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711.1008
Corner-Impact Bifurcations: a novel class of discontinuity-induced bifurcations in Cam-Follower Systems
This paper is concerned with the analysis of a class of impacting systems of relevance in applications: cam-follower systems. We show that these systems, which can be modelled as discontinuously forced impact oscillators, can exhibit complex behaviour due to the detachment at high rotational speeds between the follower and the cam. We propose that the observed phenomena can be explained in terms of a novel type of discontinuity-induced bifurcation, termed as corner-impact. We present a complete analysis of this bifurcation in the case of non-autonomous impact oscillator and explain the transition to chaos observed in a representative cam-follower example. The theoretical findings are validated numerically.
math-ph math.MP
this paper is concerned with the analysis of a class of impacting systems of relevance in applications camfollower systems we show that these systems which can be modelled as discontinuously forced impact oscillators can exhibit complex behaviour due to the detachment at high rotational speeds between the follower and the cam we propose that the observed phenomena can be explained in terms of a novel type of discontinuityinduced bifurcation termed as cornerimpact we present a complete analysis of this bifurcation in the case of nonautonomous impact oscillator and explain the transition to chaos observed in a representative camfollower example the theoretical findings are validated numerically
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711.1009
On the Casimir Effect in the High Tc Cuprates
High temperature superconductors have in common that they consist of parallel planes of copper oxide separated by layers whose composition can vary. Being ceramics, the cuprate superconductors are poor conductors above the transition temperature, T_c. Below T_c, the parallel Cu-O planes in those materials become superconducting while the layers in between stay poor conductors. Here, we ask to what extent the change in the Casimir energy that arises when the parallel Cu-O layers become superconducting could contribute to the superconducting condensation energy. Our aim here is merely to obtain an order of magnitude estimate. To this end, the material is modelled as consisting below T_c of parallel plasma sheets separated by vacuum and as without a significant Casimir effect above T_c. Due to the close proximity of the Cu-O planes the system is in the regime where the Casimir effect becomes a van der Waals type effect, dominated by contributions from TM surface plasmons propagating along the ab planes. Within this model, the Casimir energy is found to be of the same order of magnitude as the superconducting condensation energy.
cond-mat.supr-con
high temperature superconductors have in common that they consist of parallel planes of copper oxide separated by layers whose composition can vary being ceramics the cuprate superconductors are poor conductors above the transition temperature t_c below t_c the parallel cuo planes in those materials become superconducting while the layers in between stay poor conductors here we ask to what extent the change in the casimir energy that arises when the parallel cuo layers become superconducting could contribute to the superconducting condensation energy our aim here is merely to obtain an order of magnitude estimate to this end the material is modelled as consisting below t_c of parallel plasma sheets separated by vacuum and as without a significant casimir effect above t_c due to the close proximity of the cuo planes the system is in the regime where the casimir effect becomes a van der waals type effect dominated by contributions from tm surface plasmons propagating along the ab planes within this model the casimir energy is found to be of the same order of magnitude as the superconducting condensation energy
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711.101
Nature of protein family signatures: Insights from singular value analysis of position-specific scoring matrices
Position-specific scoring matrices (PSSMs) are useful for detecting weak homology in protein sequence analysis, and they are thought to contain some essential signatures of the protein families. In order to elucidate what kind of ingredients constitute such family-specific signatures, we apply singular value decomposition to a set of PSSMs and examine the properties of dominant right and left singular vectors. The first right singular vectors were correlated with various amino acid indices including relative mutability, amino acid composition in protein interior, hydropathy, or turn propensity, depending on proteins. A significant correlation between the first left singular vector and a measure of site conservation was observed. It is shown that the contribution of the first singular component to the PSSMs act to disfavor potentially but falsely functionally important residues at conserved sites. The second right singular vectors were highly correlated with hydrophobicity scales, and the corresponding left singular vectors with contact numbers of protein structures. It is suggested that sequence alignment with a PSSM is essentially equivalent to threading supplemented with functional information. The presented method may be used to separate functionally important sites from structurally important ones, and thus it may be a useful tool for predicting protein functions.
q-bio.BM
positionspecific scoring matrices pssms are useful for detecting weak homology in protein sequence analysis and they are thought to contain some essential signatures of the protein families in order to elucidate what kind of ingredients constitute such familyspecific signatures we apply singular value decomposition to a set of pssms and examine the properties of dominant right and left singular vectors the first right singular vectors were correlated with various amino acid indices including relative mutability amino acid composition in protein interior hydropathy or turn propensity depending on proteins a significant correlation between the first left singular vector and a measure of site conservation was observed it is shown that the contribution of the first singular component to the pssms act to disfavor potentially but falsely functionally important residues at conserved sites the second right singular vectors were highly correlated with hydrophobicity scales and the corresponding left singular vectors with contact numbers of protein structures it is suggested that sequence alignment with a pssm is essentially equivalent to threading supplemented with functional information the presented method may be used to separate functionally important sites from structurally important ones and thus it may be a useful tool for predicting protein functions
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711.1011
Super- and subradiant emission of two-level systems in the near-Dicke limit
We analyze the stability of super- and subradiant states in a system of identical two-level atoms in the near-Dicke limit, i.e., when the atoms are very close to each other compared to the wavelength of resonant light. The dynamics of the system are studied using a renormalized master equation, both with multipolar and minimal-coupling interaction schemes. We show that both models lead to the same result and, in contrast to unrenormalized models, predict that the relative orientation of the (co-aligned) dipoles is unimportant in the Dicke limit. Our master equation is of relevance to any system of dipole-coupled two-level atoms, and gives bounds on the strength of the dipole-dipole interaction for closely spaced atoms. Exact calculations for small atom systems in the near-Dicke limit show the increased emission times resulting from the evolution generated by the strong dipole-dipole interaction. However, for large numbers of atoms in the near-Dicke limit, it is shown that as the number of atoms increases, the effect of the dipole-dipole interaction on collective emission is reduced.
quant-ph
we analyze the stability of super and subradiant states in a system of identical twolevel atoms in the neardicke limit ie when the atoms are very close to each other compared to the wavelength of resonant light the dynamics of the system are studied using a renormalized master equation both with multipolar and minimalcoupling interaction schemes we show that both models lead to the same result and in contrast to unrenormalized models predict that the relative orientation of the coaligned dipoles is unimportant in the dicke limit our master equation is of relevance to any system of dipolecoupled twolevel atoms and gives bounds on the strength of the dipoledipole interaction for closely spaced atoms exact calculations for small atom systems in the neardicke limit show the increased emission times resulting from the evolution generated by the strong dipoledipole interaction however for large numbers of atoms in the neardicke limit it is shown that as the number of atoms increases the effect of the dipoledipole interaction on collective emission is reduced
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711.1012
Similarity search for local protein structures at atomic resolution by exploiting a database management system
A method to search for local structural similarities in proteins at atomic resolution is presented. It is demonstrated that a huge amount of structural data can be handled within a reasonable CPU time by using a conventional relational database management system with appropriate indexing of geometric data. This method, which we call geometric indexing, can enumerate ligand binding sites that are structurally similar to sub-structures of a query protein among more than 160,000 possible candidates within a few hours of CPU time on an ordinary desktop computer. After detecting a set of high scoring ligand binding sites by the geometric indexing search, structural alignments at atomic resolution are constructed by iteratively applying the Hungarian algorithm, and the statistical significance of the final score is estimated from an empirical model based on a gamma distribution. Applications of this method to several protein structures clearly shows that significant similarities can be detected between local structures of non-homologous as well as homologous proteins.
q-bio.BM
a method to search for local structural similarities in proteins at atomic resolution is presented it is demonstrated that a huge amount of structural data can be handled within a reasonable cpu time by using a conventional relational database management system with appropriate indexing of geometric data this method which we call geometric indexing can enumerate ligand binding sites that are structurally similar to substructures of a query protein among more than 160000 possible candidates within a few hours of cpu time on an ordinary desktop computer after detecting a set of high scoring ligand binding sites by the geometric indexing search structural alignments at atomic resolution are constructed by iteratively applying the hungarian algorithm and the statistical significance of the final score is estimated from an empirical model based on a gamma distribution applications of this method to several protein structures clearly shows that significant similarities can be detected between local structures of nonhomologous as well as homologous proteins
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711.1013
AGN Reddening and Ultraviolet Extinction Curves from Hubble Space Telescope Spectra
We present intrinsic extinction curves for 14 AGNs. The AGNs have reddenings, E(B-V), of up to 0.36 mag. The majority (13 out of 14) of the extinction curves are not steep in the UV. Of the seven best determined extinction curves, five have extinction curves that are as flat as the standard Galactic curve in the optical and near UV, but flatter in the far UV, and without the 2175 Angstrom feature. One AGN, B3 0754+394, has a steep SMC-like extinction curve, and another, Mrk 304, has an LMC-like extinction curve, including a probable 2175 Ang. bump. The remaining seven, lower-quality, extinction curves have overall shapes that are consistent with an LMC-like shape or a flatter shape. Two have possible 2175 features, and one might be identical to the Galactic curve. The flatter curves that predominate in our best determined extinction curves are not as flat as the Gaskell et al. (2004) extinction curve for radio-loud AGNs. This suggests that the previous radio-loud extinction curve might be slightly too flat in the range 4 < 1/lambda < 6.5 inverse microns because of luminosity-dependent reddening biases in the composite spectra, but further investigation is needed. We present a parameterized average AGN extinction curve. Observed variations in the continuum properties of the AGNs are inconsistent with intrinsic object-to-object variations because observed differences are least in the far UV where changes in the accretion disk spectrum should be greatest. We suggest that the steepening of AGN spectra around Lyman alpha is the result of a small amount of SMC-like dust (E(B-V) ~ 0.03). We find the largest object-to-object differences in spectral shape to be in the Fe II emission of the "small blue bump".
astro-ph
we present intrinsic extinction curves for 14 agns the agns have reddenings ebv of up to 036 mag the majority 13 out of 14 of the extinction curves are not steep in the uv of the seven best determined extinction curves five have extinction curves that are as flat as the standard galactic curve in the optical and near uv but flatter in the far uv and without the 2175 angstrom feature one agn b3 0754394 has a steep smclike extinction curve and another mrk 304 has an lmclike extinction curve including a probable 2175 ang bump the remaining seven lowerquality extinction curves have overall shapes that are consistent with an lmclike shape or a flatter shape two have possible 2175 features and one might be identical to the galactic curve the flatter curves that predominate in our best determined extinction curves are not as flat as the gaskell et al 2004 extinction curve for radioloud agns this suggests that the previous radioloud extinction curve might be slightly too flat in the range 4 1lambda 65 inverse microns because of luminositydependent reddening biases in the composite spectra but further investigation is needed we present a parameterized average agn extinction curve observed variations in the continuum properties of the agns are inconsistent with intrinsic objecttoobject variations because observed differences are least in the far uv where changes in the accretion disk spectrum should be greatest we suggest that the steepening of agn spectra around lyman alpha is the result of a small amount of smclike dust ebv 003 we find the largest objecttoobject differences in spectral shape to be in the fe ii emission of the small blue bump
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711.1014
Finite index subgroups of R. Thompson's group F
The authors classify the finite index subgroups of R. Thompson's group $F$. All such groups that are not isomorphic to $F$ are non-split extensions of finite cyclic groups by $F$. The classification describes precisely which finite index subgroups of $F$ are isomorphic to $F$, and also separates the isomorphism classes of the finite index subgroups of $F$ which are not isomorphic to $F$ from each other; characterizing the structure of the extensions using properties of the structure of the finite index subgroups of $Z\times Z$.
math.GR math.GN
the authors classify the finite index subgroups of r thompsons group f all such groups that are not isomorphic to f are nonsplit extensions of finite cyclic groups by f the classification describes precisely which finite index subgroups of f are isomorphic to f and also separates the isomorphism classes of the finite index subgroups of f which are not isomorphic to f from each other characterizing the structure of the extensions using properties of the structure of the finite index subgroups of ztimes z
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711.1015
Comment on Effects of transverse magnetic field on mixed convection in wall plume of power-law fluids, by Gorla, Lee, Nakamura and Pop, IJES, 1993
Comment on Effects of transverse magnetic field on mixed convection in wall plume of power-law fluids, by Rama Subba Reddy Gorla, Jin Kook Lee, Shoichiro Nakamura and Ioan Pop [International Journal of Engineering Science, 31 (1993) 1035-1045]. In the above paper the authors treat the boundary layer mixed convection flow of a power-law fluid along a vertical adiabatic surface in a transverse magnetic field with a steady thermal source at the leading edge. The governing non-similar equations are solved by means of a novel finite difference scheme. However, there are two fundamental errors in this paper and the presented results do not have any practical value.
physics.flu-dyn
comment on effects of transverse magnetic field on mixed convection in wall plume of powerlaw fluids by rama subba reddy gorla jin kook lee shoichiro nakamura and ioan pop international journal of engineering science 31 1993 10351045 in the above paper the authors treat the boundary layer mixed convection flow of a powerlaw fluid along a vertical adiabatic surface in a transverse magnetic field with a steady thermal source at the leading edge the governing nonsimilar equations are solved by means of a novel finite difference scheme however there are two fundamental errors in this paper and the presented results do not have any practical value
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711.1016
An On-the-fly Tableau-based Decision Procedure for PDL-Satisfiability
We present a tableau-based algorithm for deciding satisfiability for propositional dynamic logic (PDL) which builds a finite rooted tree with ancestor loops and passes extra information from children to parents to separate good loops from bad loops during backtracking. It is easy to implement, with potential for parallelisation, because it constructs a pseudo-model ``on the fly'' by exploring each tableau branch independently. But its worst-case behaviour is 2EXPTIME rather than EXPTIME. A prototype implementation in the TWB (http://twb.rsise.anu.edu.au) is available.
cs.LO
we present a tableaubased algorithm for deciding satisfiability for propositional dynamic logic pdl which builds a finite rooted tree with ancestor loops and passes extra information from children to parents to separate good loops from bad loops during backtracking it is easy to implement with potential for parallelisation because it constructs a pseudomodel on the fly by exploring each tableau branch independently but its worstcase behaviour is 2exptime rather than exptime a prototype implementation in the twb httptwbrsiseanueduau is available
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711.1017
Optimizing quantum process tomography with unitary 2-designs
We show that weighted unitary 2-designs define optimal measurements on the system-ancilla output state for ancilla-assisted process tomography of unital quantum channels. Examples include complete sets of mutually unbiased unitary-operator bases. Each of these specifies a minimal series of optimal orthogonal measurements. General quantum channels are also considered.
quant-ph
we show that weighted unitary 2designs define optimal measurements on the systemancilla output state for ancillaassisted process tomography of unital quantum channels examples include complete sets of mutually unbiased unitaryoperator bases each of these specifies a minimal series of optimal orthogonal measurements general quantum channels are also considered
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711.1018
Average Density of States in Disordered Graphene systems
In this paper, the average density of states (ADOS) with a binary alloy disorder in disordered graphene systems are calculated based on the recursion method. We observe an obvious resonant peak caused by interactions with surrounding impurities and an anti-resonance dip in ADOS curves near the Dirac point. We also find that the resonance energy (Er) and the dip position are sensitive to the concentration of disorders (x) and their on-site potentials (v). An linear relation, not only holds when the impurity concentration is low but this relation can be further extended to high impurity concentration regime with certain constraints. We also calculate the ADOS with a finite density of vacancies and compare our results with the previous theoretical results.
cond-mat.mes-hall
in this paper the average density of states ados with a binary alloy disorder in disordered graphene systems are calculated based on the recursion method we observe an obvious resonant peak caused by interactions with surrounding impurities and an antiresonance dip in ados curves near the dirac point we also find that the resonance energy er and the dip position are sensitive to the concentration of disorders x and their onsite potentials v an linear relation not only holds when the impurity concentration is low but this relation can be further extended to high impurity concentration regime with certain constraints we also calculate the ados with a finite density of vacancies and compare our results with the previous theoretical results
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711.1019
Discovery of Polarization Reverberation in NGC 4151
Observations of the optical polarization of NGC 4151 in 1997-2003 show variations of an order of magnitude in the polarized flux while the polarization position angle remains constant. The amplitude of variability of the polarized flux is comparable to the amplitude of variability of the total U-band flux, except that the polarized flux follows the total flux with a lag of 8 +/- 3 days. The time lag and the constancy of the position angle strongly favor a scattering origin for the variable polarization rather than a non-thermal synchrotron origin. The orientation of the position angle of the polarized flux (parallel to the radio axis) and the size of the lag imply that the polarization arises from electron scattering in a flattened region within the low-ionization component of the broad-line-region. Polarization from dust scattering in the equatorial torus is ruled out as the source of the lag in polarized flux because it would produce a larger lag and, unless the half-opening angle of the torus is more than 53 degrees, the polarization would be perpendicular to the radio axis. We note a long-term change in the percentage of polarization at similar total flux levels and this could be due either to changing non-axisymmetry in the optical continuum emission, or a change in the number of scatterers on a timescale of years.
