are critical. In the present model the duality does not lead to pure spectra in contrast to the case of Harper equation.
cond-mat.stat-mech cond-mat.mes-hall
we study one dimensional quasiperiodic system obtained from the tightbinding model on the square lattice in a uniform magnetic field with the spin orbit interaction the phase diagram with respect to the harper coupling and the rashba coupling are proposed from a number of numerical studies including a multifractal analysis there are four phases i ii iii and iv in this order from weak to strong harper coupling in the weak coupling phase i all the wave functions are extended in the intermediate coupling phases ii and iii mobility edges exist and accordingly both localized and extended wave functions exist and in the strong harper coupling phase iv all the wave functions are localized phase i and phase iv are related by the duality and phases ii and iii are related by the duality as well a localized wave function is related to an extended wave function by the duality and vice versa the boundary between phases ii and iii is the selfdual line on which all the wave functions are critical in the present model the duality does not lead to pure spectra in contrast to the case of harper equation
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710.5817
CLePAPS: Fast Pair Alignment of Protein Structures Based on Conformational Letters
Fast, efficient and reliable algorithms for pairwise alignment of protein structures are in ever increasing demand for analyzing the rapidly growing data of protein structures. CLePAPS is a tool developed for this purpose. It distinguishes itself from other existing algorithms by the use of conformational letters, which are discretized states of 3D segmental structural states. A letter corresponds to a cluster of combinations of the three angles formed by C_alpha pseudobonds of four contiguous residues. A substitution matrix called CLESUM is available to measure similarity between any two such letters. CLePAPS regards an aligned fragment pair (AFP) as an ungapped string pair with a high sum of pairwise CLESUM scores. Using CLESUM scores as the similarity measure, CLePAPS searches for AFPs by simple string comparison. The transformation which best superimposes a highly similar AFP can be used to superimpose the structure pairs under comparison. A highly scored AFP which is consistent with several other AFPs determines an initial alignment. CLePAPS then joins consistent AFPs guided by their similarity scores to extend the alignment by several `zoom-in' iteration steps. A follow-up refinement produces the final alignment. CLePAPS does not implement dynamic programming. The utility of CLePAPS is tested on various protein structure pairs.
q-bio.QM
fast efficient and reliable algorithms for pairwise alignment of protein structures are in ever increasing demand for analyzing the rapidly growing data of protein structures clepaps is a tool developed for this purpose it distinguishes itself from other existing algorithms by the use of conformational letters which are discretized states of 3d segmental structural states a letter corresponds to a cluster of combinations of the three angles formed by c_alpha pseudobonds of four contiguous residues a substitution matrix called clesum is available to measure similarity between any two such letters clepaps regards an aligned fragment pair afp as an ungapped string pair with a high sum of pairwise clesum scores using clesum scores as the similarity measure clepaps searches for afps by simple string comparison the transformation which best superimposes a highly similar afp can be used to superimpose the structure pairs under comparison a highly scored afp which is consistent with several other afps determines an initial alignment clepaps then joins consistent afps guided by their similarity scores to extend the alignment by several zoomin iteration steps a followup refinement produces the final alignment clepaps does not implement dynamic programming the utility of clepaps is tested on various protein structure pairs
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710.5818
Asymptotic behavior of Tor over complete intersections and applications
Let $R$ be a local complete intersection and $M,N$ are $R$-modules such that $\ell(\Tor_i^R(M,N))<\infty$ for $i\gg 0$. Imitating an approach by Avramov and Buchweitz, we investigate the asymptotic behavior of $\ell(\Tor_i^R(M,N))$ using Eisenbud operators and show that they have well-behaved growth. We define and study a function $\eta^R(M,N)$ which generalizes Serre's intersection multiplicity $\chi^R(M,N)$ over regular local rings and Hochster's function $\theta^R(M,N)$ over local hypersurfaces. We use good properties of $\eta^R(M,N)$ to obtain various results on complexities of $\Tor$ and $\Ext$, vanishing of $\Tor$, depth of tensor products, and dimensions of intersecting modules over local complete intersections.
math.AC
let r be a local complete intersection and mn are rmodules such that elltor_irmninfty for igg 0 imitating an approach by avramov and buchweitz we investigate the asymptotic behavior of elltor_irmn using eisenbud operators and show that they have wellbehaved growth we define and study a function etarmn which generalizes serres intersection multiplicity chirmn over regular local rings and hochsters function thetarmn over local hypersurfaces we use good properties of etarmn to obtain various results on complexities of tor and ext vanishing of tor depth of tensor products and dimensions of intersecting modules over local complete intersections
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710.5819
Molecular formations in ultracold mixtures of interacting and noninteracting atomic gases
Atom-molecule equilibrium for molecular formation processes is discussed for boson-fermion, fermion-fermion, and boson-boson mixtures of ultracold atomic gases in the framework of quasichemical equilibrium theory. After presentation of the general formulation, zero-temperature phase diagrams of the atom-molecule equilibrium states are calculated analytically; molecular, mixed, and dissociated phases are shown to appear for the change of the binding energy of the molecules. The temperature dependences of the atom or molecule densities are calculated numerically, and finite-temperature phase structures are obtained of the atom-molecule equilibrium in the mixtures. The transition temperatures of the atom or molecule Bose-Einstein condensations are also evaluated from these results. Quantum-statistical deviations of the law of mass action in atom-molecule equilibrium, which should be satisfied in mixtures of classical Maxwell-Boltzmann gases, are calculated, and the difference in the different types of quantum-statistical effects is clarified. Mean-field calculations with interparticle interactions (atom-atom, atom-molecule, and molecule-molecule) are formulated, where interaction effects are found to give the linear density-dependent term in the effective molecular binding energies. This method is applied to calculations of zero-temperature phase diagrams, where new phases with coexisting local-equilibrium states are shown to appear in the case of strongly repulsive interactions.
