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708.3649
Relationship Between Bicomplex Generalized Analytic Functions and Solutions of the Complexified Schr\"odinger Equation
Using three different representations of the bicomplex numbers $T\cong Cl_{C}(1,0) \cong Cl_{C}(0,1)$, which is a commutative ring with zero divisors defined by $T={w_0+w_1 {i_1}+w_2{i_2}+w_3 {j} | w_0,w_1,w_2,w_3 \in{R}}$ where ${i_1^{2}}=-1, {i_2^{2}}=-1, {j^{2}}=1 and {i_1}{i_2}={j}={i_2}{i_1}$, we construct three classes of bicomplex pseudoanalytic functions. In particular, we obtain some specific systems of Vekua equations of two complex variables and we established some connections between one of these systems and the classical Vekua equations. We consider also the complexification of the real stationary two-dimensional Schr{\"o}dinger equation. With the aid of any of its particular solutions, we construct a specific bicomplex Vekua equation possessing the following special property. The scalar parts of its solutions are solutions of the original complexified Schr{\"o}dinger equation and the vectorial parts are solutions of another complexified Schr{\"o}dinger equation.
math.CV
using three different representations of the bicomplex numbers tcong cl_c10 cong cl_c01 which is a commutative ring with zero divisors defined by tw_0w_1 i_1w_2i_2w_3 j w_0w_1w_2w_3 inr where i_121 i_221 j21 and i_1i_2ji_2i_1 we construct three classes of bicomplex pseudoanalytic functions in particular we obtain some specific systems of vekua equations of two complex variables and we established some connections between one of these systems and the classical vekua equations we consider also the complexification of the real stationary twodimensional schrodinger equation with the aid of any of its particular solutions we construct a specific bicomplex vekua equation possessing the following special property the scalar parts of its solutions are solutions of the original complexified schrodinger equation and the vectorial parts are solutions of another complexified schrodinger equation
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708.365
Improved Limits on the Lepton-Flavor Violating Decays tau- --> l-l+l-
A search for the neutrinoless, lepton-flavor violating decay of the tau lepton into three charged leptons has been performed using 376 fb^{-1} of data collected at an e^+e^- center-of-mass energy around 10.58 GeV with the BaBar detector at the PEP-II storage rings. In all six decay modes considered, the numbers of events found in data are compatible with the background expectations. Upper limits on the branching fractions are set in the range (4-8) x 10^{-8} at 90% confidence level.
hep-ex
a search for the neutrinoless leptonflavor violating decay of the tau lepton into three charged leptons has been performed using 376 fb1 of data collected at an ee centerofmass energy around 1058 gev with the babar detector at the pepii storage rings in all six decay modes considered the numbers of events found in data are compatible with the background expectations upper limits on the branching fractions are set in the range 48 x 108 at 90 confidence level
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708.3651
Magnetic and thermal properties of the S = 1/2 zig-zag spin-chain compound In2VO5
Static magnetic susceptibility \chi, ac susceptibility \chi_{ac} and specific heat C versus temperature T measurements on polycrystalline samples of In2VO5 and \chi and C versus T measurements on the isostructural, nonmagnetic compound In2TiO5 are reported. A Curie-Wiess fit to the \chi(T) data above 175 K for In2VO5 indicates ferromagnetic exchange between V^{4+} (S = 1/2) moments. Below 150 K the \chi(T) data deviate from the Curie-Weiss behavior but there is no signature of any long range magnetic order down to 1.8 K. There is a cusp at 2.8 K in the zero field cooled (ZFC) \chi(T) data measured in a magnetic field of 100 Oe and the ZFC and field cooled (FC) data show a bifurcation below this temperature. The frequency dependence of the \chi_{ac}(T) data indicate that below 3 K the system is in a spin-glass state. The difference \Delta C between the heat capacity of In2VO5 and In2TiO5 shows a broad anomaly peaked at 130 K. The entropy upto 300 K is more than what is expected for S = 1/2 moments. The anomaly in \Delta C and the extra entropy suggests that there may be a structural change below 130 K in In2VO5.
cond-mat.str-el cond-mat.mtrl-sci
static magnetic susceptibility chi ac susceptibility chi_ac and specific heat c versus temperature t measurements on polycrystalline samples of in2vo5 and chi and c versus t measurements on the isostructural nonmagnetic compound in2tio5 are reported a curiewiess fit to the chit data above 175 k for in2vo5 indicates ferromagnetic exchange between v4 s 12 moments below 150 k the chit data deviate from the curieweiss behavior but there is no signature of any long range magnetic order down to 18 k there is a cusp at 28 k in the zero field cooled zfc chit data measured in a magnetic field of 100 oe and the zfc and field cooled fc data show a bifurcation below this temperature the frequency dependence of the chi_act data indicate that below 3 k the system is in a spinglass state the difference delta c between the heat capacity of in2vo5 and in2tio5 shows a broad anomaly peaked at 130 k the entropy upto 300 k is more than what is expected for s 12 moments the anomaly in delta c and the extra entropy suggests that there may be a structural change below 130 k in in2vo5
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708.3652
Extensions in FormCalc 5.3
We present a new tool for editing Feynman diagrams as well as several extensions in version 5.3 of the package FormCalc for the calculation of Feynman diagrams.
hep-ph
we present a new tool for editing feynman diagrams as well as several extensions in version 53 of the package formcalc for the calculation of feynman diagrams
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708.3653
Thermonuclear Flame Spreading on Rapidly Spinning Neutron Stars: Indications of the Coriolis Force?
Millisecond period brightness oscillations during the intensity rise of thermonuclear X-ray bursts are likely caused by an azimuthally asymmetric, expanding burning region on the stellar surface. The time evolution of the oscillation amplitude during the intensity rise encodes information on how the thermonuclear flames spread across the stellar surface. This process depends on properties of the accreted burning layer, surface fluid motions, and the surface magnetic field structure, and thus can provide insight into these stellar properties. We present two examples of bursts from different sources that show a decrease in oscillation amplitude during the intensity rise. Using theoretical modeling, we demonstrate that the observed amplitude evolution of these bursts is not well described by a uniformly expanding circular burning region. We further show that by including in our model the salient aspects of the Coriolis force (as described by Spitkovsky, Levin, and Ushomirsky) we can qualitatively reproduce the observed evolution curves. Our modeling shows that the evolutionary structure of burst oscillation amplitude is sensitive to the nature of flame spreading, while the actual amplitude values can be very useful to constrain some source parameters.
astro-ph
millisecond period brightness oscillations during the intensity rise of thermonuclear xray bursts are likely caused by an azimuthally asymmetric expanding burning region on the stellar surface the time evolution of the oscillation amplitude during the intensity rise encodes information on how the thermonuclear flames spread across the stellar surface this process depends on properties of the accreted burning layer surface fluid motions and the surface magnetic field structure and thus can provide insight into these stellar properties we present two examples of bursts from different sources that show a decrease in oscillation amplitude during the intensity rise using theoretical modeling we demonstrate that the observed amplitude evolution of these bursts is not well described by a uniformly expanding circular burning region we further show that by including in our model the salient aspects of the coriolis force as described by spitkovsky levin and ushomirsky we can qualitatively reproduce the observed evolution curves our modeling shows that the evolutionary structure of burst oscillation amplitude is sensitive to the nature of flame spreading while the actual amplitude values can be very useful to constrain some source parameters
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708.3654
Proof of Lemma 6.3 in ``The crossing number of $K_{4,n}$ on the torus and the Klein bottle"
We found that Lemma 6.3 in the paper ``The crossing number of $K_{4,n}$ on the torus and the Klein bottle" is wrong.
math.CO
we found that lemma 63 in the paper the crossing number of k_4n on the torus and the klein bottle is wrong
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708.3655
Gradient regularity for elliptic equations in the Heisenberg Group
We give dimension-free regularity conditions for a class of possibly degenerate sub-elliptic equations in the Heisenberg group exhibiting super-quadratic growth in the horizontal gradient; this solves an issue raised by Manfredi & Mingione (Math. Ann. 2007) where only dimension dependent bounds for the growth exponent are given. We also obtain explicit a priori local regularity estimates, and cover the case of the horizontal p-Laplacean operator, extending some regularity proven by Domokos & Manfredi (Cont. Math. 2005). In turn, the a priori estimates found are shown to imply the suitable local Calderon-Zygmund theory for the related class of non-homogeneous, possibly degenerate equations involving discontinuous coefficients. These last results extend to the sub-elliptic setting a few classical non-linear Euclidean results of Iwaniec and Dibenedetto & Manfredi, and to the non-linear case estimates of the same nature that were available in the sub-elliptic setting only for solutions to linear equations.
math.AP math.DG
we give dimensionfree regularity conditions for a class of possibly degenerate subelliptic equations in the heisenberg group exhibiting superquadratic growth in the horizontal gradient this solves an issue raised by manfredi mingione math ann 2007 where only dimension dependent bounds for the growth exponent are given we also obtain explicit a priori local regularity estimates and cover the case of the horizontal plaplacean operator extending some regularity proven by domokos manfredi cont math 2005 in turn the a priori estimates found are shown to imply the suitable local calderonzygmund theory for the related class of nonhomogeneous possibly degenerate equations involving discontinuous coefficients these last results extend to the subelliptic setting a few classical nonlinear euclidean results of iwaniec and dibenedetto manfredi and to the nonlinear case estimates of the same nature that were available in the subelliptic setting only for solutions to linear equations
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708.3656
Memoirs of an Early String Theorist
I worked on String Theory over a period of five years during the First String Era, the most intellectually satisfying years of my scientific life. One of the early prospectors in the String Theory Mine, I was fortunate enough to contribute to the birth of this subject, which retains after these many years, its magical hold on our imaginations and expectations.
hep-th
i worked on string theory over a period of five years during the first string era the most intellectually satisfying years of my scientific life one of the early prospectors in the string theory mine i was fortunate enough to contribute to the birth of this subject which retains after these many years its magical hold on our imaginations and expectations
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708.3657
Hyperfine spectra of trapped Bosons in optical lattices
We calculate the interaction induced inhomogeneous broadening of spectral lines in a trapped Bose gas as a function of the depth of a three-dimensional cubic optical lattice. As observed in recent experiments, we find that the terraced "wedding-cake" structure of Mott plateaus splits the spectrum into a series of discrete peaks. The spectra are extremely sensitive to density corrugations and trap anharmonicities. For example, even when the majority of the cloud is superfluid the spectrum displays discrete peaks.
cond-mat.other
we calculate the interaction induced inhomogeneous broadening of spectral lines in a trapped bose gas as a function of the depth of a threedimensional cubic optical lattice as observed in recent experiments we find that the terraced weddingcake structure of mott plateaus splits the spectrum into a series of discrete peaks the spectra are extremely sensitive to density corrugations and trap anharmonicities for example even when the majority of the cloud is superfluid the spectrum displays discrete peaks
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708.3658
Structured Near-Optimal Channel-Adapted Quantum Error Correction
We present a class of numerical algorithms which adapt a quantum error correction scheme to a channel model. Given an encoding and a channel model, it was previously shown that the quantum operation that maximizes the average entanglement fidelity may be calculated by a semidefinite program (SDP), which is a convex optimization. While optimal, this recovery operation is computationally difficult for long codes. Furthermore, the optimal recovery operation has no structure beyond the completely positive trace preserving (CPTP) constraint. We derive methods to generate structured channel-adapted error recovery operations. Specifically, each recovery operation begins with a projective error syndrome measurement. The algorithms to compute the structured recovery operations are more scalable than the SDP and yield recovery operations with an intuitive physical form. Using Lagrange duality, we derive performance bounds to certify near-optimality.
quant-ph
we present a class of numerical algorithms which adapt a quantum error correction scheme to a channel model given an encoding and a channel model it was previously shown that the quantum operation that maximizes the average entanglement fidelity may be calculated by a semidefinite program sdp which is a convex optimization while optimal this recovery operation is computationally difficult for long codes furthermore the optimal recovery operation has no structure beyond the completely positive trace preserving cptp constraint we derive methods to generate structured channeladapted error recovery operations specifically each recovery operation begins with a projective error syndrome measurement the algorithms to compute the structured recovery operations are more scalable than the sdp and yield recovery operations with an intuitive physical form using lagrange duality we derive performance bounds to certify nearoptimality
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708.3659
Asymptotics of QCD traveling waves with fluctuations and running coupling effects
Extending independently the Balitsky-Kovchegov (BK) equation to running coupling or to fluctuation effects due to Pomeron loops is known to lead in both cases to qualitative changes of the traveling-wave asymptotic solutions. In this paper we study the extension of the forward BK equation, including both running coupling and fluctuations effects, using the method developed for the fixed coupling case. We derive the exact asymptotic behavior of the probabilistic distribution of the saturation scale.
hep-ph
extending independently the balitskykovchegov bk equation to running coupling or to fluctuation effects due to pomeron loops is known to lead in both cases to qualitative changes of the travelingwave asymptotic solutions in this paper we study the extension of the forward bk equation including both running coupling and fluctuations effects using the method developed for the fixed coupling case we derive the exact asymptotic behavior of the probabilistic distribution of the saturation scale
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708.366
The nature of the dense core population in the Pipe Nebula: A survey of NH3, CCS, and HC5N molecular line emission
Recent extinction studies of the Pipe Nebula (d=130 pc) reveal many cores spanning a range in mass from 0.2 to 20.4 Msun. These dense cores were identified via their high extinction and comprise a starless population in a very early stage of development. Here we present a survey of NH3 (1,1), NH3 (2,2), CCS (2_1,1_0), and HC5N (9,8) emission toward 46 of these cores. An atlas of the 2MASS extinction maps is also presented. In total, we detect 63% of the cores in NH3 (1,1) 22% in NH3 (2,2), 28% in CCS, and 9% in HC5N emission. We find the cores are associated with dense gas (~10^4 cm-3) with 9.5 < T_k < 17 K. Compared to C18O, we find the NH3 linewidths are systematically narrower, implying that the NH3 is tracing the dense component of the gas and that these cores are relatively quiescent. We find no correlation between core linewidth and size. The derived properties of the Pipe cores are similar to cores within other low-mass star-forming regions: the only differences are that the Pipe cores have weaker NH3 emision and most show no current star formation as evidenced by the lack of embedded infrared sources. Such weak NH3 emission could arise due to low column densities and abundances or reduced excitation due to relatively low core volume densities. Either alternative implies that the cores are relatively young. Thus, the Pipe cores represent an excellent sample of dense cores in which to study the initial conditions for star formation and the earliest stages of core formation and evolution.
astro-ph
recent extinction studies of the pipe nebula d130 pc reveal many cores spanning a range in mass from 02 to 204 msun these dense cores were identified via their high extinction and comprise a starless population in a very early stage of development here we present a survey of nh3 11 nh3 22 ccs 2_11_0 and hc5n 98 emission toward 46 of these cores an atlas of the 2mass extinction maps is also presented in total we detect 63 of the cores in nh3 11 22 in nh3 22 28 in ccs and 9 in hc5n emission we find the cores are associated with dense gas 104 cm3 with 95 t_k 17 k compared to c18o we find the nh3 linewidths are systematically narrower implying that the nh3 is tracing the dense component of the gas and that these cores are relatively quiescent we find no correlation between core linewidth and size the derived properties of the pipe cores are similar to cores within other lowmass starforming regions the only differences are that the pipe cores have weaker nh3 emision and most show no current star formation as evidenced by the lack of embedded infrared sources such weak nh3 emission could arise due to low column densities and abundances or reduced excitation due to relatively low core volume densities either alternative implies that the cores are relatively young thus the pipe cores represent an excellent sample of dense cores in which to study the initial conditions for star formation and the earliest stages of core formation and evolution
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708.3661
On Kalai's conjectures concerning centrally symmetric polytopes
In 1989 Kalai stated the three conjectures A, B, C of increasing strength concerning face numbers of centrally symmetric convex polytopes. The weakest conjecture, A, became known as the ``$3^d$-conjecture''. It is well-known that the three conjectures hold in dimensions d \leq 3. We show that in dimension 4 only conjectures A and B are valid, while conjecture C fails. Furthermore, we show that both conjectures B and C fail in all dimensions d \geq 5.
math.CO math.MG
in 1989 kalai stated the three conjectures a b c of increasing strength concerning face numbers of centrally symmetric convex polytopes the weakest conjecture a became known as the 3dconjecture it is wellknown that the three conjectures hold in dimensions d leq 3 we show that in dimension 4 only conjectures a and b are valid while conjecture c fails furthermore we show that both conjectures b and c fail in all dimensions d geq 5
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708.3662
On a conjecture of Hacon and McKernan in dimension three
We prove that there exists a universal constant $r_3$ such that if $X$ is a smooth projective threefold over $\mathbb{C}$ with non-negative Kodaira dimension, then the linear system $|r K_X|$ admits a fibration that is birational to the Iitaka fibration as soon as $r \geq r_3$ and sufficiently divisible. This gives an affirmative answer to a conjecture of Hacon and McKernan in the case of threefolds. Viehweg and Zhang have posted a stronger result along these lines using different methods.