astro-ph
observations of the optical polarization of ngc 4151 in 19972003 show variations of an order of magnitude in the polarized flux while the polarization position angle remains constant the amplitude of variability of the polarized flux is comparable to the amplitude of variability of the total uband flux except that the polarized flux follows the total flux with a lag of 8 3 days the time lag and the constancy of the position angle strongly favor a scattering origin for the variable polarization rather than a nonthermal synchrotron origin the orientation of the position angle of the polarized flux parallel to the radio axis and the size of the lag imply that the polarization arises from electron scattering in a flattened region within the lowionization component of the broadlineregion polarization from dust scattering in the equatorial torus is ruled out as the source of the lag in polarized flux because it would produce a larger lag and unless the halfopening angle of the torus is more than 53 degrees the polarization would be perpendicular to the radio axis we note a longterm change in the percentage of polarization at similar total flux levels and this could be due either to changing nonaxisymmetry in the optical continuum emission or a change in the number of scatterers on a timescale of years
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711.102
Electronic structure of PrCoO_3 and its temperature evolution
We investigate the detailed electronic structure of PrCoO$_3$ and its temperature evolution using state-of-the-art photoemission spectroscopy and ab initio band structure calculations. We observe that in addition to the correlation effect, spin-orbit interaction plays an important role in determining the electronic properties of this system. Pr 4$f$ states are found to be strongly hybridized with the O 2$p$ and Co 3$d$ valence electronic states, and thus influences the electronic properties significantly. The calculated results corresponding to the intermediate spin state of Co provide a good description of the experimental spectra at 300 K. The decrease in temperature from 300 K leads to a gradual enhancement of the low spin state contributions in the electronic structure. The temperature evolution of the band gap is found to be consistent with the transport data.
cond-mat.str-el
we investigate the detailed electronic structure of prcoo_3 and its temperature evolution using stateoftheart photoemission spectroscopy and ab initio band structure calculations we observe that in addition to the correlation effect spinorbit interaction plays an important role in determining the electronic properties of this system pr 4f states are found to be strongly hybridized with the o 2p and co 3d valence electronic states and thus influences the electronic properties significantly the calculated results corresponding to the intermediate spin state of co provide a good description of the experimental spectra at 300 k the decrease in temperature from 300 k leads to a gradual enhancement of the low spin state contributions in the electronic structure the temperature evolution of the band gap is found to be consistent with the transport data
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711.1021
Paraelectric-to-ferroelectric crossover and electron dynamics from time-dependent Hartree-Fock calculations
In recent years, researchers have discovered various excited states of electrons having an excited domain with a structural order different from the original one. We examine a dynamics of electron system and phonon system by using the time-dependent Hartree-Fock approximation. We examine time evolution with spin degree of freedom. We found a thermally excited paraelectric-to-ferroelectric crossover. The metastable state is spin pierls state. We also examine the Landau expansion of electron system at quarter-filled.
cond-mat.str-el cond-mat.mtrl-sci
in recent years researchers have discovered various excited states of electrons having an excited domain with a structural order different from the original one we examine a dynamics of electron system and phonon system by using the timedependent hartreefock approximation we examine time evolution with spin degree of freedom we found a thermally excited paraelectrictoferroelectric crossover the metastable state is spin pierls state we also examine the landau expansion of electron system at quarterfilled
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711.1022
Parabolic subgroups of semisimple Lie groups and Einstein solvmanifolds
In this paper, we study the solvmanifolds constructed from any parabolic subalgebras of any semisimple Lie algebras. These solvmanifolds are naturally homogeneous submanifolds of symmetric spaces of noncompact type. We show that the Ricci curvatures of our solvmanifolds coincide with the restrictions of the Ricci curvatures of the ambient symmetric spaces. Consequently, all of our solvmanifolds are Einstein, which provide a large number of new examples of noncompact homogeneous Einstein manifolds. We also show that our solvmanifolds are minimal, but not totally geodesic submanifolds of symmetric spaces.
math.DG
in this paper we study the solvmanifolds constructed from any parabolic subalgebras of any semisimple lie algebras these solvmanifolds are naturally homogeneous submanifolds of symmetric spaces of noncompact type we show that the ricci curvatures of our solvmanifolds coincide with the restrictions of the ricci curvatures of the ambient symmetric spaces consequently all of our solvmanifolds are einstein which provide a large number of new examples of noncompact homogeneous einstein manifolds we also show that our solvmanifolds are minimal but not totally geodesic submanifolds of symmetric spaces
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711.1023
CoHochschild homology of chain coalgebras
Generalizing work of Doi and of Idrissi, we define a coHochschild homology theory for chain coalgebras over any commutative ring and prove its naturality with respect to morphisms of chain coalgebras up to strong homotopy. As a consequence we obtain that if the comultiplication of a chain coalgebra $C$ is itself a morphism of chain coalgebras up to strong homotopy, then the coHochschild complex $\cohoch (C)$ admits a natural comultiplicative structure. In particular, if $K$ is a reduced simplicial set and $C_{*}K$ is its normalized chain complex, then $\cohoch (C_{*}K)$ is naturally a homotopy-coassociative chain coalgebra. We provide a simple, explicit formula for the comultiplication on $\cohoch (C_{*}K)$ when $K$ is a simplicial suspension. The coHochschild complex construction is topologically relevant. Given two simplicial maps $g,h:K\to L$, where $K$ and $L$ are reduced, the homology of the coHochschild complex of $C_{*}L$ with coefficients in $C_{*}K$ is isomorphic to the homology of the homotopy coincidence space of the geometric realizations of $g$ and $h$, and this isomorphism respects comultiplicative structure. In particular, there a isomorphism, respecting comultiplicative structure, from the homology of $\cohoch(C_{*}K)$ to $H_{*}\op L|K|$, the homology of the free loops on the geometric realization of $K$.
math.AT
generalizing work of doi and of idrissi we define a cohochschild homology theory for chain coalgebras over any commutative ring and prove its naturality with respect to morphisms of chain coalgebras up to strong homotopy as a consequence we obtain that if the comultiplication of a chain coalgebra c is itself a morphism of chain coalgebras up to strong homotopy then the cohochschild complex cohoch c admits a natural comultiplicative structure in particular if k is a reduced simplicial set and c_k is its normalized chain complex then cohoch c_k is naturally a homotopycoassociative chain coalgebra we provide a simple explicit formula for the comultiplication on cohoch c_k when k is a simplicial suspension the cohochschild complex construction is topologically relevant given two simplicial maps ghkto l where k and l are reduced the homology of the cohochschild complex of c_l with coefficients in c_k is isomorphic to the homology of the homotopy coincidence space of the geometric realizations of g and h and this isomorphism respects comultiplicative structure in particular there a isomorphism respecting comultiplicative structure from the homology of cohochc_k to h_op lk the homology of the free loops on the geometric realization of k
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711.1024
Tuning the effective coupling of an AFM lever to a thermal bath
Fabrication of Nano-Electro-Mechanical-Systems (NEMS) of high quality is nowadays extremely efficient. These NEMS will be used as sensors and actuators in integrated systems. Their use however raises questions about their interface (actuation, detection, read out) with external detection and control systems. Their operation implies many fundamental questions related to single particle effects such as Coulomb blockade, light matter interactions such as radiation pressure, thermal effects, Casimir forces and the coupling of nanosystems to external world (thermal fluctuations, back action effect). Here we specifically present how the damping of an oscillating cantilever can be tuned in two radically different ways: i) through an electro-mechanical coupling in the presence of a strong Johnson noise, ii) through an external feedback control of thermal fluctuations which is the cold damping closely related to Maxwell's demon. This shows how the interplay between MEMS or NEMS external control and their coupling to a thermal bath can lead to a wealth of effects that are nowadays extensively studied in different areas.
cond-mat.mtrl-sci
fabrication of nanoelectromechanicalsystems nems of high quality is nowadays extremely efficient these nems will be used as sensors and actuators in integrated systems their use however raises questions about their interface actuation detection read out with external detection and control systems their operation implies many fundamental questions related to single particle effects such as coulomb blockade light matter interactions such as radiation pressure thermal effects casimir forces and the coupling of nanosystems to external world thermal fluctuations back action effect here we specifically present how the damping of an oscillating cantilever can be tuned in two radically different ways i through an electromechanical coupling in the presence of a strong johnson noise ii through an external feedback control of thermal fluctuations which is the cold damping closely related to maxwells demon this shows how the interplay between mems or nems external control and their coupling to a thermal bath can lead to a wealth of effects that are nowadays extensively studied in different areas
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711.1025
NGC 5548: The AGN Energy Budget Problem and the Geometry of the Broad-Line Region and Torus
We consider in detail the spectral energy distribution (SED) and multi-wavelength variability of NGC5548. Comparison with the SEDs of other AGNs implies that the internal reddening of NGC5548 is E(B-V) = 0.17 mag. The extinction curve is consistent with the mean curve of other AGNs found by Gaskell & Benker, but inconsistent with an SMC-type reddening curve. Because most IR emission originates exterior to the broad-line region (BLR), the SED seen by the inner BLR is different from that seen by the outer BLR and from the earth. The most likely BLR covering factor is ~ 40% and it is not possible to get an overall BLR covering factor of less than 20%. This requires that the BLR is not spherically symmetric and that we are viewing through a hole. Line-continuum variability transfer functions are consistent with this geometry. The covering factor and geometry imply that near the equatorial plane the BLR covering approaches 100%. The spectrum seen by the outer regions of the BLR and by the torus is thus modified by the absorption in the inner BLR. This shielding solves the problem of observed BLR ionization stratification being much greater than implied by photoionization models. The BLR obscuration also removes the problem of the torus covering factor being greater than the BLR covering factor, and gives consistency with the observed fraction of obscured AGNs. The flux reduction at the torus also reduces the problem of AGN dust-reverberation lags giving sizes smaller than the dust-sublimation radii.
astro-ph
we consider in detail the spectral energy distribution sed and multiwavelength variability of ngc5548 comparison with the seds of other agns implies that the internal reddening of ngc5548 is ebv 017 mag the extinction curve is consistent with the mean curve of other agns found by gaskell benker but inconsistent with an smctype reddening curve because most ir emission originates exterior to the broadline region blr the sed seen by the inner blr is different from that seen by the outer blr and from the earth the most likely blr covering factor is 40 and it is not possible to get an overall blr covering factor of less than 20 this requires that the blr is not spherically symmetric and that we are viewing through a hole linecontinuum variability transfer functions are consistent with this geometry the covering factor and geometry imply that near the equatorial plane the blr covering approaches 100 the spectrum seen by the outer regions of the blr and by the torus is thus modified by the absorption in the inner blr this shielding solves the problem of observed blr ionization stratification being much greater than implied by photoionization models the blr obscuration also removes the problem of the torus covering factor being greater than the blr covering factor and gives consistency with the observed fraction of obscured agns the flux reduction at the torus also reduces the problem of agn dustreverberation lags giving sizes smaller than the dustsublimation radii
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711.1026
Finite subsets of projective space, and their ideals
Let $\mathscr{A}$ be a finite set of closed rational points in projective space, let $\mathscr{I}$ be the vanishing ideal of $\mathscr{A}$, and let $\mathscr{D}(\mathscr{A})$ be the set of exponents of those monomials which do not occur as leading monomials of elements of $\mathscr{I}$. We show that the size of $\mathscr{A}$ equals the number of axes contained in $\mathscr{D}(\mathscr{A})$. Furthermore, we present an algorithm for the construction of the Gr\"obner basis of $\mathscr{I}(\mathscr{A})$, hence also of $\mathscr{D}(\mathscr{A})$.
math.AC
let mathscra be a finite set of closed rational points in projective space let mathscri be the vanishing ideal of mathscra and let mathscrdmathscra be the set of exponents of those monomials which do not occur as leading monomials of elements of mathscri we show that the size of mathscra equals the number of axes contained in mathscrdmathscra furthermore we present an algorithm for the construction of the grobner basis of mathscrimathscra hence also of mathscrdmathscra
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711.1027
Ultrahigh energy cosmic rays as heavy nuclei from cluster accretion shocks
Large-scale accretion shocks around massive clusters of galaxies, generically expected in hierarchical scenarios of cosmological structure formation, are shown to be potential sources of the observed ultrahigh energy cosmic rays (UHECRs) by accelerating a mixture of heavy nuclei including the iron group elements. Current observations can be explained if the source composition at injection for the heavier nuclei is somewhat enhanced from simple expectations for the accreting gas. The proposed picture should be testable by current and upcoming facilities in the near future through characteristic features in the UHECR spectrum, composition and anisotropy. The associated X-ray and gamma-ray signatures are also briefly discussed.
astro-ph
largescale accretion shocks around massive clusters of galaxies generically expected in hierarchical scenarios of cosmological structure formation are shown to be potential sources of the observed ultrahigh energy cosmic rays uhecrs by accelerating a mixture of heavy nuclei including the iron group elements current observations can be explained if the source composition at injection for the heavier nuclei is somewhat enhanced from simple expectations for the accreting gas the proposed picture should be testable by current and upcoming facilities in the near future through characteristic features in the uhecr spectrum composition and anisotropy the associated xray and gammaray signatures are also briefly discussed
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711.1028
Structure on Interplanetary Shock Fronts: Type II Radio Burst Source Regions
We present \emph{in situ} observations of the source regions of interplanetary (IP) type II radio bursts, using data from the Wind spacecraft during the period 1996-2002. We show the results of this survey as well as in-depth analysis of several individual events. Each event analyzed in detail is associated with an interplanetary coronal mass ejection (ICME) and an IP shock driven by the ICME. Immediately prior to the arrival of each shock, electron beams along the interplanetary magnetic field (IMF) and associated Langmuir waves are detected, implying magnetic connection to a quasiperpendicular shock front acceleration site. These observations are analogous to those made in the terrestrial foreshock region, indicating that a similar foreshock region exists on IP shock fronts. The analogy suggests that the electron acceleration process is a fast Fermi process, and this suggestion is borne out by loss cone features in the electron distribution functions. The presence of a foreshock region requires nonplanar structure on the shock front. Using Wind burst mode data, the foreshock electrons are analyzed to estimate the dimensions of the curved region. We present the first measurement of the lateral, shock-parallel scale size of IP foreshock regions. The presence of these regions on IP shock fronts can explain the fine structure often seen in the spectra of type II bursts.
physics.space-ph
we present emphin situ observations of the source regions of interplanetary ip type ii radio bursts using data from the wind spacecraft during the period 19962002 we show the results of this survey as well as indepth analysis of several individual events each event analyzed in detail is associated with an interplanetary coronal mass ejection icme and an ip shock driven by the icme immediately prior to the arrival of each shock electron beams along the interplanetary magnetic field imf and associated langmuir waves are detected implying magnetic connection to a quasiperpendicular shock front acceleration site these observations are analogous to those made in the terrestrial foreshock region indicating that a similar foreshock region exists on ip shock fronts the analogy suggests that the electron acceleration process is a fast fermi process and this suggestion is borne out by loss cone features in the electron distribution functions the presence of a foreshock region requires nonplanar structure on the shock front using wind burst mode data the foreshock electrons are analyzed to estimate the dimensions of the curved region we present the first measurement of the lateral shockparallel scale size of ip foreshock regions the presence of these regions on ip shock fronts can explain the fine structure often seen in the spectra of type ii bursts
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711.1029
Four-quark Bound States in Chiral SU(3) Quark Model
The possibility of $QQ\bar{q}\bar{q}$ heavy-light four-quark bound states has been analyzed by means of the chiral SU(3) quark model, where $Q$ is the heavy quark ($c$ or $b$) and $q$ is the light quark ($u$, $d$ or $s$). We obtain a bound state for the $bb\bar{n}\bar{n}$ configuration with quantum number $J^{P}=1^{+},I=0$ and for the $cc\bar{n}\bar{n}$ ($J^{P}=1^{+},I=0$) configuration which is not bound but slightly above the $D^{*}D^{*}$ threshold (n is $u$ or $d$ quark). Meanwhile, we also conclude that a weakly bound state in $bb\bar{n}\bar{n}$ system can also be found without considering the chiral quark interactions between the two light quarks, yet its binding energy is weaker than that with the chiral quark interactions.
nucl-th
the possibility of qqbarqbarq heavylight fourquark bound states has been analyzed by means of the chiral su3 quark model where q is the heavy quark c or b and q is the light quark u d or s we obtain a bound state for the bbbarnbarn configuration with quantum number jp1i0 and for the ccbarnbarn jp1i0 configuration which is not bound but slightly above the dd threshold n is u or d quark meanwhile we also conclude that a weakly bound state in bbbarnbarn system can also be found without considering the chiral quark interactions between the two light quarks yet its binding energy is weaker than that with the chiral quark interactions
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711.103
Can one extract energy loss probability distributions from R_AA?
