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711.0308
The influence of bond-rigidity and cluster diffusion on the self-diffusion of hard spheres with square-well interaction
Hard spheres interacting through a square-well potential were simulated using two different methods: Brownian Cluster Dynamics (BCD) and Event Driven Brownian Dynamics (EDBD). The structure of the equilibrium states obtained by both methods were compared and found to be almost the identical. Self diffusion coefficients ($D$) were determined as a function of the interaction strength. The same values were found using BCD or EDBD. Contrary the EDBD, BCD allows one to study the effect of bond rigidity and hydrodynamic interaction within the clusters. When the bonds are flexible the effect of attraction on $D$ is relatively weak compared to systems with rigid bonds. $D$ increases first with increasing attraction strength, and then decreases for stronger interaction. Introducing intra-cluster hydrodynamic interaction weakly increases $D$ for a given interaction strength. Introducing bond rigidity causes a strong decrease of $D$ which no longer shows a maximum as function of the attraction strength.
cond-mat.soft
hard spheres interacting through a squarewell potential were simulated using two different methods brownian cluster dynamics bcd and event driven brownian dynamics edbd the structure of the equilibrium states obtained by both methods were compared and found to be almost the identical self diffusion coefficients d were determined as a function of the interaction strength the same values were found using bcd or edbd contrary the edbd bcd allows one to study the effect of bond rigidity and hydrodynamic interaction within the clusters when the bonds are flexible the effect of attraction on d is relatively weak compared to systems with rigid bonds d increases first with increasing attraction strength and then decreases for stronger interaction introducing intracluster hydrodynamic interaction weakly increases d for a given interaction strength introducing bond rigidity causes a strong decrease of d which no longer shows a maximum as function of the attraction strength
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711.0309
Recent developments in effective field theory
We will give a short introduction to the one-nucleon sector of chiral perturbation theory and will address the issue of a consistent power counting and renormalization. We will discuss the infrared regularization and the extended on-mass-shell scheme. Both allow for the inclusion of further degrees of freedom beyond pions and nucleons and the application to higher-loop calculations. As applications we consider the chiral expansion of the nucleon mass to order O(q^6) and the inclusion of vector and axial-vector mesons in the calculation of nucleon form factors.
nucl-th
we will give a short introduction to the onenucleon sector of chiral perturbation theory and will address the issue of a consistent power counting and renormalization we will discuss the infrared regularization and the extended onmassshell scheme both allow for the inclusion of further degrees of freedom beyond pions and nucleons and the application to higherloop calculations as applications we consider the chiral expansion of the nucleon mass to order oq6 and the inclusion of vector and axialvector mesons in the calculation of nucleon form factors
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711.031
Boundary state of superstring in open string channel
We derive boundary state of superstring in the open string channel. It describes the superconformal field theory of open string emission and absorption by D-brane. We define the boundary state by conformal mappings from upper half plane with operators inserted at two points corresponding to the corners of semi-infinite strip. We obtain explicit oscillator forms analytically for the fermion and superconformal ghost sectors. For the fermion sector we compare this with numerical result obtained by using naive boundary condition.
hep-th
we derive boundary state of superstring in the open string channel it describes the superconformal field theory of open string emission and absorption by dbrane we define the boundary state by conformal mappings from upper half plane with operators inserted at two points corresponding to the corners of semiinfinite strip we obtain explicit oscillator forms analytically for the fermion and superconformal ghost sectors for the fermion sector we compare this with numerical result obtained by using naive boundary condition
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711.0311
Improving the LP bound of a MILP by branching concurrently
We'll measure the differences of the dual variables and the gain of the objective function when creating new problems, which each has one inequality more than the starting LP-instance. These differences of the dual variables are naturally connected to the branches. Then we'll choose those differences of dual variables, so that for all combinations of choices at the connected branches, all dual inequalities will hold for sure. By adding the gain of each chosen branching, we get a total gain, which gives a better limit of the original problem. By this technique it is also possible to create cuts.
cs.DM cs.DS
well measure the differences of the dual variables and the gain of the objective function when creating new problems which each has one inequality more than the starting lpinstance these differences of the dual variables are naturally connected to the branches then well choose those differences of dual variables so that for all combinations of choices at the connected branches all dual inequalities will hold for sure by adding the gain of each chosen branching we get a total gain which gives a better limit of the original problem by this technique it is also possible to create cuts
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711.0312
Period Lengths for Iterated Functions
For random maps, the expected value of the order (i.e. the period of the sequence of compositional iterates) is approximated asymptotically. It is much smaller than the expected value for the product of the cycle lengths.
math.CO math.PR
for random maps the expected value of the order ie the period of the sequence of compositional iterates is approximated asymptotically it is much smaller than the expected value for the product of the cycle lengths
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711.0313
Black holes as local horizons
This talk gives a brief introduction to black hole horizons and their role in black hole thermodynamics. In particular a distinction is made between quasi-locally defined horizons and event horizons. Currently some new techniques have led to interesting developments and the field seems to be growing in two distinct directions. We will show how thermodynamics can equally well be applied to locally defined horizons and discuss some recent results. The emphasis is on giving simple intuitive pictures and mathematical details are largely omitted.
gr-qc
this talk gives a brief introduction to black hole horizons and their role in black hole thermodynamics in particular a distinction is made between quasilocally defined horizons and event horizons currently some new techniques have led to interesting developments and the field seems to be growing in two distinct directions we will show how thermodynamics can equally well be applied to locally defined horizons and discuss some recent results the emphasis is on giving simple intuitive pictures and mathematical details are largely omitted
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711.0314
Resource and Application Models for Advanced Grid Schedulers
As Grid computing is becoming an inevitable future, managing, scheduling and monitoring dynamic, heterogeneous resources will present new challenges. Solutions will have to be agile and adaptive, support self-organization and autonomous management, while maintaining optimal resource utilisation. Presented in this paper are basic principles and architectural concepts for efficient resource allocation in heterogeneous Grid environment.
cs.DC
as grid computing is becoming an inevitable future managing scheduling and monitoring dynamic heterogeneous resources will present new challenges solutions will have to be agile and adaptive support selforganization and autonomous management while maintaining optimal resource utilisation presented in this paper are basic principles and architectural concepts for efficient resource allocation in heterogeneous grid environment
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711.0315
Measuring and Monitoring Grid Resource Utilisation
Effective resource utilisation monitoring and highly granular yet adaptive measurements are prerequisites for a more efficient Grid scheduler. We present a suite of measurement applications able to monitor per-process resource utilisation, and a customisable tool for emulating observed utilisation models.
cs.DC
effective resource utilisation monitoring and highly granular yet adaptive measurements are prerequisites for a more efficient grid scheduler we present a suite of measurement applications able to monitor perprocess resource utilisation and a customisable tool for emulating observed utilisation models
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711.0316
A Study of Grid Applications: Scheduling Perspective
As the Grid evolves from a high performance cluster middleware to a multipurpose utility computing framework, a good understanding of Grid applications, their statistics and utilisation patterns is required. This study looks at job execution times and resource utilisations in a Grid environment, and their significance in cluster and network dimensioning, local level scheduling and resource management.
cs.DC
as the grid evolves from a high performance cluster middleware to a multipurpose utility computing framework a good understanding of grid applications their statistics and utilisation patterns is required this study looks at job execution times and resource utilisations in a grid environment and their significance in cluster and network dimensioning local level scheduling and resource management
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711.0317
Hastening, delaying, or averting sudden death of quantum entanglement
The finite time end of entanglement between two decohering qubits can be modified by local, unitary actions performed during the decohering process. Depending on the time when such action is taken, the end can be speeded up or slowed down, or even averted all together. This phenomenon offers practical applications for the stabilization of entangled quantum states. Details concerning hastening or delaying the finite time end of entanglement are presented for two qubits which decay spontaneously into statistically independent reservoirs.
quant-ph
the finite time end of entanglement between two decohering qubits can be modified by local unitary actions performed during the decohering process depending on the time when such action is taken the end can be speeded up or slowed down or even averted all together this phenomenon offers practical applications for the stabilization of entangled quantum states details concerning hastening or delaying the finite time end of entanglement are presented for two qubits which decay spontaneously into statistically independent reservoirs
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711.0318
Exact solution of the extended Hubbard model in the atomic limit on the Bethe Lattice
We study the phase diagram at finite temperature of a system of Fermi particles on the sites of the Bethe lattice with coordination number z and interacting through onsite U and nearest-neighbor V interactions. This is a physical realization of the extended Hubbard model in the atomic limit. By using the equations of motion method, we exactly solve the model. For an attractive intersite potential, we find, at half filling, a phase transition towards a broken particle-hole symmetry state. The critical temperature, as a function of the relevant parameters, has a re-entrant behavior as already observed in the equivalent spin-1 Ising model on the Bethe lattice.