math.AG
we prove that there exists a universal constant r_3 such that if x is a smooth projective threefold over mathbbc with nonnegative kodaira dimension then the linear system r k_x admits a fibration that is birational to the iitaka fibration as soon as r geq r_3 and sufficiently divisible this gives an affirmative answer to a conjecture of hacon and mckernan in the case of threefolds viehweg and zhang have posted a stronger result along these lines using different methods
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708.3663
How a liquid becomes a glass both on cooling and on heating
The onset of structural arrest and glass formation in a concentrated suspension of silica nanoparticles in a water-lutidine binary mixture near its consolute point is studied by exploiting the near-critical fluid degrees of freedom to control the strength of an attraction between particles and multispeckle x-ray photon correlation spectroscopy to determine the particles' collective dynamics. This model system undergoes a glass transition both on cooling and on heating, and the intermediate liquid realizes unusual logarithmic relaxations. How vitrification occurs for the two different glass transitions is characterized in detail and comparisons are drawn to recent theoretical predictions for glass formation in systems with attractive interactions.
cond-mat.soft
the onset of structural arrest and glass formation in a concentrated suspension of silica nanoparticles in a waterlutidine binary mixture near its consolute point is studied by exploiting the nearcritical fluid degrees of freedom to control the strength of an attraction between particles and multispeckle xray photon correlation spectroscopy to determine the particles collective dynamics this model system undergoes a glass transition both on cooling and on heating and the intermediate liquid realizes unusual logarithmic relaxations how vitrification occurs for the two different glass transitions is characterized in detail and comparisons are drawn to recent theoretical predictions for glass formation in systems with attractive interactions
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708.3664
Commutator maps, measure preservation, and T-systems
Let G be a finite simple group. We show that the commutator map $a : G \times G \to G$ is almost equidistributed as the order of G goes to infinity. This somewhat surprising result has many applications. It shows that for a subset X of G we have $a^{-1}(X)/|G|^2 = |X|/|G| + o(1)$, namely $a$ is almost measure preserving. From this we deduce that almost all elements $g \in G$ can be expressed as commutators $g = [x,y]$ where x,y generate G. This enables us to solve some open problems regarding T-systems and the Product Replacement Algorithm (PRA) graph. We show that the number of T-systems in G with two generators tends to infinity as the order of G goes to infinity. This settles a conjecture of Guralnick and Pak. A similar result follows for the number of connected components of the PRA graph of G with two generators. Some of our results apply for more general finite groups, and more general word maps. Our methods are based on representation theory, combining classical character theory with recent results on character degrees and values in finite simple groups. In particular the so called Witten zeta function plays a key role in the proofs.
math.GR
let g be a finite simple group we show that the commutator map a g times g to g is almost equidistributed as the order of g goes to infinity this somewhat surprising result has many applications it shows that for a subset x of g we have a1xg2 xg o1 namely a is almost measure preserving from this we deduce that almost all elements g in g can be expressed as commutators g xy where xy generate g this enables us to solve some open problems regarding tsystems and the product replacement algorithm pra graph we show that the number of tsystems in g with two generators tends to infinity as the order of g goes to infinity this settles a conjecture of guralnick and pak a similar result follows for the number of connected components of the pra graph of g with two generators some of our results apply for more general finite groups and more general word maps our methods are based on representation theory combining classical character theory with recent results on character degrees and values in finite simple groups in particular the so called witten zeta function plays a key role in the proofs
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708.3665
Symmetry of Lepton Mixing
Neutrino mixing is studied from a symmetry perspective, both bottom-up and top-down. In the bottom-up approach, we start from the tri-bimaximal mixing, or one of its three partial patterns, and construct a list of horizontal symmetry groups capable of reproducing the mixng without adjustment of parameters. This list, labeled by an integer $n\ge 3$, is explicitly calculated for $n=3$. In the top-down approach, we start from any finite group possessing a three-dimensional irreducible representation and an order-2 element, give a recipe to determine what mixing pattern it contains, and how to construct a dynamical model to reveal a particular mixing. Finally, we point out that if quark mixing is controlled by symmetry in this way, then there is an exciting possibility to determine most of the CKM mixing parameters by symmetry alone.
hep-ph
neutrino mixing is studied from a symmetry perspective both bottomup and topdown in the bottomup approach we start from the tribimaximal mixing or one of its three partial patterns and construct a list of horizontal symmetry groups capable of reproducing the mixng without adjustment of parameters this list labeled by an integer nge 3 is explicitly calculated for n3 in the topdown approach we start from any finite group possessing a threedimensional irreducible representation and an order2 element give a recipe to determine what mixing pattern it contains and how to construct a dynamical model to reveal a particular mixing finally we point out that if quark mixing is controlled by symmetry in this way then there is an exciting possibility to determine most of the ckm mixing parameters by symmetry alone
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708.3666
Jahn-Teller effect versus Hund's rule coupling in C60N-
We propose variational states for the ground state and the low-energy collective rotator excitations in negatively charged C60N- ions (N=1...5). The approach includes the linear electron-phonon coupling and the Coulomb interaction on the same level. The electron-phonon coupling is treated within the effective mode approximation (EMA) which yields the linear t_{1u} x H_g Jahn-Teller problem whereas the Coulomb interaction gives rise to Hund's rule coupling for N=2,3,4. The Hamiltonian has accidental SO(3) symmetry which allows an elegant formulation in terms of angular momenta. Trial states are constructed from coherent states and using projection operators onto angular momentum subspaces which results in good variational states for the complete parameter range. The evaluation of the corresponding energies is to a large extent analytical. We use the approach for a detailed analysis of the competition between Jahn-Teller effect and Hund's rule coupling, which determines the spin state for N=2,3,4. We calculate the low-spin/high-spin gap for N=2,3,4 as a function of the Hund's rule coupling constant J. We find that the experimentally measured gaps suggest a coupling constant in the range J=60-80meV. Using a finite value for J, we recalculate the ground state energies of the C60N- ions and find that the Jahn-Teller energy gain is partly counterbalanced by the Hund's rule coupling. In particular, the ground state energies for N=2,3,4 are almost equal.
cond-mat.supr-con
we propose variational states for the ground state and the lowenergy collective rotator excitations in negatively charged c60n ions n15 the approach includes the linear electronphonon coupling and the coulomb interaction on the same level the electronphonon coupling is treated within the effective mode approximation ema which yields the linear t_1u x h_g jahnteller problem whereas the coulomb interaction gives rise to hunds rule coupling for n234 the hamiltonian has accidental so3 symmetry which allows an elegant formulation in terms of angular momenta trial states are constructed from coherent states and using projection operators onto angular momentum subspaces which results in good variational states for the complete parameter range the evaluation of the corresponding energies is to a large extent analytical we use the approach for a detailed analysis of the competition between jahnteller effect and hunds rule coupling which determines the spin state for n234 we calculate the lowspinhighspin gap for n234 as a function of the hunds rule coupling constant j we find that the experimentally measured gaps suggest a coupling constant in the range j6080mev using a finite value for j we recalculate the ground state energies of the c60n ions and find that the jahnteller energy gain is partly counterbalanced by the hunds rule coupling in particular the ground state energies for n234 are almost equal
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708.3667
A note on the convergence of renewal and regenerative processes to a Brownian bridge
The standard functional central limit theorem for a renewal process with finite mean and variance, results in a Brownian motion limit. This note shows how to obtain a Brownian bridge process by a direct procedure that does not involve conditioning. Several examples are also considered.
math.PR
the standard functional central limit theorem for a renewal process with finite mean and variance results in a brownian motion limit this note shows how to obtain a brownian bridge process by a direct procedure that does not involve conditioning several examples are also considered
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708.3668
A simple proof of the algebraic version of a conjecture by Vogan
In a recent manuscript, D.Vogan conjectures that four canonical globalizations of Harish-Chandra modules commute with certain n-cohomology groups. In this article we prove that Vogan's conjecture holds for one of the globalizations if and only if it holds for the dual. Using a previously published result of one of the authors, which establishes the conjecture for the minimal globalization, we can therefore deduce Vogan's conjecture for the maximal globalization.
math.RT math.SP
in a recent manuscript dvogan conjectures that four canonical globalizations of harishchandra modules commute with certain ncohomology groups in this article we prove that vogans conjecture holds for one of the globalizations if and only if it holds for the dual using a previously published result of one of the authors which establishes the conjecture for the minimal globalization we can therefore deduce vogans conjecture for the maximal globalization
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708.3669
Band-Gap Engineering of Phononic Crystals: A Computational Survey of Two-Dimensional Systems
We present graphic results with high-levels of abstraction to desribe the basic principles and rules of thumb for acoustic or phononic band-gap engineering. We use these rules for developing an improved machien mount for damping acoustic vibrations, a phononic lens and a frequency selective filter in the acoustic regime.
cond-mat.mtrl-sci
we present graphic results with highlevels of abstraction to desribe the basic principles and rules of thumb for acoustic or phononic bandgap engineering we use these rules for developing an improved machien mount for damping acoustic vibrations a phononic lens and a frequency selective filter in the acoustic regime
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708.367
A covariant entropy conjecture on cosmological dynamical horizon
We here propose a covariant entropy conjecture on cosmological dynamical horizon. After the formulation of our conjecture, we test its validity in adiabatically expanding universes with open, flat and closed spatial geometry, where our conjecture can also be viewed as a cosmological version of the generalized second law of thermodynamics in some sense.
hep-th astro-ph gr-qc
we here propose a covariant entropy conjecture on cosmological dynamical horizon after the formulation of our conjecture we test its validity in adiabatically expanding universes with open flat and closed spatial geometry where our conjecture can also be viewed as a cosmological version of the generalized second law of thermodynamics in some sense
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708.3671
A Multiwavelength Analysis of the Strong Lensing Cluster RCS 022434-0002.5 at z=0.778
We present the results of two (101 ks total) Chandra observations of the z=0.778 optically selected lensing cluster RCS022434-0002.5, along with weak lensing and dynamical analyses of this object. An X-ray spectrum extracted within R(2500) (362 h(70)^(-1) kpc) results in an integrated cluster temperature of 5.1 (+0.9,-0.5) keV. The surface brightness profile of RCS022434-0002.5 indicates the presence of a slight excess of emission in the core. A hardness ratio image of this object reveals that this central emission is primarily produced by soft X-rays. Further investigation yields a cluster cooling time of 3.3 times 10^9 years, which is less than half of the age of the universe at this redshift given the current LCDM cosmology. A weak lensing analysis is performed using HST images, and our weak lensing mass estimate is found to be in good agreement with the X-ray determined mass of the cluster. Spectroscopic analysis reveals that RCS022434-0002.5 has a velocity dispersion of 900 +/- 180 km/s, consistent with its X-ray temperature. The core gas mass fraction of RCS022434-0002.5 is, however, found to be three times lower than expected universal values. The radial distribution of X-ray point sources within R(200) of this cluster peaks at ~0.7 R(200), possibly indicating that the cluster potential is influencing AGN activity at that radius. Correlations between X-ray and radio (VLA) point source positions are also examined.
astro-ph
we present the results of two 101 ks total chandra observations of the z0778 optically selected lensing cluster rcs02243400025 along with weak lensing and dynamical analyses of this object an xray spectrum extracted within r2500 362 h701 kpc results in an integrated cluster temperature of 51 0905 kev the surface brightness profile of rcs02243400025 indicates the presence of a slight excess of emission in the core a hardness ratio image of this object reveals that this central emission is primarily produced by soft xrays further investigation yields a cluster cooling time of 33 times 109 years which is less than half of the age of the universe at this redshift given the current lcdm cosmology a weak lensing analysis is performed using hst images and our weak lensing mass estimate is found to be in good agreement with the xray determined mass of the cluster spectroscopic analysis reveals that rcs02243400025 has a velocity dispersion of 900 180 kms consistent with its xray temperature the core gas mass fraction of rcs02243400025 is however found to be three times lower than expected universal values the radial distribution of xray point sources within r200 of this cluster peaks at 07 r200 possibly indicating that the cluster potential is influencing agn activity at that radius correlations between xray and radio vla point source positions are also examined
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708.3672
Reply to Comment: S. Das Sarma et al., arXiv:0708.3239
The authors of the Comment ascribe us claims never made while moderating their own previous unsubstantiated statements.
cond-mat.mes-hall cond-mat.mtrl-sci
the authors of the comment ascribe us claims never made while moderating their own previous unsubstantiated statements
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708.3673
Exploiting scale dependence in cosmological averaging
We study the role of scale dependence in the Buchert averaging method, using the flat Lemaitre-Tolman-Bondi model as a testing ground. Within this model, a single averaging scale gives too coarse predictions, but by replacing it with the distance of the objects R(z) for each redshift z, we find an O(1%) precision at z<2 in the averaged luminosity and angular diameter distances compared to their exact expressions. At low redshifts, we show the improvement for generic inhomogeneity profiles, and our numerical computations further verify it up to redshifts z~2. At higher redshifts, the method breaks down due to its inability to capture the time evolution of the inhomogeneities. We also demonstrate that the running smoothing scale R(z) can mimic acceleration, suggesting it could be at least as important as the backreaction in explaining dark energy as an inhomogeneity induced illusion.
astro-ph
we study the role of scale dependence in the buchert averaging method using the flat lemaitretolmanbondi model as a testing ground within this model a single averaging scale gives too coarse predictions but by replacing it with the distance of the objects rz for each redshift z we find an o1 precision at z2 in the averaged luminosity and angular diameter distances compared to their exact expressions at low redshifts we show the improvement for generic inhomogeneity profiles and our numerical computations further verify it up to redshifts z2 at higher redshifts the method breaks down due to its inability to capture the time evolution of the inhomogeneities we also demonstrate that the running smoothing scale rz can mimic acceleration suggesting it could be at least as important as the backreaction in explaining dark energy as an inhomogeneity induced illusion
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708.3674
Power-law expansion cosmology in Schr\"odinger-type formulation
We investigate non-linear Schr\"{o}dinger-type formulation of cosmology of which our cosmological system is a general relativistic FRLW universe containing canonical scalar field under arbitrary potential and a barotropic fluid with arbitrary spatial curvatures. We extend the formulation to include phantom field case and we have found that Schr\"{o}dinger wave function in this formulation is generally non-normalizable. Assuming power-law expansion, $a \sim t^q$, we obtain scalar field potential as function of time. The corresponding quantities in Schr\"{o}dinger-type formulation such as Schr\"{o}dinger total energy, Schr\"{o}dinger potential and wave function are also presented.
gr-qc astro-ph hep-th quant-ph
we investigate nonlinear schrodingertype formulation of cosmology of which our cosmological system is a general relativistic frlw universe containing canonical scalar field under arbitrary potential and a barotropic fluid with arbitrary spatial curvatures we extend the formulation to include phantom field case and we have found that schrodinger wave function in this formulation is generally nonnormalizable assuming powerlaw expansion a sim tq we obtain scalar field potential as function of time the corresponding quantities in schrodingertype formulation such as schrodinger total energy schrodinger potential and wave function are also presented
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708.3675
The Origin of Solar Activity in the Tachocline
Solar active regions, produced by the emergence of tubes of strong magnetic field in the photosphere, are restricted to within 35 degrees of the solar equator. The nature of the dynamo processes that create and renew these fields, and are therefore responsible for solar magnetic phenomena, are not well understood. We analyze the magneto-rotational stability of the solar tachocline for general field geometry. This thin region of strong radial and latitudinal differential rotation, between the radiative and convective zones, is unstable at latitudes above 37 degrees, yet is stable closer to the equator. We propose that small-scale magneto-rotational turbulence prevents coherent magnetic dynamo action in the tachocline except in the vicinity of the equator, thus explaining the latitudinal restriction of active regions. Tying the magnetic dynamo to the tachocline elucidates the physical conditions and processes relevant to solar magnetism.
astro-ph
solar active regions produced by the emergence of tubes of strong magnetic field in the photosphere are restricted to within 35 degrees of the solar equator the nature of the dynamo processes that create and renew these fields and are therefore responsible for solar magnetic phenomena are not well understood we analyze the magnetorotational stability of the solar tachocline for general field geometry this thin region of strong radial and latitudinal differential rotation between the radiative and convective zones is unstable at latitudes above 37 degrees yet is stable closer to the equator we propose that smallscale magnetorotational turbulence prevents coherent magnetic dynamo action in the tachocline except in the vicinity of the equator thus explaining the latitudinal restriction of active regions tying the magnetic dynamo to the tachocline elucidates the physical conditions and processes relevant to solar magnetism
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708.3676
On the Cauchy problem for higher-order nonlinear dispersive equations
We study a class of higher-order KdV equations. We show that the associated initial value problem is well posed in weighted Besov and Sobolev spaces for small initial data. We also prove ill-posedness results when in H^s(\R), for any real s.