The nuclear suppression of high transverse momentum P_T hadrons is one of the most striking findings in heavy-ion collision experiments. It has long been recognized that the suppression can be theoretically described by folding the primary parton spectrum with an energy loss probability distribution which is suitably averaged over the collision geometry. However, an interesting problem is to what degree the procedure can be inverted, i.e. given a measurement of the suppression factor R_AA with arbitrary precision, can the probability distribution of energy loss be extracted in a model-independent way? In this note, we present a conceptual study of the inversion problem for LHC energies and demonstrate that a measurement of R_AA alone is insufficient to determine the distribution, other observables such as gamma-hadron correlations must be taken into account.
hep-ph
the nuclear suppression of high transverse momentum p_t hadrons is one of the most striking findings in heavyion collision experiments it has long been recognized that the suppression can be theoretically described by folding the primary parton spectrum with an energy loss probability distribution which is suitably averaged over the collision geometry however an interesting problem is to what degree the procedure can be inverted ie given a measurement of the suppression factor r_aa with arbitrary precision can the probability distribution of energy loss be extracted in a modelindependent way in this note we present a conceptual study of the inversion problem for lhc energies and demonstrate that a measurement of r_aa alone is insufficient to determine the distribution other observables such as gammahadron correlations must be taken into account
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711.1031
Performance of Wang-Landau algorithm in continuous spin models and a case study : modified XY-model
Performance of Wang-Landau (W-L) algorithm in two continuous spin models is tested by determining the fluctuations in energy histogram. Finite size scaling is performed on a modified XY-model using different W-L sampling schemes. Difficulties faced in simulating relatively large continuous systems using W-L algorithm are discussed.
cond-mat.stat-mech
performance of wanglandau wl algorithm in two continuous spin models is tested by determining the fluctuations in energy histogram finite size scaling is performed on a modified xymodel using different wl sampling schemes difficulties faced in simulating relatively large continuous systems using wl algorithm are discussed
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711.1032
A Diagrammatic Approach for the Coefficients of the Characteristic Polynomial
In this work we provide a novel approach for computing the coefficients of the characteristic polynomial of a square matrix. We demonstrate that each coefficient can be efficiently represented by a set of circle graphs. Thus, one can employ a diagrammatic approach to determine the coefficients of the characteristic polynomial.
math-ph math.MP
in this work we provide a novel approach for computing the coefficients of the characteristic polynomial of a square matrix we demonstrate that each coefficient can be efficiently represented by a set of circle graphs thus one can employ a diagrammatic approach to determine the coefficients of the characteristic polynomial
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711.1033
Anisotropic Higgs oscillator
We present the higher-dimensional generalization of anisotropic (pseudo)spherical oscillator suggested recently in [arXiv:0710.5001], and the related spherical and pseudosperical generalizations (MICZ-)Kepler like systems with Stark term and $\cos\theta$ potential. We write down the potentials and hidden symmetry generators of these systems, in terms of ambient Euclidean space.
math-ph hep-th math.MP
we present the higherdimensional generalization of anisotropic pseudospherical oscillator suggested recently in arxiv07105001 and the related spherical and pseudosperical generalizations miczkepler like systems with stark term and costheta potential we write down the potentials and hidden symmetry generators of these systems in terms of ambient euclidean space
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711.1034
Shear viscosity of a hadronic gas mixture
We discuss in detail the shear viscosity coefficient eta and the viscosity to entropy density ratio eta/s of a hadronic gas comprised of pions and nucleons. In particular, we study the effects of baryon chemical potential on eta and eta/s. We solve the relativistic quantum Boltzmann equations with binary collisions (pi pi, pi N, and NN) for a state slightly deviated from thermal equilibrium at temperature T and baryon chemical potential mu. The use of phenomenological amplitudes in the collision terms, which are constructed to reproduce experimental data, greatly helps to extend the validity region in the T-mu plane. The total viscosity coefficient eta(T,mu)=eta^pi + eta^N increases as a function of T and mu, indirectly reflecting energy dependences of binary cross sections. The increase in mu direction is due to enhancement of the nucleon contribution eta^N while the pion contribution eta^pi diminishes with increasing mu. On the other hand, due to rapid growth of entropy density, the ratio eta/s becomes a decreasing function of T and mu in a wide region of the T-mu plane. In the kinematical region we investigated T < 180MeV, mu < 1GeV, the smallest value of eta/s is about 0.3. Thus, it never violates the conjectured lower bound eta/s= 1/4pi ~ 0.1. The smallness of eta/s in the hadronic phase and its continuity at T ~ T_c (at least for crossover at small mu) implies that the ratio will be small enough in the deconfined phase T > T_c. There is a nontrivial structure at low temperature and at around normal nuclear density. We examine its possible interpretation as the liquid-gas phase transition.
hep-ph nucl-th
we discuss in detail the shear viscosity coefficient eta and the viscosity to entropy density ratio etas of a hadronic gas comprised of pions and nucleons in particular we study the effects of baryon chemical potential on eta and etas we solve the relativistic quantum boltzmann equations with binary collisions pi pi pi n and nn for a state slightly deviated from thermal equilibrium at temperature t and baryon chemical potential mu the use of phenomenological amplitudes in the collision terms which are constructed to reproduce experimental data greatly helps to extend the validity region in the tmu plane the total viscosity coefficient etatmuetapi etan increases as a function of t and mu indirectly reflecting energy dependences of binary cross sections the increase in mu direction is due to enhancement of the nucleon contribution etan while the pion contribution etapi diminishes with increasing mu on the other hand due to rapid growth of entropy density the ratio etas becomes a decreasing function of t and mu in a wide region of the tmu plane in the kinematical region we investigated t 180mev mu 1gev the smallest value of etas is about 03 thus it never violates the conjectured lower bound etas 14pi 01 the smallness of etas in the hadronic phase and its continuity at t t_c at least for crossover at small mu implies that the ratio will be small enough in the deconfined phase t t_c there is a nontrivial structure at low temperature and at around normal nuclear density we examine its possible interpretation as the liquidgas phase transition
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711.1035
Skew domino Schensted algorithm and sign-imbalance
Using growth diagrams, we define a skew domino Schensted correspondence which is a domino analogue of the skew Robinson-Schensted correspondence due to Sagan and Stanley. The color-to-spin property of Shimozono and White is extended. As an application, we give a simple generating function for the weighted sum of skew domino tableaux, which is a generalization of Stanley's sign-imbalance formula. The generating function gives a method to calculate the generalized sign-imbalance formula. We also extend Sj{\"o}strand's theorems on sign-imbalance of skew shapes.
math.CO
using growth diagrams we define a skew domino schensted correspondence which is a domino analogue of the skew robinsonschensted correspondence due to sagan and stanley the colortospin property of shimozono and white is extended as an application we give a simple generating function for the weighted sum of skew domino tableaux which is a generalization of stanleys signimbalance formula the generating function gives a method to calculate the generalized signimbalance formula we also extend sjostrands theorems on signimbalance of skew shapes
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711.1036
Confidence Sets Based on Sparse Estimators Are Necessarily Large
Confidence sets based on sparse estimators are shown to be large compared to more standard confidence sets, demonstrating that sparsity of an estimator comes at a substantial price in terms of the quality of the estimator. The results are set in a general parametric or semiparametric framework.
math.ST stat.ME stat.TH
confidence sets based on sparse estimators are shown to be large compared to more standard confidence sets demonstrating that sparsity of an estimator comes at a substantial price in terms of the quality of the estimator the results are set in a general parametric or semiparametric framework
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711.1037
Generalizations of MICZ-Kepler system
We discuss the generalizations of the MICZ-Kepler system (the system describing the motion of the charged particle in the field of Dirac dyon), to the curved spaces, arbitrary potentials and to the multi-dyon background.
math-ph hep-th math.MP
we discuss the generalizations of the miczkepler system the system describing the motion of the charged particle in the field of dirac dyon to the curved spaces arbitrary potentials and to the multidyon background
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711.1038
Am\'elioration des Performances des Syst\`emes Automatiques de Reconnaissance de la Parole pour la Parole Non Native
In this article, we present an approach for non native automatic speech recognition (ASR). We propose two methods to adapt existing ASR systems to the non-native accents. The first method is based on the modification of acoustic models through integration of acoustic models from the mother tong. The phonemes of the target language are pronounced in a similar manner to the native language of speakers. We propose to combine the models of confused phonemes so that the ASR system could recognize both concurrent pronounciations. The second method we propose is a refinment of the pronounciation error detection through the introduction of graphemic constraints. Indeed, non native speakers may rely on the writing of words in their uttering. Thus, the pronounctiation errors might depend on the characters composing the words. The average error rate reduction that we observed is (22.5%) relative for the sentence error rate, and 34.5% (relative) in word error rate.
cs.CL
in this article we present an approach for non native automatic speech recognition asr we propose two methods to adapt existing asr systems to the nonnative accents the first method is based on the modification of acoustic models through integration of acoustic models from the mother tong the phonemes of the target language are pronounced in a similar manner to the native language of speakers we propose to combine the models of confused phonemes so that the asr system could recognize both concurrent pronounciations the second method we propose is a refinment of the pronounciation error detection through the introduction of graphemic constraints indeed non native speakers may rely on the writing of words in their uttering thus the pronounctiation errors might depend on the characters composing the words the average error rate reduction that we observed is 225 relative for the sentence error rate and 345 relative in word error rate
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711.1039
Following microscopic motion in a two dimensional glass-forming binary fluid
The dynamics of a binary mixture of large and small discs are studied at temperatures approaching the glass transition using an analysis based on the topology of the Voronoi polygon surrounding each atom. At higher temperatures we find that dynamics is dominated by fluid-like motion that involves particles entering and exiting the nearest-neighbour shells of nearby particles. As the temperature is lowered, the rate of topological moves decreases and motion becomes localised to regions of mixed pentagons and heptagons. In addition we find that in the low temperature state particles may translate significant distances without undergoing changes in their nearest neig hbour shell. These results have implications for dynamical heterogeneities in glass forming liquids.
cond-mat.soft
the dynamics of a binary mixture of large and small discs are studied at temperatures approaching the glass transition using an analysis based on the topology of the voronoi polygon surrounding each atom at higher temperatures we find that dynamics is dominated by fluidlike motion that involves particles entering and exiting the nearestneighbour shells of nearby particles as the temperature is lowered the rate of topological moves decreases and motion becomes localised to regions of mixed pentagons and heptagons in addition we find that in the low temperature state particles may translate significant distances without undergoing changes in their nearest neig hbour shell these results have implications for dynamical heterogeneities in glass forming liquids
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711.104
Statistics of Resonances in a Semi-infinite Disordered Chain
We study the average density of resonances (DOR) for a semi-infinite disordered chain, coupled to the outside world by a (semi-infinite) perfect lead. A set of equations is derived, which provides the general framework for calculating the average DOR, for an arbitrary disorder and coupling strength. These general equations are applied to the case of weak coupling and an asymptotically exact expression for the averaged DOR is derived, in the limit of small resonance width. This expression is universal, in the sense that it holds for any degree of disorder and everywhere in the (unperturbed) energy band.
cond-mat.dis-nn cond-mat.other math-ph math.MP
we study the average density of resonances dor for a semiinfinite disordered chain coupled to the outside world by a semiinfinite perfect lead a set of equations is derived which provides the general framework for calculating the average dor for an arbitrary disorder and coupling strength these general equations are applied to the case of weak coupling and an asymptotically exact expression for the averaged dor is derived in the limit of small resonance width this expression is universal in the sense that it holds for any degree of disorder and everywhere in the unperturbed energy band
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711.1041
Some Conformal Invariants from the Noncommutative Residue for Manifolds with Boundary
We review previous work of Alain Connes, and its extension by the author, on some conformal invariants obtained from the noncommutative residue on even dimensional compact manifolds without boundary. Inspired by recent work of Yong Wang, we also address possible generalizations of these conformal invariants to the setting of compact manifolds with boundary.
math.DG math-ph math.MP
we review previous work of alain connes and its extension by the author on some conformal invariants obtained from the noncommutative residue on even dimensional compact manifolds without boundary inspired by recent work of yong wang we also address possible generalizations of these conformal invariants to the setting of compact manifolds with boundary
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711.1042
Efficient light coupling from integrated single-mode waveguides to supercollimating photonic crystals on silicon-on-insulator platforms
We propose a practical and efficient solution for the coupling of light from integrated single-mode waveguides to supercollimating planar photonic crystals on conventional silicon-on-insulator platforms. The device consists of a rib waveguide, designed to sustain spatially extended single-modes and matched to a supercollimating photonic crystal, which has been truncated at its boundary to improve impedance matching between the two photonic components. Three-dimensional simulations show transmission efficiencies up to 96 % and reflections below 0.2 % at wavelengths close to 1.55 microns. This approach constitutes a significant step toward the integration of supercollimating structures on photonic chips.
physics.optics
we propose a practical and efficient solution for the coupling of light from integrated singlemode waveguides to supercollimating planar photonic crystals on conventional silicononinsulator platforms the device consists of a rib waveguide designed to sustain spatially extended singlemodes and matched to a supercollimating photonic crystal which has been truncated at its boundary to improve impedance matching between the two photonic components threedimensional simulations show transmission efficiencies up to 96 and reflections below 02 at wavelengths close to 155 microns this approach constitutes a significant step toward the integration of supercollimating structures on photonic chips
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711.1043
Cosmological models in scalar tensor theories of gravity and observations: a class of general solutions
We consider cosmological models in scalar tensor theories of gravity that describe an accelerating universe, and we study a family of inverse power law potentials, for which exact solutions of the Einstein equations are known. We also compare theoretical predictions of our models with observations. For this we use the following data: the publicly available catalogs of type Ia supernovae and high redshift Gamma Ray Bursts, the parameters of large scale structure determined by the 2-degree Field Galaxy Redshift Survey (2dFGRS), and measurements of cosmological distances based on the Sunyaev-Zel'dovich effect, among others.
astro-ph
we consider cosmological models in scalar tensor theories of gravity that describe an accelerating universe and we study a family of inverse power law potentials for which exact solutions of the einstein equations are known we also compare theoretical predictions of our models with observations for this we use the following data the publicly available catalogs of type ia supernovae and high redshift gamma ray bursts the parameters of large scale structure determined by the 2degree field galaxy redshift survey 2dfgrs and measurements of cosmological distances based on the sunyaevzeldovich effect among others
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711.1044
Can Massive Dark Haloes Destroy the Disks of Dwarf Galaxies?
Recent high-resolution simulations together with theoretical studies of the dynamical evolution of galactic disks have shown that contrary to wide-held beliefs a `live', dynamically responsive, dark halo surrounding a disk does not stabilize the disk against dynamical instabilities. We generalize Toomre's Q stability parameter for a disk-halo system and show that if a disk, which would be otherwise stable, is embedded in a halo, which is too massive and cold, the combined disk-halo system can become locally Jeans unstable. The good news is, on the other hand, that this will not happen in real dark haloes, which are in radial hydrostatic equilibrium. Even very low-mass disks are not prone to such dynamical instabilities.
astro-ph
recent highresolution simulations together with theoretical studies of the dynamical evolution of galactic disks have shown that contrary to wideheld beliefs a live dynamically responsive dark halo surrounding a disk does not stabilize the disk against dynamical instabilities we generalize toomres q stability parameter for a diskhalo system and show that if a disk which would be otherwise stable is embedded in a halo which is too massive and cold the combined diskhalo system can become locally jeans unstable the good news is on the other hand that this will not happen in real dark haloes which are in radial hydrostatic equilibrium even very lowmass disks are not prone to such dynamical instabilities
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711.1045
Mirrorfolds with K3 Fibrations
We study a class of non-geometric string vacua realized as completely soluble superconformal field theory (SCFT). These models are defined as `interpolating orbifolds' of $K3 \times S^1$ by the mirror transformation acting on the $K3$ fiber combined with the half-shift on the $S^1$-base. They are variants of the T-folds, the interpolating orbifolds by T-duality transformations, and thus may be called `mirrorfolds'. Starting with arbitrary (compact or non-compact) Gepner models for the $K3$ fiber, we construct modular invariant partition functions of general mirrorfold models. In the case of compact $K3$ fiber the mirrorfolds only yield non-supersymmetric string vacua. They exhibit IR instability due to winding tachyon condensation which is similar to the Scherk-Schwarz type circle compactification. When the fiber SCFT is non-compact (say, the ALE space in the simplest case), on the other hand, both supersymmetric and non-supersymmetric vacua can be constructed. The non-compact non-supersymmetric mirrorfolds can get stabilised at the level of string perturbation theory. We also find that in the non-compact supersymmeric mirrorfolds D-branes are {\em always} non-BPS. These D-branes can get stabilized against both open- and closed-string marginal deformations.