cond-mat.soft cond-mat.other
atommolecule equilibrium for molecular formation processes is discussed for bosonfermion fermionfermion and bosonboson mixtures of ultracold atomic gases in the framework of quasichemical equilibrium theory after presentation of the general formulation zerotemperature phase diagrams of the atommolecule equilibrium states are calculated analytically molecular mixed and dissociated phases are shown to appear for the change of the binding energy of the molecules the temperature dependences of the atom or molecule densities are calculated numerically and finitetemperature phase structures are obtained of the atommolecule equilibrium in the mixtures the transition temperatures of the atom or molecule boseeinstein condensations are also evaluated from these results quantumstatistical deviations of the law of mass action in atommolecule equilibrium which should be satisfied in mixtures of classical maxwellboltzmann gases are calculated and the difference in the different types of quantumstatistical effects is clarified meanfield calculations with interparticle interactions atomatom atommolecule and moleculemolecule are formulated where interaction effects are found to give the linear densitydependent term in the effective molecular binding energies this method is applied to calculations of zerotemperature phase diagrams where new phases with coexisting localequilibrium states are shown to appear in the case of strongly repulsive interactions
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710.582
The C-(symmetric) quadrilateral lattice, its transformations and the algebro-geometric construction
The C-quadrilateral lattice (CQL), called also the symmetric lattice, provides geometric interpretation of the discrete CKP equation within the quadrilateral lattice (QL) theory. We discuss affine-geometric properties of the lattice emphasizing the role of the Gallucci theorem in the multidimensional consistency of the CQL. Then we give the algebro-geometric construction of the lattice. We also present the reduction of the vectorial fundamental transformation of the QL to the CQL case. In the Appendix we show a relation between the QL and the so called Darboux maps.
nlin.SI
the cquadrilateral lattice cql called also the symmetric lattice provides geometric interpretation of the discrete ckp equation within the quadrilateral lattice ql theory we discuss affinegeometric properties of the lattice emphasizing the role of the gallucci theorem in the multidimensional consistency of the cql then we give the algebrogeometric construction of the lattice we also present the reduction of the vectorial fundamental transformation of the ql to the cql case in the appendix we show a relation between the ql and the so called darboux maps
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710.5821
Geometry dependence of the charge transfer at YBa2Cu3O7-metal interfaces
Transport in electronic devices based on high-Tc superconductors depends critically on the charge redistribution at interfaces, since the band structure is modified on a local scale. Using the density functional theory approach for relaxed YBa2Cu3O7-metal contacts, the charge transfer into the superconductor has been studied in Appl. Phys. Lett. 90, 192502 (2007). In the present paper we discuss the systematics inherent in the local electronic structure of the near-contact YBa2Cu3O7 sites, in particular the dependence on the contact geometry.
cond-mat.supr-con
transport in electronic devices based on hightc superconductors depends critically on the charge redistribution at interfaces since the band structure is modified on a local scale using the density functional theory approach for relaxed yba2cu3o7metal contacts the charge transfer into the superconductor has been studied in appl phys lett 90 192502 2007 in the present paper we discuss the systematics inherent in the local electronic structure of the nearcontact yba2cu3o7 sites in particular the dependence on the contact geometry
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710.5822
Hard X-ray variability of Magnetar's Tails observed with INTEGRAL
Magnetar's persistent emission above 10 keV was recently discovered thanks to the imaging capabilities of the IBIS coded mask telescope on board the INTEGRAL satellite. The only two sources that show some degree of long term variability are SGR 1806-20 and 1RXS J170849.0-400910. We find some indications that variability of these hard tails could be the driver of the spectral variability measured in these sources below 10 keV. In addition we report for the first time the detection at 2.8 sigma level of pulsations in the hard X-ray tail of SGR 1806-20.
astro-ph
magnetars persistent emission above 10 kev was recently discovered thanks to the imaging capabilities of the ibis coded mask telescope on board the integral satellite the only two sources that show some degree of long term variability are sgr 180620 and 1rxs j1708490400910 we find some indications that variability of these hard tails could be the driver of the spectral variability measured in these sources below 10 kev in addition we report for the first time the detection at 28 sigma level of pulsations in the hard xray tail of sgr 180620
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710.5823
The complex relation between production and scattering amplitudes
The unitarity relation, Im(A)=T* A, is derived for a three-body production amplitude, A, that consists of a complex linear combination of elements of the two-body scattering amplitude, T. We conclude that the unitarity relation does not impose a realness condition on the coefficients in the expansion of, A, in terms of, T.
hep-ph
the unitarity relation imat a is derived for a threebody production amplitude a that consists of a complex linear combination of elements of the twobody scattering amplitude t we conclude that the unitarity relation does not impose a realness condition on the coefficients in the expansion of a in terms of t
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710.5824
Inhomogeneous charge ordering of a spinless fermionic system on the Bethe lattice
We show that a system of spinless Fermi particles, localized on the sites of the Bethe lattice with coordination number z and interacting through a repulsive nearest-neighbor interaction, exhibits a phase transition to a charge-ordered state. The phase diagram in the n-T plane is derived. Relevant thermodynamic quantities, such as the free energy, the specific heat, the entropy and the compressibility are analyzed in detail.
cond-mat.str-el cond-mat.stat-mech
we show that a system of spinless fermi particles localized on the sites of the bethe lattice with coordination number z and interacting through a repulsive nearestneighbor interaction exhibits a phase transition to a chargeordered state the phase diagram in the nt plane is derived relevant thermodynamic quantities such as the free energy the specific heat the entropy and the compressibility are analyzed in detail
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710.5825
Evolution of the genetic code. Emergence of stop codons
What could cause the emergence of non-encoding codons in the course of evolution of the genetic code? Hypothesis of evolution of the genetic code from GC to the AGUC-alphabet account for existence of stop codons.