cond-mat.str-el cond-mat.stat-mech
we study the phase diagram at finite temperature of a system of fermi particles on the sites of the bethe lattice with coordination number z and interacting through onsite u and nearestneighbor v interactions this is a physical realization of the extended hubbard model in the atomic limit by using the equations of motion method we exactly solve the model for an attractive intersite potential we find at half filling a phase transition towards a broken particlehole symmetry state the critical temperature as a function of the relevant parameters has a reentrant behavior as already observed in the equivalent spin1 ising model on the bethe lattice
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711.0319
Observation and properties of the orbitally excited B_{s2}* Meson
We report the direct observation of the excited L=1 state B_{s2}* in fully reconstructed decays to B+K-. The mass of the B_{s2}* meson is measured to be {5839.6 +- 1.1 (stat.) +- 0.7 (syst.) MeV/c^2, and its production rate relative to the B+ meson is measured to be [1.15 +- 0.23 (stat.) +- 0.13 (syst.)] %.
hep-ex
we report the direct observation of the excited l1 state b_s2 in fully reconstructed decays to bk the mass of the b_s2 meson is measured to be 58396 11 stat 07 syst mevc2 and its production rate relative to the b meson is measured to be 115 023 stat 013 syst
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711.032
Electric-field controlled spin reversal in a quantum dot with ferromagnetic contacts
Manipulation of the spin-states of a quantum dot by purely electrical means is a highly desirable property of fundamental importance for the development of spintronic devices such as spin-filters, spin-transistors and single-spin memory as well as for solid-state qubits. An electrically gated quantum dot in the Coulomb blockade regime can be tuned to hold a single unpaired spin-1/2, which is routinely spin-polarized by an applied magnetic field. Using ferromagnetic electrodes, however, the properties of the quantum dot become directly spin-dependent and it has been demonstrated that the ferromagnetic electrodes induce a local exchange-field which polarizes the localized spin in the absence of any external fields. Here we report on the experimental realization of this tunneling-induced spin-splitting in a carbon nanotube quantum dot coupled to ferromagnetic nickel-electrodes. We study the intermediate coupling regime in which single-electron states remain well defined, but with sufficiently good tunnel-contacts to give rise to a sizable exchange-field. Since charge transport in this regime is dominated by the Kondo-effect, we can utilize this sharp many-body resonance to read off the local spin-polarization from the measured bias-spectroscopy. We show that the exchange-field can be compensated by an external magnetic field, thus restoring a zero-bias Kondo-resonance, and we demonstrate that the exchange-field itself, and hence the local spin-polarization, can be tuned and reversed merely by tuning the gate-voltage. This demonstrates a very direct electrical control over the spin-state of a quantum dot which, in contrast to an applied magnetic field, allows for rapid spin-reversal with a very localized addressing.
cond-mat.mes-hall cond-mat.str-el
manipulation of the spinstates of a quantum dot by purely electrical means is a highly desirable property of fundamental importance for the development of spintronic devices such as spinfilters spintransistors and singlespin memory as well as for solidstate qubits an electrically gated quantum dot in the coulomb blockade regime can be tuned to hold a single unpaired spin12 which is routinely spinpolarized by an applied magnetic field using ferromagnetic electrodes however the properties of the quantum dot become directly spindependent and it has been demonstrated that the ferromagnetic electrodes induce a local exchangefield which polarizes the localized spin in the absence of any external fields here we report on the experimental realization of this tunnelinginduced spinsplitting in a carbon nanotube quantum dot coupled to ferromagnetic nickelelectrodes we study the intermediate coupling regime in which singleelectron states remain well defined but with sufficiently good tunnelcontacts to give rise to a sizable exchangefield since charge transport in this regime is dominated by the kondoeffect we can utilize this sharp manybody resonance to read off the local spinpolarization from the measured biasspectroscopy we show that the exchangefield can be compensated by an external magnetic field thus restoring a zerobias kondoresonance and we demonstrate that the exchangefield itself and hence the local spinpolarization can be tuned and reversed merely by tuning the gatevoltage this demonstrates a very direct electrical control over the spinstate of a quantum dot which in contrast to an applied magnetic field allows for rapid spinreversal with a very localized addressing
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711.0321
The rare decays $B^+_u\to\pi^+\ell^+\ell^-$, $\rho^+\ell^+\ell^-$ and $B^0_d\to \ell^+\ell^-$ in the R-parity violating supersymmetry
We study the rare decays $B^{+}_u\to \pi^{+}\ell^{+}\ell^{-}$, $\rho^{+}\ell^{+}\ell^{-}$ and $B^{0}_d \to \ell^{+} \ell^{-}(\ell=e,\mu)$ in the R-parity violating supersymmetric standard model. From the latest upper limits of $\mathcal{B}(B^+_u\to\pi^+\ell^+\ell^-)$ and $\mathcal{B}(B^0_d\to\ell^+\ell^-)$, we have derived new upper bounds on the relevant R-parity violating couplings products, which are stronger than the existing ones. Using the constrained parameter space, we present the R-parity violating effects on the branching ratios and the forward-backward asymmetries of these decays. We find that $\mathcal{B}(B^0_d\to \ell^+\ell^-)$ and $\mathcal{B}(B^+_u \to\rho^+\ell^+\ell^-)$ could be enhanced several orders by the R-parity violating sneutrino and squark exchanges, respectively. The R-parity violating effects on the dilepton invariant mass spectra of $B^+_u\to \pi^+\ell^+\ell^-$, $\rho^+\ell^+\ell^-$ and the normalized forward-backward asymmetry $\mathcal{A}_{FB}(B^+_u\to\pi^+\ell^+\ell^-)$ and $\mathcal{A}_{FB}(B^+_u \to\rho^+\ell^+\ell^-)$ are studied in detail. Our results could be used to probe the R-parity violating effects and will correlate with searches for the direct R-parity violating signals at the future experiments.
hep-ph
we study the rare decays b_uto piellell rhoellell and b0_d to ell ellellemu in the rparity violating supersymmetric standard model from the latest upper limits of mathcalbb_utopiellell and mathcalbb0_dtoellell we have derived new upper bounds on the relevant rparity violating couplings products which are stronger than the existing ones using the constrained parameter space we present the rparity violating effects on the branching ratios and the forwardbackward asymmetries of these decays we find that mathcalbb0_dto ellell and mathcalbb_u torhoellell could be enhanced several orders by the rparity violating sneutrino and squark exchanges respectively the rparity violating effects on the dilepton invariant mass spectra of b_uto piellell rhoellell and the normalized forwardbackward asymmetry mathcala_fbb_utopiellell and mathcala_fbb_u torhoellell are studied in detail our results could be used to probe the rparity violating effects and will correlate with searches for the direct rparity violating signals at the future experiments
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711.0322
The Formation of Hydrogen Deficient Stars through Common Envelope Evolution
We present preliminary results from Smooth Particle Hydrodynamics (SPH) simulations of common envelope evolution. We qualitatively compare the interaction between a 0.9M red giant with two different companion masses: a 0.05M brown dwarf and a 0.25M white dwarf companion.
astro-ph
we present preliminary results from smooth particle hydrodynamics sph simulations of common envelope evolution we qualitatively compare the interaction between a 09m red giant with two different companion masses a 005m brown dwarf and a 025m white dwarf companion
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711.0323
Single Spin Effects in Collisions of Hadrons and Heavy Ions at High Energy
Experimental data on transverse single-spin asymmetry, hyperon polarization and vector meson alignment in h+h, h+A and A+A-collisions have been analyzed. A new mechanism for the origin of single spin effects is proposed, which takes into account the interaction of massive constituent quarks via their chromomagnetic moment with an effective inhomogeneous chromomagnetic field of strings, produced after the initial color exchange. Quark spin precession in the color field is taken into account, which can be the reason for an oscillation of the single spin observables as a function of Feynman $x_{F}$ and its energy dependence. The model predictions are compared with the experimental data, in particular with the heavy ion collision data. The data are consistent with a large negative anomalous chromomagnetic moment of the constituent quarks which is predicted in the instanton model.
hep-ph
experimental data on transverse singlespin asymmetry hyperon polarization and vector meson alignment in hh ha and aacollisions have been analyzed a new mechanism for the origin of single spin effects is proposed which takes into account the interaction of massive constituent quarks via their chromomagnetic moment with an effective inhomogeneous chromomagnetic field of strings produced after the initial color exchange quark spin precession in the color field is taken into account which can be the reason for an oscillation of the single spin observables as a function of feynman x_f and its energy dependence the model predictions are compared with the experimental data in particular with the heavy ion collision data the data are consistent with a large negative anomalous chromomagnetic moment of the constituent quarks which is predicted in the instanton model
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711.0324
Tensor product for symmetric monoidal categories
We introduce a tensor product for symmetric monoidal categories with the following properties. Let SMC denote the 2-category with objects small symmetric monoidal categories, arrows symmetric monoidal functors and 2-cells monoidal natural transformations. Our tensor product together with a suitable unit is part of a structure on SMC that is a 2-categorical version of the symmetric monoidal closed categories. This structure is surprisingly simple. In particular the arrows involved in the associativity and symmetry laws for the tensor and in the unit cancellation laws are 2-natural and satisfy coherence axioms which are strictly commuting diagrams. We also show that the category quotient of SMC by the congruence generated by its 2-cells admits a symmetric monoidal closed structure.