hep-th
we study a class of nongeometric string vacua realized as completely soluble superconformal field theory scft these models are defined as interpolating orbifolds of k3 times s1 by the mirror transformation acting on the k3 fiber combined with the halfshift on the s1base they are variants of the tfolds the interpolating orbifolds by tduality transformations and thus may be called mirrorfolds starting with arbitrary compact or noncompact gepner models for the k3 fiber we construct modular invariant partition functions of general mirrorfold models in the case of compact k3 fiber the mirrorfolds only yield nonsupersymmetric string vacua they exhibit ir instability due to winding tachyon condensation which is similar to the scherkschwarz type circle compactification when the fiber scft is noncompact say the ale space in the simplest case on the other hand both supersymmetric and nonsupersymmetric vacua can be constructed the noncompact nonsupersymmetric mirrorfolds can get stabilised at the level of string perturbation theory we also find that in the noncompact supersymmeric mirrorfolds dbranes are em always nonbps these dbranes can get stabilized against both open and closedstring marginal deformations
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711.1046
Classical probability waves
Probability waves in the configuration space are associated with coherent solutions of the classical Liouville or Fokker-Planck equations. Distributions localized in the momentum space provide action waves, specified by the probability density and the generating function of the Hamilton-Jacobi theory. It is shown that by introducing a minimum distance in the coordinate space, the action distributions aquire the energy dispersion specific to the quantum objects. At finite temperature, probability density waves propagating with the sound velocity are obtained as nonstationary solutions of the classical Fokker-Planck equation. The results suggest that in a system of quantum Brownian particles, a transition from complex to real probability waves could be observed.
quant-ph gr-qc math-ph math.MP
probability waves in the configuration space are associated with coherent solutions of the classical liouville or fokkerplanck equations distributions localized in the momentum space provide action waves specified by the probability density and the generating function of the hamiltonjacobi theory it is shown that by introducing a minimum distance in the coordinate space the action distributions aquire the energy dispersion specific to the quantum objects at finite temperature probability density waves propagating with the sound velocity are obtained as nonstationary solutions of the classical fokkerplanck equation the results suggest that in a system of quantum brownian particles a transition from complex to real probability waves could be observed
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711.1047
Core polarization in coupled-cluster theory induced by a parity and time-reversal violating interaction
The effects of parity and time reversal violating potential, in particular the tensor-pseudotensor electron nucleus interaction are studied. We establish that selected terms representing the interplay of these effects and the residual Coulomb interaction in the coupled-cluster method are equivalent to the coupled perturbed Hartree-Fock. We have shown that the {\em normal} CPHF diagrams have a one-one correspondance in the coupled-cluster theory, but the CPHF pseudo diagrams are present in a subtle way. We have studied the {\em pseudo} diagrams in great detail and have shown explicitly their origin in coupled-cluster theory. This is demonstrated by considering the case of the permanent electric dipole moment of atomic Hg and our results are compared with the results of an earlier calculation.
physics.atom-ph
the effects of parity and time reversal violating potential in particular the tensorpseudotensor electron nucleus interaction are studied we establish that selected terms representing the interplay of these effects and the residual coulomb interaction in the coupledcluster method are equivalent to the coupled perturbed hartreefock we have shown that the em normal cphf diagrams have a oneone correspondance in the coupledcluster theory but the cphf pseudo diagrams are present in a subtle way we have studied the em pseudo diagrams in great detail and have shown explicitly their origin in coupledcluster theory this is demonstrated by considering the case of the permanent electric dipole moment of atomic hg and our results are compared with the results of an earlier calculation
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711.1048
Hamiltonian of two spinning compact bodies with next-to-leading order gravitational spin-orbit coupling
A Hamiltonian formulation is given for the gravitational dynamics of two spinning compact bodies to next-to-leading order ($G/c^4$ and $G^2/c^4$) in the spin-orbit interaction. We use a novel approach (valid to linear order in the spins), which starts from the second-post-Newtonian metric (in ADM coordinates) generated by two spinless bodies, and computes the next-to-leading order precession, in this metric, of suitably redefined ``constant-magnitude'' 3-dimensional spin vectors ${\bf S}_1$, ${\bf S}_2$. We prove the Poincar\'e invariance of our Hamiltonian by explicitly constructing ten phase-space generators realizing the Poincar\'e algebra. A remarkable feature of our approach is that it allows one to derive the {\it orbital} equations of motion of spinning binaries to next-to-leading order in spin-orbit coupling without having to solve Einstein's field equations with a spin-dependent stress tensor. We show that our Hamiltonian (orbital and spin) dynamics is equivalent to the dynamics recently obtained by Faye, Blanchet, and Buonanno, by solving Einstein's equations in harmonic coordinates.
gr-qc
a hamiltonian formulation is given for the gravitational dynamics of two spinning compact bodies to nexttoleading order gc4 and g2c4 in the spinorbit interaction we use a novel approach valid to linear order in the spins which starts from the secondpostnewtonian metric in adm coordinates generated by two spinless bodies and computes the nexttoleading order precession in this metric of suitably redefined constantmagnitude 3dimensional spin vectors bf s_1 bf s_2 we prove the poincare invariance of our hamiltonian by explicitly constructing ten phasespace generators realizing the poincare algebra a remarkable feature of our approach is that it allows one to derive the it orbital equations of motion of spinning binaries to nexttoleading order in spinorbit coupling without having to solve einsteins field equations with a spindependent stress tensor we show that our hamiltonian orbital and spin dynamics is equivalent to the dynamics recently obtained by faye blanchet and buonanno by solving einsteins equations in harmonic coordinates
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711.1049
Non-unitary leptonic mixing and CP-violation
Some theories of new physics accounting for neutrino masses can give rise to a low-energy non-unitary leptonic mixing matrix. It is shown that the CP-asymmetries in the $\nu_\mu\to \nu_\tau$ channel are an excellent probe of such new physics. In adition, we clarify the relationship betweeen our framework and the so called "non-standard neutrino interactions" scenarios: the sensitivities explored here apply as well to such constructions, except for extremely fine-tuned cancellations.
hep-ph
some theories of new physics accounting for neutrino masses can give rise to a lowenergy nonunitary leptonic mixing matrix it is shown that the cpasymmetries in the nu_muto nu_tau channel are an excellent probe of such new physics in adition we clarify the relationship betweeen our framework and the so called nonstandard neutrino interactions scenarios the sensitivities explored here apply as well to such constructions except for extremely finetuned cancellations
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711.105
On the backwards difference filter
It is usual in helioseismology to remove unwanted instrumental low-frequency trends by applying high-pass filters to the time series. However, the choice of the filter is very important because it can keep the periodic signals throughout the spectrum. At the same time, these filters should not introduce any spurious effects on the remaining signal, which would modify the periodic signatures in the Fourier domain. One of the most used filters is the so-called backwards difference filter that can be applied when the time series are regularly sampled. The problem of this filter is that the amplitudes and the phases of the periodic signals in the Fourier domain are modified and, therefore, their extracted amplitudes are biased when the frequency of the periodic signals decreases. The objective of this research note is to give a correction that could be applied to the power spectrum to over come this problem. We properly derive the transfer function of the backwards difference filter and we show how this can be applied to the power spectrum to correct the amplitudes. For the amplitude spectrum and the time series, we also derive a correction for the phase. The amplitudes of the periodic signals in the resultant power spectrum density are corrected from the cut-off frequency down to zero.
astro-ph
it is usual in helioseismology to remove unwanted instrumental lowfrequency trends by applying highpass filters to the time series however the choice of the filter is very important because it can keep the periodic signals throughout the spectrum at the same time these filters should not introduce any spurious effects on the remaining signal which would modify the periodic signatures in the fourier domain one of the most used filters is the socalled backwards difference filter that can be applied when the time series are regularly sampled the problem of this filter is that the amplitudes and the phases of the periodic signals in the fourier domain are modified and therefore their extracted amplitudes are biased when the frequency of the periodic signals decreases the objective of this research note is to give a correction that could be applied to the power spectrum to over come this problem we properly derive the transfer function of the backwards difference filter and we show how this can be applied to the power spectrum to correct the amplitudes for the amplitude spectrum and the time series we also derive a correction for the phase the amplitudes of the periodic signals in the resultant power spectrum density are corrected from the cutoff frequency down to zero
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711.1051
Low-energy structure of the intertwining double-chain ferrimagnets A_3_Cu_3_(PO_4_)_4_ (A=Ca,Sr,Pb)
Motivated by the homometallic intertwining double-chain ferrimagnets A_3_Cu_3_(PO_4_)_4_ (A=Ca,Sr,Pb), we investigate the low-energy structure of their model Hamiltonian H=\sum_n_[J_1_(S_{n :1}_+S_{n :3}_) +J_2_(S_{n+1:1}+S_{n-1:3}_)]\cdotS_{n:2}_, where S_{n:l}_ stands for the Cu^{2+}^ ion spin labeled l in the nth trimer unit, with particular emphasis on the range of bond alternation 0<J_2/J_1<1. Although the spin-wave theory, whether up to O(S^1^) or up to O(S^0^), claims that there exists a flat band in the excitation spectrum regardless of bond alternation, a perturbational treatment as well as the exact diagonalization of the Hamiltonian reveals its weak but nonvanishing momentum dispersion unless J_2_=J_1_ or J_2_=0. Quantum Monte Carlo calculations of the static structure factor further convince us of the low-lying excitation mechanism, elucidating similarities and differences between the present system and alternating-spin linear-chain ferrimagnets.
cond-mat.str-el cond-mat.stat-mech
motivated by the homometallic intertwining doublechain ferrimagnets a_3_cu_3_po_4__4_ acasrpb we investigate the lowenergy structure of their model hamiltonian hsum_n_j_1_s_n 1_s_n 3_ j_2_s_n11s_n13_cdots_n2_ where s_nl_ stands for the cu2 ion spin labeled l in the nth trimer unit with particular emphasis on the range of bond alternation 0j_2j_11 although the spinwave theory whether up to os1 or up to os0 claims that there exists a flat band in the excitation spectrum regardless of bond alternation a perturbational treatment as well as the exact diagonalization of the hamiltonian reveals its weak but nonvanishing momentum dispersion unless j_2_j_1_ or j_2_0 quantum monte carlo calculations of the static structure factor further convince us of the lowlying excitation mechanism elucidating similarities and differences between the present system and alternatingspin linearchain ferrimagnets
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711.1052
Optical characterization of platinum-halide ladder compounds
New varieties of quasi-one-dimensional halogen (X)-bridged transition-metal (M) complexes, (C_8_H_6_N_4_)[Pt(C_2_H_8_N_2_)X]_2_X(ClO_4_)_3_\cdotH_2_O (X=Br,Cl) and (C_10_H_8_N_2_)[Pt(C_4_H_13_N_3_)Br]_2_Br_4_\cdot2H_2_O, comprising two-leg ladders of mixed-valent platinum ions, are described in terms of a multiband extended Peierls-Hubbard Hamiltonian. The polarized optical conductivity spectra are theoretically reproduced and the ground-state valence distributions are reasonably determined. The latter variety, whose interchain valence arrangement is out of phase, is reminiscent of conventional MX single-chain compounds, while the former variety, whose interchain valence arrangement is in phase, reveals itself as a novel d-p-\pi-hybridized multiband ladder material.
cond-mat.str-el cond-mat.mtrl-sci
new varieties of quasionedimensional halogen xbridged transitionmetal m complexes c_8_h_6_n_4_ptc_2_h_8_n_2_x_2_xclo_4__3_cdoth_2_o xbrcl and c_10_h_8_n_2_ptc_4_h_13_n_3_br_2_br_4_cdot2h_2_o comprising twoleg ladders of mixedvalent platinum ions are described in terms of a multiband extended peierlshubbard hamiltonian the polarized optical conductivity spectra are theoretically reproduced and the groundstate valence distributions are reasonably determined the latter variety whose interchain valence arrangement is out of phase is reminiscent of conventional mx singlechain compounds while the former variety whose interchain valence arrangement is in phase reveals itself as a novel dppihybridized multiband ladder material
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711.1053
Microscopic modeling of a spin crossover transition
In spin crossover materials, an abrupt phase transition between a low spin state and a high spin state can be driven by temperature, pressure or by light irradiation. Of a special relevance are Fe(II) based coordination polymers where, in contrast to molecular systems, the phase transition between a spin S=0 and a spin S=2 state shows a pronounced hysteresis which is desirable for technical applications. A satisfactory microscopic explanation of this large cooperative phenomenon has been sought for a long time. The lack of X-ray data has been one of the reasons for the absence of microscopic studies. In this work, we present an efficient route to prepare reliable model structures and within an ab initio density functional theory analysis and effective model considerations we show that in polymeric spin crossover compounds magnetic exchange between high spin Fe(II) centers is as important as elastic couplings for understanding the phase transition. We discuss the relevance of these interactions for the cooperative behavior in these materials.
cond-mat.mtrl-sci
in spin crossover materials an abrupt phase transition between a low spin state and a high spin state can be driven by temperature pressure or by light irradiation of a special relevance are feii based coordination polymers where in contrast to molecular systems the phase transition between a spin s0 and a spin s2 state shows a pronounced hysteresis which is desirable for technical applications a satisfactory microscopic explanation of this large cooperative phenomenon has been sought for a long time the lack of xray data has been one of the reasons for the absence of microscopic studies in this work we present an efficient route to prepare reliable model structures and within an ab initio density functional theory analysis and effective model considerations we show that in polymeric spin crossover compounds magnetic exchange between high spin feii centers is as important as elastic couplings for understanding the phase transition we discuss the relevance of these interactions for the cooperative behavior in these materials
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711.1054
Heralded Generation of Ultrafast Single Photons in Pure Quantum States
We present an experimental demonstration of heralded single photons prepared in pure quantum states from a parametric downconversion source. It is shown that, through controlling the modal structure of the photon pair emission, one can generate pairs in factorable states and thence eliminate the need for spectral filters in multiple-source interference schemes. Indistinguishable heralded photons were generated in two independent spectrally engineered sources, and, by performing a Hong-Ou-Mandel interference between them without spectral filters at a raw visibility of 94.4%, their purity was measured to be over 95%.
quant-ph
we present an experimental demonstration of heralded single photons prepared in pure quantum states from a parametric downconversion source it is shown that through controlling the modal structure of the photon pair emission one can generate pairs in factorable states and thence eliminate the need for spectral filters in multiplesource interference schemes indistinguishable heralded photons were generated in two independent spectrally engineered sources and by performing a hongoumandel interference between them without spectral filters at a raw visibility of 944 their purity was measured to be over 95
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711.1055
Simple Recursive Games
We define the class of "simple recursive games". A simple recursive game is defined as a simple stochastic game (a notion due to Anne Condon), except that we allow arbitrary real payoffs but disallow moves of chance. We study the complexity of solving simple recursive games and obtain an almost-linear time comparison-based algorithm for computing an equilibrium of such a game. The existence of a linear time comparison-based algorithm remains an open problem.
cs.GT cs.DS
we define the class of simple recursive games a simple recursive game is defined as a simple stochastic game a notion due to anne condon except that we allow arbitrary real payoffs but disallow moves of chance we study the complexity of solving simple recursive games and obtain an almostlinear time comparisonbased algorithm for computing an equilibrium of such a game the existence of a linear time comparisonbased algorithm remains an open problem
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711.1056
Bounds on the Number of Iterations for Turbo-Like Ensembles over the Binary Erasure Channe
This paper provides simple lower bounds on the number of iterations which is required for successful message-passing decoding of some important families of graph-based code ensembles (including low-density parity-check codes and variations of repeat-accumulate codes). The transmission of the code ensembles is assumed to take place over a binary erasure channel, and the bounds refer to the asymptotic case where we let the block length tend to infinity. The simplicity of the bounds derived in this paper stems from the fact that they are easily evaluated and are expressed in terms of some basic parameters of the ensemble which include the fraction of degree-2 variable nodes, the target bit erasure probability and the gap between the channel capacity and the design rate of the ensemble. This paper demonstrates that the number of iterations which is required for successful message-passing decoding scales at least like the inverse of the gap (in rate) to capacity, provided that the fraction of degree-2 variable nodes of these turbo-like ensembles does not vanish (hence, the number of iterations becomes unbounded as the gap to capacity vanishes).
cs.IT math.IT
this paper provides simple lower bounds on the number of iterations which is required for successful messagepassing decoding of some important families of graphbased code ensembles including lowdensity paritycheck codes and variations of repeataccumulate codes the transmission of the code ensembles is assumed to take place over a binary erasure channel and the bounds refer to the asymptotic case where we let the block length tend to infinity the simplicity of the bounds derived in this paper stems from the fact that they are easily evaluated and are expressed in terms of some basic parameters of the ensemble which include the fraction of degree2 variable nodes the target bit erasure probability and the gap between the channel capacity and the design rate of the ensemble this paper demonstrates that the number of iterations which is required for successful messagepassing decoding scales at least like the inverse of the gap in rate to capacity provided that the fraction of degree2 variable nodes of these turbolike ensembles does not vanish hence the number of iterations becomes unbounded as the gap to capacity vanishes
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711.1057
Junction Conditions and Consequences of Quasi-Spherical Space-Time with Electro-Magnetic Field and Vaidya Matric
In this work the junction conditions between the exterior Reissner-Nordstrom-Vaidya space-time with the interior quasi-spherical Szekeres space-time have been studied for analyzing gravitational collapse in the presence of a magneto-hydrodynamic fluid undergoing dissipation in the form of heat flow. We have discussed about the apparent horizon and have evaluated the time difference between the formation of apparent horizon and central singularity.