q-bio.PE q-bio.BM
what could cause the emergence of nonencoding codons in the course of evolution of the genetic code hypothesis of evolution of the genetic code from gc to the agucalphabet account for existence of stop codons
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710.5826
On a random recursion related to absorption times of death Markov chains
Let $X_1,X_2,...$ be a sequence of random variables satisfying the distributional recursion $X_1=0$ and $X_n= X_{n-I_n}+1$ for $n=2,3,...$, where $I_n$ is a random variable with values in $\{1,...,n-1\}$ which is independent of $X_2,...,X_{n-1}$. The random variable $X_n$ can be interpreted as the absorption time of a suitable death Markov chain with state space ${\mathbb N}:=\{1,2,...\}$ and absorbing state 1, conditioned that the chain starts in the initial state $n$. This paper focuses on the asymptotics of $X_n$ as $n$ tends to infinity under the particular but important assumption that the distribution of $I_n$ satisfies ${\mathbb P}\{I_n=k\}=p_k/(p_1+...+p_{n-1})$ for some given probability distribution $p_k={\mathbb P}\{\xi=k\}$, $k\in{\mathbb N}$. Depending on the tail behaviour of the distribution of $\xi$, several scalings for $X_n$ and corresponding limiting distributions come into play, among them stable distributions and distributions of exponential integrals of subordinators. The methods used in this paper are mainly probabilistic. The key tool is a coupling technique which relates the distribution of $X_n$ to a random walk, which explains, for example, the appearance of the Mittag-Leffler distribution in this context. The results are applied to describe the asymptotics of the number of collisions for certain beta-coalescent processes.
math.PR math.ST stat.TH
let x_1x_2 be a sequence of random variables satisfying the distributional recursion x_10 and x_n x_ni_n1 for n23 where i_n is a random variable with values in 1n1 which is independent of x_2x_n1 the random variable x_n can be interpreted as the absorption time of a suitable death markov chain with state space mathbb n12 and absorbing state 1 conditioned that the chain starts in the initial state n this paper focuses on the asymptotics of x_n as n tends to infinity under the particular but important assumption that the distribution of i_n satisfies mathbb pi_nkp_kp_1p_n1 for some given probability distribution p_kmathbb pxik kinmathbb n depending on the tail behaviour of the distribution of xi several scalings for x_n and corresponding limiting distributions come into play among them stable distributions and distributions of exponential integrals of subordinators the methods used in this paper are mainly probabilistic the key tool is a coupling technique which relates the distribution of x_n to a random walk which explains for example the appearance of the mittagleffler distribution in this context the results are applied to describe the asymptotics of the number of collisions for certain betacoalescent processes
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710.5827
A reversible theory of entanglement and its relation to the second law
We consider the manipulation of multipartite entangled states in the limit of many copies under quantum operations that asymptotically cannot generate entanglement. As announced in [Brandao and Plenio, Nature Physics 4, 8 (2008)], and in stark contrast to the manipulation of entanglement under local operations and classical communication, the entanglement shared by two or more parties can be reversibly interconverted in this setting. The unique entanglement measure is identified as the regularized relative entropy of entanglement, which is shown to be equal to a regularized and smoothed version of the logarithmic robustness of entanglement. Here we give a rigorous proof of this result, which is fundamentally based on a certain recent extension of quantum Stein's Lemma proved in [Brandao and Plenio, Commun. Math. 295, 791 (2010)], giving the best measurement strategy for discriminating several copies of an entangled state from an arbitrary sequence of non-entangled states, with an optimal distinguishability rate equal to the regularized relative entropy of entanglement. We moreover analyse the connection of our approach to axiomatic formulations of the second law of thermodynamics.
quant-ph
we consider the manipulation of multipartite entangled states in the limit of many copies under quantum operations that asymptotically cannot generate entanglement as announced in brandao and plenio nature physics 4 8 2008 and in stark contrast to the manipulation of entanglement under local operations and classical communication the entanglement shared by two or more parties can be reversibly interconverted in this setting the unique entanglement measure is identified as the regularized relative entropy of entanglement which is shown to be equal to a regularized and smoothed version of the logarithmic robustness of entanglement here we give a rigorous proof of this result which is fundamentally based on a certain recent extension of quantum steins lemma proved in brandao and plenio commun math 295 791 2010 giving the best measurement strategy for discriminating several copies of an entangled state from an arbitrary sequence of nonentangled states with an optimal distinguishability rate equal to the regularized relative entropy of entanglement we moreover analyse the connection of our approach to axiomatic formulations of the second law of thermodynamics
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710.5828
Midgap states in corrugated graphene: Ab-initio calculations and effective field theory
We investigate the electronic properties of corrugated graphene and show how rippling-induced pseudomagnetic fields alter graphene's low-energy electronic properties by combining first principles calculations with an effective field theory. The formation of flat bands near the Fermi level corresponding to pseudo-Landau levels is studied as a function of the rippling parameters. Quenched and relaxed ripples turn out to be fundamentally different is this respect: It is demonstrated, both numerically and analytically, that annealing of quenched ripples can destroy the flat bands.
cond-mat.mes-hall
we investigate the electronic properties of corrugated graphene and show how ripplinginduced pseudomagnetic fields alter graphenes lowenergy electronic properties by combining first principles calculations with an effective field theory the formation of flat bands near the fermi level corresponding to pseudolandau levels is studied as a function of the rippling parameters quenched and relaxed ripples turn out to be fundamentally different is this respect it is demonstrated both numerically and analytically that annealing of quenched ripples can destroy the flat bands
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710.5829
Decay of low-lying 12C resonances within a 3alpha cluster model
We compute energy distributions of three $\alpha$-particles emerging from the decay of $^{12}$C resonances by means of the hyperspherical adiabatic expansion method combined with complex scaling. The large distance continuum properties of the wave functions are crucial and must be accurately calculated. The substantial changes from small to large distances determine the decay mechanisms. We illustrate by computing the energy distributions from decays of the $1^{+}$ and $3^-$-resonances in $^{12}$C. These states are dominated by direct and sequential decays into the three-body continuum respectively.