math.CT math.AT
we introduce a tensor product for symmetric monoidal categories with the following properties let smc denote the 2category with objects small symmetric monoidal categories arrows symmetric monoidal functors and 2cells monoidal natural transformations our tensor product together with a suitable unit is part of a structure on smc that is a 2categorical version of the symmetric monoidal closed categories this structure is surprisingly simple in particular the arrows involved in the associativity and symmetry laws for the tensor and in the unit cancellation laws are 2natural and satisfy coherence axioms which are strictly commuting diagrams we also show that the category quotient of smc by the congruence generated by its 2cells admits a symmetric monoidal closed structure
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711.0325
Self-Organising management of Grid environments
This paper presents basic concepts, architectural principles and algorithms for efficient resource and security management in cluster computing environments and the Grid. The work presented in this paper is funded by BTExacT and the EPSRC project SO-GRM (GR/S21939).
cs.DC
this paper presents basic concepts architectural principles and algorithms for efficient resource and security management in cluster computing environments and the grid the work presented in this paper is funded by btexact and the epsrc project sogrm grs21939
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711.0326
Enabling Adaptive Grid Scheduling and Resource Management
Wider adoption of the Grid concept has led to an increasing amount of federated computational, storage and visualisation resources being available to scientists and researchers. Distributed and heterogeneous nature of these resources renders most of the legacy cluster monitoring and management approaches inappropriate, and poses new challenges in workflow scheduling on such systems. Effective resource utilisation monitoring and highly granular yet adaptive measurements are prerequisites for a more efficient Grid scheduler. We present a suite of measurement applications able to monitor per-process resource utilisation, and a customisable tool for emulating observed utilisation models. We also outline our future work on a predictive and probabilistic Grid scheduler. The research is undertaken as part of UK e-Science EPSRC sponsored project SO-GRM (Self-Organising Grid Resource Management) in cooperation with BT.
cs.DC
wider adoption of the grid concept has led to an increasing amount of federated computational storage and visualisation resources being available to scientists and researchers distributed and heterogeneous nature of these resources renders most of the legacy cluster monitoring and management approaches inappropriate and poses new challenges in workflow scheduling on such systems effective resource utilisation monitoring and highly granular yet adaptive measurements are prerequisites for a more efficient grid scheduler we present a suite of measurement applications able to monitor perprocess resource utilisation and a customisable tool for emulating observed utilisation models we also outline our future work on a predictive and probabilistic grid scheduler the research is undertaken as part of uk escience epsrc sponsored project sogrm selforganising grid resource management in cooperation with bt
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711.0327
Managing Uncertainty: A Case for Probabilistic Grid Scheduling
The Grid technology is evolving into a global, service-orientated architecture, a universal platform for delivering future high demand computational services. Strong adoption of the Grid and the utility computing concept is leading to an increasing number of Grid installations running a wide range of applications of different size and complexity. In this paper we address the problem of elivering deadline/economy based scheduling in a heterogeneous application environment using statistical properties of job historical executions and its associated meta-data. This approach is motivated by a study of six-month computational load generated by Grid applications in a multi-purpose Grid cluster serving a community of twenty e-Science projects. The observed job statistics, resource utilisation and user behaviour is discussed in the context of management approaches and models most suitable for supporting a probabilistic and autonomous scheduling architecture.
cs.DC
the grid technology is evolving into a global serviceorientated architecture a universal platform for delivering future high demand computational services strong adoption of the grid and the utility computing concept is leading to an increasing number of grid installations running a wide range of applications of different size and complexity in this paper we address the problem of elivering deadlineeconomy based scheduling in a heterogeneous application environment using statistical properties of job historical executions and its associated metadata this approach is motivated by a study of sixmonth computational load generated by grid applications in a multipurpose grid cluster serving a community of twenty escience projects the observed job statistics resource utilisation and user behaviour is discussed in the context of management approaches and models most suitable for supporting a probabilistic and autonomous scheduling architecture
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711.0328
Intermediate long X-ray bursts from the ultra-compact binary source SLX 1737-282
Aims: The low persistent X-ray burster source SLX 1737-282 is classified as an ultra-compact binary candidate. We compare the data on SLX 1737-282 with the other similar objects and attempt to derive constraints on the physical processes responsible for the formation of intermediate long bursts. Methods: Up to now only three intermediate long bursts, all with duration between ~15-30 minutes, have been recorded for SLX 1737-282. The properties of two intermediate long X-ray bursts observed by INTEGRAL from SLX 1737-282 are investigated. The broadband spectrum of the persistent emission in the 3-100 keV energy band is studied with the INTEGRAL data. Results: The persistent emission is measured to be < 1% Eddington luminosity. From the photospheric radius expansion observed during the bursts we derive the source distance at 7.3 kpc. The observed intermediate long burst properties from SLX 1737-282 are consistent with helium ignition at the column depth of 7-8 x 10E-9 g cm-2 and a burst energy release of 1E41 erg. The apparent recurrence time of ~80 days between the intermediate long bursts from SLX 1737-282 suggests a regime of unstable burning of a thick, pure helium layer slowly accreted from a helium donor star.
astro-ph
aims the low persistent xray burster source slx 1737282 is classified as an ultracompact binary candidate we compare the data on slx 1737282 with the other similar objects and attempt to derive constraints on the physical processes responsible for the formation of intermediate long bursts methods up to now only three intermediate long bursts all with duration between 1530 minutes have been recorded for slx 1737282 the properties of two intermediate long xray bursts observed by integral from slx 1737282 are investigated the broadband spectrum of the persistent emission in the 3100 kev energy band is studied with the integral data results the persistent emission is measured to be 1 eddington luminosity from the photospheric radius expansion observed during the bursts we derive the source distance at 73 kpc the observed intermediate long burst properties from slx 1737282 are consistent with helium ignition at the column depth of 78 x 10e9 g cm2 and a burst energy release of 1e41 erg the apparent recurrence time of 80 days between the intermediate long bursts from slx 1737282 suggests a regime of unstable burning of a thick pure helium layer slowly accreted from a helium donor star
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711.0329
The Monitor project: Rotation of low-mass stars in the open cluster NGC 2547
We report on the results of an I-band time-series photometric survey of NGC 2547 using the MPG/ESO 2.2m telescope with WFI, achieving better than 1% photometric precision per data point over 14 <~ I <~ 18. Candidate cluster members were selected from a V vs V-I colour magnitude diagram over 12.5 < V < 24 (covering masses from 0.9 Msol down to below the brown dwarf limit), finding 800 candidates, of which we expect ~330 to be real cluster members, taking into account contamination from the field (which is most severe at the extremes of our mass range). Searching for periodic variations in these gave 176 detections over the mass range 0.1 <~ M/Msol <~ 0.9. The rotation period distributions were found to show a clear mass-dependent morphology, qualitatively intermediate between the distributions obtained from similar surveys in NGC 2362 and NGC 2516, as would be expected from the age of this cluster. Models of the rotational evolution were investigated, finding that the evolution from NGC 2362 to NGC 2547 was qualitatively reproduced (given the uncertainty in the age of NGC 2547) by solid body and core-envelope decoupled models from our earlier NGC 2516 study without need for significant modification.
astro-ph
we report on the results of an iband timeseries photometric survey of ngc 2547 using the mpgeso 22m telescope with wfi achieving better than 1 photometric precision per data point over 14 i 18 candidate cluster members were selected from a v vs vi colour magnitude diagram over 125 v 24 covering masses from 09 msol down to below the brown dwarf limit finding 800 candidates of which we expect 330 to be real cluster members taking into account contamination from the field which is most severe at the extremes of our mass range searching for periodic variations in these gave 176 detections over the mass range 01 mmsol 09 the rotation period distributions were found to show a clear massdependent morphology qualitatively intermediate between the distributions obtained from similar surveys in ngc 2362 and ngc 2516 as would be expected from the age of this cluster models of the rotational evolution were investigated finding that the evolution from ngc 2362 to ngc 2547 was qualitatively reproduced given the uncertainty in the age of ngc 2547 by solid body and coreenvelope decoupled models from our earlier ngc 2516 study without need for significant modification
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711.033
Assessing statistical significance of periodogram peaks
The least-squares (or Lomb-Scargle) periodogram is a powerful tool which is used routinely in many branches of astronomy to search for periodicities in observational data. The problem of assessing statistical significance of candidate periodicities for different periodograms is considered. Based on results in extreme value theory, improved analytic estimations of false alarm probabilities are given. They include an upper limit to the false alarm probability (or a lower limit to the significance). These estimations are tested numerically in order to establish regions of their practical applicability.
astro-ph
the leastsquares or lombscargle periodogram is a powerful tool which is used routinely in many branches of astronomy to search for periodicities in observational data the problem of assessing statistical significance of candidate periodicities for different periodograms is considered based on results in extreme value theory improved analytic estimations of false alarm probabilities are given they include an upper limit to the false alarm probability or a lower limit to the significance these estimations are tested numerically in order to establish regions of their practical applicability
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711.0331
X-ray Observables of Magnetically Dominated Cavities in Clusters
We present results from magneto-hydrodynamic jet simulations in the magnetically dominated regime and find that they inflate cavities into the intracluster medium. Mock Chandra X-ray observations of our simulations show a strong resemblance to real cavities observed in X-ray images of clusters, both in terms of their morphology and thermodynamic structure. An analysis of the evolution of bubble sizes in the multi-cavity system Hydra A, as well as in a large sample of 64 cavities in 32 clusters shows that bubbles tend to expand much faster than expected in the purely adiabatic regime. Instead, we find that the bubbles follow more closely a trend predicted by our current-carrying jet models.