math.AP
we study a class of higherorder kdv equations we show that the associated initial value problem is well posed in weighted besov and sobolev spaces for small initial data we also prove illposedness results when in hsr for any real s
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708.3677
Comment on "Limits on the Time Variation of the Electromagnetic Fine-Structure Constant in the Low Energy Limit from Absorption Lines in the Spectra of Distant Quasars"
In their Letter [Phys. Rev. Lett. 92, 121302 (2004)] (also [Astron. Astrophys. 417, 853 (2004)]), Srianand et al. analysed optical spectra of heavy-element species in 23 absorption systems along background quasar sight-lines, reporting limits on relative variations in the fine-structure constant: da/a=(-0.06+/-0.06) x 10^{-5}. Here we demonstrate basic flaws in their analysis, using the same data and absorption profile fits, which led to spurious values of da/a and significantly underestimated uncertainties. We conclude that these data and fits offer no stringent test of previous evidence for a varying alpha. In their Reply (arXiv:0711.1742) to this Comment, Srianand et al. state or argue several points regarding their original analysis and our new analysis. We discuss these points here, dismissing all of them because they are demonstrably incorrect or because they rely on a flawed application of simple statistical arguments.
astro-ph hep-th physics.atom-ph
in their letter phys rev lett 92 121302 2004 also astron astrophys 417 853 2004 srianand et al analysed optical spectra of heavyelement species in 23 absorption systems along background quasar sightlines reporting limits on relative variations in the finestructure constant daa006006 x 105 here we demonstrate basic flaws in their analysis using the same data and absorption profile fits which led to spurious values of daa and significantly underestimated uncertainties we conclude that these data and fits offer no stringent test of previous evidence for a varying alpha in their reply arxiv07111742 to this comment srianand et al state or argue several points regarding their original analysis and our new analysis we discuss these points here dismissing all of them because they are demonstrably incorrect or because they rely on a flawed application of simple statistical arguments
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708.3678
A large population of mid-infrared selected, obscured active galaxies in the Bootes field
We identify a population of 640 obscured and 839 unobscured AGNs at redshifts 0.7<z<~3 using multiwavelength observations of the 9 deg^2 NOAO Deep Wide-Field Survey (NDWFS) region in Bootes. We select AGNs on the basis of Spitzer IRAC colors obtained by the IRAC Shallow Survey. Redshifts are obtained from optical spectroscopy or photometric redshift estimators. We classify the IR-selected AGNs as IRAGN 1 (unobscured) and IRAGN 2 (obscured) using a simple criterion based on the observed optical to mid-IR color, with a selection boundary of R-[4.5]=6.1, where R and [4.5] are the Vega magnitudes in the R and IRAC 4.5 micron bands, respectively. We verify this selection using X-ray stacking analyses with data from the Chandra XBootes survey, as well as optical photometry from NDWFS and spectroscopy from MMT/AGES. We show that (1) these sources are indeed AGNs, and (2) the optical/IR color selection separates obscured sources (with average N_H~3x10^22 cm^-2 obtained from X-ray hardness ratios, and optical colors and morphologies typical of galaxies) and unobscured sources (with no X-ray absorption, and quasar colors and morphologies), with a reliability of >~80%. The observed numbers of IRAGNs are comparable to predictions from previous X-ray, optical, and IR luminosity functions, for the given redshifts and IRAC flux limits. We observe a bimodal distribution in R-[4.5] color, suggesting that luminous IR-selected AGNs have either low or significant dust extinction, which may have implications for models of AGN obscuration.
astro-ph
we identify a population of 640 obscured and 839 unobscured agns at redshifts 07z3 using multiwavelength observations of the 9 deg2 noao deep widefield survey ndwfs region in bootes we select agns on the basis of spitzer irac colors obtained by the irac shallow survey redshifts are obtained from optical spectroscopy or photometric redshift estimators we classify the irselected agns as iragn 1 unobscured and iragn 2 obscured using a simple criterion based on the observed optical to midir color with a selection boundary of r4561 where r and 45 are the vega magnitudes in the r and irac 45 micron bands respectively we verify this selection using xray stacking analyses with data from the chandra xbootes survey as well as optical photometry from ndwfs and spectroscopy from mmtages we show that 1 these sources are indeed agns and 2 the opticalir color selection separates obscured sources with average n_h3x1022 cm2 obtained from xray hardness ratios and optical colors and morphologies typical of galaxies and unobscured sources with no xray absorption and quasar colors and morphologies with a reliability of 80 the observed numbers of iragns are comparable to predictions from previous xray optical and ir luminosity functions for the given redshifts and irac flux limits we observe a bimodal distribution in r45 color suggesting that luminous irselected agns have either low or significant dust extinction which may have implications for models of agn obscuration
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708.3679
Adiabatic cross-polarization
A scheme of adiabatic cross-polarization is described. It is based on demagnetization - remagnetization, when the Zeeman order of abundant nuclei in the laboratory frame is first adiabatically converted into the dipolar order, and then, into the Zeeman order of rare nuclei. The scheme, implemented with two low-power frequency-sweeping pulses, is very efficient for static samples and can significantly increase polarization of rare nuclei, compared to the conventional Hartmann-Hahn cross-polarization. The experimental examples are presented for solids, liquid crystal, and molecules in a liquid-crystalline solvent.
cond-mat.other
a scheme of adiabatic crosspolarization is described it is based on demagnetization remagnetization when the zeeman order of abundant nuclei in the laboratory frame is first adiabatically converted into the dipolar order and then into the zeeman order of rare nuclei the scheme implemented with two lowpower frequencysweeping pulses is very efficient for static samples and can significantly increase polarization of rare nuclei compared to the conventional hartmannhahn crosspolarization the experimental examples are presented for solids liquid crystal and molecules in a liquidcrystalline solvent
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708.368
Black Holes, Entropy, and Information
Black holes are a continuing source of mystery. Although their classical properties have been understood since the 1970's, their quantum properties raise some of the deepest questions in theoretical physics. Some of these questions have recently been answered using string theory. I will review these fundamental questions, and the aspects of string theory needed to answer them. I will then explain the recent developments and new insights into black holes that they provide. Some remaining puzzles are mentioned in the conclusion.
astro-ph gr-qc
black holes are a continuing source of mystery although their classical properties have been understood since the 1970s their quantum properties raise some of the deepest questions in theoretical physics some of these questions have recently been answered using string theory i will review these fundamental questions and the aspects of string theory needed to answer them i will then explain the recent developments and new insights into black holes that they provide some remaining puzzles are mentioned in the conclusion
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708.3681
The family of analytic Poisson brackets for the Camassa--Holm hierarchy
We consider the integrable Camassa--Holm hierarchy on the line with positive initial data rapidly decaying at infinity. It is known that flows of the hierarchy can be formulated in a Hamiltonian form using two compatible Poisson brackets. In this note we propose a new approach to Hamiltonian theory of the CH equation. In terms of associated Riemann surface and the Weyl function we write an analytic formula which produces a family of compatible Poisson brackets. The formula includes an entire function $f(z)$ as a parameter. The simplest choice $f(z)=1$ or $f(z)=z$ corresponds to the rational or trigonometric solutions of the Yang-Baxter equation and produces two original Poisson brackets. All other Poisson brackets corresponding to other choices of the function $f(z)$ are new.
math-ph math.AG math.MP
we consider the integrable camassaholm hierarchy on the line with positive initial data rapidly decaying at infinity it is known that flows of the hierarchy can be formulated in a hamiltonian form using two compatible poisson brackets in this note we propose a new approach to hamiltonian theory of the ch equation in terms of associated riemann surface and the weyl function we write an analytic formula which produces a family of compatible poisson brackets the formula includes an entire function fz as a parameter the simplest choice fz1 or fzz corresponds to the rational or trigonometric solutions of the yangbaxter equation and produces two original poisson brackets all other poisson brackets corresponding to other choices of the function fz are new
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708.3682
Entanglement in Disordered Systems at Criticality
Entanglement is a physical resource of a quantum system just like mass, charge or energy. Moreover it is an essential tool for many purposes of nowadays quantum information processing, e.g. quantum teleportation, quantum cryptography or quantum computation. In this work we investigate an extended system of N qubits. In our system a qubit is the absence or presence of an electron at a site of a tight-binding system. Several measures of entanglement between a given qubit and the rest of the system and also the entanglement between two qubits and the rest of the system is calculated in a one-electron picture in the presence of disorder. We invoke the power law band random matrix model which even in one dimension is able to produce multifractal states that fluctuate at all length scales. The concurrence, the tangle and the entanglement entropy all show interesting scaling properties.
cond-mat.dis-nn quant-ph
entanglement is a physical resource of a quantum system just like mass charge or energy moreover it is an essential tool for many purposes of nowadays quantum information processing eg quantum teleportation quantum cryptography or quantum computation in this work we investigate an extended system of n qubits in our system a qubit is the absence or presence of an electron at a site of a tightbinding system several measures of entanglement between a given qubit and the rest of the system and also the entanglement between two qubits and the rest of the system is calculated in a oneelectron picture in the presence of disorder we invoke the power law band random matrix model which even in one dimension is able to produce multifractal states that fluctuate at all length scales the concurrence the tangle and the entanglement entropy all show interesting scaling properties
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708.3683
Formal equivalence between Tsallis and extended Boltzmann-Gibbs statistics
A formal correspondence between the q-distribution obtained from the Tsallis entropy and non-maxwellian distributions obtained from the Boltzmann-Gibbs entropy is afforded.
quant-ph
a formal correspondence between the qdistribution obtained from the tsallis entropy and nonmaxwellian distributions obtained from the boltzmanngibbs entropy is afforded
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708.3684
The influence of cluster emission and the symmetry energy on neutron-proton spectral double ratios
Emissions of free neutrons and protons from the central collisions of 124Sn+124Sn and 112Sn+112Sn reactions are simulated using the Improved Quantum Molecular Dynamics model with two different density dependence of the symmetry energy in the nuclear equation of state. The constructed double ratios of the neutron to proton ratios of the two reaction systems are found to be sensitive to the symmetry terms in the EOS. The effect of cluster formation is examined and found to affect the double ratios mainly in the low energy region. In order to extract better information on symmetry energy with transport models, it is therefore important to have accurate data in the high energy region which also is affected minimally by sequential decays.
nucl-th nucl-ex
emissions of free neutrons and protons from the central collisions of 124sn124sn and 112sn112sn reactions are simulated using the improved quantum molecular dynamics model with two different density dependence of the symmetry energy in the nuclear equation of state the constructed double ratios of the neutron to proton ratios of the two reaction systems are found to be sensitive to the symmetry terms in the eos the effect of cluster formation is examined and found to affect the double ratios mainly in the low energy region in order to extract better information on symmetry energy with transport models it is therefore important to have accurate data in the high energy region which also is affected minimally by sequential decays
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708.3685
On representations of certain pseudo-Anosov maps of Riemann surfaces with punctures
Let $S$ be a Riemann surface of type $(p,n)$ with $3p+n>4$ and $n\geq 1$. Let $\alpha_1,\alpha_2\subset S$ be two simple closed geodesics such that $\{\alpha_1, \alpha_2\}$ fills $S$. It was shown by Thurston that most maps obtained through Dehn twists along $\alpha_1$ and $\alpha_2$ are pseudo-Anosov. Let $a$ be a puncture. In this paper, we study the family $\mathcal{F}(S,a)$ of pseudo-Anosov maps on $S$ that projects to the trivial map as $a$ is filled in, and show that there are infinitely many elements in $\mathcal{F}(S,a)$ that cannot be obtained from Dehn twists along two filling geodesics. We further characterize all elements in $\mathcal{F}(S,a)$ that can be constructed by two filling geodesics. Finally, for any point $b\in S$, we obtain a family $\mathcal{H}$ of pseudo-Anosov maps on $S\backslash \{b\}$ that is not obtained from Thurston's construction and projects to an element $\chi\in \mathcal{F}(S,a)$ as $b$ is filled in, some properties of elements in $\mathcal{H}$ are also discussed.
math.CV math.GT
let s be a riemann surface of type pn with 3pn4 and ngeq 1 let alpha_1alpha_2subset s be two simple closed geodesics such that alpha_1 alpha_2 fills s it was shown by thurston that most maps obtained through dehn twists along alpha_1 and alpha_2 are pseudoanosov let a be a puncture in this paper we study the family mathcalfsa of pseudoanosov maps on s that projects to the trivial map as a is filled in and show that there are infinitely many elements in mathcalfsa that cannot be obtained from dehn twists along two filling geodesics we further characterize all elements in mathcalfsa that can be constructed by two filling geodesics finally for any point bin s we obtain a family mathcalh of pseudoanosov maps on sbackslash b that is not obtained from thurstons construction and projects to an element chiin mathcalfsa as b is filled in some properties of elements in mathcalh are also discussed
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708.3686
Accuracy of a teleported trapped field state inside a single bimodal cavity
We propose a simplified scheme to teleport a superposition of coherent states from one mode to another of the same bimodal lossy cavity. Based on current experimental capabilities, we present a calculation of the fidelity that can be achieved, demonstrating accurate teleportation if the mean photon number of each mode is at most 1.5. Our scheme applies as well for teleportation of coherent states from one mode of a cavity to another mode of a second cavity, both cavities embedded in a common reservoir.
quant-ph
we propose a simplified scheme to teleport a superposition of coherent states from one mode to another of the same bimodal lossy cavity based on current experimental capabilities we present a calculation of the fidelity that can be achieved demonstrating accurate teleportation if the mean photon number of each mode is at most 15 our scheme applies as well for teleportation of coherent states from one mode of a cavity to another mode of a second cavity both cavities embedded in a common reservoir
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708.3687
Multiplicity in Supersymmetric Spin Chains
We discuss a simple procedure for obtaining new integrable spin chains from old by replacing each single state of the original model by some collection of states. This works whenever the Lax matrix of the chain has a certain form. The simplest example is the su(n) XX model. We apply the techniques of the nested algebraic Bethe ansatz to solve such systems, in the bosonic and supersymmetric cases.
math-ph math.MP
we discuss a simple procedure for obtaining new integrable spin chains from old by replacing each single state of the original model by some collection of states this works whenever the lax matrix of the chain has a certain form the simplest example is the sun xx model we apply the techniques of the nested algebraic bethe ansatz to solve such systems in the bosonic and supersymmetric cases
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708.3688
Localization and delocalization errors in density functional theory and implications for band-gap prediction
The band-gap problem and other systematic failures of approximate functionals are explained from an analysis of total energy for fractional charges. The deviation from the correct intrinsic linear behavior in finite systems leads to delocalization and localization errors in large or bulk systems. Functionals whose energy is convex for fractional charges such as LDA display an incorrect apparent linearity in the bulk limit, due to the delocalization error. Concave functionals also have an incorrect apparent linearity in the bulk calculation, due to the localization error and imposed symmetry. This resolves an important paradox and opens the possibility to obtain accurate band-gaps from DFT.
cond-mat.mtrl-sci
the bandgap problem and other systematic failures of approximate functionals are explained from an analysis of total energy for fractional charges the deviation from the correct intrinsic linear behavior in finite systems leads to delocalization and localization errors in large or bulk systems functionals whose energy is convex for fractional charges such as lda display an incorrect apparent linearity in the bulk limit due to the delocalization error concave functionals also have an incorrect apparent linearity in the bulk calculation due to the localization error and imposed symmetry this resolves an important paradox and opens the possibility to obtain accurate bandgaps from dft
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708.3689
Arithmetic structures in smooth subsets of F_p
Fix integers a_1,...,a_d satisfying a_1 + ... + a_d = 0. Suppose that f : Z_N -> [0,1], where N is prime. We show that if f is ``smooth enough'' then we can bound from below the sum of f(x_1)...f(x_d) over all solutions (x_1,...,x_d) in Z_N to a_1 x_1 + ... + a_d x_d == 0 (mod N). Note that d = 3 and a_1 = a_2 = 1 and a_3 = -2 is the case where x_1,x_2,x_3 are in arithmetic progression. By ``smooth enough'' we mean that the sum of squares of the lower order Fourier coefficients of f is ``small'', a property shared by many naturally-occurring functions, among them certain ones supported on sumsets and on certain types of pseudoprimes. The paper can be thought of as a generalization of another result of the author, which dealt with a F_p^n analogue of the problem. It appears that the method in that paper, and to a more limited extent the present paper, uses ideas similar to those of B. Green's ``arithmetic regularity lemma'', as we explain in the paper.