nucl-th
we compute energy distributions of three alphaparticles emerging from the decay of 12c resonances by means of the hyperspherical adiabatic expansion method combined with complex scaling the large distance continuum properties of the wave functions are crucial and must be accurately calculated the substantial changes from small to large distances determine the decay mechanisms we illustrate by computing the energy distributions from decays of the 1 and 3resonances in 12c these states are dominated by direct and sequential decays into the threebody continuum respectively
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710.583
Stability analysis of a max-min fair Rate Control Protocol (RCP) in a small buffer regime
In this note we analyse various stability properties of the max-min fair Rate Control Protocol (RCP) operating with small buffers. We first tackle the issue of stability for networks with arbitrary topologies. We prove that the max-min fair RCP fluid model is globally stable in the absence of propagation delays, and also derive a set of conditions for local stability when arbitrary heterogeneous propagation delays are present. The network delay stability result assumes that, at equilibrium, there is only one bottleneck link along each route. Lastly, in the simpler setting of a single link, single delay model, we investigate the impact of the loss of local stability via a Hopf bifurcation.
cs.NI
in this note we analyse various stability properties of the maxmin fair rate control protocol rcp operating with small buffers we first tackle the issue of stability for networks with arbitrary topologies we prove that the maxmin fair rcp fluid model is globally stable in the absence of propagation delays and also derive a set of conditions for local stability when arbitrary heterogeneous propagation delays are present the network delay stability result assumes that at equilibrium there is only one bottleneck link along each route lastly in the simpler setting of a single link single delay model we investigate the impact of the loss of local stability via a hopf bifurcation
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710.5831
A new search strategy for microquasar candidates using NVSS/2MASS and XMM-Newton data
Microquasars are ideal natural laboratories for understanding accretion/ejection processes, studying the physics of relativistic jets, and testing gravitational phenomena. Nevertheless, these objects are difficult to find in our Galaxy. The main goal of this work is to increase the number of known systems of this kind. We have developed an improved search strategy based on positional cross-identification with very restrictive selection criteria to find new MQs, taking advantage of more sensitive modern radio and X-ray data. We find 86 sources with positional coincidence in the NVSS/XMM catalogs at |b|<10 deg. Among them, 24 are well-known objects and the remaining 62 sources are unidentified. For the fully coincident sources, whenever possible, we analyzed color-color and hardness ratio diagrams and found that at least 3 of them display high-mass X-ray binary characteristics, making them potential microquasar candidates.
astro-ph
microquasars are ideal natural laboratories for understanding accretionejection processes studying the physics of relativistic jets and testing gravitational phenomena nevertheless these objects are difficult to find in our galaxy the main goal of this work is to increase the number of known systems of this kind we have developed an improved search strategy based on positional crossidentification with very restrictive selection criteria to find new mqs taking advantage of more sensitive modern radio and xray data we find 86 sources with positional coincidence in the nvssxmm catalogs at b10 deg among them 24 are wellknown objects and the remaining 62 sources are unidentified for the fully coincident sources whenever possible we analyzed colorcolor and hardness ratio diagrams and found that at least 3 of them display highmass xray binary characteristics making them potential microquasar candidates
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710.5832
Semiclassical Description of Exotic Nuclear Shapes
Exotic nuclear structures such as bubbles and tori are analyzed through semiclassical extended Thomas-Fermi calculations with the Skyrme force SkM$^*$. The variational equations for neutron and proton densities are solved fully self-consistently in spherical (bubbles) and cylindrical (tori) symmetries. The possible existence of bubble configurations in some astrophysical scenarios is discussed. The stability of toroidal structures against change of quadrupole moment is studied. A global minimum of the energy is found in heavy
nucl-th
exotic nuclear structures such as bubbles and tori are analyzed through semiclassical extended thomasfermi calculations with the skyrme force skm the variational equations for neutron and proton densities are solved fully selfconsistently in spherical bubbles and cylindrical tori symmetries the possible existence of bubble configurations in some astrophysical scenarios is discussed the stability of toroidal structures against change of quadrupole moment is studied a global minimum of the energy is found in heavy
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710.5833
Right-handed sneutrinos as self-interacting dark matter in supersymmetric economical 3-3-1 model
In this work we show that the supersymmetric economical SU(3)_C X SU(3)_L X U(1)_X (3-3-1) gauge model has a realistic candidate for self-interacting dark matter. In the model under consideration, the right-handed sneutrino is in bottom of the triplet, which is a singlet of the Standard Model SU(2)_L group. In addition, the right-handed sneutrino is the lightest slepton. By these properties, the right-handed sneutrino is weakly interacting with the Standard Model and stable without introduction of extra symmetry. From the Spergel-Steinhardt condition, the typical mass limit $\leq 10 $ MeV is derived. With self-interacting coupling constant fixed by supersymmetry, this limit is deduced without any approximation. The condition for thermal generated self-interacting dark matter in the Universe is also obtained.
hep-ph
in this work we show that the supersymmetric economical su3_c x su3_l x u1_x 331 gauge model has a realistic candidate for selfinteracting dark matter in the model under consideration the righthanded sneutrino is in bottom of the triplet which is a singlet of the standard model su2_l group in addition the righthanded sneutrino is the lightest slepton by these properties the righthanded sneutrino is weakly interacting with the standard model and stable without introduction of extra symmetry from the spergelsteinhardt condition the typical mass limit leq 10 mev is derived with selfinteracting coupling constant fixed by supersymmetry this limit is deduced without any approximation the condition for thermal generated selfinteracting dark matter in the universe is also obtained
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710.5834
Rheology of dilute polymer solutions with time-dependent screening of hydrodynamic interactions
The screening of hydrodynamic interactions (HI) essentially affects macroscopic properties of polymeric solutions. This screening depends not only on the polymer concentration but has a dynamic nature. In the present work, a bead-spring theory is developed, in which this phenomenon is described for solutions of nonentangled polymer coils. The equation of motion for the beads of a test polymer is solved together with the Brinkman's equation for the solvent velocity that takes into account the presence of other coils in solution. The time correlation functions for the polymer normal modes are found. A tendency to the screening of HI is demonstrated on the coil diffusion as well as on the relaxation of its internal modes. With the growing concentration of the coils they both show a transition to the exact Rouse behavior. The viscosity of the solution and some other observable quantities are calculated. As the time increaes, the time-dependent quantities change their behavior from the Rouse regime through the Zimm one again to the Rouse dynamics at long times.