astro-ph
we present results from magnetohydrodynamic jet simulations in the magnetically dominated regime and find that they inflate cavities into the intracluster medium mock chandra xray observations of our simulations show a strong resemblance to real cavities observed in xray images of clusters both in terms of their morphology and thermodynamic structure an analysis of the evolution of bubble sizes in the multicavity system hydra a as well as in a large sample of 64 cavities in 32 clusters shows that bubbles tend to expand much faster than expected in the purely adiabatic regime instead we find that the bubbles follow more closely a trend predicted by our currentcarrying jet models
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711.0332
Summary of session A4 at the GRG18 conference: Alternative Theories of Gravity
More than 50 abstracts were submitted to the A4 session on "Alternatives Theories of Gravity" at the GRG18 conference. About 30 of them were scheduled as oral presentations, that we summarize below. We do not intend to give a critical review, but rather pointers to the corresponding papers. The main topics were (i) brane models both from the mathematical and the phenomenological viewpoints; (ii) Einstein-Gauss-Bonnet gravity in higher dimensions or coupled to a scalar field; (iii) modified Newtonian dynamics (MOND); (iv) scalar-tensor and f(R) theories; (v) alternative models involving Lorentz violations, noncommutative spacetimes or Chern-Simons corrections.
gr-qc
more than 50 abstracts were submitted to the a4 session on alternatives theories of gravity at the grg18 conference about 30 of them were scheduled as oral presentations that we summarize below we do not intend to give a critical review but rather pointers to the corresponding papers the main topics were i brane models both from the mathematical and the phenomenological viewpoints ii einsteingaussbonnet gravity in higher dimensions or coupled to a scalar field iii modified newtonian dynamics mond iv scalartensor and fr theories v alternative models involving lorentz violations noncommutative spacetimes or chernsimons corrections
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711.0333
Magnetic resonance as an orbital state probe
Magnetic resonance in ordered state is shown to be the direct method for distinguishing the orbital ground state. The example of perovskite titanates, particularly, LaTiO3 and YTiO3, is considered. External magnetic field resonance spectra of these crystals reveal glaring qualitative dependence on assumed orbital state of the compounds: orbital liquid or static orbital structure. Theoretical basis for using the method as an orbital state probe is grounded.
cond-mat.str-el
magnetic resonance in ordered state is shown to be the direct method for distinguishing the orbital ground state the example of perovskite titanates particularly latio3 and ytio3 is considered external magnetic field resonance spectra of these crystals reveal glaring qualitative dependence on assumed orbital state of the compounds orbital liquid or static orbital structure theoretical basis for using the method as an orbital state probe is grounded
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711.0334
Ueber Eigenwerte, Integrale und pi^2/6: Die Idee der Spurformel (On eigenvalues, integrals and pi^2/6: The idea of the trace formula)
This is an expository article that results from a talk given to second year students at Oldenburg university. The aim of the talk was to show what beautiful and unexpected results may be obtained if one plays with daring analogies in a way that is usually not done in undergraduate education (unfortunately): We start from the fact that the sum of diagonal entries of a symmetric matrix equals the sum of its eigenvalues. We then guess an analogous formula where the matrix is replaced by a function of two real variables and sums are replaced by integrals in a systematic way. We show that this is indeed a worthwhile process: In a special case it yields that the sum of inverse squares of the positive integers is pi^2/6. Finally, an outline of the proof of the guessed formula is given, and further applications, for example to the connection between billiards and the frequencies of a drum, are explained.
math.HO math.GM math.SP
this is an expository article that results from a talk given to second year students at oldenburg university the aim of the talk was to show what beautiful and unexpected results may be obtained if one plays with daring analogies in a way that is usually not done in undergraduate education unfortunately we start from the fact that the sum of diagonal entries of a symmetric matrix equals the sum of its eigenvalues we then guess an analogous formula where the matrix is replaced by a function of two real variables and sums are replaced by integrals in a systematic way we show that this is indeed a worthwhile process in a special case it yields that the sum of inverse squares of the positive integers is pi26 finally an outline of the proof of the guessed formula is given and further applications for example to the connection between billiards and the frequencies of a drum are explained
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711.0335
On the enhanced cosmic-ray ionization rate in the diffuse cloud towards Zeta Persei
The spatial distribution of the cosmic-ray flux is important in understanding the Interstellar Medium (ISM) of the Galaxy. This distribution can be analyzed by studying different molecular species along different sight lines whose abundances are sensitive to the cosmic-ray ionization rate. Recently several groups have reported an enhanced cosmic-ray ionization rate in diffuse clouds compared to the standard value, zeta(average)=2.5e-17 s^-1, measured toward dense molecular clouds. In an earlier work we reported an enhancement in the cosmic ray rate of 20 towards HD185418. McCall et al. have reported enhancements of 48 towards zeta Persei based on the observed abundance of H$_{3}^+ while Le Petit et al. found a cosmic ray enhancement of ~10 to be consistent with their models for this same sight line. Here we revisit zeta Persei and perform a detailed calculation using a self-consistent treatment of the hydrogen chemistry, grain physics, energy and ionization balance, and excitation physics. We show that the value of zeta deduced from the H$_{3}^+$ column density in the diffuse region of the sightline depends strongly on the properties of the grains because they remove free electrons and change the hydrogen chemistry. The observations are largely consistent with a cosmic ray enhancement of 40, with several diagnostics indicating higher values. This underscores the importance of a full treatment of grain physics in studies of interstellar chemistry.
astro-ph
the spatial distribution of the cosmicray flux is important in understanding the interstellar medium ism of the galaxy this distribution can be analyzed by studying different molecular species along different sight lines whose abundances are sensitive to the cosmicray ionization rate recently several groups have reported an enhanced cosmicray ionization rate in diffuse clouds compared to the standard value zetaaverage25e17 s1 measured toward dense molecular clouds in an earlier work we reported an enhancement in the cosmic ray rate of 20 towards hd185418 mccall et al have reported enhancements of 48 towards zeta persei based on the observed abundance of h_3 while le petit et al found a cosmic ray enhancement of 10 to be consistent with their models for this same sight line here we revisit zeta persei and perform a detailed calculation using a selfconsistent treatment of the hydrogen chemistry grain physics energy and ionization balance and excitation physics we show that the value of zeta deduced from the h_3 column density in the diffuse region of the sightline depends strongly on the properties of the grains because they remove free electrons and change the hydrogen chemistry the observations are largely consistent with a cosmic ray enhancement of 40 with several diagnostics indicating higher values this underscores the importance of a full treatment of grain physics in studies of interstellar chemistry
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711.0336
QCD Thermodynamics
Recent results on QCD thermodynamics are presented. The nature of the T>0 transition is determined, which turns out to be an analytic cross-over. The absolute scale for this transition is calculated. The temperature dependent static potential is given. The results were obtained by using a Symanzik improved gauge and stout-link improved fermionic action. In order to approach the continuum limit four different sets of lattice spacings were used with temporal extensions N_t=4, 6, 8 and 10 (they correspond to lattice spacings a \sim 0.3, 0.2, 0.15 and 0.12 fm). A new technique is presented, which --in contrast to earlier methods-- enables one to determine the equation of state at very large temperatures.
hep-lat
recent results on qcd thermodynamics are presented the nature of the t0 transition is determined which turns out to be an analytic crossover the absolute scale for this transition is calculated the temperature dependent static potential is given the results were obtained by using a symanzik improved gauge and stoutlink improved fermionic action in order to approach the continuum limit four different sets of lattice spacings were used with temporal extensions n_t4 6 8 and 10 they correspond to lattice spacings a sim 03 02 015 and 012 fm a new technique is presented which in contrast to earlier methods enables one to determine the equation of state at very large temperatures
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711.0337
Linear Stark Shifts to Measure the Fr Weak Nuclear Charge with Small Atom Samples
We study the chirality of ground-state alkali atoms in E and B fields, dressed with a circularly-polarized laser beam close-detuned from an E-field-assisted forbidden transition, such as 7S-8S in Fr. We predict a parity violating energy shift of their sublevels, linear in E, and the weak nuclear charge Q_W$. A dressing beam of 10 kW/cm$^2$ at 506 nm produces a shift of $\sim100 \mu$Hz at E=100 V/cm, B $\gtrsim$30 mG. It should be observable with $\sim 10^4$ Fr atoms confined in an optical dipole trap. We discuss optimal conditions, parameter reversals and a calibration procedure to measure $Q_W$.
physics.atom-ph hep-ph
we study the chirality of groundstate alkali atoms in e and b fields dressed with a circularlypolarized laser beam closedetuned from an efieldassisted forbidden transition such as 7s8s in fr we predict a parity violating energy shift of their sublevels linear in e and the weak nuclear charge q_w a dressing beam of 10 kwcm2 at 506 nm produces a shift of sim100 muhz at e100 vcm b gtrsim30 mg it should be observable with sim 104 fr atoms confined in an optical dipole trap we discuss optimal conditions parameter reversals and a calibration procedure to measure q_w
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711.0338
Structure constants of the OSP(1|2) WZNW model
We propose exact formulas for the 2- and 3-point functions of the WZNW model on the non-compact supergroup OSP(1|2). Using the path integral approach that was recently developed in arXiv:0706.1030 we show how local correlation functions in the OSP(p|2) WZNW models can be obtained from those of N=p supersymmetric Liouville field theory for p=1,2. We then employ known results on correlators in N=1 Liouville theory to determine the structure constants of the OSP(1|2) theory.