math.NT math.CO
fix integers a_1a_d satisfying a_1 a_d 0 suppose that f z_n 01 where n is prime we show that if f is smooth enough then we can bound from below the sum of fx_1fx_d over all solutions x_1x_d in z_n to a_1 x_1 a_d x_d 0 mod n note that d 3 and a_1 a_2 1 and a_3 2 is the case where x_1x_2x_3 are in arithmetic progression by smooth enough we mean that the sum of squares of the lower order fourier coefficients of f is small a property shared by many naturallyoccurring functions among them certain ones supported on sumsets and on certain types of pseudoprimes the paper can be thought of as a generalization of another result of the author which dealt with a f_pn analogue of the problem it appears that the method in that paper and to a more limited extent the present paper uses ideas similar to those of b greens arithmetic regularity lemma as we explain in the paper
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708.369
Two-dimensional quantum-dot helium in a magnetic field: Variational theory
A trial wave function for two-dimensional quantum dot helium in an arbitrary perpendicular magnetic field (a system of two interacting electrons in a two-dimensional parabolic confinement potential) is introduced. A key ingredient of this trial wave function is a Jastrow pair correlation factor that has a displaced Gaussian form. The above choice of the pair correlation factor is instrumental on assuring the overall quality of the wave function at all values of the magnetic field.Exact numerical diagonalization results are used to gauge the quality of the proposed trial wave function.We find out that this trial wave function is an excellent representation of the true ground state at all values of the magnetic field including weak (or zero) and strong magnetic fields.
cond-mat.mes-hall cond-mat.str-el
a trial wave function for twodimensional quantum dot helium in an arbitrary perpendicular magnetic field a system of two interacting electrons in a twodimensional parabolic confinement potential is introduced a key ingredient of this trial wave function is a jastrow pair correlation factor that has a displaced gaussian form the above choice of the pair correlation factor is instrumental on assuring the overall quality of the wave function at all values of the magnetic fieldexact numerical diagonalization results are used to gauge the quality of the proposed trial wave functionwe find out that this trial wave function is an excellent representation of the true ground state at all values of the magnetic field including weak or zero and strong magnetic fields
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708.3691
Time dependent black holes and thermal equilibration
We study aspects of a recently proposed exact time dependent black hole solution of IIB string theory using the AdS/CFT correspondence. The dual field theory is a thermal system in which initially a vacuum density for a non-conserved operator is turned on. We can see that in agreement with general thermal field theory expectation the system equilibrates: the expectation value of the non-conserved operator goes to zero exponentially and the entropy increases. In the field theory the process can be described quantitatively in terms of a thermofield state and exact agreement with the gravity answers is found.
hep-th gr-qc
we study aspects of a recently proposed exact time dependent black hole solution of iib string theory using the adscft correspondence the dual field theory is a thermal system in which initially a vacuum density for a nonconserved operator is turned on we can see that in agreement with general thermal field theory expectation the system equilibrates the expectation value of the nonconserved operator goes to zero exponentially and the entropy increases in the field theory the process can be described quantitatively in terms of a thermofield state and exact agreement with the gravity answers is found
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708.3692
Influence of the N*(1440) and N*(1535) Resonances in Intermediate Energy pp and np Scattering
Motivated by a recent measurement of proton-proton elastic scattering observables up to 3.0 GeV, we investigate the description of those data within models of the nucleon-nucleon (NN) interaction valid above the pion production threshold. In addition to including the well known Delta resonance we incorporate two low-lying N* resonances, the N*(1440) and the N*(1535), and study their influence on pp and np observables for projectile laboratory kinetic energies up to 1.5 GeV.
nucl-th nucl-ex
motivated by a recent measurement of protonproton elastic scattering observables up to 30 gev we investigate the description of those data within models of the nucleonnucleon nn interaction valid above the pion production threshold in addition to including the well known delta resonance we incorporate two lowlying n resonances the n1440 and the n1535 and study their influence on pp and np observables for projectile laboratory kinetic energies up to 15 gev
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708.3693
An Ergodic Result
A rather general ergodic type scheme is presented on arbitrary sets X, as they are generated by arbitrary mappings T : X \longrightarrow X. The structures considered on X are given by suitable subsets of the set of all of its finite partitions. Ergodicity is studied not with respect to subsets of X, but with the {\it inverse limits} of families of finite partitions.
math.GM math.DS
a rather general ergodic type scheme is presented on arbitrary sets x as they are generated by arbitrary mappings t x longrightarrow x the structures considered on x are given by suitable subsets of the set of all of its finite partitions ergodicity is studied not with respect to subsets of x but with the it inverse limits of families of finite partitions
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708.3694
Electronic, dynamical, and thermal properties of ultra-incompressible superhard rhenium diboride: A combined first-principles and neutron scattering study
Rhenium diboride is a recently recognized ultra-incompressible superhard material. Here we report the electronic (e), phonon (p), e-p coupling and thermal properties of ReB$_2$ from first-principles density-functional theory (DFT) calculations and neutron scattering measurements. Our calculated elastic constants ($c_{11}$ = 641 GPa, $c_{12}$ = 159 GPa, $c_{13}$ = 128 GPa, $c_{33}$ = 1037 GPa, and $c_{44}$ = 271 GPa), bulk modulus ($B$ $\approx$ 350 GPa) and hardness ($H$ $\approx$ 46 GPa) are in good agreement with the reported experimental data. The calculated phonon density of states (DOS) agrees very well with our neutron vibrational spectroscopy result. Electronic and phonon analysis indicates that the strong covalent B-B and Re-B bonding is the main reason for the super incompressibility and hardness of ReB$_2$. The thermal expansion coefficients, calculated within the quasi-harmonic approximation and measured by neutron powder diffraction, are found to be nearly isotropic in $a$ and $c$ directions and only slightly larger than that of diamond in terms of magnitude. The excellent agreement found between calculations and experimental measurements indicate that first-principles calculations capture the main interactions in this class of superhard materials, and thus can be used to search, predict, and design new materials with desired properties.
cond-mat.mtrl-sci
rhenium diboride is a recently recognized ultraincompressible superhard material here we report the electronic e phonon p ep coupling and thermal properties of reb_2 from firstprinciples densityfunctional theory dft calculations and neutron scattering measurements our calculated elastic constants c_11 641 gpa c_12 159 gpa c_13 128 gpa c_33 1037 gpa and c_44 271 gpa bulk modulus b approx 350 gpa and hardness h approx 46 gpa are in good agreement with the reported experimental data the calculated phonon density of states dos agrees very well with our neutron vibrational spectroscopy result electronic and phonon analysis indicates that the strong covalent bb and reb bonding is the main reason for the super incompressibility and hardness of reb_2 the thermal expansion coefficients calculated within the quasiharmonic approximation and measured by neutron powder diffraction are found to be nearly isotropic in a and c directions and only slightly larger than that of diamond in terms of magnitude the excellent agreement found between calculations and experimental measurements indicate that firstprinciples calculations capture the main interactions in this class of superhard materials and thus can be used to search predict and design new materials with desired properties
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708.3695
Near-horizon geometries of supersymmetric AdS(5) black holes
We provide a classification of near-horizon geometries of supersymmetric, asymptotically anti-de Sitter, black holes of five-dimensional U(1)^3-gauged supergravity which admit two rotational symmetries. We find three possibilities: a topologically spherical horizon, an S^1 \times S^2 horizon and a toroidal horizon. The near-horizon geometry of the topologically spherical case turns out to be that of the most general known supersymmetric, asymptotically anti-de Sitter, black hole of U(1)^3-gauged supergravity. The other two cases have constant scalars and only exist in particular regions of this moduli space -- in particular they do not exist within minimal gauged supergravity. We also find a solution corresponding to the near-horizon geometry of a three-charge supersymmetric black ring held in equilibrium by a conical singularity; when lifted to type IIB supergravity this solution can be made regular, resulting in a discrete family of warped AdS(3) geometries. Analogous results are presented in U(1)^n gauged supergravity.
hep-th
we provide a classification of nearhorizon geometries of supersymmetric asymptotically antide sitter black holes of fivedimensional u13gauged supergravity which admit two rotational symmetries we find three possibilities a topologically spherical horizon an s1 times s2 horizon and a toroidal horizon the nearhorizon geometry of the topologically spherical case turns out to be that of the most general known supersymmetric asymptotically antide sitter black hole of u13gauged supergravity the other two cases have constant scalars and only exist in particular regions of this moduli space in particular they do not exist within minimal gauged supergravity we also find a solution corresponding to the nearhorizon geometry of a threecharge supersymmetric black ring held in equilibrium by a conical singularity when lifted to type iib supergravity this solution can be made regular resulting in a discrete family of warped ads3 geometries analogous results are presented in u1n gauged supergravity
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708.3696
Relative-Error CUR Matrix Decompositions
Many data analysis applications deal with large matrices and involve approximating the matrix using a small number of ``components.'' Typically, these components are linear combinations of the rows and columns of the matrix, and are thus difficult to interpret in terms of the original features of the input data. In this paper, we propose and study matrix approximations that are explicitly expressed in terms of a small number of columns and/or rows of the data matrix, and thereby more amenable to interpretation in terms of the original data. Our main algorithmic results are two randomized algorithms which take as input an $m \times n$ matrix $A$ and a rank parameter $k$. In our first algorithm, $C$ is chosen, and we let $A'=CC^+A$, where $C^+$ is the Moore-Penrose generalized inverse of $C$. In our second algorithm $C$, $U$, $R$ are chosen, and we let $A'=CUR$. ($C$ and $R$ are matrices that consist of actual columns and rows, respectively, of $A$, and $U$ is a generalized inverse of their intersection.) For each algorithm, we show that with probability at least $1-\delta$: $$ ||A-A'||_F \leq (1+\epsilon) ||A-A_k||_F, $$ where $A_k$ is the ``best'' rank-$k$ approximation provided by truncating the singular value decomposition (SVD) of $A$. The number of columns of $C$ and rows of $R$ is a low-degree polynomial in $k$, $1/\epsilon$, and $\log(1/\delta)$. Our two algorithms are the first polynomial time algorithms for such low-rank matrix approximations that come with relative-error guarantees; previously, in some cases, it was not even known whether such matrix decompositions exist. Both of our algorithms are simple, they take time of the order needed to approximately compute the top $k$ singular vectors of $A$, and they use a novel, intuitive sampling method called ``subspace sampling.''
cs.DS
many data analysis applications deal with large matrices and involve approximating the matrix using a small number of components typically these components are linear combinations of the rows and columns of the matrix and are thus difficult to interpret in terms of the original features of the input data in this paper we propose and study matrix approximations that are explicitly expressed in terms of a small number of columns andor rows of the data matrix and thereby more amenable to interpretation in terms of the original data our main algorithmic results are two randomized algorithms which take as input an m times n matrix a and a rank parameter k in our first algorithm c is chosen and we let acca where c is the moorepenrose generalized inverse of c in our second algorithm c u r are chosen and we let acur c and r are matrices that consist of actual columns and rows respectively of a and u is a generalized inverse of their intersection for each algorithm we show that with probability at least 1delta aa_f leq 1epsilon aa_k_f where a_k is the best rankk approximation provided by truncating the singular value decomposition svd of a the number of columns of c and rows of r is a lowdegree polynomial in k 1epsilon and log1delta our two algorithms are the first polynomial time algorithms for such lowrank matrix approximations that come with relativeerror guarantees previously in some cases it was not even known whether such matrix decompositions exist both of our algorithms are simple they take time of the order needed to approximately compute the top k singular vectors of a and they use a novel intuitive sampling method called subspace sampling
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708.3697
Homotopy characterization of ANR mapping spaces
Let Y be an absolute neighborhood retract (ANR) for the class of metric spaces and let X be a Hausdorff space. Let map(X,Y) denote the space of continuous maps from X to Y with the compact open topology. It is shown that if X is a CW complex then map(X,Y) is an ANR for the class of metric spaces if and only if map(X,Y) is metrizable and has the homotopy type of a CW complex. The same holds also when X is a compactly generated hemicompact space (metrizability assumption is void in this case).
math.AT math.GN
let y be an absolute neighborhood retract anr for the class of metric spaces and let x be a hausdorff space let mapxy denote the space of continuous maps from x to y with the compact open topology it is shown that if x is a cw complex then mapxy is an anr for the class of metric spaces if and only if mapxy is metrizable and has the homotopy type of a cw complex the same holds also when x is a compactly generated hemicompact space metrizability assumption is void in this case
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708.3698
Upper limit for circumstellar gas around the Type Ia SN 2000cx
The nature of the companion stars in Type Ia Supernova (SNe) progenitor systems remains unclear. One possible way to discriminate between different scenarios is the presence (or absence) of circumstellar material, the left overs from the progenitor evolution that may be revealed by their interaction with the SN. A new method to probe the circumstellar environment has been exploited for the normal Type Ia SN 2006X, leading for the first time to the direct detection of material which escaped the progenitor system. In this paper we apply the same analysis to the peculiar Type Ia SN 2000cx, with the aim of constraining the properties of its progenitor system. Using multi-epoch, high-resolution spectroscopy we have studied the spectral region where narrow, time-variable NaID absorption features are expected in case circumstellar material is present along the line of sight. No NaID absorption is detected in the rest-frame of the host galaxy to a level of a few mA, setting a stringent upper limit to the column density of the absorbing material (N(NaI)<=2 x 10^10 cm-2). In this respect the peculiar Type Ia SN 2000cx is different from the normal Ia SN 2006X. Whether this is to be attributed to a different progenitor system, to viewing-angle effects or to a low metallicity remains to be clarified.
astro-ph
the nature of the companion stars in type ia supernova sne progenitor systems remains unclear one possible way to discriminate between different scenarios is the presence or absence of circumstellar material the left overs from the progenitor evolution that may be revealed by their interaction with the sn a new method to probe the circumstellar environment has been exploited for the normal type ia sn 2006x leading for the first time to the direct detection of material which escaped the progenitor system in this paper we apply the same analysis to the peculiar type ia sn 2000cx with the aim of constraining the properties of its progenitor system using multiepoch highresolution spectroscopy we have studied the spectral region where narrow timevariable naid absorption features are expected in case circumstellar material is present along the line of sight no naid absorption is detected in the restframe of the host galaxy to a level of a few ma setting a stringent upper limit to the column density of the absorbing material nnai2 x 1010 cm2 in this respect the peculiar type ia sn 2000cx is different from the normal ia sn 2006x whether this is to be attributed to a different progenitor system to viewingangle effects or to a low metallicity remains to be clarified
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708.3699
Convolutional Entanglement Distillation
We develop a theory of entanglement distillation that exploits a convolutional coding structure. We provide a method for converting an arbitrary classical binary or quaternary convolutional code into a convolutional entanglement distillation protocol. The imported classical convolutional code does not have to be dual-containing or self-orthogonal. The yield and error-correcting properties of such a protocol depend respectively on the rate and error-correcting properties of the imported classical convolutional code. A convolutional entanglement distillation protocol has several other benefits. Two parties sharing noisy ebits can distill noiseless ebits ``online'' as they acquire more noisy ebits. Distillation yield is high and decoding complexity is simple for a convolutional entanglement distillation protocol. Our theory of convolutional entanglement distillation reduces the problem of finding a good convolutional entanglement distillation protocol to the well-established problem of finding a good classical convolutional code.
quant-ph cs.IT math.IT
we develop a theory of entanglement distillation that exploits a convolutional coding structure we provide a method for converting an arbitrary classical binary or quaternary convolutional code into a convolutional entanglement distillation protocol the imported classical convolutional code does not have to be dualcontaining or selforthogonal the yield and errorcorrecting properties of such a protocol depend respectively on the rate and errorcorrecting properties of the imported classical convolutional code a convolutional entanglement distillation protocol has several other benefits two parties sharing noisy ebits can distill noiseless ebits online as they acquire more noisy ebits distillation yield is high and decoding complexity is simple for a convolutional entanglement distillation protocol our theory of convolutional entanglement distillation reduces the problem of finding a good convolutional entanglement distillation protocol to the wellestablished problem of finding a good classical convolutional code
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708.37
Memory Effect and Fast Spinodal Decomposition
We consider the modification of the Cahn-Hilliard equation when a time delay process through a memory function is taken into account. We then study the process of spinodal decomposition in fast phase transitions associated with a conserved order parameter. The introduced memory effect plays an important role to obtain a finite group velocity. Then, we discuss the constraint for the parameters to satisfy causality. The memory effect is seen to affect the dynamics of phase transition at short times and has the effect of delaying, in a significant way, the process of rapid growth of the order parameter that follows a quench into the spinodal region.
nucl-th cond-mat.soft hep-ph
we consider the modification of the cahnhilliard equation when a time delay process through a memory function is taken into account we then study the process of spinodal decomposition in fast phase transitions associated with a conserved order parameter the introduced memory effect plays an important role to obtain a finite group velocity then we discuss the constraint for the parameters to satisfy causality the memory effect is seen to affect the dynamics of phase transition at short times and has the effect of delaying in a significant way the process of rapid growth of the order parameter that follows a quench into the spinodal region
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708.3701
Classical analogs for Rabi-oscillations, Ramsey-fringes, and spin-echo in Josephson junctions
We investigate the results of recently published experiments on the quantum behavior of Josephson circuits in terms of the classical modelling based on the resistively and capacitively-shunted (RCSJ) junction model. Our analysis shows evidence for a close analogy between the nonlinear behavior of a pulsed microwave-driven Josephson junction at low temperature and low dissipation and the experimental observations reported for the Josephson circuits. Specifically, we demonstrate that Rabi-oscillations, Ramsey-fringes, and spin-echo observations are not phenomena with a unique quantum interpretation. In fact, they are natural consequences of transients to phase-locking in classical nonlinear dynamics and can be observed in a purely classical model of a Josephson junction when the experimental recipe for the application of microwaves is followed and the experimental detection scheme followed. We therefore conclude that classical nonlinear dynamics can contribute to the understanding of relevant experimental observations of Josephson response to various microwave perturbations at very low temperature and low dissipation.