gr-qc
in this work the junction conditions between the exterior reissnernordstromvaidya spacetime with the interior quasispherical szekeres spacetime have been studied for analyzing gravitational collapse in the presence of a magnetohydrodynamic fluid undergoing dissipation in the form of heat flow we have discussed about the apparent horizon and have evaluated the time difference between the formation of apparent horizon and central singularity
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711.1058
Equivalent hyperon-nucleon interactions in low-momentum space
Equivalent interactions in a low-momentum space for the $\Lambda N$, $\Sigma N$ and $\Xi N$ interactions are calculated, using the SU$_6$ quark model potential as well as the Nijmegen OBEP model as the input bare interaction. Because the two-body scattering data has not been accumulated sufficiently to determine the hyperon-nucleon interactions unambiguously, the construction of the potential even in low-energy regions has to rely on a theoretical model. The equivalent interaction after removing high-momentum components is still model dependent. Because this model dependence reflects the character of the underlying potential model, it is instructive for better understanding of baryon-baryon interactions in the strangeness sector to study the low-momentum space $YN$ interactions.
nucl-th
equivalent interactions in a lowmomentum space for the lambda n sigma n and xi n interactions are calculated using the su_6 quark model potential as well as the nijmegen obep model as the input bare interaction because the twobody scattering data has not been accumulated sufficiently to determine the hyperonnucleon interactions unambiguously the construction of the potential even in lowenergy regions has to rely on a theoretical model the equivalent interaction after removing highmomentum components is still model dependent because this model dependence reflects the character of the underlying potential model it is instructive for better understanding of baryonbaryon interactions in the strangeness sector to study the lowmomentum space yn interactions
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711.1059
Photometric Redshifts for the Dark Energy Survey and VISTA and Implications for Large Scale Structure
We conduct a detailed analysis of the photometric redshift requirements for the proposed Dark Energy Survey (DES) using two sets of mock galaxy simulations and an artificial neural network code - ANNz. In particular, we examine how optical photometry in the DES grizY bands can be complemented with near infra-red photometry from the planned VISTA Hemisphere Survey (VHS) in the JHK_s bands. We find that the rms scatter on the photometric redshift estimate over 1<z<2 is sigma_z=0.2 from DES alone and sigma_z=0.15 from DES+VISTA, i.e. an improvement of more than 30%. We draw attention to the effects of galaxy formation scenarios such as reddening on the photo-z estimate and using our neural network code, calculate the extinction, A_v for these reddened galaxies. We also look at the impact of using different training sets when calculating photometric redshifts. In particular, we find that using the ongoing DEEP2 and VVDS-Deep spectroscopic surveys to calibrate photometric redshifts for DES, will prove effective. However we need to be aware of uncertainties in the photometric redshift bias that arise when using different training sets as these will translate into errors in the dark energy equation of state parameter, w. Furthermore, we show that the neural network error estimate on the photometric redshift may be used to remove outliers from our samples before any kind of cosmological analysis, in particular for large-scale structure experiments. By removing all galaxies with a neural network photo-z error estimate of greater than 0.1 from our DES+VHS sample, we can constrain the galaxy power spectrum out to a redshift of 2 and reduce the fractional error on this power spectrum by ~15-20% compared to using the entire catalogue.
astro-ph
we conduct a detailed analysis of the photometric redshift requirements for the proposed dark energy survey des using two sets of mock galaxy simulations and an artificial neural network code annz in particular we examine how optical photometry in the des grizy bands can be complemented with near infrared photometry from the planned vista hemisphere survey vhs in the jhk_s bands we find that the rms scatter on the photometric redshift estimate over 1z2 is sigma_z02 from des alone and sigma_z015 from desvista ie an improvement of more than 30 we draw attention to the effects of galaxy formation scenarios such as reddening on the photoz estimate and using our neural network code calculate the extinction a_v for these reddened galaxies we also look at the impact of using different training sets when calculating photometric redshifts in particular we find that using the ongoing deep2 and vvdsdeep spectroscopic surveys to calibrate photometric redshifts for des will prove effective however we need to be aware of uncertainties in the photometric redshift bias that arise when using different training sets as these will translate into errors in the dark energy equation of state parameter w furthermore we show that the neural network error estimate on the photometric redshift may be used to remove outliers from our samples before any kind of cosmological analysis in particular for largescale structure experiments by removing all galaxies with a neural network photoz error estimate of greater than 01 from our desvhs sample we can constrain the galaxy power spectrum out to a redshift of 2 and reduce the fractional error on this power spectrum by 1520 compared to using the entire catalogue
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711.106
Well-posedness and ill-posedness of the fifth order modifed KdV equation
We consider the initial value problem of the fifth order modified KdV equation on the Sobolev spaces. \partial_t u - \partial_x^5u + c_1\partial_x^3(u^3) + c_2u\partial_x u\partial_x^2 u + c_3uu\partial_x^3 u =0, u(x,0)= u_0(x) where $ u:R\timesR \to R $ and $c_j$'s are real. We show the local well-posedness in H^s(R) for s \geq 3/4 via the contraction principle on $X^{s,b}$ space. Also, we show that the solution map from data to the solutions fails to be uniformly continuous below $H^{3/4}(R)$. The counter example is obtained by approximating the fifth order mKdV equation by the cubic NLS equation.
math.AP
we consider the initial value problem of the fifth order modified kdv equation on the sobolev spaces partial_t u partial_x5u c_1partial_x3u3 c_2upartial_x upartial_x2 u c_3uupartial_x3 u 0 ux0 u_0x where urtimesr to r and c_js are real we show the local wellposedness in hsr for s geq 34 via the contraction principle on xsb space also we show that the solution map from data to the solutions fails to be uniformly continuous below h34r the counter example is obtained by approximating the fifth order mkdv equation by the cubic nls equation
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711.1061
Evidence for compact cooperatively rearranging regions in a supercooled liquid
We examine structural relaxation in a supercooled glass-forming liquid simulated by NVE molecular dynamics. Time correlations of the total kinetic energy fluctuations are used as a comprehensive measure of the system's approach to the ergodic equilibrium. We find that, under cooling, the total structural relaxation becomes delayed as compared with the decay of the component of the intermediate scattering function corresponding to the main peak of the structure factor. This observation can be explained by collective movements of particles preserving many-body structural correlations within compact 3D cooperatively rearranging regions.
cond-mat.soft cond-mat.stat-mech
we examine structural relaxation in a supercooled glassforming liquid simulated by nve molecular dynamics time correlations of the total kinetic energy fluctuations are used as a comprehensive measure of the systems approach to the ergodic equilibrium we find that under cooling the total structural relaxation becomes delayed as compared with the decay of the component of the intermediate scattering function corresponding to the main peak of the structure factor this observation can be explained by collective movements of particles preserving manybody structural correlations within compact 3d cooperatively rearranging regions
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711.1062
Spin-flip scattering and non-ideal interfaces in dirty ferromagnet/superconductor junctions
We study the proximity-induced superconducting correlations as well as the local density of states of a ferromagnet, in a ferromagnet/s-wave superconductor heterostructure. We include the effects of spin-flip scattering, non-ideal interfaces, and the presence of impurities in the sample. We employ the quasiclassical theory of superconductivity, solving the Usadel equation with emphasis on obtaining transparent analytical results. As our main result, we report that in a certain parameter regime the spatial oscillations of the anomalous (superconducting) part of the Green's function induced in the ferromagnet by the proximity effect from the s-wave superconductor, are damped out due to the presence of spin-flip processes. As a consequence, spin-flip scattering may under certain conditions actually enhance the local density of states due to the oscillatory behaviour of the latter in ferromagnet/superconductor structures. We also conjecture that the damping could be manifested in the behaviour of the critical temperature ($T_c$) of the s-wave superconductor in contact with the ferromagnet. More specifically, we argue that the non-monotonic decrease of $T_c$ in ferromagnet/s-wave superconductor junctions without magnetic impurities is altered to a monotonic, non-oscillatory decrease when the condition $1>16\tau_\text{sf}^2h^2$ is fulfilled, where $\tau_\text{sf}$ is the spin-flip relaxation time and $h$ is the exchange field.
cond-mat.supr-con
we study the proximityinduced superconducting correlations as well as the local density of states of a ferromagnet in a ferromagnetswave superconductor heterostructure we include the effects of spinflip scattering nonideal interfaces and the presence of impurities in the sample we employ the quasiclassical theory of superconductivity solving the usadel equation with emphasis on obtaining transparent analytical results as our main result we report that in a certain parameter regime the spatial oscillations of the anomalous superconducting part of the greens function induced in the ferromagnet by the proximity effect from the swave superconductor are damped out due to the presence of spinflip processes as a consequence spinflip scattering may under certain conditions actually enhance the local density of states due to the oscillatory behaviour of the latter in ferromagnetsuperconductor structures we also conjecture that the damping could be manifested in the behaviour of the critical temperature t_c of the swave superconductor in contact with the ferromagnet more specifically we argue that the nonmonotonic decrease of t_c in ferromagnetswave superconductor junctions without magnetic impurities is altered to a monotonic nonoscillatory decrease when the condition 116tau_textsf2h2 is fulfilled where tau_textsf is the spinflip relaxation time and h is the exchange field
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711.1063
On the Quantum Reconstruction of the Riemann zeros
We discuss a possible spectral realization of the Riemann zeros based on the Hamiltonian $H = xp$ perturbed by a term that depends on two potentials, which are related to the Berry-Keating semiclassical constraints. We find perturbatively the potentials whose Jost function is given by the zeta function $\zeta(\sigma - i t)$ for $\sigma > 1$. For $\sigma = 1/2$ we find the potentials that yield the smooth approximation to the zeros. We show that the existence of potentials realizing the zeta function at $\sigma = 1/2$, as a Jost function, would imply that the Riemann zeros are point like spectrum embedded in the continuum, resolving in that way the emission/spectral interpretation.
math-ph math.MP
we discuss a possible spectral realization of the riemann zeros based on the hamiltonian h xp perturbed by a term that depends on two potentials which are related to the berrykeating semiclassical constraints we find perturbatively the potentials whose jost function is given by the zeta function zetasigma i t for sigma 1 for sigma 12 we find the potentials that yield the smooth approximation to the zeros we show that the existence of potentials realizing the zeta function at sigma 12 as a jost function would imply that the riemann zeros are point like spectrum embedded in the continuum resolving in that way the emissionspectral interpretation
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711.1064
Fluctuation-Response Relation and modeling in systems with fast and slow dynamics
We show how a general formulation of the Fluctuation-Response Relation is able to describe in detail the connection between response properties to external perturbations and spontaneous fluctuations in systems with fast and slow variables. The method is tested by using the 360-variable Lorenz-96 model, where slow and fast variables are coupled to one another with reciprocal feedback, and a simplified low dimensional system. In the Fluctuation-Response context, the influence of the fast dynamics on the slow dynamics relies in a non trivial behavior of a suitable quadratic response function. This has important consequences for the modeling of the slow dynamics in terms of a Langevin equation: beyond a certain intrinsic time interval even the optimal model can give just statistical prediction.
nlin.CD
we show how a general formulation of the fluctuationresponse relation is able to describe in detail the connection between response properties to external perturbations and spontaneous fluctuations in systems with fast and slow variables the method is tested by using the 360variable lorenz96 model where slow and fast variables are coupled to one another with reciprocal feedback and a simplified low dimensional system in the fluctuationresponse context the influence of the fast dynamics on the slow dynamics relies in a non trivial behavior of a suitable quadratic response function this has important consequences for the modeling of the slow dynamics in terms of a langevin equation beyond a certain intrinsic time interval even the optimal model can give just statistical prediction
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711.1065
Optically-stimulated desorption of 'hot' excimers from pre-irradiated Ar solids
Electronically-induced desorption from solid Ar pre-irradiated by a low-energy electron beam was investigated by activation spectroscopy methods - photon-stimulated exoelectron emission and photon-stimulated luminescence in combination with spectrally-resolved measurements in the VUV range of the spectrum. Desorption of vibrationally excited argon molecules Ar2^*(v) from the surface of pre-irradiated solid Ar was observed for the first time. It was shown that desorption of 'hot' Ar2^*(v) molecules is caused by recombination of self-trapped holes with electrons released from traps by visible range photons. The possibility of optical stimulation of the phenomenon is evidenced.
cond-mat.other
electronicallyinduced desorption from solid ar preirradiated by a lowenergy electron beam was investigated by activation spectroscopy methods photonstimulated exoelectron emission and photonstimulated luminescence in combination with spectrallyresolved measurements in the vuv range of the spectrum desorption of vibrationally excited argon molecules ar2v from the surface of preirradiated solid ar was observed for the first time it was shown that desorption of hot ar2v molecules is caused by recombination of selftrapped holes with electrons released from traps by visible range photons the possibility of optical stimulation of the phenomenon is evidenced
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711.1066
Role of Interlayer Electron Hopping for Spin Density Wave State in the Zero-Gap Organic Conductor
We investigate the formation of density waves in the zero-gap state (ZGS) which has been found in the quasi-two-dimensional organic conductor $\alpha$-(BEDT-TTF)$_2$I$_3$ salt under the hydrostatic pressure. The ZGS exhibits the cone-like dispersion for both the conduction band and the valence band which degenerate each other at the two-dimensional wave vectors, $\pm\mib{k}_0$ forming a zero gap. By using the extended Hubbard model with repulsive interaction we calculate the onset temperature of the spin density wave (SDW) as a function of the interlayer electron hopping, which by itself does not break the cone-like dispersion. It is shown that the SDW with wave number $2\mib{k}_0$ is induced by the combined effect of the interaction, the inter-band excitation across the zero-gap and the interlayer hopping.
cond-mat.str-el
we investigate the formation of density waves in the zerogap state zgs which has been found in the quasitwodimensional organic conductor alphabedtttf_2i_3 salt under the hydrostatic pressure the zgs exhibits the conelike dispersion for both the conduction band and the valence band which degenerate each other at the twodimensional wave vectors pmmibk_0 forming a zero gap by using the extended hubbard model with repulsive interaction we calculate the onset temperature of the spin density wave sdw as a function of the interlayer electron hopping which by itself does not break the conelike dispersion it is shown that the sdw with wave number 2mibk_0 is induced by the combined effect of the interaction the interband excitation across the zerogap and the interlayer hopping
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711.1067
Subleading terms in asymptotic Passarino-Veltman functions
We write explicit and self-contained asymptotic expressions for the tensorial B, C and D Passarino-Veltman functions. These include quadratic and linear logarithmic terms, as well as subleading constant terms. Only mass-suppressed O(m^2/s) contributions are neglected. We discuss the usefulness of such expressions, particularly for studying one-loop effects in 2-to-2 body processes at high energy.
hep-ph
we write explicit and selfcontained asymptotic expressions for the tensorial b c and d passarinoveltman functions these include quadratic and linear logarithmic terms as well as subleading constant terms only masssuppressed om2s contributions are neglected we discuss the usefulness of such expressions particularly for studying oneloop effects in 2to2 body processes at high energy
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711.1068
A conservative evolution of the Brownian excursion
We consider the problem of conditioning the Brownian excursion to have a fixed time average over the interval [0,1] and we study an associated stochastic partial differential equation with reflection at 0 and with the constraint of conservation of the space average. The equation is driven by the derivative in space of a space-time white noise and contains a double Laplacian in the drift. Due to the lack of the maximum principle for the double Laplacian, the standard techniques based on the penalization method do not yield existence of a solution.
math.PR
we consider the problem of conditioning the brownian excursion to have a fixed time average over the interval 01 and we study an associated stochastic partial differential equation with reflection at 0 and with the constraint of conservation of the space average the equation is driven by the derivative in space of a spacetime white noise and contains a double laplacian in the drift due to the lack of the maximum principle for the double laplacian the standard techniques based on the penalization method do not yield existence of a solution
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711.1069
Numerical analysis of solitons profiles in a composite model for DNA to rsion dynamics
We present the results of our numerical analysis of a "composite" model of DNA which generalizes a well-known elementary torsional model of Yakushevich by allowing bases to move independently from the backbone. The model shares with the Yakushevich model many features and results but it represents an improvement from both the conceptual and the phenomenological point of view. It provides a more realistic description of DNA and possibly a justification for the use of models which consider the DNA chain as uniform. It shows that the existence of solitons is a generic feature of the underlying nonlinear dynamics and is to a large extent independent of the detailed modelling of DNA. As opposite to the Yakushevich model, where it is needed to use an unphysical value for the torsion in order to induce the correct velocity of sound, the model we consider supports solitonic solutions, qualitatively and quantitatively very similar to the Yakushevich solitons, in a fully realistic range of all the physical parameters characterizing the DNA.