hep-th
we propose exact formulas for the 2 and 3point functions of the wznw model on the noncompact supergroup osp12 using the path integral approach that was recently developed in arxiv07061030 we show how local correlation functions in the ospp2 wznw models can be obtained from those of np supersymmetric liouville field theory for p12 we then employ known results on correlators in n1 liouville theory to determine the structure constants of the osp12 theory
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711.0339
Twisted Gromov-Witten r-spin potential and Givental's quantization
The universal curve p:C->\Mbar over the moduli space \Mbar of stable r-spin maps to a target K\"ahler manifold X carries a universal spinor bundle L->C. Therefore the moduli space \Mbar itself carries a natural K-theory class Rp_*L. We introduce a twisted r-spin Gromov-Witten potential of X enriched with Chern characters of Rp_*L. We show that the twisted potential can be reconstructed from the ordinary r-spin Gromov-Witten potential of X via an operator that assumes a particularly simple form in Givental's quantization formalism.
math.AG
the universal curve pcmbar over the moduli space mbar of stable rspin maps to a target kahler manifold x carries a universal spinor bundle lc therefore the moduli space mbar itself carries a natural ktheory class rp_l we introduce a twisted rspin gromovwitten potential of x enriched with chern characters of rp_l we show that the twisted potential can be reconstructed from the ordinary rspin gromovwitten potential of x via an operator that assumes a particularly simple form in giventals quantization formalism
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711.034
Origin of ferromagnetic response in diluted magnetic semiconductors and oxides
This paper reviews the present understanding of the origin of ferromagnetic response of diluted magnetic semiconductors and diluted magnetic oxides as well as in some nominally magnetically undoped materials. It is argued that these systems can be grouped into four classes. To the first belong composite materials in which precipitations of a known ferromagnetic, ferrimagnetic or antiferromagnetic compound account for magnetic characteristics at high temperatures. The second class forms alloys showing chemical nano-scale phase separation into the regions with small and large concentrations of the magnetic constituent. To the third class belong (Ga,Mn)As, heavily doped p-(Zn,Mn)Te, and related semiconductors. In these solid solutions the theory built on p-d Zener's model of hole-mediated ferromagnetism and on either the Kohn-Luttinger kp theory or the multi-orbital tight-binding approach describes qualitatively, and often quantitatively many relevant properties. Finally, in a number of carrier-doped DMS and DMO a competition between long-range ferromagnetic and short-range antiferromagnetic interactions and/or the proximity of the localisation boundary lead to an electronic nano-scale phase separation.
cond-mat.mtrl-sci cond-mat.str-el
this paper reviews the present understanding of the origin of ferromagnetic response of diluted magnetic semiconductors and diluted magnetic oxides as well as in some nominally magnetically undoped materials it is argued that these systems can be grouped into four classes to the first belong composite materials in which precipitations of a known ferromagnetic ferrimagnetic or antiferromagnetic compound account for magnetic characteristics at high temperatures the second class forms alloys showing chemical nanoscale phase separation into the regions with small and large concentrations of the magnetic constituent to the third class belong gamnas heavily doped pznmnte and related semiconductors in these solid solutions the theory built on pd zeners model of holemediated ferromagnetism and on either the kohnluttinger kp theory or the multiorbital tightbinding approach describes qualitatively and often quantitatively many relevant properties finally in a number of carrierdoped dms and dmo a competition between longrange ferromagnetic and shortrange antiferromagnetic interactions andor the proximity of the localisation boundary lead to an electronic nanoscale phase separation
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711.0341
ASPID-SR: Prototype of a VO-compliant Science-Ready Data Archive
ASPID stands for the "Archive of Spectral, Photometric, and Interferometric Data". The world largest collection of raw 3D spectroscopic observations of galactic and extragalactic sources is provided. ASPID-SR is a prototype of an archive of heterogeneous science ready data, fed by ASPID, where we try to exploit all the power of the IVOA Characterisation Data Model. Multi-level Characterisation metadata is provided for every dataset. The archive provides powerful metadata query mechanism with access to every data model element, vital for the efficient scientific usage of a complex informational system. We provide a set of access interfaces: SIAP/SSAP, HTTP-based characterisation metadata query, Web-service accepting ADQL/x.
astro-ph
aspid stands for the archive of spectral photometric and interferometric data the world largest collection of raw 3d spectroscopic observations of galactic and extragalactic sources is provided aspidsr is a prototype of an archive of heterogeneous science ready data fed by aspid where we try to exploit all the power of the ivoa characterisation data model multilevel characterisation metadata is provided for every dataset the archive provides powerful metadata query mechanism with access to every data model element vital for the efficient scientific usage of a complex informational system we provide a set of access interfaces siapssap httpbased characterisation metadata query webservice accepting adqlx
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711.0342
Comprehensive Metadata Query Interface for Heterogeneous Data Archives Based on Open Source PostgreSQL ORDBMS
We use PostgreSQL DBMS for storing XML metadata, described by the IVOA Characterisation Data Model. Initial XML type support in the PostgreSQL has recently been implemented. We make heavy use of this feature in order to provide comprehensive search over Characterisation metadata tree. We built a prototype of the Characterisation metadata query service, implementing two access methods: (1) HTTP-GET/POST based interface implements almost direct translation of the query parameter name into XPath of the data model element in the XML serialisation; (2) Web-Service based interface to receive XQuery which is also directly translated into XPath. This service will be used in the ASPID-SR archive, containing science-ready data obtained with the Russian 6-m telescope.
astro-ph
we use postgresql dbms for storing xml metadata described by the ivoa characterisation data model initial xml type support in the postgresql has recently been implemented we make heavy use of this feature in order to provide comprehensive search over characterisation metadata tree we built a prototype of the characterisation metadata query service implementing two access methods 1 httpgetpost based interface implements almost direct translation of the query parameter name into xpath of the data model element in the xml serialisation 2 webservice based interface to receive xquery which is also directly translated into xpath this service will be used in the aspidsr archive containing scienceready data obtained with the russian 6m telescope
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711.0343
Origin and control of ferromagnetism in dilute magnetic semiconductors and oxides
The author reviews the present understanding of the hole-mediated ferromagnetism in magnetically doped semiconductors and oxides as well as the origin of high temperature ferromagnetism in materials containing no valence band holes. It is argued that in these systems spinodal decomposition into regions with a large and a small concentration of magnetic component takes place. This self-organized assembling of magnetic nanocrystals can be controlled by co-doping and growth conditions. Functionalities of these multicomponent systems are described together with prospects for their applications in spintronics, nanoelectronics, photonics, plasmonics, and thermoelectrics.
cond-mat.mtrl-sci
the author reviews the present understanding of the holemediated ferromagnetism in magnetically doped semiconductors and oxides as well as the origin of high temperature ferromagnetism in materials containing no valence band holes it is argued that in these systems spinodal decomposition into regions with a large and a small concentration of magnetic component takes place this selforganized assembling of magnetic nanocrystals can be controlled by codoping and growth conditions functionalities of these multicomponent systems are described together with prospects for their applications in spintronics nanoelectronics photonics plasmonics and thermoelectrics
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711.0344
Automatic Coding Rule Conformance Checking Using Logic Programs
Some approaches to increasing program reliability involve a disciplined use of programming languages so as to minimise the hazards introduced by error-prone features. This is realised by writing code that is constrained to a subset of the a priori admissible programs, and that, moreover, may use only a subset of the language. These subsets are determined by a collection of so-called coding rules.
cs.PL cs.SE
some approaches to increasing program reliability involve a disciplined use of programming languages so as to minimise the hazards introduced by errorprone features this is realised by writing code that is constrained to a subset of the a priori admissible programs and that moreover may use only a subset of the language these subsets are determined by a collection of socalled coding rules
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711.0345
A Prolog-based Environment for Reasoning about Programming Languages (Extended abstract)
ECLAIR is a Prolog-based prototype system aiming to provide a functionally complete environment for the study, development and evaluation of programming language analysis and implementation tools. In this paper, we sketch the overall structure of the system, outlining the main methodologies and technologies underlying its components. We also discuss the appropriateness of Prolog as the implementation language for the system: besides highlighting its strengths, we also point out a few potential weaknesses, hinting at possible solutions.
cs.PL cs.SE
eclair is a prologbased prototype system aiming to provide a functionally complete environment for the study development and evaluation of programming language analysis and implementation tools in this paper we sketch the overall structure of the system outlining the main methodologies and technologies underlying its components we also discuss the appropriateness of prolog as the implementation language for the system besides highlighting its strengths we also point out a few potential weaknesses hinting at possible solutions
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711.0346
Poincar\'e duality for $K$-theory of equivariant complex projective spaces
We make explicit Poincar\'{e} duality for the equivariant $K$-theory of equivariant complex projective spaces. The case of the trivial group provides a new approach to the $K$-theory orientation.