cond-mat.supr-con cond-mat.stat-mech
we investigate the results of recently published experiments on the quantum behavior of josephson circuits in terms of the classical modelling based on the resistively and capacitivelyshunted rcsj junction model our analysis shows evidence for a close analogy between the nonlinear behavior of a pulsed microwavedriven josephson junction at low temperature and low dissipation and the experimental observations reported for the josephson circuits specifically we demonstrate that rabioscillations ramseyfringes and spinecho observations are not phenomena with a unique quantum interpretation in fact they are natural consequences of transients to phaselocking in classical nonlinear dynamics and can be observed in a purely classical model of a josephson junction when the experimental recipe for the application of microwaves is followed and the experimental detection scheme followed we therefore conclude that classical nonlinear dynamics can contribute to the understanding of relevant experimental observations of josephson response to various microwave perturbations at very low temperature and low dissipation
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708.3702
Measurements of Partial Branching Fractions for Bbar --> X_u ell nubar and Determination of |V_{ub}|
We present partial branching fractions for inclusive charmless semileptonic B decays Bbar --> X_u ell nubar, and the determination of the CKM matrix element |V_{ub}|. The analysis is based on a sample of 383 million Y(4S) decays into B Bbar pairs collected with the BaBar detector at the PEP-II e+ e- storage rings. We select events using either the invariant mass M_X of the hadronic system, the invariant mass squared, q^2, of the lepton and neutrino pair, the kinematic variable P_+ or one of their combinations. We then determine partial branching fractions in limited regions of phase space: Delta B = (1.18 +- 0.09_{stat.} +- 0.07_{syst.} +- 0.01_{theo.}) x 10^{-3} (M_X < 1.55 GeV/c^2), Delta B = (0.95 +- 0.10_{stat.} +- 0.08_{syst.} +- 0.01_{theo.}) x 10^{-3} (P_+ < 0.66 GeV/c), and Delta B = (0.81 +- 0.08_{stat.} +- 0.07_{syst.} +- 0.02_{theo.}) x 10^{-3} (M_X < 1.7 GeV/c^2, q^2 > 8 GeV^2/c^4). Corresponding values of |V_{ub}| are extracted using several theoretical calculations.
hep-ex
we present partial branching fractions for inclusive charmless semileptonic b decays bbar x_u ell nubar and the determination of the ckm matrix element v_ub the analysis is based on a sample of 383 million y4s decays into b bbar pairs collected with the babar detector at the pepii e e storage rings we select events using either the invariant mass m_x of the hadronic system the invariant mass squared q2 of the lepton and neutrino pair the kinematic variable p_ or one of their combinations we then determine partial branching fractions in limited regions of phase space delta b 118 009_stat 007_syst 001_theo x 103 m_x 155 gevc2 delta b 095 010_stat 008_syst 001_theo x 103 p_ 066 gevc and delta b 081 008_stat 007_syst 002_theo x 103 m_x 17 gevc2 q2 8 gev2c4 corresponding values of v_ub are extracted using several theoretical calculations
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708.3703
Testing the evolution of the DB white dwarf GD 358: First results of a new approach using asteroseismology
We present a new method that investigates the evolutionary history of the pulsating DB white dwarf GD358 using asteroseismology. This is done considering the internal C/O profile, which describes the relative abundances of carbon and oxygen from the core of the star to its surface. Different evolutionary channels lead to the generation of different C/O profiles, and these affect the pulsation periods. We used C/O profiles associated with white dwarfs that evolved through binary evolution channels where the progenitor experienced one or two episodes of mass loss during one or two common envelope (CE) phases, and two profiles from single star evolution. We computed models using these different profiles and used a genetic algorithm (GA) to optimize the search in the parameter space in order to find the best-fit to the observed pulsation periods. We used three-parameter models, adjusting the stellar mass, the effective temperature, and the helium mass of the external layer. Our results suggest that binary evolution profiles may provide a better match to the pulsation periods of GD 358. The best-fit to the observations is obtained using a profile related to an evolutionary history where two episodes of mass loss happen during two CE phases. The best-fit model has a mass close to the mean mass for DB white dwarfs found in various works, and a temperature consistent with UV spectra obtained with the IUE satellite.
astro-ph
we present a new method that investigates the evolutionary history of the pulsating db white dwarf gd358 using asteroseismology this is done considering the internal co profile which describes the relative abundances of carbon and oxygen from the core of the star to its surface different evolutionary channels lead to the generation of different co profiles and these affect the pulsation periods we used co profiles associated with white dwarfs that evolved through binary evolution channels where the progenitor experienced one or two episodes of mass loss during one or two common envelope ce phases and two profiles from single star evolution we computed models using these different profiles and used a genetic algorithm ga to optimize the search in the parameter space in order to find the bestfit to the observed pulsation periods we used threeparameter models adjusting the stellar mass the effective temperature and the helium mass of the external layer our results suggest that binary evolution profiles may provide a better match to the pulsation periods of gd 358 the bestfit to the observations is obtained using a profile related to an evolutionary history where two episodes of mass loss happen during two ce phases the bestfit model has a mass close to the mean mass for db white dwarfs found in various works and a temperature consistent with uv spectra obtained with the iue satellite
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708.3704
About Goldbach strong conjecture
In this work we use the number classification in families of the form 6n+1, and 6n+5 with n integer (Such families contain all odd prime numbers greater than 3 and other compound numbers related with primes). We will use this kind of classification in order to attempt an approach to Goldbach strong conjecture. By means of a geometric method of binary bands of numbers we conceive a new form of study of the stated problem.
math.GM
in this work we use the number classification in families of the form 6n1 and 6n5 with n integer such families contain all odd prime numbers greater than 3 and other compound numbers related with primes we will use this kind of classification in order to attempt an approach to goldbach strong conjecture by means of a geometric method of binary bands of numbers we conceive a new form of study of the stated problem
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708.3705
Lattice QCD Calculation of the $\rho$ Meson Decay Width
We present a lattice QCD calculation of the $\rho$ meson decay width via the $P$-wave scattering phase shift for the I=1 two-pion system. Our calculation uses full QCD gauge configurations for $N_f=2$ flavors generated using a renormalization group improved gauge action and an improved Wilson fermion action on a $12^3\times24$ lattice at $m_\pi/m_\rho=0.41$ and the lattice spacing $1/a=0.92 {\rm GeV}$. The phase shift calculated with the use of the finite size formula for the two-pion system in the moving frame shows a behavior consistent with the existence of a resonance at a mass close to the vector meson mass obtained in spectroscopy. The decay width estimated from the phase shift is consistent with the experiment, when the quark mass is scaled to the realistic value.
hep-lat
we present a lattice qcd calculation of the rho meson decay width via the pwave scattering phase shift for the i1 twopion system our calculation uses full qcd gauge configurations for n_f2 flavors generated using a renormalization group improved gauge action and an improved wilson fermion action on a 123times24 lattice at m_pim_rho041 and the lattice spacing 1a092 rm gev the phase shift calculated with the use of the finite size formula for the twopion system in the moving frame shows a behavior consistent with the existence of a resonance at a mass close to the vector meson mass obtained in spectroscopy the decay width estimated from the phase shift is consistent with the experiment when the quark mass is scaled to the realistic value
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708.3706
D3/D7 holographic Gauge theory and Chemical potential
N=2 supersymmetric Yang-Mills theory with flavor hypermultiplets at finite temperature and in the dS${}_4$ are studied for finite quark number density ($n_b$) by a dual supergravity background with non-trivial dilaton and axion. The quarks and its number density $n_b$ are introduced by embedding a probe D7 brane. We find a critical value of the chemical potential at the limit of $n_b=0$, and it coincides with the effective quark mass given in each theory for $n_b=0$. At this point, a transition of the D7 embedding configurations occurs between their two typical ones. The phase diagrams of this transition are shown in the plane of chemical potential versus temperature and cosmological constant for YM theory at finite temperature and in dS${}_4$ respectively. In this phase transition, the order parameter is considered as $n_b$. % and the critical value of the chemical potential This result seems to be reasonable since both theories are in the quark deconfinement phase.
hep-th
n2 supersymmetric yangmills theory with flavor hypermultiplets at finite temperature and in the ds_4 are studied for finite quark number density n_b by a dual supergravity background with nontrivial dilaton and axion the quarks and its number density n_b are introduced by embedding a probe d7 brane we find a critical value of the chemical potential at the limit of n_b0 and it coincides with the effective quark mass given in each theory for n_b0 at this point a transition of the d7 embedding configurations occurs between their two typical ones the phase diagrams of this transition are shown in the plane of chemical potential versus temperature and cosmological constant for ym theory at finite temperature and in ds_4 respectively in this phase transition the order parameter is considered as n_b and the critical value of the chemical potential this result seems to be reasonable since both theories are in the quark deconfinement phase
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708.3707
First order approach and index theorems for discrete and metric graphs
The aim of the present paper is to introduce the notion of first order (supersymmetric) Dirac operators on discrete and metric (``quantum'') graphs. In order to cover all self-adjoint boundary conditions for the associated metric graph Laplacian, we develop systematically a new type of discrete graph operators acting on a decorated graph. The decoration at each vertex of degree-d is given by a subspace of $\C^d$, generalising the fact that a function on the standard vertex space has only a scalar value. We develop the notion of exterior derivative, differential forms, Dirac and Laplace operators in the discrete and metric case, using a supersymmetric framework. We calculate the (supersymmetric) index of the discrete Dirac operator generalising the standard index formula involving the Euler characteristic of a graph. Finally, we show that the corresponding index for the metric Dirac operator agrees with the discrete one.
math.SP math-ph math.CO math.FA math.MP
the aim of the present paper is to introduce the notion of first order supersymmetric dirac operators on discrete and metric quantum graphs in order to cover all selfadjoint boundary conditions for the associated metric graph laplacian we develop systematically a new type of discrete graph operators acting on a decorated graph the decoration at each vertex of degreed is given by a subspace of cd generalising the fact that a function on the standard vertex space has only a scalar value we develop the notion of exterior derivative differential forms dirac and laplace operators in the discrete and metric case using a supersymmetric framework we calculate the supersymmetric index of the discrete dirac operator generalising the standard index formula involving the euler characteristic of a graph finally we show that the corresponding index for the metric dirac operator agrees with the discrete one
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708.3708
Super-bicharacter construction of quantum vertex algebras
We extend the bicharacter construction of quantum vertex algebras first proposed by Borcherds to the case of super Hopf algebras. We give a bicharacter description of the charged free fermion super vertex algebra, which allows us to construct different quantizations of it in the sense of $H_D$-quantum vertex algebras, or specializations to Etingof-Kazhdan quantum vertex algebras. We give formulas for the analytic continuation of product of fields, the operator product expansion and the normal ordered product in terms of the super-bicharacters.
math-ph math.MP math.QA
we extend the bicharacter construction of quantum vertex algebras first proposed by borcherds to the case of super hopf algebras we give a bicharacter description of the charged free fermion super vertex algebra which allows us to construct different quantizations of it in the sense of h_dquantum vertex algebras or specializations to etingofkazhdan quantum vertex algebras we give formulas for the analytic continuation of product of fields the operator product expansion and the normal ordered product in terms of the superbicharacters
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708.3709
An elementary sieve
In this paper we review the properties of families of numbers of the form $6n\pm1$, with $n$ integer (in which there are all prime numbers greater than 3 and other compound numbers with particular properties) to later use them in a new sieve that allows the separation of numbers $n$ that generate primes from those that only generate compounds. In principle, this can be used to find the amount of prime numbers up to a given number $h$; this means, $\pi(h)$.
math.GM
in this paper we review the properties of families of numbers of the form 6npm1 with n integer in which there are all prime numbers greater than 3 and other compound numbers with particular properties to later use them in a new sieve that allows the separation of numbers n that generate primes from those that only generate compounds in principle this can be used to find the amount of prime numbers up to a given number h this means pih
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708.371
Real World Interpretations of Quantum Theory
I propose a new class of interpretations, {\it real world interpretations}, of the quantum theory of closed systems. These interpretations postulate a preferred factorization of Hilbert space and preferred projective measurements on one factor. They give a mathematical characterisation of the different possible worlds arising in an evolving closed quantum system, in which each possible world corresponds to a (generally mixed) evolving quantum state. In a realistic model, the states corresponding to different worlds should be expected to tend towards orthogonality as different possible quasiclassical structures emerge or as measurement-like interactions produce different classical outcomes. However, as the worlds have a precise mathematical definition, real world interpretations need no definition of quasiclassicality, measurement, or other concepts whose imprecision is problematic in other interpretational approaches. It is natural to postulate that precisely one world is chosen randomly, using the natural probability distribution, as the world realised in Nature, and that this world's mathematical characterisation is a complete description of reality.
quant-ph
i propose a new class of interpretations it real world interpretations of the quantum theory of closed systems these interpretations postulate a preferred factorization of hilbert space and preferred projective measurements on one factor they give a mathematical characterisation of the different possible worlds arising in an evolving closed quantum system in which each possible world corresponds to a generally mixed evolving quantum state in a realistic model the states corresponding to different worlds should be expected to tend towards orthogonality as different possible quasiclassical structures emerge or as measurementlike interactions produce different classical outcomes however as the worlds have a precise mathematical definition real world interpretations need no definition of quasiclassicality measurement or other concepts whose imprecision is problematic in other interpretational approaches it is natural to postulate that precisely one world is chosen randomly using the natural probability distribution as the world realised in nature and that this worlds mathematical characterisation is a complete description of reality
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708.3711
Mean-field description of the nucleus-nucleus optical potential
A new finite-range representation of the JLM effective nucleon-nucleon interaction is suggested based on the CDM3Y density dependent functional and M3Y-Paris interaction. The density dependence has been carefully adjusted at each energy so that the nucleon optical potential (OP) given by the new density dependent interaction in the Hartree-Fock calculation of nuclear matter closely matches the JLM nucleon OP given by the Brueckner-Hatree-Fock calculation. The new interaction has been used in the double-folding model to calculate the OP for the elastic $^{6}$Li,$^{6}$He,$^{12}$C + $^{12}$C scattering at different energies.
nucl-th nucl-ex
a new finiterange representation of the jlm effective nucleonnucleon interaction is suggested based on the cdm3y density dependent functional and m3yparis interaction the density dependence has been carefully adjusted at each energy so that the nucleon optical potential op given by the new density dependent interaction in the hartreefock calculation of nuclear matter closely matches the jlm nucleon op given by the bruecknerhatreefock calculation the new interaction has been used in the doublefolding model to calculate the op for the elastic 6li6he12c 12c scattering at different energies
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708.3712
Canonical Charmonium Interpretation for Y(4360) and Y(4660)
In this work, we consider the canonical charmonium assignments for Y(4360) and Y(4660). Y(4660) is good candidate of $\rm 5 ^3S_1$ $c\bar{c}$ state, the possibility of Y(4360) as a $\rm 3 ^3D_1$ $c\bar{c}$ state is studied, and the charmonium hybrid interpretation of Y(4360) can not be excluded completely. We evaluate the $e^{+}e^{-}$ leptonic widths, E1 transitions, M1 transitions and the open flavor strong decays of Y(4360) and Y(4660). Experimental tests for the charmonium assignments are suggested.
hep-ph
in this work we consider the canonical charmonium assignments for y4360 and y4660 y4660 is good candidate of rm 5 3s_1 cbarc state the possibility of y4360 as a rm 3 3d_1 cbarc state is studied and the charmonium hybrid interpretation of y4360 can not be excluded completely we evaluate the ee leptonic widths e1 transitions m1 transitions and the open flavor strong decays of y4360 and y4660 experimental tests for the charmonium assignments are suggested
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708.3713
A field theoretic approach to master equations and a variational method beyond the Poisson ansatz
We develop a variational scheme in a field theoretic approach to a stochastic process. While various stochastic processes can be expressed using master equations, in general it is difficult to solve the master equations exactly, and it is also hard to solve the master equations numerically because of the curse of dimensionality. The field theoretic approach has been used in order to study such complicated master equations, and the variational scheme achieves tremendous reduction in the dimensionality of master equations. For the variational method, only the Poisson ansatz has been used, in which one restricts the variational function to a Poisson distribution. Hence, one has dealt with only restricted fluctuation effects. We develop the variational method further, which enables us to treat an arbitrary variational function. It is shown that the variational scheme developed gives a quantitatively good approximation for master equations which describe a stochastic gene regulatory network.