q-bio.BM q-bio.QM
we present the results of our numerical analysis of a composite model of dna which generalizes a wellknown elementary torsional model of yakushevich by allowing bases to move independently from the backbone the model shares with the yakushevich model many features and results but it represents an improvement from both the conceptual and the phenomenological point of view it provides a more realistic description of dna and possibly a justification for the use of models which consider the dna chain as uniform it shows that the existence of solitons is a generic feature of the underlying nonlinear dynamics and is to a large extent independent of the detailed modelling of dna as opposite to the yakushevich model where it is needed to use an unphysical value for the torsion in order to induce the correct velocity of sound the model we consider supports solitonic solutions qualitatively and quantitatively very similar to the yakushevich solitons in a fully realistic range of all the physical parameters characterizing the dna
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711.107
Adaptive Eigenvalue Computation - Complexity Estimates
This paper is concerned with the design and analysis of a fully adaptive eigenvalue solver for linear symmetric operators. After transforming the original problem into an equivalent one formulated on $\ell_2$, the space of square summable sequences, the problem becomes sufficiently well conditioned so that a gradient type iteration can be shown to reduce the error by some fixed factor per step. It then remains to realize these (ideal) iterations within suitable dynamically updated error tolerances. It is shown under which circumstances the adaptive scheme exhibits in some sense asymptotically optimal complexity.
math.NA
this paper is concerned with the design and analysis of a fully adaptive eigenvalue solver for linear symmetric operators after transforming the original problem into an equivalent one formulated on ell_2 the space of square summable sequences the problem becomes sufficiently well conditioned so that a gradient type iteration can be shown to reduce the error by some fixed factor per step it then remains to realize these ideal iterations within suitable dynamically updated error tolerances it is shown under which circumstances the adaptive scheme exhibits in some sense asymptotically optimal complexity
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711.1071
Double-Resonance g Factor Measurements by Quantum Jump Spectroscopy
With the advent of high-precision frequency combs that can bridge large frequency intervals, new possibilities have opened up for the laser spectroscopy of atomic transitions. Here, we show that laser spectroscopic techniques can also be used to determine the ground-state g factor of a bound electron: Our proposal is based on a double-resonance experiment, where the spin state of a ground-state electron is constantly being read out by laser excitation to the atomic L shell, while the spin flip transitions are being induced simultaneously by a resonant microwave field, leading to a detection of the quantum jumps between the ground-state Zeeman sublevels. The magnetic moments of electrons in light hydrogen-like ions could thus be measured with advanced laser technology. Corresponding theoretical predictions are also presented.
physics.atom-ph
with the advent of highprecision frequency combs that can bridge large frequency intervals new possibilities have opened up for the laser spectroscopy of atomic transitions here we show that laser spectroscopic techniques can also be used to determine the groundstate g factor of a bound electron our proposal is based on a doubleresonance experiment where the spin state of a groundstate electron is constantly being read out by laser excitation to the atomic l shell while the spin flip transitions are being induced simultaneously by a resonant microwave field leading to a detection of the quantum jumps between the groundstate zeeman sublevels the magnetic moments of electrons in light hydrogenlike ions could thus be measured with advanced laser technology corresponding theoretical predictions are also presented
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711.1072
Test of the Schr\"odinger functional with chiral fermions in the Gross-Neveu model
The recently proposed construction of chiral fermions on lattices with boundaries is tested in an interacting theory up to first order of perturbation theory. We confirm that, in the bulk of the lattice, the chiral Ward identities take their continuum value up to cutoff effects without any tuning. Universal quantities are defined that have an expansion in the renormalised couplings with coefficients that are functions of the physical size and the periodicity in the spatial direction. These coefficient functions have to be identical for different discretisations. We find agreement with the standard Wilson fermions. The computation is done in the asymptotically free Gross-Neveu model with continuous chiral symmetry.
hep-lat
the recently proposed construction of chiral fermions on lattices with boundaries is tested in an interacting theory up to first order of perturbation theory we confirm that in the bulk of the lattice the chiral ward identities take their continuum value up to cutoff effects without any tuning universal quantities are defined that have an expansion in the renormalised couplings with coefficients that are functions of the physical size and the periodicity in the spatial direction these coefficient functions have to be identical for different discretisations we find agreement with the standard wilson fermions the computation is done in the asymptotically free grossneveu model with continuous chiral symmetry
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711.1073
Structure, Time Propagation and Dissipative Terms for Resonances
For odd anharmonic oscillators, it is well known that complex scaling can be used to determine resonance energy eigenvalues and the corresponding eigenvectors in complex rotated space. We briefly review and discuss various methods for the numerical determination of such eigenvalues, and also discuss the connection to the case of purely imaginary coupling, which is PT-symmetric. Moreover, we show that a suitable generalization of the complex scaling method leads to an algorithm for the time propagation of wave packets in potentials which give rise to unstable resonances. This leads to a certain unification of the structure and the dynamics. Our time propagation results agree with known quantum dynamics solvers and allow for a natural incorporation of structural perturbations (e.g., due to dissipative processes) into the quantum dynamics.
math-ph math.MP
for odd anharmonic oscillators it is well known that complex scaling can be used to determine resonance energy eigenvalues and the corresponding eigenvectors in complex rotated space we briefly review and discuss various methods for the numerical determination of such eigenvalues and also discuss the connection to the case of purely imaginary coupling which is ptsymmetric moreover we show that a suitable generalization of the complex scaling method leads to an algorithm for the time propagation of wave packets in potentials which give rise to unstable resonances this leads to a certain unification of the structure and the dynamics our time propagation results agree with known quantum dynamics solvers and allow for a natural incorporation of structural perturbations eg due to dissipative processes into the quantum dynamics
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711.1074
Charged Rotating Black Holes on DGP Brane
We consider charged rotating black holes localized on a three-brane in the DGP model. Assuming a $Z_2$-symmetry across the brane and with a stationary and axisymmetric metric ansatz on the brane, a particular solution is obtained in the Kerr-Schild form. This solution belongs to the accelerated branch of the DGP model and has the characteristic of the Kerr-Newman-de Sitter type solution in general relativity. Using a modified version of Boyer-Lindquist coordinates we examine the structures of the horizon and ergosphere.
hep-th gr-qc
we consider charged rotating black holes localized on a threebrane in the dgp model assuming a z_2symmetry across the brane and with a stationary and axisymmetric metric ansatz on the brane a particular solution is obtained in the kerrschild form this solution belongs to the accelerated branch of the dgp model and has the characteristic of the kerrnewmande sitter type solution in general relativity using a modified version of boyerlindquist coordinates we examine the structures of the horizon and ergosphere
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711.1075
Combining CPT-conjugate Neutrino channels at Fermilab
We explore an alternative strategy to determine the neutrino mass hierarchy by making use of possible future neutrino facilities at Fermilab. Here, we use CPT-conjugate neutrino channels, exploiting a nu_mu beam from the NuMI beamline and a barnu_e beam from a betabeam experimental setup. Both experiments are performed at approximately the same E/L. We present different possible accelerator scenarios for the betabeam neutrino setup and fluxes. This CPT-conjugate neutrino channel scenario can extract the neutrino mass hierarchy down to sin^2 (2 theta_13) \approx 0.02.
hep-ph
we explore an alternative strategy to determine the neutrino mass hierarchy by making use of possible future neutrino facilities at fermilab here we use cptconjugate neutrino channels exploiting a nu_mu beam from the numi beamline and a barnu_e beam from a betabeam experimental setup both experiments are performed at approximately the same el we present different possible accelerator scenarios for the betabeam neutrino setup and fluxes this cptconjugate neutrino channel scenario can extract the neutrino mass hierarchy down to sin2 2 theta_13 approx 002
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711.1076
Modelling element distributions in the atmospheres of magnetic Ap stars
In recent papers convincing evidence has been presented for chemical stratification in Ap star atmospheres, and surface abundance maps have been shown to correlate with the magnetic field direction. Radiatively driven diffusion in magnetic fields is among the processes responsible for these inhomogeneities. Here we explore the hypothesis that equilibrium stratifications can, in a number of cases, explain the observed abundance maps and vertical distributions of the various elements. The investigation of equilibrium stratifications in stellar atmospheres with temperatures from 8500K to 12000K and fields up to 10 kG reveals considerable variations in the vertical distribution of the 5 elements studied (Mg, Si, Ca, Ti, Fe), often with zones of large over- or under-abundances and with indications of other competing processes (such as mass loss). Horizontal magnetic fields can be very efficient in helping the accumulation of elements in higher layers. A comparison between our calculations and the vertical abundance profiles and surface maps derived by magnetic Doppler imaging reveals that equilibrium stratifications are in a number of cases consistent with the main trends inferred from observed spectra. However, it is not clear whether such equilibrium solutions will ever be reached during the evolution of an Ap star.
astro-ph
in recent papers convincing evidence has been presented for chemical stratification in ap star atmospheres and surface abundance maps have been shown to correlate with the magnetic field direction radiatively driven diffusion in magnetic fields is among the processes responsible for these inhomogeneities here we explore the hypothesis that equilibrium stratifications can in a number of cases explain the observed abundance maps and vertical distributions of the various elements the investigation of equilibrium stratifications in stellar atmospheres with temperatures from 8500k to 12000k and fields up to 10 kg reveals considerable variations in the vertical distribution of the 5 elements studied mg si ca ti fe often with zones of large over or underabundances and with indications of other competing processes such as mass loss horizontal magnetic fields can be very efficient in helping the accumulation of elements in higher layers a comparison between our calculations and the vertical abundance profiles and surface maps derived by magnetic doppler imaging reveals that equilibrium stratifications are in a number of cases consistent with the main trends inferred from observed spectra however it is not clear whether such equilibrium solutions will ever be reached during the evolution of an ap star
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711.1077
Implications of HERA measurements for LHC
I discuss the theoretical understanding of key measurements at HERA and their relevance for physics at LHC, focusing on recent developments for structure functions and for diffraction.
hep-ph
i discuss the theoretical understanding of key measurements at hera and their relevance for physics at lhc focusing on recent developments for structure functions and for diffraction
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711.1078
Comment on "Reply to Comment on Time-dependent Quasi-Hermitian Hamiltonians and the Unitary Quantum Evolution"
I point out that if one defines the operator $U_R(t)$ as done by M. Znojil in his reply [arXiv:0711.0514v1] to my comment [arXiv:0711.0137v1] and also accepts the validity of the defining relation of $U_R(t)$ as given in his paper [arXiv:0710.5653v1], one finds that the time-evolution of the associated quantum system is not governed by the Schr\"odinger equation for the Hamiltonian operator $H$ but an operator $H'$ which differs from $H$ if the metric operator is time-dependent. In the latter case this effective Hamiltonian $H'$ is not observable. This is consistent with the conclusions of my paper [Phys. Lett. B 650, 208 (2007), arXiv:0706.1872v2] which allow for unitary time-evolution generated by unobservable Hamiltonians.
quant-ph
i point out that if one defines the operator u_rt as done by m znojil in his reply arxiv07110514v1 to my comment arxiv07110137v1 and also accepts the validity of the defining relation of u_rt as given in his paper arxiv07105653v1 one finds that the timeevolution of the associated quantum system is not governed by the schrodinger equation for the hamiltonian operator h but an operator h which differs from h if the metric operator is timedependent in the latter case this effective hamiltonian h is not observable this is consistent with the conclusions of my paper phys lett b 650 208 2007 arxiv07061872v2 which allow for unitary timeevolution generated by unobservable hamiltonians
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711.1079
70Ge(p,gamma)71As and 76Ge(p,n)76As cross sections for the astrophysical p process: sensitivity of the optical proton potential at low energies
The cross sections of the 70Ge(p,gamma)71As and 76Ge(p,n)76As reactions have been measured with the activation method in the Gamow window for the astrophysical p process. The experiments were carried out at the Van de Graaff and cyclotron accelerators of ATOMKI. The cross sections have been derived by measuring the decay gamma-radiation of the reaction products. The results are compared to the predictions of Hauser-Feshbach statistical model calculations using the code NON-SMOKER. Good agreement between theoretical and experimental S factors is found. Based on the new data, modifications of the optical potential used for low-energy protons are discussed.
nucl-ex
the cross sections of the 70gepgamma71as and 76gepn76as reactions have been measured with the activation method in the gamow window for the astrophysical p process the experiments were carried out at the van de graaff and cyclotron accelerators of atomki the cross sections have been derived by measuring the decay gammaradiation of the reaction products the results are compared to the predictions of hauserfeshbach statistical model calculations using the code nonsmoker good agreement between theoretical and experimental s factors is found based on the new data modifications of the optical potential used for lowenergy protons are discussed
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711.108
Thermal expansion and magnetostriction of pure and doped RAgSb2 (R = Y, Sm, La) single crystals
Data on temperature-dependent, anisotropic thermal expansion in pure and doped RAgSb2 (R = Y, Sm, La) single crystals are presented. Using the Ehrenfest relation and heat capacity measurements, uniaxial pressure derivatives for long range magnetic ordering and charge density wave transition temperatures are evaluated and compared with the results of the direct measurements under hydrostatic pressure. In-plane and c-axis pressure have opposite effect on the phase transitions in these materials, with in-plane effects being significantly weaker. Quantum oscillations in magnetostriction were observed for the three pure compounds, with the possible detection of new frequencies in SmAgSb2 and LaAgSb2. The uniaxial (along the c-axis) pressure derivatives of the dominant extreme orbits (beta) were evaluated for YAgSb2 and LaAgSb2.
cond-mat.mtrl-sci
data on temperaturedependent anisotropic thermal expansion in pure and doped ragsb2 r y sm la single crystals are presented using the ehrenfest relation and heat capacity measurements uniaxial pressure derivatives for long range magnetic ordering and charge density wave transition temperatures are evaluated and compared with the results of the direct measurements under hydrostatic pressure inplane and caxis pressure have opposite effect on the phase transitions in these materials with inplane effects being significantly weaker quantum oscillations in magnetostriction were observed for the three pure compounds with the possible detection of new frequencies in smagsb2 and laagsb2 the uniaxial along the caxis pressure derivatives of the dominant extreme orbits beta were evaluated for yagsb2 and laagsb2
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711.1081
Short-time dynamics of a packing of polyhedral grains under horizontal vibrations
We analyze the dynamics of a 3D granular packing composed of particles of irregular polyhedral shape confined inside a rectangular box with a retaining wall sub jected to horizontal harmonic forcing. The simulations are performed by means of the contact dynamics method for a broad set of loading parameters. We explore the vibrational dynamics of the packing, the evolution of solid fraction and the scaling of dy- namics with the loading parameters. We show that the motion of the retaining wall is strongly anharmonic as a result of jamming and grain rearrangements. It is found that the mean particle displacement scales with inverse square of frequency, the inverse of the force amplitude and the square of gravity. The short- time compaction rate grows in proportion to frequency up to a characteristic frequency, corresponding to collective particle rearrangements between equilibrium states, and then it declines in inverse proportion to frequency.
physics.class-ph
we analyze the dynamics of a 3d granular packing composed of particles of irregular polyhedral shape confined inside a rectangular box with a retaining wall sub jected to horizontal harmonic forcing the simulations are performed by means of the contact dynamics method for a broad set of loading parameters we explore the vibrational dynamics of the packing the evolution of solid fraction and the scaling of dy namics with the loading parameters we show that the motion of the retaining wall is strongly anharmonic as a result of jamming and grain rearrangements it is found that the mean particle displacement scales with inverse square of frequency the inverse of the force amplitude and the square of gravity the short time compaction rate grows in proportion to frequency up to a characteristic frequency corresponding to collective particle rearrangements between equilibrium states and then it declines in inverse proportion to frequency
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711.1082
Multivariate normal approximation with Stein's method of exchangeable pairs under a general linearity condition
In this paper we establish a multivariate exchangeable pairs approach within the framework of Stein's method to assess distributional distances to potentially singular multivariate normal distributions. By extending the statistics into a higher-dimensional space, we also propose an embedding method which allows for a normal approximation even when the corresponding statistics of interest do not lend themselves easily to Stein's exchangeable pairs approach. To illustrate the method, we provide the examples of runs on the line as well as double-indexed permutation statistics.