math.AT
we make explicit poincare duality for the equivariant ktheory of equivariant complex projective spaces the case of the trivial group provides a new approach to the ktheory orientation
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711.0347
A theoretical analysis of the resolution due to diffusion and size-dispersion of particles in deterministic lateral displacement devices
We present a model including diffusion and particle-size dispersion for separation of particles in deterministic lateral displacement devices also known as bumper arrays. We determine the upper critical diameter for diffusion-dominated motion and the lower critical diameter for pure convection-induced displacement. Our model explains the systematic deviation, observed for small particles in several experiments, from the critical diameter for separation given by simple laminar flow considerations.
physics.flu-dyn physics.comp-ph
we present a model including diffusion and particlesize dispersion for separation of particles in deterministic lateral displacement devices also known as bumper arrays we determine the upper critical diameter for diffusiondominated motion and the lower critical diameter for pure convectioninduced displacement our model explains the systematic deviation observed for small particles in several experiments from the critical diameter for separation given by simple laminar flow considerations
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711.0348
Compiling ER Specifications into Declarative Programs
This paper proposes an environment to support high-level database programming in a declarative programming language. In order to ensure safe database updates, all access and update operations related to the database are generated from high-level descriptions in the entity- relationship (ER) model. We propose a representation of ER diagrams in the declarative language Curry so that they can be constructed by various tools and then translated into this representation. Furthermore, we have implemented a compiler from this representation into a Curry program that provides access and update operations based on a high-level API for database programming.
cs.PL cs.SE
this paper proposes an environment to support highlevel database programming in a declarative programming language in order to ensure safe database updates all access and update operations related to the database are generated from highlevel descriptions in the entity relationship er model we propose a representation of er diagrams in the declarative language curry so that they can be constructed by various tools and then translated into this representation furthermore we have implemented a compiler from this representation into a curry program that provides access and update operations based on a highlevel api for database programming
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711.0349
Adaptive multiresolution for wavelet analysis
We present a new method of wavelet packet decomposition to be used in gravitational wave detection. An issue in wavelet analysis is what is the time-frequency resolution which is best suited to analyze data when in quest of a signal of unknown shape, like a burst. In the other wavelet methods currently employed, like LIGO WaveBurst, the analysis is performed at some trial resolutions. We propose a decomposition which automatically selects at any frequency the best resolution. The criterion for resolution selection is based on minimization of a function of the data, named entropy in analogy with the information theory. As a qualitative application we show how a multiresolution time-frequency scalogram looks in the case of a sample signal injected over Gaussian noise. For a more quantitative application of the method we tested its efficiency as a non-linear filter of simulated data for burst searches, finding that it is able to lower the false alarm rate of the WaveBurst algorithm with negligible effects on the efficiency.
gr-qc
we present a new method of wavelet packet decomposition to be used in gravitational wave detection an issue in wavelet analysis is what is the timefrequency resolution which is best suited to analyze data when in quest of a signal of unknown shape like a burst in the other wavelet methods currently employed like ligo waveburst the analysis is performed at some trial resolutions we propose a decomposition which automatically selects at any frequency the best resolution the criterion for resolution selection is based on minimization of a function of the data named entropy in analogy with the information theory as a qualitative application we show how a multiresolution timefrequency scalogram looks in the case of a sample signal injected over gaussian noise for a more quantitative application of the method we tested its efficiency as a nonlinear filter of simulated data for burst searches finding that it is able to lower the false alarm rate of the waveburst algorithm with negligible effects on the efficiency
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711.035
Intermittent estimation of stationary time series
Let $\{X_n\}_{n=0}^{\infty}$ be a stationary real-valued time series with unknown distribution. Our goal is to estimate the conditional expectation of $X_{n+1}$ based on the observations $X_i$, $0\le i\le n$ in a strongly consistent way. Bailey and Ryabko proved that this is not possible even for ergodic binary time series if one estimates at all values of $n$. We propose a very simple algorithm which will make prediction infinitely often at carefully selected stopping times chosen by our rule. We show that under certain conditions our procedure is strongly (pointwise) consistent, and $L_2$ consistent without any condition. An upper bound on the growth of the stopping times is also presented in this paper.
math.PR cs.IT math.IT
let x_n_n0infty be a stationary realvalued time series with unknown distribution our goal is to estimate the conditional expectation of x_n1 based on the observations x_i 0le ile n in a strongly consistent way bailey and ryabko proved that this is not possible even for ergodic binary time series if one estimates at all values of n we propose a very simple algorithm which will make prediction infinitely often at carefully selected stopping times chosen by our rule we show that under certain conditions our procedure is strongly pointwise consistent and l_2 consistent without any condition an upper bound on the growth of the stopping times is also presented in this paper
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711.0351
Noise threshold for universality of 2-input gates
Evans and Pippenger showed in 1998 that noisy gates with 2 inputs are universal for arbitrary computation (i.e. can compute any function with bounded error), if all gates fail independently with probability epsilon and epsilon<theta, where theta is roughly 8.856%. We show that formulas built from gates with 2 inputs, in which each gate fails with probability at least theta cannot be universal. Hence, there is a threshold on the tolerable noise for formulas with 2-input gates and it is theta. We conjecture that the same threshold also holds for circuits.
cs.IT cs.CC math.IT
evans and pippenger showed in 1998 that noisy gates with 2 inputs are universal for arbitrary computation ie can compute any function with bounded error if all gates fail independently with probability epsilon and epsilontheta where theta is roughly 8856 we show that formulas built from gates with 2 inputs in which each gate fails with probability at least theta cannot be universal hence there is a threshold on the tolerable noise for formulas with 2input gates and it is theta we conjecture that the same threshold also holds for circuits
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711.0352
The Twisted Higher Harmonic Signature for Foliations
We prove that the higher harmonic signature of an even dimensional oriented Riemannian foliation of a compact Riemannian manifold with coefficients in a leafwise U(p,q)-flat complex bundle is a leafwise homotopy invariant. We also prove the leafwise homotopy invariance of the twisted higher Betti classes. Consequences for the Novikov conjecture for foliations and for groups are investigated. Replaces The Higher Harmonic Signature for Foliations I: The Untwisted Case, and contains significant improvements.
math.KT math.DG
we prove that the higher harmonic signature of an even dimensional oriented riemannian foliation of a compact riemannian manifold with coefficients in a leafwise upqflat complex bundle is a leafwise homotopy invariant we also prove the leafwise homotopy invariance of the twisted higher betti classes consequences for the novikov conjecture for foliations and for groups are investigated replaces the higher harmonic signature for foliations i the untwisted case and contains significant improvements
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711.0353
The IceCube Collaboration: contributions to the 30th International Cosmic Ray Conference (ICRC 2007)
This paper bundles 40 contributions by the IceCube collaboration that were submitted to the 30th International Cosmic Ray Conference ICRC 2007. The articles cover studies on cosmic rays and atmospheric neutrinos, searches for non-localized, extraterrestrial electron, muon and tau neutrino signals, scans for steady and intermittent neutrino point sources, searches for dark matter candidates, magnetic monopoles and other exotic particles, improvements in analysis techniques, as well as future detector extensions. The IceCube observatory will be finalized in 2011 to form a cubic-kilometer ice-Cherenkov detector at the location of the geographic South Pole. At the present state of construction, IceCube consists of 52 paired IceTop surface tanks and 22 IceCube strings with a total of 1426 Digital Optical Modules deployed at depths up to 2350 m. The observatory also integrates the 19 string AMANDA subdetector, that was completed in 2000 and extends IceCube's reach to lower energies. Before the deployment of IceTop, cosmic air showers were registered with the 30 station SPASE-2 surface array. IceCube's low noise Digital Optical Modules are very reliable, show a uniform response and record waveforms of arriving photons that are resolvable with nanosecond precision over a large dynamic range. Data acquisition, reconstruction and simulation software are running in production mode and the analyses, profiting from the improved data quality and increased overall sensitivity, are well under way.
astro-ph
this paper bundles 40 contributions by the icecube collaboration that were submitted to the 30th international cosmic ray conference icrc 2007 the articles cover studies on cosmic rays and atmospheric neutrinos searches for nonlocalized extraterrestrial electron muon and tau neutrino signals scans for steady and intermittent neutrino point sources searches for dark matter candidates magnetic monopoles and other exotic particles improvements in analysis techniques as well as future detector extensions the icecube observatory will be finalized in 2011 to form a cubickilometer icecherenkov detector at the location of the geographic south pole at the present state of construction icecube consists of 52 paired icetop surface tanks and 22 icecube strings with a total of 1426 digital optical modules deployed at depths up to 2350 m the observatory also integrates the 19 string amanda subdetector that was completed in 2000 and extends icecubes reach to lower energies before the deployment of icetop cosmic air showers were registered with the 30 station spase2 surface array icecubes low noise digital optical modules are very reliable show a uniform response and record waveforms of arriving photons that are resolvable with nanosecond precision over a large dynamic range data acquisition reconstruction and simulation software are running in production mode and the analyses profiting from the improved data quality and increased overall sensitivity are well under way
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711.0354
Investigations of the NS-alpha model using a lid-driven cavity flow
In this paper we investigate a subgrid model based on an anisotropic version of the NS-$\alpha$ model using a lid-driven cavity flow at a Reynolds number of 10,000. Previously the NS-$\alpha$ model has only been used numerically in the isotropic form. The subgrid model is developed from the Eulerian-averaged anisotropic equations [Holm, \textit{Physica D}, v.133, pp 215-269, 1999]. It was found that when $\alpha^{2}$ was based on the mesh numerical oscillations developed which manifested themselves in the appearance of streamwise vortices and a `mixing out' of the velocity profile. This is analogous to the Craik-Leibovich mechanism, with the difference being that the oscillations here are not physical but numerical. The problem could be traced back to the discontinuity in $\alpha^{2}$ encountered when $\alpha^{2}=0$ on the endwalls. An alternative definition of $\alpha^{2}$ based on velocity gradients, rather than mesh spacing, is proposed and tested. Using this definition the results with the model shown a significant improvement. The splitting of the downstream wall jet, rms and shear stress profiles are correctly captured a coarse mesh. The model is shown to predict both positive and negative energy transfer in the jet impingement region, in qualitative agreement with DNS results.