cond-mat.stat-mech
we develop a variational scheme in a field theoretic approach to a stochastic process while various stochastic processes can be expressed using master equations in general it is difficult to solve the master equations exactly and it is also hard to solve the master equations numerically because of the curse of dimensionality the field theoretic approach has been used in order to study such complicated master equations and the variational scheme achieves tremendous reduction in the dimensionality of master equations for the variational method only the poisson ansatz has been used in which one restricts the variational function to a poisson distribution hence one has dealt with only restricted fluctuation effects we develop the variational method further which enables us to treat an arbitrary variational function it is shown that the variational scheme developed gives a quantitatively good approximation for master equations which describe a stochastic gene regulatory network
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708.3714
Orbits of particles in noncommutative Schwarzschild spacetime
By considering particles as smeared objects, we investigate the effects of space noncommutativity on the orbits of particles in Schwarzschild spacetime. The effects of space noncommutativity on the value of the precession of the perihelion of particle orbit and deflection of light ray in Schwarzschild geometry are calculated and the stability of circular orbits is discussed.
gr-qc
by considering particles as smeared objects we investigate the effects of space noncommutativity on the orbits of particles in schwarzschild spacetime the effects of space noncommutativity on the value of the precession of the perihelion of particle orbit and deflection of light ray in schwarzschild geometry are calculated and the stability of circular orbits is discussed
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708.3715
Three String Junction and N=4 Dyon Spectrum
The exact spectrum of dyons in a class of N=4 supersymmetric string theories gives us information about dyon spectrum in N=4 supersymmetric gauge theories. This in turn can be translated into prediction about the BPS spectrum of three string junctions on a configuration of three parallel D3-branes. We show that this prediction agrees with the known spectrum of three string junction in different domains in the moduli space separated by walls of marginal stability.
hep-th
the exact spectrum of dyons in a class of n4 supersymmetric string theories gives us information about dyon spectrum in n4 supersymmetric gauge theories this in turn can be translated into prediction about the bps spectrum of three string junctions on a configuration of three parallel d3branes we show that this prediction agrees with the known spectrum of three string junction in different domains in the moduli space separated by walls of marginal stability
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708.3716
The Impact of a Percolating IGM on Redshifted 21 cm Observations of Quasar HII Regions
We assess the impact of inhomogeneous reionization on detection of HII regions surrounding luminous high redshift quasars using planned low frequency radio telescopes. Our approach is to implement a semi-numerical scheme to calculate the 3-dimensional structure of ionized regions surrounding a massive halo at high redshift, including the ionizing influence of a luminous quasar. As part of our analysis we briefly contrast our scheme with published semi-numerical models. We calculate mock 21cm spectra along the line of sight towards high redshift quasars, and estimate the ability of the planned Murchison Widefield Array to detect the presence of HII regions. The signal-to-noise for detection will drop as the characteristic bubble size grows during reionization because the quasar's influence becomes less prominent. However, quasars will imprint a detectable signature on observed 21cm spectra that is distinct from a region of typical IGM. At epochs where the mean hydrogen neutral fraction is ~30% or greater we find that neutral gas in the IGM surrounding a single quasar will be detectable (at a significance of 5 sigma) within 100 hour integrations in more than 50% of cases. 1000 hour integrations will be required to detect a smaller neutral fraction of 15% in more than 50% of cases. A highly significant detection will be possible in only 100 hours for a stack of 10 smaller 3 proper Mpc HII regions. The accurate measurement of the global average neutral fraction (<x_HI>) will be limited by systematic fluctuations between lines of sight for single HII regions. We estimate the accuracy with which the global neutral fraction could be measured from a single HII region to be 50%, 30% and 20% for <x_HI> ~ 0.15, 0.3 and 0.5 respectively.
astro-ph
we assess the impact of inhomogeneous reionization on detection of hii regions surrounding luminous high redshift quasars using planned low frequency radio telescopes our approach is to implement a seminumerical scheme to calculate the 3dimensional structure of ionized regions surrounding a massive halo at high redshift including the ionizing influence of a luminous quasar as part of our analysis we briefly contrast our scheme with published seminumerical models we calculate mock 21cm spectra along the line of sight towards high redshift quasars and estimate the ability of the planned murchison widefield array to detect the presence of hii regions the signaltonoise for detection will drop as the characteristic bubble size grows during reionization because the quasars influence becomes less prominent however quasars will imprint a detectable signature on observed 21cm spectra that is distinct from a region of typical igm at epochs where the mean hydrogen neutral fraction is 30 or greater we find that neutral gas in the igm surrounding a single quasar will be detectable at a significance of 5 sigma within 100 hour integrations in more than 50 of cases 1000 hour integrations will be required to detect a smaller neutral fraction of 15 in more than 50 of cases a highly significant detection will be possible in only 100 hours for a stack of 10 smaller 3 proper mpc hii regions the accurate measurement of the global average neutral fraction x_hi will be limited by systematic fluctuations between lines of sight for single hii regions we estimate the accuracy with which the global neutral fraction could be measured from a single hii region to be 50 30 and 20 for x_hi 015 03 and 05 respectively
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708.3717
Evidence For The Production Of Slow Antiprotonic Hydrogen In Vacuum
We present evidence showing how antiprotonic hydrogen, the quasistable antiproton-proton (pbar-p) bound system, has been synthesized following the interaction of antiprotons with the hydrogen molecular ion (H2+) in a nested Penning trap environment. From a careful analysis of the spatial distributions of antiproton annihilation events, evidence is presented for antiprotonic hydrogen production with sub-eV kinetic energies in states around n=70, and with low angular momenta. The slow antiprotonic hydrogen may be studied using laser spectroscopic techniques.
hep-ex
we present evidence showing how antiprotonic hydrogen the quasistable antiprotonproton pbarp bound system has been synthesized following the interaction of antiprotons with the hydrogen molecular ion h2 in a nested penning trap environment from a careful analysis of the spatial distributions of antiproton annihilation events evidence is presented for antiprotonic hydrogen production with subev kinetic energies in states around n70 and with low angular momenta the slow antiprotonic hydrogen may be studied using laser spectroscopic techniques
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708.3718
Zero product preservers of C*-algebras
Let T be be a zero-product preserving bounded linear map between C*-algebras A and B. Here neither A nor B is necessarily unital. In this note, we investigate when T gives rise to a Jordan homomorphism. In particular, we show that A and B are isomorphic as Jordan algebras if T is bijective and sends zero products of self-adjoint elements to zero products. They are isomorphic as C*-algebras if T is bijective and preserves the full zero product structure.
math.OA math.FA
let t be be a zeroproduct preserving bounded linear map between calgebras a and b here neither a nor b is necessarily unital in this note we investigate when t gives rise to a jordan homomorphism in particular we show that a and b are isomorphic as jordan algebras if t is bijective and sends zero products of selfadjoint elements to zero products they are isomorphic as calgebras if t is bijective and preserves the full zero product structure
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708.3719
Evolution of Star Clusters near the Galactic Center: Fully Self-consistent N-body Simulations
We have performed fully self-consistent $N$-body simulations of star clusters near the Galactic center (GC). Such simulations have not been performed because it is difficult to perform fast and accurate simulations of such systems using conventional methods. We used the Bridge code, which integrates the parent galaxy using the tree algorithm and the star cluster using the fourth-order Hermite scheme with individual timestep. The interaction between the parent galaxy and the star cluster is calculate with the tree algorithm. Therefore, the Bridge code can handle both the orbital and internal evolutions of star clusters correctly at the same time. We investigated the evolution of star clusters using the Bridge code and compared the results with previous studies. We found that 1) the inspiral timescale of the star clusters is shorter than that obtained with "traditional" simulations, in which the orbital evolution of star clusters is calculated analytically using the dynamical friction formula and 2) the core collapse of the star cluster increases the core density and help the cluster survive. The initial conditions of star clusters is not so severe as previously suggested.
astro-ph
we have performed fully selfconsistent nbody simulations of star clusters near the galactic center gc such simulations have not been performed because it is difficult to perform fast and accurate simulations of such systems using conventional methods we used the bridge code which integrates the parent galaxy using the tree algorithm and the star cluster using the fourthorder hermite scheme with individual timestep the interaction between the parent galaxy and the star cluster is calculate with the tree algorithm therefore the bridge code can handle both the orbital and internal evolutions of star clusters correctly at the same time we investigated the evolution of star clusters using the bridge code and compared the results with previous studies we found that 1 the inspiral timescale of the star clusters is shorter than that obtained with traditional simulations in which the orbital evolution of star clusters is calculated analytically using the dynamical friction formula and 2 the core collapse of the star cluster increases the core density and help the cluster survive the initial conditions of star clusters is not so severe as previously suggested
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708.372
Dirac concentrations in Lotka-Volterra parabolic PDEs
We consider parabolic partial differential equations of Lotka-Volterra type, with a non-local nonlinear term. This models, at the population level, the darwinian evolution of a population; the Laplace term represents mutations and the nonlinear birth/death term represents competition leading to selection. Once rescaled with a small diffusion, we prove that the solutions converge to a moving Dirac mass. The velocity and weights cannot be obtained by a simple expression, e.g., an ordinary differential equation. We show that they are given by a constrained Hamilton-Jacobi equation. This extends several earlier results to the parabolic case and to general nonlinearities. Technical new ingredients are a $BV$ estimate in time on the non-local nonlinearity, a characterization of the concentration point (in a monomorphic situation) and, surprisingly, some counter-examples showing that jumps on the Dirac locations are indeed possible.
math.AP
we consider parabolic partial differential equations of lotkavolterra type with a nonlocal nonlinear term this models at the population level the darwinian evolution of a population the laplace term represents mutations and the nonlinear birthdeath term represents competition leading to selection once rescaled with a small diffusion we prove that the solutions converge to a moving dirac mass the velocity and weights cannot be obtained by a simple expression eg an ordinary differential equation we show that they are given by a constrained hamiltonjacobi equation this extends several earlier results to the parabolic case and to general nonlinearities technical new ingredients are a bv estimate in time on the nonlocal nonlinearity a characterization of the concentration point in a monomorphic situation and surprisingly some counterexamples showing that jumps on the dirac locations are indeed possible
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708.3721
Verified Real Number Calculations: A Library for Interval Arithmetic
Real number calculations on elementary functions are remarkably difficult to handle in mechanical proofs. In this paper, we show how these calculations can be performed within a theorem prover or proof assistant in a convenient and highly automated as well as interactive way. First, we formally establish upper and lower bounds for elementary functions. Then, based on these bounds, we develop a rational interval arithmetic where real number calculations take place in an algebraic setting. In order to reduce the dependency effect of interval arithmetic, we integrate two techniques: interval splitting and taylor series expansions. This pragmatic approach has been developed, and formally verified, in a theorem prover. The formal development also includes a set of customizable strategies to automate proofs involving explicit calculations over real numbers. Our ultimate goal is to provide guaranteed proofs of numerical properties with minimal human theorem-prover interaction.
cs.MS cs.LO
real number calculations on elementary functions are remarkably difficult to handle in mechanical proofs in this paper we show how these calculations can be performed within a theorem prover or proof assistant in a convenient and highly automated as well as interactive way first we formally establish upper and lower bounds for elementary functions then based on these bounds we develop a rational interval arithmetic where real number calculations take place in an algebraic setting in order to reduce the dependency effect of interval arithmetic we integrate two techniques interval splitting and taylor series expansions this pragmatic approach has been developed and formally verified in a theorem prover the formal development also includes a set of customizable strategies to automate proofs involving explicit calculations over real numbers our ultimate goal is to provide guaranteed proofs of numerical properties with minimal human theoremprover interaction
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708.3722
Formally Verified Argument Reduction with a Fused-Multiply-Add
Cody & Waite argument reduction technique works perfectly for reasonably large arguments but as the input grows there are no bit left to approximate the constant with enough accuracy. Under mild assumptions, we show that the result computed with a fused-multiply-add provides a fully accurate result for many possible values of the input with a constant almost accurate to the full working precision. We also present an algorithm for a fully accurate second reduction step to reach double full accuracy (all the significand bits of two numbers are significant) even in the worst cases of argument reduction. Our work recalls the common algorithms and presents proofs of correctness. All the proofs are formally verified using the Coq automatic proof checker.
cs.MS cs.PF
cody waite argument reduction technique works perfectly for reasonably large arguments but as the input grows there are no bit left to approximate the constant with enough accuracy under mild assumptions we show that the result computed with a fusedmultiplyadd provides a fully accurate result for many possible values of the input with a constant almost accurate to the full working precision we also present an algorithm for a fully accurate second reduction step to reach double full accuracy all the significand bits of two numbers are significant even in the worst cases of argument reduction our work recalls the common algorithms and presents proofs of correctness all the proofs are formally verified using the coq automatic proof checker
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708.3723
Parametric Stiffness Analysis of the Orthoglide
This paper presents a parametric stiffness analysis of the Orthoglide, a 3-DOF translational Parallel Kinematic Machine. First, a compliant modeling of the Orthoglide is conducted based on an existing method. Then stiffness matrix is symbolically computed. This allows one to easily study the influence of the geometric design parameters on the matrix elements. Critical links are displayed. Cutting forces are then modeled so that static displacements of the Orthoglide tool during slot milling are symbolically computed. Influence of the geometric design parameters on the static displacements is checked as well. Other machining operations can be modeled. This parametric stiffness analysis can be applied to any parallel manipulator for which stiffness is a critical issue.
cs.RO
this paper presents a parametric stiffness analysis of the orthoglide a 3dof translational parallel kinematic machine first a compliant modeling of the orthoglide is conducted based on an existing method then stiffness matrix is symbolically computed this allows one to easily study the influence of the geometric design parameters on the matrix elements critical links are displayed cutting forces are then modeled so that static displacements of the orthoglide tool during slot milling are symbolically computed influence of the geometric design parameters on the static displacements is checked as well other machining operations can be modeled this parametric stiffness analysis can be applied to any parallel manipulator for which stiffness is a critical issue
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708.3724
Compton telescope with coded aperture mask: Imaging with the INTEGRAL/IBIS Compton mode
Compton telescopes provide a good sensitivity over a wide field of view in the difficult energy range running from a few hundred keV to several MeV. Their angular resolution is, however, poor and strongly energy dependent. We present a novel experimental design associating a coded mask and a Compton detection unit to overcome these pitfalls. It maintains the Compton performance while improving the angular resolution by at least an order of magnitude in the field of view subtended by the mask. This improvement is obtained only at the expense of the efficiency that is reduced by a factor of two. In addition, the background corrections benefit from the coded mask technique, i.e. a simultaneous measurement of the source and background. This design is implemented and tested using the IBIS telescope on board the INTEGRAL satellite to construct images with a 12' resolution over a 29 degrees x 29 degrees field of view in the energy range from 200 keV to a few MeV. The details of the analysis method and the resulting telescope performance, particularly in terms of sensitivity, are presented.
astro-ph
compton telescopes provide a good sensitivity over a wide field of view in the difficult energy range running from a few hundred kev to several mev their angular resolution is however poor and strongly energy dependent we present a novel experimental design associating a coded mask and a compton detection unit to overcome these pitfalls it maintains the compton performance while improving the angular resolution by at least an order of magnitude in the field of view subtended by the mask this improvement is obtained only at the expense of the efficiency that is reduced by a factor of two in addition the background corrections benefit from the coded mask technique ie a simultaneous measurement of the source and background this design is implemented and tested using the ibis telescope on board the integral satellite to construct images with a 12 resolution over a 29 degrees x 29 degrees field of view in the energy range from 200 kev to a few mev the details of the analysis method and the resulting telescope performance particularly in terms of sensitivity are presented
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708.3725
Temperature Dependent Polarity Reversal in Au/Nb:SrTiO3 Schottky Junctions
We have observed temperature-dependent reversal of the rectifying polarity in Au/Nb:SrTiO3 Schottky junctions. By simulating current-voltage characteristics we have found that the permittivity of SrTiO3 near the interface exhibits temperature dependence opposite to that observed in the bulk, significantly reducing the barrier width. At low temperature, tunneling current dominates the junction transport due both to such barrier narrowing and to suppressed thermal excitations. The present results demonstrate that novel junction properties can be induced by the interface permittivity.
cond-mat.str-el cond-mat.mtrl-sci
we have observed temperaturedependent reversal of the rectifying polarity in aunbsrtio3 schottky junctions by simulating currentvoltage characteristics we have found that the permittivity of srtio3 near the interface exhibits temperature dependence opposite to that observed in the bulk significantly reducing the barrier width at low temperature tunneling current dominates the junction transport due both to such barrier narrowing and to suppressed thermal excitations the present results demonstrate that novel junction properties can be induced by the interface permittivity
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708.3726
Nonadiabatic factor accompanying magnetic translation of a charged particle
The quantum adiabatic theorem incorporating the Berry phase phenomenon can be characterized as a factorization of the time evolution operator into a path-dependent geometric factor, a usual dynamical factor and a non-adiabatic factor that approaches the identity in the adiabatic limit. We study a case where all these three factors can be constructed explicitly and where the instantaneous Hamiltonian has infinitely degenerate energy eigenstates associated with magnetic translation symmetry. Significance of the non-adiabatic factor in terms of transition probabilities is discussed.