cond-mat.soft
the screening of hydrodynamic interactions hi essentially affects macroscopic properties of polymeric solutions this screening depends not only on the polymer concentration but has a dynamic nature in the present work a beadspring theory is developed in which this phenomenon is described for solutions of nonentangled polymer coils the equation of motion for the beads of a test polymer is solved together with the brinkmans equation for the solvent velocity that takes into account the presence of other coils in solution the time correlation functions for the polymer normal modes are found a tendency to the screening of hi is demonstrated on the coil diffusion as well as on the relaxation of its internal modes with the growing concentration of the coils they both show a transition to the exact rouse behavior the viscosity of the solution and some other observable quantities are calculated as the time increaes the timedependent quantities change their behavior from the rouse regime through the zimm one again to the rouse dynamics at long times
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710.5835
On finite index subgroups of a universal group
The orbifold group of the Borromean rings with singular angle 90 degrees, $U$, is a universal group, because every closed oriented 3--manifold $M^{3}$ occurs as a quotient space $M^{3} = H^{3}/G$, where $G$ is a finite index subgroup of $U$. Therefore, an interesting, but quite difficult problem, is to classify the finite index subgroups of the universal group $U$. One of the purposes of this paper is to begin this classification. In particular we analyze the classification of the finite index subgroups of $U$ that are generated by rotations.
math.GT
the orbifold group of the borromean rings with singular angle 90 degrees u is a universal group because every closed oriented 3manifold m3 occurs as a quotient space m3 h3g where g is a finite index subgroup of u therefore an interesting but quite difficult problem is to classify the finite index subgroups of the universal group u one of the purposes of this paper is to begin this classification in particular we analyze the classification of the finite index subgroups of u that are generated by rotations
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710.5836
Tidal synchronization of the subdwarf B binary PG 0101+039
Tidally locked rotation is a frequently applied assumption that helps to measure masses of invisible compact companions in close binaries. The calculations of synchronization times are affected by large uncertainties in particular for stars with radiative envelopes calling for observational constraints. We aim at verifying tidally locked rotation for the binary PG 0101+039, a subdwarf B star + white dwarf binary from its tiny (0.025 %) light variations measured with the MOST satellite (Randall et al. 2005). Binary parameters were derived from the mass function, apparent rotation and surface gravity of PG 0101+039 assuming a canonical mass of 0.47 Mo and tidally locked rotation. The light curve was then synthesised and was found to match the observed amplitude well. We verified that the light variations are due to ellipsoidal deformation and that tidal synchronization is established for PG 0101+039. We conclude that this assumption should hold for all sdB binaries with orbital periods of less than half a day. Hence the masses can be derived from systems too faint to measure tiny light variations.
astro-ph
tidally locked rotation is a frequently applied assumption that helps to measure masses of invisible compact companions in close binaries the calculations of synchronization times are affected by large uncertainties in particular for stars with radiative envelopes calling for observational constraints we aim at verifying tidally locked rotation for the binary pg 0101039 a subdwarf b star white dwarf binary from its tiny 0025 light variations measured with the most satellite randall et al 2005 binary parameters were derived from the mass function apparent rotation and surface gravity of pg 0101039 assuming a canonical mass of 047 mo and tidally locked rotation the light curve was then synthesised and was found to match the observed amplitude well we verified that the light variations are due to ellipsoidal deformation and that tidal synchronization is established for pg 0101039 we conclude that this assumption should hold for all sdb binaries with orbital periods of less than half a day hence the masses can be derived from systems too faint to measure tiny light variations
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710.5837
On estimating covariances between many assets with histories of highly variable length
Quantitative portfolio allocation requires the accurate and tractable estimation of covariances between a large number of assets, whose histories can greatly vary in length. Such data are said to follow a monotone missingness pattern, under which the likelihood has a convenient factorization. Upon further assuming that asset returns are multivariate normally distributed, with histories at least as long as the total asset count, maximum likelihood (ML) estimates are easily obtained by performing repeated ordinary least squares (OLS) regressions, one for each asset. Things get more interesting when there are more assets than historical returns. OLS becomes unstable due to rank--deficient design matrices, which is called a "big p small n" problem. We explore remedies that involve making a change of basis, as in principal components or partial least squares regression, or by applying shrinkage methods like ridge regression or the lasso. This enables the estimation of covariances between large sets of assets with histories of essentially arbitrary length, and offers improvements in accuracy and interpretation. We further extend the method by showing how external factors can be incorporated. This allows for the adaptive use of factors without the restrictive assumptions common in factor models. Our methods are demonstrated on randomly generated data, and then benchmarked by the performance of balanced portfolios using real historical financial returns. An accompanying R package called monomvn, containing code implementing the estimators described herein, has been made freely available on CRAN.