math.PR
in this paper we establish a multivariate exchangeable pairs approach within the framework of steins method to assess distributional distances to potentially singular multivariate normal distributions by extending the statistics into a higherdimensional space we also propose an embedding method which allows for a normal approximation even when the corresponding statistics of interest do not lend themselves easily to steins exchangeable pairs approach to illustrate the method we provide the examples of runs on the line as well as doubleindexed permutation statistics
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711.1083
The Faint and Extremely Red K-band Selected Galaxy Population in the DEEP2/Palomar Fields
We present in this paper an analysis of the faint and red near-infrared selected galaxy population found in near-infrared imaging from the Palomar Observatory Wide-Field Infrared Survey. This survey covers 1.53 deg^2 to 5-sigma detection limits of K_vega = 20.5-21 and J_vega = 22.5, and overlaps with the DEEP2 spectroscopic redshift survey. We discuss the details of this NIR survey, including our J and K band counts. We show that the K-band galaxy population has a redshift distribution that varies with K-magnitude, with most K < 17 galaxies at z < 1.5 and a significant fraction (38.3+/-0.3%) of K > 19 systems at z > 1.5. We further investigate the stellar masses and morphological properties of K-selected galaxies, particularly extremely red objects, as defined by (R-K) > 5.3 and (I-K) > 4. One of our conclusions is that the ERO selection is a good method for picking out galaxies at z > 1.2, and within our magnitude limits, the most massive galaxies at these redshifts. The ERO limit finds 75% of all M_* > 10^{11} M_0 galaxies at z ~ 1.5 down to K_vega = 19.7. We further find that the morphological break-down of K < 19.7 EROs is dominated by early-types (57+/-3%) and peculiars (34+/-3%). However, about a fourth of the early-types are distorted ellipticals, and within CAS parameter space these bridge the early-type and peculiar population, suggesting a morphological evolutionary sequence. We also investigate the use of a (I-K) > 4 selection to locate EROs, finding that it selects galaxies at slightly higher average redshifts (<z> = 1.43+/-0.32) than the (R-K) > 5.3 limit with <z> = 1.28+/-0.23. Finally, by using the redshift distribution of K < 20 selected galaxies, and the properties of our EROs, we are able to rule out all monolithic collapse models for the formation of massive galaxies.
astro-ph
we present in this paper an analysis of the faint and red nearinfrared selected galaxy population found in nearinfrared imaging from the palomar observatory widefield infrared survey this survey covers 153 deg2 to 5sigma detection limits of k_vega 20521 and j_vega 225 and overlaps with the deep2 spectroscopic redshift survey we discuss the details of this nir survey including our j and k band counts we show that the kband galaxy population has a redshift distribution that varies with kmagnitude with most k 17 galaxies at z 15 and a significant fraction 38303 of k 19 systems at z 15 we further investigate the stellar masses and morphological properties of kselected galaxies particularly extremely red objects as defined by rk 53 and ik 4 one of our conclusions is that the ero selection is a good method for picking out galaxies at z 12 and within our magnitude limits the most massive galaxies at these redshifts the ero limit finds 75 of all m_ 1011 m_0 galaxies at z 15 down to k_vega 197 we further find that the morphological breakdown of k 197 eros is dominated by earlytypes 573 and peculiars 343 however about a fourth of the earlytypes are distorted ellipticals and within cas parameter space these bridge the earlytype and peculiar population suggesting a morphological evolutionary sequence we also investigate the use of a ik 4 selection to locate eros finding that it selects galaxies at slightly higher average redshifts z 143032 than the rk 53 limit with z 128023 finally by using the redshift distribution of k 20 selected galaxies and the properties of our eros we are able to rule out all monolithic collapse models for the formation of massive galaxies
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711.1084
Microstructure and mechanical properties of constrained shape-memory alloy nanograins and nanowires
We use the phase-field method to study the martensitic transformation at the nanoscale. For nanosystems such as nanowires and nanograins embedded in a stiff matrix, the geometric constraints and boundary conditions have an impact on martensite formation, leading to new microstructures --such as dots aligned on a square lattice with axes along <01>-- or preventing martensite formation altogether. We also perform tension tests on the nanowires. The stress-strain curves are very different from bulk results. Moreover, they are weakly affected by microstructures -- the mechanical response of nanowires with different microstructures may be similar, while nanowires with the same microstructure may have a different mechanical behavior. We also observe that at the transition temperature, or slightly below it, the narrowest wires behave pseudoelastically whereas wider wires are in the memory-shape regime. Moreover the yield stress does not change monotonically with width: it has a minimum value at intermediate width.
cond-mat.mtrl-sci
we use the phasefield method to study the martensitic transformation at the nanoscale for nanosystems such as nanowires and nanograins embedded in a stiff matrix the geometric constraints and boundary conditions have an impact on martensite formation leading to new microstructures such as dots aligned on a square lattice with axes along 01 or preventing martensite formation altogether we also perform tension tests on the nanowires the stressstrain curves are very different from bulk results moreover they are weakly affected by microstructures the mechanical response of nanowires with different microstructures may be similar while nanowires with the same microstructure may have a different mechanical behavior we also observe that at the transition temperature or slightly below it the narrowest wires behave pseudoelastically whereas wider wires are in the memoryshape regime moreover the yield stress does not change monotonically with width it has a minimum value at intermediate width
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711.1085
Phase transitions and topology in 2+k XY mean-field models
The thermodynamics and topology of mean-field models with 2+k body interaction terms (generalizing XY model) are derived. Focusing on two particular cases (2+4 and 2+6 body interaction terms), a comparison between thermodynamic (phase transition energy, thermodynamically forbidden energy regions) and topological (singularity and curvature of saddle entropy) properties is performed. We find that i) a topological change is present at the phase transition energy; however, ii) only one topological change occurs, also for those models exhibiting two phase transitions; iii) the order of a phase transition is not completely signaled by the curvature of topological quantities.
cond-mat.stat-mech
the thermodynamics and topology of meanfield models with 2k body interaction terms generalizing xy model are derived focusing on two particular cases 24 and 26 body interaction terms a comparison between thermodynamic phase transition energy thermodynamically forbidden energy regions and topological singularity and curvature of saddle entropy properties is performed we find that i a topological change is present at the phase transition energy however ii only one topological change occurs also for those models exhibiting two phase transitions iii the order of a phase transition is not completely signaled by the curvature of topological quantities
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711.1086
Large x Resummation in Q^2 Evolution
The standard analytic solution to the DGLAP equation in Mellin space is improved by resumming the large x divergences. Explicit results are given to next-to-leading order and next-to-leading logarithmic accuracy. Numerically, the theoretical error is found to be reduced by the resummation for a large range of x.
hep-ph
the standard analytic solution to the dglap equation in mellin space is improved by resumming the large x divergences explicit results are given to nexttoleading order and nexttoleading logarithmic accuracy numerically the theoretical error is found to be reduced by the resummation for a large range of x
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711.1087
On function spaces on symmetric spaces
Let Y=G/H be a semisimple symmetric space. It is shown that the smooth vectors for the regular representation of G on L^p(Y) vanish at infinity.
math.RT
let ygh be a semisimple symmetric space it is shown that the smooth vectors for the regular representation of g on lpy vanish at infinity
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711.1088
Modeling extended contacts to nanotube and graphene devices
Carrier injection into carbon nanotubes and graphene nanoribbons, contacted by a metal coating over an arbitrary length, is studied by various means: Minimal models allow for exact analytic solutions which can be transferred to the original system with high precision. Microscopic ab initio calculations of the electronic structure at the carbon-metal interface allow us to extract -- for Ti and Pd as contacting materials -- realistic parameters, which are then used in large scale tight-binding models for transport calculations. The results are shown to be robust against nonepitaxially grown electrodes and general disorder at the interface, as well as various refinements of the model.
cond-mat.mes-hall
carrier injection into carbon nanotubes and graphene nanoribbons contacted by a metal coating over an arbitrary length is studied by various means minimal models allow for exact analytic solutions which can be transferred to the original system with high precision microscopic ab initio calculations of the electronic structure at the carbonmetal interface allow us to extract for ti and pd as contacting materials realistic parameters which are then used in large scale tightbinding models for transport calculations the results are shown to be robust against nonepitaxially grown electrodes and general disorder at the interface as well as various refinements of the model
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711.1089
Periodic variations in 6.7-GHz methanol masers
An intensive monitoring program of 54 6.7-GHz methanol maser sources was carried out at the Hartebeesthoek Radio Astronomy Observatory from January 1999 to April 2003. The monitoring program was subsequently continued on 19 sources of interest. Analysis of the resulting time-series stretching over eight years shows that six of the sources are periodic, with periods ranging from 133 days to 504 days. The waveforms in individual sources range from sinusoidal fluctuations to sharp flares and there can be other long term trends in the time-series. The amplitudes of the variations can also change from cycle to cycle. The time-series of the periodic masers will be presented, and possible causes of the variability discussed.
astro-ph
an intensive monitoring program of 54 67ghz methanol maser sources was carried out at the hartebeesthoek radio astronomy observatory from january 1999 to april 2003 the monitoring program was subsequently continued on 19 sources of interest analysis of the resulting timeseries stretching over eight years shows that six of the sources are periodic with periods ranging from 133 days to 504 days the waveforms in individual sources range from sinusoidal fluctuations to sharp flares and there can be other long term trends in the timeseries the amplitudes of the variations can also change from cycle to cycle the timeseries of the periodic masers will be presented and possible causes of the variability discussed
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711.109
TDDFT with Skyrme Forces: Effect of Time-Odd Densities on Electric Giant Resonances
Time-odd densities and their effect on electric giant resonances are investigated within the self-consistent separable random-phase-approximation (SRPA) model for various Skyrme forces (SkT6, SkO, SkM*, SIII, SGII, SLy4, SLy6, SkI3). Time-odd densities restore Galilean invariance of the Skyrme functional, violated by the effective-mass and spin-orbital terms. In even-even nuclei these densities do not contribute to the ground state but can affect the dynamics. As a particular case, we explore the role of the current density in description of isovector E1 and isoscalar E2 giant resonances in a chain of Nd spherical and deformed isotopes with A=134-158. Relation of the current to the effective masses and relevant parameters of the Skyrme functional is analyzed. It is shown that current contribution to E1 and E2 resonances is generally essential and fully determined by the values and signs of the isovector and isoscalar effective-mass parameters of the force. The contribution is the same for all the isotope chain, i.e. for both standard and exotic nuclei.
nucl-th
timeodd densities and their effect on electric giant resonances are investigated within the selfconsistent separable randomphaseapproximation srpa model for various skyrme forces skt6 sko skm siii sgii sly4 sly6 ski3 timeodd densities restore galilean invariance of the skyrme functional violated by the effectivemass and spinorbital terms in eveneven nuclei these densities do not contribute to the ground state but can affect the dynamics as a particular case we explore the role of the current density in description of isovector e1 and isoscalar e2 giant resonances in a chain of nd spherical and deformed isotopes with a134158 relation of the current to the effective masses and relevant parameters of the skyrme functional is analyzed it is shown that current contribution to e1 and e2 resonances is generally essential and fully determined by the values and signs of the isovector and isoscalar effectivemass parameters of the force the contribution is the same for all the isotope chain ie for both standard and exotic nuclei
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711.1091
Convergence to equilibrium distribution. The Klein-Gordon equation coupled to a particle
We consider the Hamiltonian system consisting of a Klein-Gordon vector field and a particle in $\R^3$. The initial date of the system is a random function with a finite mean density of energy which also satisfies a Rosenblatt- or Ibragimov-type mixing condition. Moreover, initial correlation functions are translation-invariant. We study the distribution $\mu_t$ of the solution at time $t\in\R$. The main result is the convergence of $\mu_t$ to a Gaussian measure as $t\to\infty$, where $\mu_\infty$ is translation-invariant.
math-ph math.MP
we consider the hamiltonian system consisting of a kleingordon vector field and a particle in r3 the initial date of the system is a random function with a finite mean density of energy which also satisfies a rosenblatt or ibragimovtype mixing condition moreover initial correlation functions are translationinvariant we study the distribution mu_t of the solution at time tinr the main result is the convergence of mu_t to a gaussian measure as ttoinfty where mu_infty is translationinvariant
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711.1092
Hidden Structure in Tilings, Conjectured Asymptotic Expansion for lambda_d in Multidimensional Dimer Problem
The dimer problem arose in a thermodynamic study of diatomic molecules, and was abstracted into one of the most basic and natural problems in both statistical mechanics and combinatoric mathematics. Given a rectangular lattice of volume V in d dimensions, the dimer problem loosely speaking is to count the number of different ways dimers (dominoes) may be layed down on the lattice to completely cover it. It is known that the number of such coverings is roughly exp(lambda_d V) for some number lambda_d. The first terms in the expansion of lambda_d have been known for about thirty years lambda_d ~ (1/2)ln(2d)-1/2 Herein we present a mathematical argument for an asymptotic expansion lambda_d ~ (1/2)ln(2d) -1/2 +(1/8)/d + (5/96)/d^2 +... with the first few terms given explicitly.
math-ph cond-mat.stat-mech math.MP
the dimer problem arose in a thermodynamic study of diatomic molecules and was abstracted into one of the most basic and natural problems in both statistical mechanics and combinatoric mathematics given a rectangular lattice of volume v in d dimensions the dimer problem loosely speaking is to count the number of different ways dimers dominoes may be layed down on the lattice to completely cover it it is known that the number of such coverings is roughly explambda_d v for some number lambda_d the first terms in the expansion of lambda_d have been known for about thirty years lambda_d 12ln2d12 herein we present a mathematical argument for an asymptotic expansion lambda_d 12ln2d 12 18d 596d2 with the first few terms given explicitly
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711.1093
CO investigation of z=0.4-1.5 galaxies
We report on the results of an IRAM-30m search for CO emission lines in three galaxies at intermediate redshifts. The idea was to investigate the molecular content of galaxies bright in the infrared at z=0.4-1.5, a redshift desert for molecular line studies, poorly investigated as of yet. We integrated 8-10h per source and did not succeed in detecting any of the sources. From our upper limits, we are able to constrain the molecular gas content in these systems to less than 4 to 8 x 10^9 Mo, assuming a CO-to-H_2 conversion factor (\alpha=0.8 Mo/(K km s^-1 pc^2)). We stress the current difficulty of selecting sources with a detectable molecular content, a problem that will be faced by the ALMA First Science projects.
astro-ph
we report on the results of an iram30m search for co emission lines in three galaxies at intermediate redshifts the idea was to investigate the molecular content of galaxies bright in the infrared at z0415 a redshift desert for molecular line studies poorly investigated as of yet we integrated 810h per source and did not succeed in detecting any of the sources from our upper limits we are able to constrain the molecular gas content in these systems to less than 4 to 8 x 109 mo assuming a cotoh_2 conversion factor alpha08 mok km s1 pc2 we stress the current difficulty of selecting sources with a detectable molecular content a problem that will be faced by the alma first science projects
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711.1094
Search for anisotropic effects of hcp solid helium on optical lines of cesium impurities
The anisotropic effect of a hcp 4He solid matrix on cesium atoms has been proposed as a tool to reveal the parity violating anapole moment of its nucleus. It should also result in splitting the D2 optical excitation line in a way depending on the light polarization. An experimental investigation has been set up using oriented hcp helium crystals in which cesium metal grains are embedded. Atoms are created by laser sputtering from this grains. Optical absorption spectra of the D2 line have been recorded in the temperature range of 1.0 to 1.4 K at liquid/solid coexistence pressure by monitoring the fluorescence on the D2 line at 950 nm. No significant effect of the light polarization has been found, suggesting a statistically isotropic disordered solid environment for the cesium atoms.
quant-ph cond-mat.other physics.atom-ph
the anisotropic effect of a hcp 4he solid matrix on cesium atoms has been proposed as a tool to reveal the parity violating anapole moment of its nucleus it should also result in splitting the d2 optical excitation line in a way depending on the light polarization an experimental investigation has been set up using oriented hcp helium crystals in which cesium metal grains are embedded atoms are created by laser sputtering from this grains optical absorption spectra of the d2 line have been recorded in the temperature range of 10 to 14 k at liquidsolid coexistence pressure by monitoring the fluorescence on the d2 line at 950 nm no significant effect of the light polarization has been found suggesting a statistically isotropic disordered solid environment for the cesium atoms
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711.1095
Aging and quenched localization for one-dimensional random walks in random environment in the sub-ballistic regime
We consider transient one-dimensional random walks in random environment with zero asymptotic speed. An aging phenomenon involving the generalized Arcsine law is proved using the localization of the walk at the foot of "valleys" of height $\log t$. In the quenched setting, we also sharply estimate the distribution of the walk at time $t$.
math.PR math-ph math.MP
we consider transient onedimensional random walks in random environment with zero asymptotic speed an aging phenomenon involving the generalized arcsine law is proved using the localization of the walk at the foot of valleys of height log t in the quenched setting we also sharply estimate the distribution of the walk at time t
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711.1096
Piezo-ferroelectrics: Pressure-induced phase transitions in Pb(Zr1-xTix)O3 (PZT)
Piezoelectric PZT solid solutions were studied as a function of pressure and temperature. Moderate pressure is found to induce phase transitions to monoclinic phases (Cm,Cc) for Ti-rich PZT, which are the same ferroelectric phases responsible for the high piezoelectric properties of the MPB. The following transformation sequence P4mm -> Cm -> Cc -> F1 -> F-1 was identified upon increasing pressure. Compression behaviour is dominated by: (1) a rotation and a reduction of the spontaneouspolarization and (2) octahedral tilting leading to unit cell doubling. Future studies as a function of pressure, temperature and electric field on single crystals of heterovalent relaxor ferroelectric isotypes of PZT are proposed in order to better understand these potentially technologically-important piezoferroelectric materials.