physics.flu-dyn
in this paper we investigate a subgrid model based on an anisotropic version of the nsalpha model using a liddriven cavity flow at a reynolds number of 10000 previously the nsalpha model has only been used numerically in the isotropic form the subgrid model is developed from the eulerianaveraged anisotropic equations holm textitphysica d v133 pp 215269 1999 it was found that when alpha2 was based on the mesh numerical oscillations developed which manifested themselves in the appearance of streamwise vortices and a mixing out of the velocity profile this is analogous to the craikleibovich mechanism with the difference being that the oscillations here are not physical but numerical the problem could be traced back to the discontinuity in alpha2 encountered when alpha20 on the endwalls an alternative definition of alpha2 based on velocity gradients rather than mesh spacing is proposed and tested using this definition the results with the model shown a significant improvement the splitting of the downstream wall jet rms and shear stress profiles are correctly captured a coarse mesh the model is shown to predict both positive and negative energy transfer in the jet impingement region in qualitative agreement with dns results
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711.0355
Energies of ions in water and nanopores within Density Functional Theory
Accurate calculations of electrostatic potentials and treatment of substrate polarizability are critical for predicting the permeation of ions inside water-filled nanopores. The {\it ab initio} molecular dynamics method (AIMD), based on Density Functional Theory (DFT), accounts for the polarizability of materials, water, and solutes, and it should be the method of choice for predicting accurate electrostatic energies of ions. In practice, DFT coupled with the use of periodic boundary conditions in a charged system leads to large energy shifts. Results obtained using different DFT packages may vary because of the way pseudopotentials and long-range electrostatics are implemented. Using maximally localized Wannier functions, we apply robust corrections that yield relatively unambiguous ion energies in select molecular and aqueous systems and inside carbon nanotubes. Large binding energies are predicted for ions in metallic carbon nanotube arrays, while with consistent definitions Na$^+$ and Cl$^-$ energies are found to exhibit asymmetries comparable with those computed using non-polarizable water force fields.
cond-mat.mtrl-sci
accurate calculations of electrostatic potentials and treatment of substrate polarizability are critical for predicting the permeation of ions inside waterfilled nanopores the it ab initio molecular dynamics method aimd based on density functional theory dft accounts for the polarizability of materials water and solutes and it should be the method of choice for predicting accurate electrostatic energies of ions in practice dft coupled with the use of periodic boundary conditions in a charged system leads to large energy shifts results obtained using different dft packages may vary because of the way pseudopotentials and longrange electrostatics are implemented using maximally localized wannier functions we apply robust corrections that yield relatively unambiguous ion energies in select molecular and aqueous systems and inside carbon nanotubes large binding energies are predicted for ions in metallic carbon nanotube arrays while with consistent definitions na and cl energies are found to exhibit asymmetries comparable with those computed using nonpolarizable water force fields
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711.0356
Data Transmission in the Fourth Dimension
Alice wants to send an arbitrary binary word to Bob. We show here that there is no problem for her to do that with only two bits. Of course, we consider here information like a signal in 4D.
physics.gen-ph
alice wants to send an arbitrary binary word to bob we show here that there is no problem for her to do that with only two bits of course we consider here information like a signal in 4d
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711.0357
Observations of Transient Active Region Heating with Hinode
We present observations of transient active region heating events observed with the Extreme Ultraviolet Imaging Spectrometer (EIS) and X-ray Telescope (XRT) on Hinode. This initial investigation focuses on NOAA active region 10940 as observed by Hinode on February 1, 2007 between 12 and 19 UT. In these observations we find numerous examples of transient heating events within the active region. The high spatial resolution and broad temperature coverage of these instruments allows us to track the evolution of coronal plasma. The evolution of the emission observed with XRT and EIS during these events is generally consistent with loops that have been heated and are cooling. We have analyzed the most energetic heating event observed during this period, a small GOES B-class flare, in some detail and present some of the spectral signatures of the event, such as relative Doppler shifts at one of the loop footpoints and enhanced line widths during the rise phase of the event. While the analysis of these transient events has the potential to yield insights into the coronal heating mechanism, these observations do not rule out the possibility that there is a strong steady heating level in the active region. Detailed statistical analysis will be required to address this question definitively.
astro-ph
we present observations of transient active region heating events observed with the extreme ultraviolet imaging spectrometer eis and xray telescope xrt on hinode this initial investigation focuses on noaa active region 10940 as observed by hinode on february 1 2007 between 12 and 19 ut in these observations we find numerous examples of transient heating events within the active region the high spatial resolution and broad temperature coverage of these instruments allows us to track the evolution of coronal plasma the evolution of the emission observed with xrt and eis during these events is generally consistent with loops that have been heated and are cooling we have analyzed the most energetic heating event observed during this period a small goes bclass flare in some detail and present some of the spectral signatures of the event such as relative doppler shifts at one of the loop footpoints and enhanced line widths during the rise phase of the event while the analysis of these transient events has the potential to yield insights into the coronal heating mechanism these observations do not rule out the possibility that there is a strong steady heating level in the active region detailed statistical analysis will be required to address this question definitively
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711.0358
Critical values of moment maps on quantizable manifolds
Let $M$ be a quantizable symplectic manifold acted on by $T=(S^1)^r$ in a Hamiltonian fashion and $J$ a moment map for this action. Suppose that the set $M^{T}$ of fixed points is discrete and denote by ${\alpha}_{pj}\in{\mathbb Z}^r$ the weights of the isotropy representation at $p$. By means of the $\alpha_{pj}$'s we define a partition ${\mathcal Q}_+$, ${\mathcal Q}_-$ of $M^T$. (When $r=1$, ${\mathcal Q}_{\pm}$ will be the set of fixed points such that the half of the Morse index of $J$ at them is even (odd)). We prove the existence of a map $\pi_{\pm}:{\mathcal Q}_{\pm}\to{\mathcal Q}_{\mp}$ such that $J(q)-J(\pi_{\pm}(q))\in I_{\mp}$, for all $q\in {\mathcal Q}_{\pm}$, where $I_{\pm}$ is the lattice generated by the $\alpha_{pj}$'s with $p\in{\mathcal Q}_{\pm}.$ We define partition functions $N_p$ similar to the ones of Kostant \cite{Gui} and we prove that $\sum_{p\in{\mathcal Q}_+}N_p(l)=\sum_{p\in{\mathcal Q}_-}N_p(l)$, for any $l\in{\mathbb Z}^r$ with $|l|$ sufficiently large.
math.SG
let m be a quantizable symplectic manifold acted on by ts1r in a hamiltonian fashion and j a moment map for this action suppose that the set mt of fixed points is discrete and denote by alpha_pjinmathbb zr the weights of the isotropy representation at p by means of the alpha_pjs we define a partition mathcal q_ mathcal q_ of mt when r1 mathcal q_pm will be the set of fixed points such that the half of the morse index of j at them is even odd we prove the existence of a map pi_pmmathcal q_pmtomathcal q_mp such that jqjpi_pmqin i_mp for all qin mathcal q_pm where i_pm is the lattice generated by the alpha_pjs with pinmathcal q_pm we define partition functions n_p similar to the ones of kostant citegui and we prove that sum_pinmathcal q_n_plsum_pinmathcal q_n_pl for any linmathbb zr with l sufficiently large
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711.0359
Dark energy FRW cosmology - dynamical system reconstruction
We develop a simple method of dark energy reconstruction using a geometrical form of the luminosity-distance relation. In this method the FRW dynamical system with dark energy is reconstructed instead of the equation of state parameter. We give several examples which illustrate the usefulness of our method in fitting the redshift transition from the decelerating to accelerating phase as the value of the Hubble function at the transition.