stat.ME stat.AP stat.CO
quantitative portfolio allocation requires the accurate and tractable estimation of covariances between a large number of assets whose histories can greatly vary in length such data are said to follow a monotone missingness pattern under which the likelihood has a convenient factorization upon further assuming that asset returns are multivariate normally distributed with histories at least as long as the total asset count maximum likelihood ml estimates are easily obtained by performing repeated ordinary least squares ols regressions one for each asset things get more interesting when there are more assets than historical returns ols becomes unstable due to rankdeficient design matrices which is called a big p small n problem we explore remedies that involve making a change of basis as in principal components or partial least squares regression or by applying shrinkage methods like ridge regression or the lasso this enables the estimation of covariances between large sets of assets with histories of essentially arbitrary length and offers improvements in accuracy and interpretation we further extend the method by showing how external factors can be incorporated this allows for the adaptive use of factors without the restrictive assumptions common in factor models our methods are demonstrated on randomly generated data and then benchmarked by the performance of balanced portfolios using real historical financial returns an accompanying r package called monomvn containing code implementing the estimators described herein has been made freely available on cran
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710.5838
2-level fractional factorial designs which are the union of non trivial regular designs
Every fraction is a union of points, which are trivial regular fractions. To characterize non trivial decomposition, we derive a condition for the inclusion of a regular fraction as follows. Let $F = \sum_\alpha b_\alpha X^\alpha$ be the indicator polynomial of a generic fraction, see Fontana et al, JSPI 2000, 149-172. Regular fractions are characterized by $R = \frac 1l \sum_{\alpha \in \mathcal L} e_\alpha X^\alpha$, where $\alpha \mapsto e_\alpha$ is an group homeomorphism from $\mathcal L \subset \mathbb Z_2^d$ into $\{-1,+1\}$. The regular $R$ is a subset of the fraction $F$ if $FR = R$, which in turn is equivalent to $\sum_t F(t)R(t) = \sum_t R(t)$. If $\mathcal H = \{\alpha_1 >... \alpha_k\}$ is a generating set of $\mathcal L$, and $R = \frac1{2^k}(1 + e_1X^{\alpha_1}) ... (1 + e_kX^{\alpha_k})$, $e_j = \pm 1$, $j=1 ... k$, the inclusion condition in term of the $b_\alpha$'s is % \begin{equation}b_0 + e_1 b_{\alpha_1} + >... + e_1 ... e_k b_{\alpha_1 + ... + \alpha_k} = 1. \tag{*}\end{equation} % The last part of the paper will discuss some examples to investigate the practical applicability of the previous condition (*). This paper is an offspring of the Alcotra 158 EU research contract on the planning of sequential designs for sample surveys in tourism statistics.
stat.ME
every fraction is a union of points which are trivial regular fractions to characterize non trivial decomposition we derive a condition for the inclusion of a regular fraction as follows let f sum_alpha b_alpha xalpha be the indicator polynomial of a generic fraction see fontana et al jspi 2000 149172 regular fractions are characterized by r frac 1l sum_alpha in mathcal l e_alpha xalpha where alpha mapsto e_alpha is an group homeomorphism from mathcal l subset mathbb z_2d into 11 the regular r is a subset of the fraction f if fr r which in turn is equivalent to sum_t ftrt sum_t rt if mathcal h alpha_1 alpha_k is a generating set of mathcal l and r frac12k1 e_1xalpha_1 1 e_kxalpha_k e_j pm 1 j1 k the inclusion condition in term of the b_alphas is beginequationb_0 e_1 b_alpha_1 e_1 e_k b_alpha_1 alpha_k 1 tagendequation the last part of the paper will discuss some examples to investigate the practical applicability of the previous condition this paper is an offspring of the alcotra 158 eu research contract on the planning of sequential designs for sample surveys in tourism statistics
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710.5839
Algebras of unbounded operators over the ring of measurable functions and their derivations and automorphisms
In the present paper derivations and *-automorphisms of algebras of unbounded operators over the ring of measurable functions are investigated and it is shown that all L^0-linear derivations and L^{0}-linear *-automorphisms are inner. Moreover, it is proved that each L^0-linear automorphism of the algebra of all linear operators on a bo-dense submodule of a Kaplansky-Hilbert module over the ring of measurable functions is spatial.
math.FA math.OA
in the present paper derivations and automorphisms of algebras of unbounded operators over the ring of measurable functions are investigated and it is shown that all l0linear derivations and l0linear automorphisms are inner moreover it is proved that each l0linear automorphism of the algebra of all linear operators on a bodense submodule of a kaplanskyhilbert module over the ring of measurable functions is spatial
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710.584
Comment on "Pinched Flow Fractionation: Continuous Size Separation of Particles Utilizing a Laminar Flow Profile in a Pinched Microchannel"
[First paragraph] In a recent paper Yamada et al. propose the novel concept of "pinched flow fractionation" (PFF) for the continuous size separation and analysis of particles in microfabricated lab-on-a-chip devices. In their description of the basic principle they claim that especially the width of the pinched and broadened segments will affect theseparation performance. In the following we comment on the physics behind this statement.
physics.flu-dyn
first paragraph in a recent paper yamada et al propose the novel concept of pinched flow fractionation pff for the continuous size separation and analysis of particles in microfabricated labonachip devices in their description of the basic principle they claim that especially the width of the pinched and broadened segments will affect theseparation performance in the following we comment on the physics behind this statement
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710.5841
Nuclear and particle physics aspects of the 2nbb-decay of 150Nd
A discussion is given on possible realization of the Single State Dominance (SSD) hypothesis in the case of the two-neutrino double beta decay(2nbb-decay) of 150Nd with 1^- ground state of the intermediate nucleus. We conclude that the SSD hypothesis is expected to be ruled out by precision measurement of differential characteristics of this process in running NEMO 3 or planed SuperNEMO experiments unlike some unknown low-lying 1^+ state of 150Pm does exist. This problem can be solved via (d,2He) charge-exchange experiment on 150Sm. Further, we address the question about possible violation of the Pauli exclusion principle for neutrinos and its consequences for the energy distributions of the 2nbb-decay of 150Nd. This phenomenon might be a subject of interest of NEMO 3 and SuperNEMO experiments as well.