quant-ph
the quantum adiabatic theorem incorporating the berry phase phenomenon can be characterized as a factorization of the time evolution operator into a pathdependent geometric factor a usual dynamical factor and a nonadiabatic factor that approaches the identity in the adiabatic limit we study a case where all these three factors can be constructed explicitly and where the instantaneous hamiltonian has infinitely degenerate energy eigenstates associated with magnetic translation symmetry significance of the nonadiabatic factor in terms of transition probabilities is discussed
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708.3727
Galois cohomology of completed link groups
In this paper we compute the Galois cohomology of the pro-p completion of primitive link groups. Here, a primitive link group is the fundamental group of a tame link in the 3-sphere whose linking number diagram is irreducible modulo p (e.g. none of the linking numbers is divisible by p). The result is that (with Z/pZ-coefficients) the Galois cohomology is naturally isomorphic to the Z/pZ-cohomology of the discrete link group. The main application of this result is that for such groups the Baum-Connes conjecture or the Atiyah conjecture are true for every finite extension (or even every elementary amenable extension), if they are true for the group itself.
math.GR math.AG
in this paper we compute the galois cohomology of the prop completion of primitive link groups here a primitive link group is the fundamental group of a tame link in the 3sphere whose linking number diagram is irreducible modulo p eg none of the linking numbers is divisible by p the result is that with zpzcoefficients the galois cohomology is naturally isomorphic to the zpzcohomology of the discrete link group the main application of this result is that for such groups the baumconnes conjecture or the atiyah conjecture are true for every finite extension or even every elementary amenable extension if they are true for the group itself
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708.3728
Quasi-particle interference and superconducting gap in a high-temperature superconductor Ca2-xNaxCuO2Cl2
High-transition-temperature (high-Tc) superconductivity is ubiquitous in the cuprates containing CuO2 planes but each cuprate has its own character. The study of the material dependence of the d-wave superconducting gap (SG) should provide important insights into the mechanism of high-Tc. However, because of the 'pseudogap' phenomenon, it is often unclear whether the energy gaps observed by spectroscopic techniques really represent the SG. Here, we report spectroscopic imaging scanning tunneling microscopy (SI-STM) studies of nearly-optimally-doped Ca2-xNaxCuO2Cl2 (Na-CCOC) with Tc = 25 ~ 28 K. They enable us to observe the quasi-particle interference (QPI) effect in this material, through which unambiguous new information on the SG is obtained. The analysis of QPI in Na-CCOC reveals that the SG dispersion near the gap node is almost identical to that of Bi2Sr2CaCu2Oy (Bi2212) at the same doping level, while Tc of Bi2212 is 3 times higher than that of Na-CCOC. We also find that SG in Na-CCOC is confined in narrower energy and momentum ranges than Bi2212. This explains at least in part the remarkable material dependence of Tc
cond-mat.supr-con cond-mat.str-el
hightransitiontemperature hightc superconductivity is ubiquitous in the cuprates containing cuo2 planes but each cuprate has its own character the study of the material dependence of the dwave superconducting gap sg should provide important insights into the mechanism of hightc however because of the pseudogap phenomenon it is often unclear whether the energy gaps observed by spectroscopic techniques really represent the sg here we report spectroscopic imaging scanning tunneling microscopy sistm studies of nearlyoptimallydoped ca2xnaxcuo2cl2 naccoc with tc 25 28 k they enable us to observe the quasiparticle interference qpi effect in this material through which unambiguous new information on the sg is obtained the analysis of qpi in naccoc reveals that the sg dispersion near the gap node is almost identical to that of bi2sr2cacu2oy bi2212 at the same doping level while tc of bi2212 is 3 times higher than that of naccoc we also find that sg in naccoc is confined in narrower energy and momentum ranges than bi2212 this explains at least in part the remarkable material dependence of tc
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708.3729
From Unruh temperature to generalized Bousso bound
In a classical spacetime satisfying Einstein's equation and the null convergence condition, the same quantum mechanical effects that cause black holes to have a temperature are found to imply, if joined to the macroscopic nature of entropy, the covariant entropy bound in its generalized form. This is obtained from thermodynamics, as applied across the local Rindler causal horizon through every point p of the null hypersurfaces L the covariant entropy bound refers to, in the direction of the null geodesics generating L.
gr-qc
in a classical spacetime satisfying einsteins equation and the null convergence condition the same quantum mechanical effects that cause black holes to have a temperature are found to imply if joined to the macroscopic nature of entropy the covariant entropy bound in its generalized form this is obtained from thermodynamics as applied across the local rindler causal horizon through every point p of the null hypersurfaces l the covariant entropy bound refers to in the direction of the null geodesics generating l
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708.373
Densities for Rough Differential Equations under Hoermander's Condition
We consider stochastic differential equations dY=V(Y)dX driven by a multidimensional Gaussian process X in the rough path sense. Using Malliavin Calculus we show that Y(t) admits a density for t in (0,T] provided (i) the vector fields V=(V_1,...,V_d) satisfy Hoermander's condition and (ii) the Gaussian driving signal X satisfies certain conditions. Examples of driving signals include fractional Brownian motion with Hurst parameter H>1/4, the Brownian Bridge returning to zero after time T and the Ornstein-Uhlenbeck process.
math.PR
we consider stochastic differential equations dyvydx driven by a multidimensional gaussian process x in the rough path sense using malliavin calculus we show that yt admits a density for t in 0t provided i the vector fields vv_1v_d satisfy hoermanders condition and ii the gaussian driving signal x satisfies certain conditions examples of driving signals include fractional brownian motion with hurst parameter h14 the brownian bridge returning to zero after time t and the ornsteinuhlenbeck process
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708.3731
Differences between charged-current coefficient functions
Second- and third-order results are presented for the structure functions of charged-current deep-inelastic scattering in the framework of massless perturbative QCD. We write down the two-loop differences between the corresponding crossing-even and -odd coefficient functions, including those for the longitudinal structure function not covered in the literature so far. At three loops we compute the lowest five moments of these differences for all three structure functions and provide approximate expressions in Bjorken-$x$ space. Also calculated is the related third-order coefficient-function correction to the Gottfried sum rule. We confirm the conjectured suppression of these quantities if the number of colours is large. Finally we derive the second- and third-order QCD contributions to the Paschos-Wolfenstein ratio used for the determination of the weak mixing angle from neutrino-nucleon deep-inelastic scattering. These contributions are found to be small.
hep-ph
second and thirdorder results are presented for the structure functions of chargedcurrent deepinelastic scattering in the framework of massless perturbative qcd we write down the twoloop differences between the corresponding crossingeven and odd coefficient functions including those for the longitudinal structure function not covered in the literature so far at three loops we compute the lowest five moments of these differences for all three structure functions and provide approximate expressions in bjorkenx space also calculated is the related thirdorder coefficientfunction correction to the gottfried sum rule we confirm the conjectured suppression of these quantities if the number of colours is large finally we derive the second and thirdorder qcd contributions to the paschoswolfenstein ratio used for the determination of the weak mixing angle from neutrinonucleon deepinelastic scattering these contributions are found to be small
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708.3732
Evolution of the gaps through the cuprate phase-diagram
The actual physical origin of the gap at the antinodes, and a clear identification of the superconducting gap are fundamental open issues in the physics of high-$T_c$ superconductors. Here, we present a systematic electronic Raman scattering study of a mercury-based single layer cuprate, as a function of both doping level and temperature. On the deeply overdoped side, we show that the antinodal gap is a true superconducting gap. In contrast, on the underdoped side, our results reveal the existence of a break point close to optimal doping below which the antinodal gap is gradually disconnected from superconductivity. The nature of both the superconducting and normal state is distinctly different on each side of this breakpoint.
cond-mat.supr-con cond-mat.str-el
the actual physical origin of the gap at the antinodes and a clear identification of the superconducting gap are fundamental open issues in the physics of hight_c superconductors here we present a systematic electronic raman scattering study of a mercurybased single layer cuprate as a function of both doping level and temperature on the deeply overdoped side we show that the antinodal gap is a true superconducting gap in contrast on the underdoped side our results reveal the existence of a break point close to optimal doping below which the antinodal gap is gradually disconnected from superconductivity the nature of both the superconducting and normal state is distinctly different on each side of this breakpoint
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708.3733
Luminosity function, sizes and FR dichotomy of radio-loud AGN
The radio luminosity function (RLF) of radio galaxies and radio-loud quasars is often modelled as a broken power-law. The break luminosity is close to the dividing line between the two Fanaroff-Riley (FR) morphological classes for the large-scale radio structure of these objects. We use an analytical model for the luminosity and size evolution of FRII-type objects together with a simple prescription for FRI-type sources to construct the RLF. We postulate that all sources start out with an FRII-type morphology. Weaker jets subsequently disrupt within the quasi-constant density cores of their host galaxies and develop turbulent lobes of type FRI. With this model we recover the slopes of the power laws and the break luminosity of the RLF determined from observations. The rate at which AGN with jets of jet power $Q$ appear in the universe is found to be proportional to $Q^{-1.6}$. The model also roughly predicts the distribution of the radio lobe sizes for FRII-type objects, if the radio luminosity of the turbulent jets drops significantly at the point of disruption. We show that our model is consistent with recent ideas of two distinct accretion modes in jet-producing AGN, if radiative efficiency of the accretion process is correlated with jet power.
astro-ph
the radio luminosity function rlf of radio galaxies and radioloud quasars is often modelled as a broken powerlaw the break luminosity is close to the dividing line between the two fanaroffriley fr morphological classes for the largescale radio structure of these objects we use an analytical model for the luminosity and size evolution of friitype objects together with a simple prescription for fritype sources to construct the rlf we postulate that all sources start out with an friitype morphology weaker jets subsequently disrupt within the quasiconstant density cores of their host galaxies and develop turbulent lobes of type fri with this model we recover the slopes of the power laws and the break luminosity of the rlf determined from observations the rate at which agn with jets of jet power q appear in the universe is found to be proportional to q16 the model also roughly predicts the distribution of the radio lobe sizes for friitype objects if the radio luminosity of the turbulent jets drops significantly at the point of disruption we show that our model is consistent with recent ideas of two distinct accretion modes in jetproducing agn if radiative efficiency of the accretion process is correlated with jet power
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708.3734
Searching for a dangerous host: randomized vs. deterministic
A Black Hole is an harmful host in a network that destroys incoming agents without leaving any trace of such event. The problem of locating the black hole in a network through a team of agent coordinated by a common protocol is usually referred in literature as the Black Hole Search problem (or BHS for brevity) and it is a consolidated research topic in the area of distributed algorithms. The aim of this paper is to extend the results for BHS by considering more general (and hence harder) classes of dangerous host. In particular we introduce rB-hole as a probabilistic generalization of the Black Hole, in which the destruction of an incoming agent is a purely random event happening with some fixed probability (like flipping a biased coin). The main result we present is that if we tolerate an arbitrarily small error probability in the result then the rB-hole Search problem, or RBS, is not harder than the usual BHS. We establish this result in two different communication model, specifically both in presence or absence of whiteboards non-located at the homebase. The core of our methods is a general reduction tool for transforming algorithms for the black hole into algorithms for the rB-hole.
cs.DC
a black hole is an harmful host in a network that destroys incoming agents without leaving any trace of such event the problem of locating the black hole in a network through a team of agent coordinated by a common protocol is usually referred in literature as the black hole search problem or bhs for brevity and it is a consolidated research topic in the area of distributed algorithms the aim of this paper is to extend the results for bhs by considering more general and hence harder classes of dangerous host in particular we introduce rbhole as a probabilistic generalization of the black hole in which the destruction of an incoming agent is a purely random event happening with some fixed probability like flipping a biased coin the main result we present is that if we tolerate an arbitrarily small error probability in the result then the rbhole search problem or rbs is not harder than the usual bhs we establish this result in two different communication model specifically both in presence or absence of whiteboards nonlocated at the homebase the core of our methods is a general reduction tool for transforming algorithms for the black hole into algorithms for the rbhole
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708.3735
Pattern formation in the damped Nikolaevskiy equation
The Nikolaevskiy equation has been proposed as a model for seismic waves, electroconvection and weak turbulence; we show that it can also be used to model transverse instabilities of fronts. This equation possesses a large-scale "Goldstone" mode that significantly influences the stability of spatially periodic steady solutions; indeed, all such solutions are unstable at onset, and the equation exhibits so-called soft-mode turbulence. In many applications, a weak damping of this neutral mode will be present, and we study the influence of this damping on solutions to the Nikolaevskiy equation. We examine the transition to the usual Eckhaus instability as the damping of the large-scale mode is increased, through numerical calculation and weakly nonlinear analysis. The latter is accomplished using asymptotically consistent systems of coupled amplitude equations. We find that there is a critical value of the damping below which (for a given value of the supercriticality parameter) all periodic steady states are unstable. The last solutions to lose stability lie in a cusp close to the left-hand side of the marginal stability curve.
nlin.PS
the nikolaevskiy equation has been proposed as a model for seismic waves electroconvection and weak turbulence we show that it can also be used to model transverse instabilities of fronts this equation possesses a largescale goldstone mode that significantly influences the stability of spatially periodic steady solutions indeed all such solutions are unstable at onset and the equation exhibits socalled softmode turbulence in many applications a weak damping of this neutral mode will be present and we study the influence of this damping on solutions to the nikolaevskiy equation we examine the transition to the usual eckhaus instability as the damping of the largescale mode is increased through numerical calculation and weakly nonlinear analysis the latter is accomplished using asymptotically consistent systems of coupled amplitude equations we find that there is a critical value of the damping below which for a given value of the supercriticality parameter all periodic steady states are unstable the last solutions to lose stability lie in a cusp close to the lefthand side of the marginal stability curve
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708.3736
A convergent finite difference method for a nonlinear variational wave equation
We establish rigorously convergence of a semi-discrete upwind scheme for the nonlinear variational wave equation $u_{tt} - c(u)(c(u) u_x)_x = 0$ with $u|_{t=0}=u_0$ and $u_t|_{t=0}=v_0$. Introducing Riemann invariants $R=u_t+c u_x$ and $S=u_t-c u_x$, the variational wave equation is equivalent to $R_t-c R_x=\tilde c (R^2-S^2)$ and $S_t+c S_x=-\tilde c (R^2-S^2)$ with $\tilde c=c'/(4c)$. An upwind scheme is defined for this system. We assume that the the speed $c$ is positive, increasing and both $c$ and its derivative are bounded away from zero and that $R|_{t=0}, S|_{t=0}\in L^1\cap L^3$ are nonpositive. The numerical scheme is illustrated on several examples.
math.AP math.NA
we establish rigorously convergence of a semidiscrete upwind scheme for the nonlinear variational wave equation u_tt cucu u_x_x 0 with u_t0u_0 and u_t_t0v_0 introducing riemann invariants ru_tc u_x and su_tc u_x the variational wave equation is equivalent to r_tc r_xtilde c r2s2 and s_tc s_xtilde c r2s2 with tilde cc4c an upwind scheme is defined for this system we assume that the the speed c is positive increasing and both c and its derivative are bounded away from zero and that r_t0 s_t0in l1cap l3 are nonpositive the numerical scheme is illustrated on several examples
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708.3737
Joint deprojection of Sunyaev-Zeldovich and X-ray images of galaxy clusters
We present two non-parametric deprojection methods aimed at recovering the three-dimensional density and temperature profiles of galaxy clusters from spatially resolved thermal Sunyaev-Zeldovich (tSZ) and X-ray surface brightness maps, thus avoiding the use of X-ray spectroscopic data. In both methods, clusters are assumed to be spherically symmetric and modeled with an onion-skin structure. The first method follows a direct geometrical approach. The second method is based on the maximization of a single joint (tSZ and X-ray) likelihood function, which allows one to fit simultaneously the two signals by following a Monte Carlo Markov Chain approach. These techniques are tested against a set of cosmological simulations of clusters, with and without instrumental noise. We project each cluster along the three orthogonal directions defined by the principal axes of the momentum of inertia tensor. This enables us to check any bias in the deprojection associated to the cluster elongation along the line of sight. After averaging over all the three projection directions, we find an overall good reconstruction, with a small (<~10 per cent) overestimate of the gas density profile. This turns into a comparable overestimate of the gas mass within the virial radius, which we ascribe to the presence of residual gas clumping. Apart from this small bias the reconstruction has an intrinsic scatter of about 5 per cent, which is dominated by gas clumpiness. Cluster elongation along the line of sight biases the deprojected temperature profile upwards at r<~0.2r_vir and downwards at larger radii. A comparable bias is also found in the deprojected temperature profile. Overall, this turns into a systematic underestimate of the gas mass, up to 10 percent. (Abridged)
astro-ph
we present two nonparametric deprojection methods aimed at recovering the threedimensional density and temperature profiles of galaxy clusters from spatially resolved thermal sunyaevzeldovich tsz and xray surface brightness maps thus avoiding the use of xray spectroscopic data in both methods clusters are assumed to be spherically symmetric and modeled with an onionskin structure the first method follows a direct geometrical approach the second method is based on the maximization of a single joint tsz and xray likelihood function which allows one to fit simultaneously the two signals by following a monte carlo markov chain approach these techniques are tested against a set of cosmological simulations of clusters with and without instrumental noise we project each cluster along the three orthogonal directions defined by the principal axes of the momentum of inertia tensor this enables us to check any bias in the deprojection associated to the cluster elongation along the line of sight after averaging over all the three projection directions we find an overall good reconstruction with a small 10 per cent overestimate of the gas density profile this turns into a comparable overestimate of the gas mass within the virial radius which we ascribe to the presence of residual gas clumping apart from this small bias the reconstruction has an intrinsic scatter of about 5 per cent which is dominated by gas clumpiness cluster elongation along the line of sight biases the deprojected temperature profile upwards at r02r_vir and downwards at larger radii a comparable bias is also found in the deprojected temperature profile overall this turns into a systematic underestimate of the gas mass up to 10 percent abridged
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708.3738
Killing superalgebra deformations of ten-dimensional supergravity backgrounds
We explore Lie superalgebra deformations of the Killing superalgebras of some ten-dimensional supergravity backgrounds. We prove the rigidity of the Poincare superalgebras in types I, IIA and IIB, as well as of the Killing superalgebra of the Freund-Rubin vacuum of type IIB supergravity. We also prove rigidity of the Killing superalgebras of the NS5, D0, D3, D4 and D5 branes, whereas we exhibit the possible deformations of the D1, D2, D6 and D7 brane Killing superalgebras, as well as of that of the type II fundamental string solutions. We relate the superalgebra deformations of the D2 and D6 branes to those of the (delocalised) M2 brane and the Kaluza-Klein monopole, respectively. The good behaviour under Kaluza-Klein reduction suggests that the deformed superalgebras ought to have a geometric interpretation.