cond-mat.mtrl-sci
piezoelectric pzt solid solutions were studied as a function of pressure and temperature moderate pressure is found to induce phase transitions to monoclinic phases cmcc for tirich pzt which are the same ferroelectric phases responsible for the high piezoelectric properties of the mpb the following transformation sequence p4mm cm cc f1 f1 was identified upon increasing pressure compression behaviour is dominated by 1 a rotation and a reduction of the spontaneouspolarization and 2 octahedral tilting leading to unit cell doubling future studies as a function of pressure temperature and electric field on single crystals of heterovalent relaxor ferroelectric isotypes of pzt are proposed in order to better understand these potentially technologicallyimportant piezoferroelectric materials
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711.1097
Multipolar analysis of spinning binaries
We present a preliminary study of the multipolar structure of gravitational radiation from spinning black hole binary mergers. We consider three different spinning binary configurations: (1) one "hang-up" run, where the black holes have equal masses and large spins initially aligned with the orbital angular momentum; (2) seven "spin-flip" runs, where the holes have a mass ratio q=4, the spins are anti-aligned with the orbital angular momentum, and the initial Kerr parameters of the holes j_1=j_2=j_i are fine-tuned to produce a Schwarzschild remnant after merger; (3) three "super-kick" runs where the mass ratio q=M_1/M_2=1, 2, 4 and the spins of the two holes are initially located on the orbital plane, pointing in opposite directions. For all of these simulations we compute the multipolar energy distribution and the Kerr parameter of the final hole. For the hang-up run, we show that including leading-order spin-orbit and spin-spin terms in a multipolar decomposition of the post-Newtonian waveforms improves the agreement with the numerical simulation.
gr-qc
we present a preliminary study of the multipolar structure of gravitational radiation from spinning black hole binary mergers we consider three different spinning binary configurations 1 one hangup run where the black holes have equal masses and large spins initially aligned with the orbital angular momentum 2 seven spinflip runs where the holes have a mass ratio q4 the spins are antialigned with the orbital angular momentum and the initial kerr parameters of the holes j_1j_2j_i are finetuned to produce a schwarzschild remnant after merger 3 three superkick runs where the mass ratio qm_1m_21 2 4 and the spins of the two holes are initially located on the orbital plane pointing in opposite directions for all of these simulations we compute the multipolar energy distribution and the kerr parameter of the final hole for the hangup run we show that including leadingorder spinorbit and spinspin terms in a multipolar decomposition of the postnewtonian waveforms improves the agreement with the numerical simulation
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711.1098
A Cosmological Sector in Loop Quantum Gravity
We use the method of embedding a subsystem (i.e. its observable algebra) into a larger quantum system to extract a cosmological sector from full Loop Quantum Gravity. The application of this method provides a setting for a systematic study of the interplay between diffeomorphism invariance and symmetry reduction. The non-triviality of this relation is shown by extracting a cosmological system that has configurations variables that are very similar to the ones of a super-selection sector of standard Loop Quantum Cosmology. The full operator algebra however turns out to be different from standard Loop Quantum Cosmology. The homogeneous isotropic sector of pure gravity turns out to be quantum mechanics on a circle. The dynamics of our system seems pathological at first sight, and we give both mathematical and physical reasons for this behavior and we explain a strategy to cure these pathologies.
gr-qc
we use the method of embedding a subsystem ie its observable algebra into a larger quantum system to extract a cosmological sector from full loop quantum gravity the application of this method provides a setting for a systematic study of the interplay between diffeomorphism invariance and symmetry reduction the nontriviality of this relation is shown by extracting a cosmological system that has configurations variables that are very similar to the ones of a superselection sector of standard loop quantum cosmology the full operator algebra however turns out to be different from standard loop quantum cosmology the homogeneous isotropic sector of pure gravity turns out to be quantum mechanics on a circle the dynamics of our system seems pathological at first sight and we give both mathematical and physical reasons for this behavior and we explain a strategy to cure these pathologies
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711.1099
Approximating Perpetuities
We propose and analyze an algorithm to approximate distribution functions and densities of perpetuities. Our algorithm refines an earlier approach based on iterating discretized versions of the fixed point equation that defines the perpetuity. We significantly reduce the complexity of the earlier algorithm. Also one particular perpetuity arising in the analysis of the selection algorithm Quickselect is studied in more detail. Our approach works well for distribution functions. For densities we have weaker error bounds although computer experiments indicate that densities can also be approximated well.
math.PR
we propose and analyze an algorithm to approximate distribution functions and densities of perpetuities our algorithm refines an earlier approach based on iterating discretized versions of the fixed point equation that defines the perpetuity we significantly reduce the complexity of the earlier algorithm also one particular perpetuity arising in the analysis of the selection algorithm quickselect is studied in more detail our approach works well for distribution functions for densities we have weaker error bounds although computer experiments indicate that densities can also be approximated well
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711.11
The square gradient model in a two-phase mixture II. Non-equilibrium properties of a 2D-isotropic interface
In earlier work \cite{bedeaux/vdW/I, bedeaux/vdW/II, bedeaux/vdW/III} a systematic extension of the van der Waals square gradient model to non-equilibrium one-component systems was given. In this work the focus was on heat and mass transfer through the liquid-vapor interface as caused by a temperature difference or an over or under pressure. It was established that the surface as described using Gibbs excess densities was in local equilibrium. Heat and mass transfer coefficients were evaluated. In our first paper \cite{glav/gradient/eq/I} we discussed the equilibrium properties of a multi-component system following the same procedure. In particular, we derived an explicit expression for the pressure tensor and discussed the validity of the Gibbs relation in the interfacial region. In this paper we will give an extension of this approach to multi-component non-equilibrium systems in the systematic context of non-equilibrium thermodynamics. The two-dimensional isotropy of the interface is discussed. Furthermore we give numerically obtained profiles of the concentration, the mole fraction and the temperature, which illustrate the solution for some special cases.
cond-mat.soft cond-mat.stat-mech
in earlier work citebedeauxvdwi bedeauxvdwii bedeauxvdwiii a systematic extension of the van der waals square gradient model to nonequilibrium onecomponent systems was given in this work the focus was on heat and mass transfer through the liquidvapor interface as caused by a temperature difference or an over or under pressure it was established that the surface as described using gibbs excess densities was in local equilibrium heat and mass transfer coefficients were evaluated in our first paper citeglavgradienteqi we discussed the equilibrium properties of a multicomponent system following the same procedure in particular we derived an explicit expression for the pressure tensor and discussed the validity of the gibbs relation in the interfacial region in this paper we will give an extension of this approach to multicomponent nonequilibrium systems in the systematic context of nonequilibrium thermodynamics the twodimensional isotropy of the interface is discussed furthermore we give numerically obtained profiles of the concentration the mole fraction and the temperature which illustrate the solution for some special cases
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711.1101
Magnetic properties of bi-phase micro- and nanotubes
The magnetic configurations of bi-phase micro- and nanotubes consisting of a ferromagnetic internal tube, an intermediate non-magnetic spacer, and an external magnetic shell are investigated as a function of their geometry. Based on a continuum approach we obtained analytical expressions for the energy which lead us to obtain phase diagrams giving the relative stability of characteristic internal magnetic configurations of the bi-phase tubes.
cond-mat.mtrl-sci cond-mat.soft
the magnetic configurations of biphase micro and nanotubes consisting of a ferromagnetic internal tube an intermediate nonmagnetic spacer and an external magnetic shell are investigated as a function of their geometry based on a continuum approach we obtained analytical expressions for the energy which lead us to obtain phase diagrams giving the relative stability of characteristic internal magnetic configurations of the biphase tubes
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711.1102
Approche p\'edagogique sur l'innocuit\'e des technologies de r\'eseaux sans fil
The wireless networks technologies are becoming more prevalent. As part of our courses, we have to deal with the technical aspects of these technologies. However, the experience of mobile telephony has shown fears that these products can lead to the general public. The latter comes from the use of electromagnetic waves at frequencies close to the frequencies of microwaves oven(2.45 GHz). Studies are under way for years in order to identify the possible effects on the body related to prolonged use of mobile phones. Wireless networks like WiFi or ZigBee for example works with microwave frequencies. On the other hand, problems relating to electromagnetic compatibility waves with the electronic devices must also be studied. The question of the safety of these technologies must be addressed with the students. They will may need to install such equipment. We have integrated the teaching of wireless networks in a chapter dealing with current standards of exposure to electromagnetic waves for living beings and the electronic devices. The aim of our approach is the obtention of knowledges by the student. so he will be able to form an opinion and to provide a speech enlightened to future users of these networks. To this end, we have developed a visualization tool for the distribution of electromagnetic fields. This tool being used will help you understand the electromagnetic environment in which we live and quantify the values of electromagnetic fields (telephony, television, radio, WiFi, Bluetooth, ZigBee, microwave oven, etc.).
physics.ed-ph physics.pop-ph
the wireless networks technologies are becoming more prevalent as part of our courses we have to deal with the technical aspects of these technologies however the experience of mobile telephony has shown fears that these products can lead to the general public the latter comes from the use of electromagnetic waves at frequencies close to the frequencies of microwaves oven245 ghz studies are under way for years in order to identify the possible effects on the body related to prolonged use of mobile phones wireless networks like wifi or zigbee for example works with microwave frequencies on the other hand problems relating to electromagnetic compatibility waves with the electronic devices must also be studied the question of the safety of these technologies must be addressed with the students they will may need to install such equipment we have integrated the teaching of wireless networks in a chapter dealing with current standards of exposure to electromagnetic waves for living beings and the electronic devices the aim of our approach is the obtention of knowledges by the student so he will be able to form an opinion and to provide a speech enlightened to future users of these networks to this end we have developed a visualization tool for the distribution of electromagnetic fields this tool being used will help you understand the electromagnetic environment in which we live and quantify the values of electromagnetic fields telephony television radio wifi bluetooth zigbee microwave oven etc
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711.1103
From Dirac spinor fields to ELKO
Dual-helicity eigenspinors of the charge conjugation operator (ELKO spinor fields) belong, together with Majorana spinor fields, to a wider class of spinor fields, the so-called flagpole spinor fields, corresponding to the class (5), according to Lounesto spinor field classification based on the relations and values taken by their associated bilinear covariants. There exists only six such disjoint classes: the first three corresponding to Dirac spinor fields, and the other three respectively corresponding to flagpole, flag-dipole and Weyl spinor fields. This paper is devoted to investigate and provide the necessary and sufficient conditions to map Dirac spinor fields to ELKO, in order to naturally extend the Standard Model to spinor fields possessing mass dimension one. As ELKO is a prime candidate to describe dark matter, an adequate and necessary formalism is introduced and developed here, to better understand the algebraic, geometric and physical properties of ELKO spinor fields, and their underlying relationship to Dirac spinor fields.
math-ph hep-th math.MP
dualhelicity eigenspinors of the charge conjugation operator elko spinor fields belong together with majorana spinor fields to a wider class of spinor fields the socalled flagpole spinor fields corresponding to the class 5 according to lounesto spinor field classification based on the relations and values taken by their associated bilinear covariants there exists only six such disjoint classes the first three corresponding to dirac spinor fields and the other three respectively corresponding to flagpole flagdipole and weyl spinor fields this paper is devoted to investigate and provide the necessary and sufficient conditions to map dirac spinor fields to elko in order to naturally extend the standard model to spinor fields possessing mass dimension one as elko is a prime candidate to describe dark matter an adequate and necessary formalism is introduced and developed here to better understand the algebraic geometric and physical properties of elko spinor fields and their underlying relationship to dirac spinor fields
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711.1104
Selection Principles and Baire spaces
We prove that if X is a separable metric space with the Hurewicz covering property, then the Banach-Mazur game played on X is determined. The implication is not true when "Hurewicz covering property" is replaced with "Menger covering property".
math.GN
we prove that if x is a separable metric space with the hurewicz covering property then the banachmazur game played on x is determined the implication is not true when hurewicz covering property is replaced with menger covering property
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711.1105
The fine-grained phase-space structure of Cold Dark Matter halos
We present a new and completely general technique for calculating the fine-grained phase-space structure of dark matter throughout the Galactic halo. Our goal is to understand this structure on the scales relevant for direct and indirect detection experiments. Our method is based on evaluating the geodesic deviation equation along the trajectories of individual DM particles. It requires no assumptions about the symmetry or stationarity of the halo formation process. In this paper we study general static potentials which exhibit more complex behaviour than the separable potentials studied previously. For ellipsoidal logarithmic potentials with a core, phase mixing is sensitive to the resonance structure, as indicated by the number of independent orbital frequencies. Regions of chaotic mixing can be identified by the very rapid decrease in the real space density of the associated dark matter streams. We also study the evolution of stream density in ellipsoidal NFW halos with radially varying isopotential shape, showing that if such a model is applied to the Galactic halo, at least $10^5$ streams are expected near the Sun. The most novel aspect of our approach is that general non-static systems can be studied through implementation in a cosmological N-body code. Such an implementation allows a robust and accurate evaluation of the enhancements in annihilation radiation due to fine-scale structure such as caustics. We embed the scheme in the current state-of-the-art code GADGET-3 and present tests which demonstrate that N-body discreteness effects can be kept under control in realistic configurations.
astro-ph
we present a new and completely general technique for calculating the finegrained phasespace structure of dark matter throughout the galactic halo our goal is to understand this structure on the scales relevant for direct and indirect detection experiments our method is based on evaluating the geodesic deviation equation along the trajectories of individual dm particles it requires no assumptions about the symmetry or stationarity of the halo formation process in this paper we study general static potentials which exhibit more complex behaviour than the separable potentials studied previously for ellipsoidal logarithmic potentials with a core phase mixing is sensitive to the resonance structure as indicated by the number of independent orbital frequencies regions of chaotic mixing can be identified by the very rapid decrease in the real space density of the associated dark matter streams we also study the evolution of stream density in ellipsoidal nfw halos with radially varying isopotential shape showing that if such a model is applied to the galactic halo at least 105 streams are expected near the sun the most novel aspect of our approach is that general nonstatic systems can be studied through implementation in a cosmological nbody code such an implementation allows a robust and accurate evaluation of the enhancements in annihilation radiation due to finescale structure such as caustics we embed the scheme in the current stateoftheart code gadget3 and present tests which demonstrate that nbody discreteness effects can be kept under control in realistic configurations
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711.1106
Ageing in homogeneous systems at criticality
Ageing phenomena are observed in a large variety of dynamical systems exhibiting a slow relaxation from a non-equilibrium initial state. Ageing can be characterised in terms of the linear response R(t,s) at time t to a local perturbation at time s<t. Usually one distinguishes two dynamical regimes, namely, the quasi-stationary regime, where the response is translationally invariant in time, and the ageing regime, where this invariance is broken. In general these two regimes are separate in the sense that the two limits of (a) taking t,s to infinity while keeping t/s fixed, and (b) taking t,s to infinity with fixed t-s, give different results. In recent years, ageing was also investigated in the context of homogeneous critical systems such as the Glauber-Ising model and the contact process. Here we argue that, in contrast to a widespread believe, homogeneous critical systems do not have a separate quasi-stationary regime, hence the two limits do commute. Moreover, it is discussed under which conditions two particular exponents, denoted as a and a' in the literature, have to be identical.
cond-mat.stat-mech
ageing phenomena are observed in a large variety of dynamical systems exhibiting a slow relaxation from a nonequilibrium initial state ageing can be characterised in terms of the linear response rts at time t to a local perturbation at time st usually one distinguishes two dynamical regimes namely the quasistationary regime where the response is translationally invariant in time and the ageing regime where this invariance is broken in general these two regimes are separate in the sense that the two limits of a taking ts to infinity while keeping ts fixed and b taking ts to infinity with fixed ts give different results in recent years ageing was also investigated in the context of homogeneous critical systems such as the glauberising model and the contact process here we argue that in contrast to a widespread believe homogeneous critical systems do not have a separate quasistationary regime hence the two limits do commute moreover it is discussed under which conditions two particular exponents denoted as a and a in the literature have to be identical
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711.1107
Correlated X-ray and Optical Variability in Mkn 509
We present results of a 3 year monitoring campaign of the Seyfert 1 galaxy Markarian 509, using X-ray data from the Rossi X-ray Timing Explorer (RXTE) and optical data taken by the SMARTS consortium. Both light curves show significant variations, and are strongly correlated with the optical flux leading the X-ray flux by 15 days. The X-ray power spectrum shows a steep high-frequency slope of -2.0, breaking to a slope of -1.0 at at timescale of 34 days. The lag from optical to X-ray emission is most likely caused by variations in the accretion disk propagating inward.
astro-ph
we present results of a 3 year monitoring campaign of the seyfert 1 galaxy markarian 509 using xray data from the rossi xray timing explorer rxte and optical data taken by the smarts consortium both light curves show significant variations and are strongly correlated with the optical flux leading the xray flux by 15 days the xray power spectrum shows a steep highfrequency slope of 20 breaking to a slope of 10 at at timescale of 34 days the lag from optical to xray emission is most likely caused by variations in the accretion disk propagating inward
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