hep-ph
a discussion is given on possible realization of the single state dominance ssd hypothesis in the case of the twoneutrino double beta decay2nbbdecay of 150nd with 1 ground state of the intermediate nucleus we conclude that the ssd hypothesis is expected to be ruled out by precision measurement of differential characteristics of this process in running nemo 3 or planed supernemo experiments unlike some unknown lowlying 1 state of 150pm does exist this problem can be solved via d2he chargeexchange experiment on 150sm further we address the question about possible violation of the pauli exclusion principle for neutrinos and its consequences for the energy distributions of the 2nbbdecay of 150nd this phenomenon might be a subject of interest of nemo 3 and supernemo experiments as well
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710.5842
Fermionic systems with charge correlations on the Bethe lattice
A fermionic model, built up of q species of localized Fermi particles, interacting by charge correlations, is isomorphic to a spin-q/2 Ising model. However, the equivalence is only formal and the two systems exhibit a different physical behavior. By considering a Bethe lattice with q=1, we have exactly solved the models. There exists a critical temperature below which there is a spontaneous breakdown of the particle-hole symmetry for the first model, and of the spin symmetry for the second. While the spin system is always stable and exhibits a homogeneous ferromagnetic phase below T_{c}, the fermionic system for T<T_{c} is unstable against the formation of inhomogeneous phases with charge separation.
cond-mat.str-el cond-mat.stat-mech
a fermionic model built up of q species of localized fermi particles interacting by charge correlations is isomorphic to a spinq2 ising model however the equivalence is only formal and the two systems exhibit a different physical behavior by considering a bethe lattice with q1 we have exactly solved the models there exists a critical temperature below which there is a spontaneous breakdown of the particlehole symmetry for the first model and of the spin symmetry for the second while the spin system is always stable and exhibits a homogeneous ferromagnetic phase below t_c the fermionic system for tt_c is unstable against the formation of inhomogeneous phases with charge separation
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710.5843
Renormalization of concurrence: the application of quantum renormalization group to the quantum information systems
We have combined the idea of renormalization group and quantum information theory. We have shown how the entanglement or concurrence evolve as the size of the system being large, i.e. the finite size scaling is obtained. Moreover, It introduces how the renormalization group approach can be implemented to obtain the quantum information properties of a many body system. We have obtained the concurrence as a measure of entanglement, its derivatives and their scaling behavior versus the size of system for the one dimensional Ising model in transverse field. We have found that the derivative of concurrence between two blocks each containing half of the system size diverges at the critical point with the exponent which is directly associated with the divergence of the correlation length.
quant-ph cond-mat.str-el
we have combined the idea of renormalization group and quantum information theory we have shown how the entanglement or concurrence evolve as the size of the system being large ie the finite size scaling is obtained moreover it introduces how the renormalization group approach can be implemented to obtain the quantum information properties of a many body system we have obtained the concurrence as a measure of entanglement its derivatives and their scaling behavior versus the size of system for the one dimensional ising model in transverse field we have found that the derivative of concurrence between two blocks each containing half of the system size diverges at the critical point with the exponent which is directly associated with the divergence of the correlation length
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710.5844
Lessons from (2+1)-dimensional quantum gravity
Proposals that quantum gravity gives rise to non-commutative spacetime geometry and deformations of Poincare symmetry are examined in the context of (2+1)-dimensional quantum gravity. The results are expressed in five lessons, which summarise how the gravitational constant, Planck's constant and the cosmological constant enter the non-commutative and non-cocommutative structures arising in (2+1)-dimensional quantum gravity. It is emphasised that the much studied bicrossproduct kappa-Poincare algebra does not arise directly in (2+1)-dimensional quantum gravity.
gr-qc hep-th math-ph math.MP
proposals that quantum gravity gives rise to noncommutative spacetime geometry and deformations of poincare symmetry are examined in the context of 21dimensional quantum gravity the results are expressed in five lessons which summarise how the gravitational constant plancks constant and the cosmological constant enter the noncommutative and noncocommutative structures arising in 21dimensional quantum gravity it is emphasised that the much studied bicrossproduct kappapoincare algebra does not arise directly in 21dimensional quantum gravity
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710.5845
Sturm numbers and substitution invariance of 3iet words
In this paper, we give a necessary condition for an infinite word defined by a non-degenerate interval exchange on three intervals (3iet word) to be invariant by a substitution: a natural parameter associated to this word must be a Sturm number. We deduce some algebraic consequences from this condition concerning the incidence matrix of the associated substitution. As a by-product of our proof, we give a combinatorial characterization of 3iet words.
math.CO math.DS
in this paper we give a necessary condition for an infinite word defined by a nondegenerate interval exchange on three intervals 3iet word to be invariant by a substitution a natural parameter associated to this word must be a sturm number we deduce some algebraic consequences from this condition concerning the incidence matrix of the associated substitution as a byproduct of our proof we give a combinatorial characterization of 3iet words
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710.5846
Relations between GPDs and TMDs: model results and beyond
Comparing the respective structures of the correlators defining generalized and transverse momentum dependent parton distributions, one finds possible relations between these two objects. Although it looks like the relations found do not hold in general, we show that they can be established at least in simple spectator model calculations. In addition, we discuss these relations in the context of generalized transverse momentum dependent parton distributions.
hep-ph
comparing the respective structures of the correlators defining generalized and transverse momentum dependent parton distributions one finds possible relations between these two objects although it looks like the relations found do not hold in general we show that they can be established at least in simple spectator model calculations in addition we discuss these relations in the context of generalized transverse momentum dependent parton distributions
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710.5847
Deformed Reissner--Nordstrom solutions in noncommutative gravity
The leading order corrections to Reissner--Nordstrom solutions of the Einstein's equations on noncommutative space time have been worked out basing on a noncommutative gauge theory of gravity. From the corrcted metric the horizons have been derived and the curvature scalar is also computed. The introduction of noncommutativity leads to the removal of the coordinate singularities.
hep-th
the leading order corrections to reissnernordstrom solutions of the einsteins equations on noncommutative space time have been worked out basing on a noncommutative gauge theory of gravity from the corrcted metric the horizons have been derived and the curvature scalar is also computed the introduction of noncommutativity leads to the removal of the coordinate singularities
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710.5848
Ising model fog drip: the first two droplets
We present here a simple model describing coexistence of solid and vapour phases. The two phases are separated by an interface. We show that when the concentration of supersaturated vapour reaches the dew-point, the droplet of solid is created spontaneously on the interface, adding to it a monolayer of a visible size.