hep-th
we explore lie superalgebra deformations of the killing superalgebras of some tendimensional supergravity backgrounds we prove the rigidity of the poincare superalgebras in types i iia and iib as well as of the killing superalgebra of the freundrubin vacuum of type iib supergravity we also prove rigidity of the killing superalgebras of the ns5 d0 d3 d4 and d5 branes whereas we exhibit the possible deformations of the d1 d2 d6 and d7 brane killing superalgebras as well as of that of the type ii fundamental string solutions we relate the superalgebra deformations of the d2 and d6 branes to those of the delocalised m2 brane and the kaluzaklein monopole respectively the good behaviour under kaluzaklein reduction suggests that the deformed superalgebras ought to have a geometric interpretation
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708.3739
Exact Statistical Mechanical Investigation of a Finite Model Protein in its environment: A Small System Paradigm
We consider a general incompressible finite model protein of size M in its environment, which we represent by a semiflexible copolymer consisting of amino acid residues classified into only two species (H and P, see text) following Lau and Dill. We allow various interactions between chemically unbonded residues in a given sequence and the solvent (water), and exactly enumerate the number of conformations W(E) as a function of the energy E on an infinite lattice under two different conditions: (i) we allow conformations that are restricted to be compact (known as Hamilton walk conformations), and (ii) we allow unrestricted conformations that can also be non-compact. It is easily demonstrated using plausible arguments that our model does not possess any energy gap even though it is supposed to exhibit a sharp folding transition in the thermodynamic limit. The enumeration allows us to investigate exactly the effects of energetics on the native state(s), and the effect of small size on protein thermodynamics and, in particular, on the differences between the microcanonical and canonical ensembles. We find that the canonical entropy is much larger than the microcanonical entropy for finite systems. We investigate the property of self-averaging and conclude that small proteins do not self-average. We also present results that (i) provide some understanding of the energy landscape, and (ii) shed light on the free energy landscape at different temperatures.
cond-mat.stat-mech q-bio.BM
we consider a general incompressible finite model protein of size m in its environment which we represent by a semiflexible copolymer consisting of amino acid residues classified into only two species h and p see text following lau and dill we allow various interactions between chemically unbonded residues in a given sequence and the solvent water and exactly enumerate the number of conformations we as a function of the energy e on an infinite lattice under two different conditions i we allow conformations that are restricted to be compact known as hamilton walk conformations and ii we allow unrestricted conformations that can also be noncompact it is easily demonstrated using plausible arguments that our model does not possess any energy gap even though it is supposed to exhibit a sharp folding transition in the thermodynamic limit the enumeration allows us to investigate exactly the effects of energetics on the native states and the effect of small size on protein thermodynamics and in particular on the differences between the microcanonical and canonical ensembles we find that the canonical entropy is much larger than the microcanonical entropy for finite systems we investigate the property of selfaveraging and conclude that small proteins do not selfaverage we also present results that i provide some understanding of the energy landscape and ii shed light on the free energy landscape at different temperatures
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708.374
Plate-forme Magicien d'Oz pour l'\'etude de l'apport des ACAs \`a l'interaction
In order to evaluate the contribution of Embodied (Animated) Conversational Agents (ECAs) to the effectiveness and usability of human-computer interaction, we developed a software platform meant to collect usage data. This platform, which implements the wizard of Oz paradigm, makes it possible to simulate user interfaces integrating ACAs for any Windows software application. It can also save and "replay" a rich interaction trace including user and system events, screen captures, users' speech and eye fixations. This platform has been used to assess users' subjective judgements and reactions to a multimodal online help system meant to facilitate the use of software for the general public (Flash). The online help system is embodied using a 3D talking head (developed by FT R&D) which "says" oral help messages illustrated with Flash screen copies.
cs.HC
in order to evaluate the contribution of embodied animated conversational agents ecas to the effectiveness and usability of humancomputer interaction we developed a software platform meant to collect usage data this platform which implements the wizard of oz paradigm makes it possible to simulate user interfaces integrating acas for any windows software application it can also save and replay a rich interaction trace including user and system events screen captures users speech and eye fixations this platform has been used to assess users subjective judgements and reactions to a multimodal online help system meant to facilitate the use of software for the general public flash the online help system is embodied using a 3d talking head developed by ft rd which says oral help messages illustrated with flash screen copies
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708.3741
The correct relatively stable category for idempotent modules
We answer a question posed by Carlson, Peng, and Wheeler, and demonstrate that in general Rickard modules in relatively stable categories are not idempotent modules even if one localizes with respect to a tensor ideal subcategory. We also show that there is a modification one can make so as to recover the idempotent behaviour.
math.RT
we answer a question posed by carlson peng and wheeler and demonstrate that in general rickard modules in relatively stable categories are not idempotent modules even if one localizes with respect to a tensor ideal subcategory we also show that there is a modification one can make so as to recover the idempotent behaviour
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708.3742
Interfaces adaptatives Adaptation dynamique \`a l'utilisateur courant
We present a survey of recent research studies of the implementation of adaptive user models in human-computer interaction. A classification of research directions on adaptive user interfaces is first proposed; it takes account of the user characteristics that are modelled, the distribution of initiative and control of the system evolution between user and system, and the role of dynamic adaptation. Then, a few representative research studies are briefly presented to illustrate this classification. In the conclusion, some major issues regarding the utility and usability of adaptive user interfaces and the design of an appropriate methodology for assessing the ergonomic quality of this new form of interaction are mentioned.
cs.HC
we present a survey of recent research studies of the implementation of adaptive user models in humancomputer interaction a classification of research directions on adaptive user interfaces is first proposed it takes account of the user characteristics that are modelled the distribution of initiative and control of the system evolution between user and system and the role of dynamic adaptation then a few representative research studies are briefly presented to illustrate this classification in the conclusion some major issues regarding the utility and usability of adaptive user interfaces and the design of an appropriate methodology for assessing the ergonomic quality of this new form of interaction are mentioned
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708.3743
The Universe expansion and Energy problems
In this paper we construct a physical modelization of the universe expansion. The universe then reduces to a Riemannian space $0.2cm$ $(B(O,R(t)),g_t)$, where $R(t) \sim t$ for $t \gg $0, and $g_t$ is a time - dependent Riemannian metric which reflects and characterizes the dynamical matter - energy distribution $E_t(X)$ on $B(O,R(t))$ according to the Mach - Einstein principle. Our model allows us to resolve several major problems of Physics. It is consistent in the sense that all Newtonian and classical physical laws are valid as particular cases in classical situations. Moreover, our model permits to recover some confirmed principles and postulates such as the famous Einstein's relationship $ E = mc^2$ and to specify some approximate results of modern Physics. After showing, rigorously, the deficiency of the second part of the special relativity second postulate and after specifying the role of the wave quantum Mechanics and the quantum Statistics, we adapt the Einstein's general relativity theory and the (Einstein - de Sitter - Friedmann) homogeneous isotropic cosmology to our setting. This readaptation allows us to determine the age, the size and the total energy of our universe and to prove that only the total energy E, the electromagnetic constant $ke^2$ and the speed of light c are time - independent universal constants. The other fundamental constants of Physics (such as G,$\bar{h}$, $K_B 0.05cm T$, $\alpha$...) are indeed time - dependent and naturally related to the previous ones. Consequently, we realize the unification of all Physics' domains The expanding universe is so reduced to four basic elements (E, c, $ke^2$, t) and dynamically described by a (reviewed) general relativity theory.
physics.gen-ph
in this paper we construct a physical modelization of the universe expansion the universe then reduces to a riemannian space 02cm bortg_t where rt sim t for t gg 0 and g_t is a time dependent riemannian metric which reflects and characterizes the dynamical matter energy distribution e_tx on bort according to the mach einstein principle our model allows us to resolve several major problems of physics it is consistent in the sense that all newtonian and classical physical laws are valid as particular cases in classical situations moreover our model permits to recover some confirmed principles and postulates such as the famous einsteins relationship e mc2 and to specify some approximate results of modern physics after showing rigorously the deficiency of the second part of the special relativity second postulate and after specifying the role of the wave quantum mechanics and the quantum statistics we adapt the einsteins general relativity theory and the einstein de sitter friedmann homogeneous isotropic cosmology to our setting this readaptation allows us to determine the age the size and the total energy of our universe and to prove that only the total energy e the electromagnetic constant ke2 and the speed of light c are time independent universal constants the other fundamental constants of physics such as gbarh k_b 005cm t alpha are indeed time dependent and naturally related to the previous ones consequently we realize the unification of all physics domains the expanding universe is so reduced to four basic elements e c ke2 t and dynamically described by a reviewed general relativity theory
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708.3744
The Aharonov-Casher effect
The Aharonov-Casher effect, entry in the Compendium of Quantum Physics: Concepts, Experiments, History and Philosophy, ed. F. Weinert, K. Hentschel, D. Greenberger and B. Falkenburg (Springer), to appear
quant-ph
the aharonovcasher effect entry in the compendium of quantum physics concepts experiments history and philosophy ed f weinert k hentschel d greenberger and b falkenburg springer to appear
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708.3745
Spectral Mapping Reconstruction of Extended Sources
Three dimensional spectroscopy of extended sources is typically performed with dedicated integral field spectrographs. We describe a method of reconstructing full spectral cubes, with two spatial and one spectral dimension, from rastered spectral mapping observations employing a single slit in a traditional slit spectrograph. When the background and image characteristics are stable, as is often achieved in space, the use of traditional long slits for integral field spectroscopy can substantially reduce instrument complexity over dedicated integral field designs, without loss of mapping efficiency -- particularly compelling when a long slit mode for single unresolved source followup is separately required. We detail a custom flux-conserving cube reconstruction algorithm, discuss issues of extended source flux calibration, and describe CUBISM, a tool which implements these methods for spectral maps obtained with ther Spitzer Space Telescope's Infrared Spectrograph.
astro-ph
three dimensional spectroscopy of extended sources is typically performed with dedicated integral field spectrographs we describe a method of reconstructing full spectral cubes with two spatial and one spectral dimension from rastered spectral mapping observations employing a single slit in a traditional slit spectrograph when the background and image characteristics are stable as is often achieved in space the use of traditional long slits for integral field spectroscopy can substantially reduce instrument complexity over dedicated integral field designs without loss of mapping efficiency particularly compelling when a long slit mode for single unresolved source followup is separately required we detail a custom fluxconserving cube reconstruction algorithm discuss issues of extended source flux calibration and describe cubism a tool which implements these methods for spectral maps obtained with ther spitzer space telescopes infrared spectrograph
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708.3746
Energy-dependent tunnelling from few-electron dynamic quantum dots
We measure the electron escape-rate from surface-acoustic-wave dynamic quantum dots (QDs) through a tunnel barrier. Rate-equations are used to extract the tunnelling rates, which change by an order of magnitude with tunnel-barrier gate voltage. We find that the tunnelling rates depend on the number of electrons in each dynamic QD because of Coulomb energy. By comparing this dependence to a saddle-point-potential model, the addition energies of the second and third electron in each dynamic QD are estimated. The scale (a few meV) is comparable to those in static QDs as expected.
cond-mat.mes-hall cond-mat.other
we measure the electron escaperate from surfaceacousticwave dynamic quantum dots qds through a tunnel barrier rateequations are used to extract the tunnelling rates which change by an order of magnitude with tunnelbarrier gate voltage we find that the tunnelling rates depend on the number of electrons in each dynamic qd because of coulomb energy by comparing this dependence to a saddlepointpotential model the addition energies of the second and third electron in each dynamic qd are estimated the scale a few mev is comparable to those in static qds as expected
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708.3747
Special correspondences and Chow traces of Landweber-Novikov operations
We prove that the function field of a variety which possesses a special correspondence in the sense of M. Rost preserves the rationality of cycles of small codimensions. This fact was proven by Vishik in the case of quadrics and played the crucial role in his construction of fields with $u$-invariant $2^r+1$. The main technical tools are algebraic cobordism of Levine-Morel, generalized Rost degree formula and divisibility of Chow traces of certain Landweber-Novikov operations. As a direct application of our methods we prove the Vishik's Theorem for all $F_4$-varieties.
math.AG
we prove that the function field of a variety which possesses a special correspondence in the sense of m rost preserves the rationality of cycles of small codimensions this fact was proven by vishik in the case of quadrics and played the crucial role in his construction of fields with uinvariant 2r1 the main technical tools are algebraic cobordism of levinemorel generalized rost degree formula and divisibility of chow traces of certain landwebernovikov operations as a direct application of our methods we prove the vishiks theorem for all f_4varieties
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708.3748
Unveiling the nature and interaction of the intermediate/high-mass YSOs in IRAS 20343+4129
In order to elucidate the nature of the brightest infrared sources associated with IRAS 20343+4129, IRS1 and IRS3, we observed with the Submillimeter Array (SMA) the 1.3 mm continuum and CO(2-1) emission of the region. Faint millimeter dust continuum emission was detected toward IRS1, and we derived an associated gas mass of ~0.8 Msun. The IRS1 spectral energy distribution agrees with IRS1 being an intermediate-mass Class I source of about 1000 Lsun, whose circumstellar material is producing the observed large infrared excess. We have discovered a high-velocity CO bipolar outflow in the east-west direction, which is clearly associated with IRS1, and the outflow parameters are similar to those of intermediate-mass young stellar objects. Associated with the blue large scale CO outflow lobe, detected with single-dish observations, we only found two elongated low-velocity structures on either side of IRS3. The large-scale outflow lobe is almost completely resolved out by the SMA. Our detected low-velocity CO structures are coincident with elongated H2 emission features. The strongest millimeter continuum condensations in the region are found on either side of IRS3, where the infrared emission is extremely weak, and the CO and H2 elongated structures follow the border of the millimeter continuum emission that is facing IRS3. All these results suggest that the dust is associated with the walls of an expanding cavity driven by IRS3, estimated to be a B2 star. Within and beyond the expanding cavity, the millimeter continuum sources can be sites of future low-mass star formation.
astro-ph
in order to elucidate the nature of the brightest infrared sources associated with iras 203434129 irs1 and irs3 we observed with the submillimeter array sma the 13 mm continuum and co21 emission of the region faint millimeter dust continuum emission was detected toward irs1 and we derived an associated gas mass of 08 msun the irs1 spectral energy distribution agrees with irs1 being an intermediatemass class i source of about 1000 lsun whose circumstellar material is producing the observed large infrared excess we have discovered a highvelocity co bipolar outflow in the eastwest direction which is clearly associated with irs1 and the outflow parameters are similar to those of intermediatemass young stellar objects associated with the blue large scale co outflow lobe detected with singledish observations we only found two elongated lowvelocity structures on either side of irs3 the largescale outflow lobe is almost completely resolved out by the sma our detected lowvelocity co structures are coincident with elongated h2 emission features the strongest millimeter continuum condensations in the region are found on either side of irs3 where the infrared emission is extremely weak and the co and h2 elongated structures follow the border of the millimeter continuum emission that is facing irs3 all these results suggest that the dust is associated with the walls of an expanding cavity driven by irs3 estimated to be a b2 star within and beyond the expanding cavity the millimeter continuum sources can be sites of future lowmass star formation
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