math-ph math.MP
we present here a simple model describing coexistence of solid and vapour phases the two phases are separated by an interface we show that when the concentration of supersaturated vapour reaches the dewpoint the droplet of solid is created spontaneously on the interface adding to it a monolayer of a visible size
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710.5849
Status of the EDELWEISS-2 Dark Matter Search
The Edelweiss programme is dedicated to the direct search for Dark Matter as massive weakly interacting particles (WIMPs) with Germanium cryogenic detectors operated in the Laboratoire Souterrain de Modane in the French Alps at a depth of 4800 mwe. After the initial phase Edelweiss I, which involved a total mass of 1 kg, the second step of the programme, Edelweiss II, currently operates 9 kg of detectors and an active shielding of 100 m^2 muon veto detectors and is now in its commissioning phase. The current status and performance of the Edelweiss II set-up in terms of backgrounds will be given, the underground muon flux measured with the muon veto system will be presented.
astro-ph
the edelweiss programme is dedicated to the direct search for dark matter as massive weakly interacting particles wimps with germanium cryogenic detectors operated in the laboratoire souterrain de modane in the french alps at a depth of 4800 mwe after the initial phase edelweiss i which involved a total mass of 1 kg the second step of the programme edelweiss ii currently operates 9 kg of detectors and an active shielding of 100 m2 muon veto detectors and is now in its commissioning phase the current status and performance of the edelweiss ii setup in terms of backgrounds will be given the underground muon flux measured with the muon veto system will be presented
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710.585
25-nm diamond crystals hosting single NV color centers sorted by photon-correlation near-field microscopy
Diamond nanocrystals containing highly photoluminescent color centers are attractive non-classical and near-field light sources. For near-field applications the size of the nanocrystal is crucial since it defines the optical resolution. NV (Nitrogen-Vacancy) color centers are efficiently created by proton irradiation and annealing of a nanodiamond powder. Using near-field microscopy and photon statistics measurements, we show that nanodiamond with size down to 25 nm can hold a single NV color center with bright and stable photoluminescence.
cond-mat.mtrl-sci physics.optics
diamond nanocrystals containing highly photoluminescent color centers are attractive nonclassical and nearfield light sources for nearfield applications the size of the nanocrystal is crucial since it defines the optical resolution nv nitrogenvacancy color centers are efficiently created by proton irradiation and annealing of a nanodiamond powder using nearfield microscopy and photon statistics measurements we show that nanodiamond with size down to 25 nm can hold a single nv color center with bright and stable photoluminescence
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710.5851
Realization of efficient electroabsorption using intersubband transitions in step quantum wells
We have demonstrated efficient intersubband electroabsorption in InGaAs/InAlGaAs/InAlAs step quantum wells grown by metal-organic vapor phase epitaxy (MOVPE). An absorption modulation of 6 dB at $\lambda=6.0 \mu$m due to Stark shift of the IS absorption was achieved at a low voltage swing of $\pm 0.5$ V in a multipass waveguide structure. Based on the experimental results it is estimated that an electroabsorption modulator with a low peak-to-peak voltage of $V_{pp}=0.9$ V can yield a modulation speed of $f_{3dB} \approx 120$ GHz with the present material by using a strongly confining surface plasmon waveguide of 30 $\mu$m length.
physics.optics
we have demonstrated efficient intersubband electroabsorption in ingaasinalgaasinalas step quantum wells grown by metalorganic vapor phase epitaxy movpe an absorption modulation of 6 db at lambda60 mum due to stark shift of the is absorption was achieved at a low voltage swing of pm 05 v in a multipass waveguide structure based on the experimental results it is estimated that an electroabsorption modulator with a low peaktopeak voltage of v_pp09 v can yield a modulation speed of f_3db approx 120 ghz with the present material by using a strongly confining surface plasmon waveguide of 30 mum length
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710.5852
Anderson localization in quantum chaos: scaling and universality
The one parameter scaling theory is a powerful tool to investigate Anderson localization effects in disordered systems. In this paper we show this theory can be adapted to the context of quantum chaos provided that the classical phase space is homogeneous, not mixed. The localization problem in this case is defined in momentum, not in real space. We then employ the one parameter scaling theory to: a) propose a precise characterization of the type of classical dynamics related to the Wigner-Dyson and Poisson statistics which also predicts in what situations Anderson localization corrections invalidate the relation between classical chaos and random matrix theory encoded in the Bohigas-Schmit-Giannoni conjecture, b) to identify the universality class associated with the metal-insulator transition in quantum chaos. In low dimensions it is characterized by classical superdiffusion, in higher dimensions it has in general a quantum origin as in the case of disordered systems. We illustrate these two cases by studying 1$d$ kicked rotors with non analytical potentials and a 3$d$ kicked rotor with a smooth potential.
cond-mat.dis-nn cond-mat.mes-hall
the one parameter scaling theory is a powerful tool to investigate anderson localization effects in disordered systems in this paper we show this theory can be adapted to the context of quantum chaos provided that the classical phase space is homogeneous not mixed the localization problem in this case is defined in momentum not in real space we then employ the one parameter scaling theory to a propose a precise characterization of the type of classical dynamics related to the wignerdyson and poisson statistics which also predicts in what situations anderson localization corrections invalidate the relation between classical chaos and random matrix theory encoded in the bohigasschmitgiannoni conjecture b to identify the universality class associated with the metalinsulator transition in quantum chaos in low dimensions it is characterized by classical superdiffusion in higher dimensions it has in general a quantum origin as in the case of disordered systems we illustrate these two cases by studying 1d kicked rotors with non analytical potentials and a 3d kicked rotor with a smooth potential
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