astro-ph
we develop a simple method of dark energy reconstruction using a geometrical form of the luminositydistance relation in this method the frw dynamical system with dark energy is reconstructed instead of the equation of state parameter we give several examples which illustrate the usefulness of our method in fitting the redshift transition from the decelerating to accelerating phase as the value of the hubble function at the transition
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711.036
Detecting Order and Chaos by the Linear Dependence Index (LDI) Method
We introduce a new methodology for a fast and reliable discrimination between ordered and chaotic orbits in multidimensional Hamiltonian systems which we call the Linear Dependence Index (LDI). The new method is based on the recently introduced theory of the Generalized Alignment Indices (GALI). LDI takes advantage of the linear dependence (or independence) of deviation vectors of a given orbit, using the method of Singular Value Decomposition at every time step of the integration. We show that the LDI produces estimates which numerically coincide with those of the GALI method for the same number of $m$ deviation vectors, while its main advantage is that it requires considerable less CPU time than GALI especially in Hamiltonian systems of many degrees of freedom
nlin.CD
we introduce a new methodology for a fast and reliable discrimination between ordered and chaotic orbits in multidimensional hamiltonian systems which we call the linear dependence index ldi the new method is based on the recently introduced theory of the generalized alignment indices gali ldi takes advantage of the linear dependence or independence of deviation vectors of a given orbit using the method of singular value decomposition at every time step of the integration we show that the ldi produces estimates which numerically coincide with those of the gali method for the same number of m deviation vectors while its main advantage is that it requires considerable less cpu time than gali especially in hamiltonian systems of many degrees of freedom
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711.0361
On the integration of Poisson homogeneous spaces
We study a reduction procedure for describing the symplectic groupoid of a Poisson homogeneous space obtained by quotient of a coisotropic subgroup. We perform it as a reduction of the Lu-Weinstein symplectic groupoid integrating Poisson Lie groups, that is suitable even for the non complete case.
math.SG
we study a reduction procedure for describing the symplectic groupoid of a poisson homogeneous space obtained by quotient of a coisotropic subgroup we perform it as a reduction of the luweinstein symplectic groupoid integrating poisson lie groups that is suitable even for the non complete case
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711.0362
On the Asymptotic Solution for the Fourier-Bessel Multiple Scattering Coefficients of an Infinite Grating of Insulating Dielectric Circular Cylinders at Oblique Incidence
In this article, we present the asymptotic solution for the matrix system of equations representing the multiple scattering coefficients of an infinite grating of insulating dielectric circular cylinders associated with vertically polarized obliquely incident plane electromagnetic waves.
math-ph math.MP
in this article we present the asymptotic solution for the matrix system of equations representing the multiple scattering coefficients of an infinite grating of insulating dielectric circular cylinders associated with vertically polarized obliquely incident plane electromagnetic waves
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711.0363
Dyson-Schwinger Equation and Quantum Phase Transitions in Massless QCD
We study the stability of the highest symmetric solution (Wigner-solution) of Dyson-Schwinger equations in chiral limit and at zero temperature. Our results confirm that if the chemical potential is not very large, the QCD vacuum is in the chiral symmetry breaking phase and the quantum phase-transition of the chiral symmetry restoration is in first order. Meanwhile it seems that there is not competition between chiral symmetry breaking phase and color superconductivity phase since the color superconductivity phase appears only if the chemical potential is very large. Moreover, we propose that chiral symmetry breaking arises from the positive feedback with respect to the mass perturbation.
hep-ph
we study the stability of the highest symmetric solution wignersolution of dysonschwinger equations in chiral limit and at zero temperature our results confirm that if the chemical potential is not very large the qcd vacuum is in the chiral symmetry breaking phase and the quantum phasetransition of the chiral symmetry restoration is in first order meanwhile it seems that there is not competition between chiral symmetry breaking phase and color superconductivity phase since the color superconductivity phase appears only if the chemical potential is very large moreover we propose that chiral symmetry breaking arises from the positive feedback with respect to the mass perturbation
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711.0364
Discriminating spin through quantum interference
Many of the proposed solutions to the hierarchy and naturalness problems postulate new `partner' fields to the standard model particles. Determining the spins of these new particles will be critical in distinguishing among the various possible SM extensions, yet proposed methods rely on the underlying models. We propose a new model-independent method for spin measurements which takes advantage of quantum interference among helicity states. We demonstrate that this method will be able to discriminate scalar particles from higher spin states at the ILC, and discuss application to higher spins and possible uses at the LHC.
hep-ph
many of the proposed solutions to the hierarchy and naturalness problems postulate new partner fields to the standard model particles determining the spins of these new particles will be critical in distinguishing among the various possible sm extensions yet proposed methods rely on the underlying models we propose a new modelindependent method for spin measurements which takes advantage of quantum interference among helicity states we demonstrate that this method will be able to discriminate scalar particles from higher spin states at the ilc and discuss application to higher spins and possible uses at the lhc
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711.0365
Properties of tunnel Josephson junctions with a ferromagnetic interlayer
We investigate superconductor/insulator/ferromagnet/superconductor (SIFS) tunnel Josephson junctions in the dirty limit, using the quasiclassical theory. We formulate a quantitative model describing the oscillations of critical current as a function of thickness of the ferromagnetic layer and use this model to fit recent experimental data. We also calculate quantitatively the density of states (DOS) in this type of junctions and compare DOS oscillations with those of the critical current.
cond-mat.supr-con
we investigate superconductorinsulatorferromagnetsuperconductor sifs tunnel josephson junctions in the dirty limit using the quasiclassical theory we formulate a quantitative model describing the oscillations of critical current as a function of thickness of the ferromagnetic layer and use this model to fit recent experimental data we also calculate quantitatively the density of states dos in this type of junctions and compare dos oscillations with those of the critical current
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711.0366
Shannon Theoretic Limits on Noisy Compressive Sampling
In this paper, we study the number of measurements required to recover a sparse signal in ${\mathbb C}^M$ with $L$ non-zero coefficients from compressed samples in the presence of noise. For a number of different recovery criteria, we prove that $O(L)$ (an asymptotically linear multiple of $L$) measurements are necessary and sufficient if $L$ grows linearly as a function of $M$. This improves on the existing literature that is mostly focused on variants of a specific recovery algorithm based on convex programming, for which $O(L\log(M-L))$ measurements are required. We also show that $O(L\log(M-L))$ measurements are required in the sublinear regime ($L = o(M)$).
cs.IT math.IT
in this paper we study the number of measurements required to recover a sparse signal in mathbb cm with l nonzero coefficients from compressed samples in the presence of noise for a number of different recovery criteria we prove that ol an asymptotically linear multiple of l measurements are necessary and sufficient if l grows linearly as a function of m this improves on the existing literature that is mostly focused on variants of a specific recovery algorithm based on convex programming for which ollogml measurements are required we also show that ollogml measurements are required in the sublinear regime l om
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711.0367
Nonparametric inference for ergodic, stationary time series
The setting is a stationary, ergodic time series. The challenge is to construct a sequence of functions, each based on only finite segments of the past, which together provide a strongly consistent estimator for the conditional probability of the next observation, given the infinite past. Ornstein gave such a construction for the case that the values are from a finite set, and recently Algoet extended the scheme to time series with coordinates in a Polish space. The present study relates a different solution to the challenge. The algorithm is simple and its verification is fairly transparent. Some extensions to regression, pattern recognition, and on-line forecasting are mentioned.
math.PR cs.IT math.IT
the setting is a stationary ergodic time series the challenge is to construct a sequence of functions each based on only finite segments of the past which together provide a strongly consistent estimator for the conditional probability of the next observation given the infinite past ornstein gave such a construction for the case that the values are from a finite set and recently algoet extended the scheme to time series with coordinates in a polish space the present study relates a different solution to the challenge the algorithm is simple and its verification is fairly transparent some extensions to regression pattern recognition and online forecasting are mentioned
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711.0368
Fast computation of Lyot-style coronagraph propagation
We present a new method for numerical propagation through Lyot-style coronagraphs using finite occulting masks. Standard methods for coronagraphic simulations involve Fast Fourier Transforms (FFT) of very large arrays, and computing power is an issue for the design and tolerancing of coronagraphs on segmented Extremely Large Telescopes (ELT) in order to handle both the speed and memory requirements. Our method combines a semi-analytical approach with non-FFT based Fourier transform algorithms. It enables both fast and memory-efficient computations without introducing any additional approximations. Typical speed improvements based on computation costs are of about ten to fifty for propagations from pupil to Lyot plane, with thirty to sixty times less memory needed. Our method makes it possible to perform numerical coronagraphic studies even in the case of ELTs using a contemporary commercial laptop computer, or any standard commercial workstation computer.
astro-ph
we present a new method for numerical propagation through lyotstyle coronagraphs using finite occulting masks standard methods for coronagraphic simulations involve fast fourier transforms fft of very large arrays and computing power is an issue for the design and tolerancing of coronagraphs on segmented extremely large telescopes elt in order to handle both the speed and memory requirements our method combines a semianalytical approach with nonfft based fourier transform algorithms it enables both fast and memoryefficient computations without introducing any additional approximations typical speed improvements based on computation costs are of about ten to fifty for propagations from pupil to lyot plane with thirty to sixty times less memory needed our method makes it possible to perform numerical coronagraphic studies even in the case of elts using a contemporary commercial laptop computer or any standard commercial workstation computer
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711.0369
Some considerations of finite dimensional spin glasses
In talk I will review the theoretical results that have been obtained for spin glasses, paying a particular attention to finite dimensional spin glasses. I will concentrate my attention on the formulation of the mean field approach and on its numerical and experimental verifications. I will mainly considered equilibrium properties at zero magnetic field, where the situation is clear and it should be not controversial. I will present the various hypothesis at the basis of the theory and I will discuss their physical status.
cond-mat.dis-nn
in talk i will review the theoretical results that have been obtained for spin glasses paying a particular attention to finite dimensional spin glasses i will concentrate my attention on the formulation of the mean field approach and on its numerical and experimental verifications i will mainly considered equilibrium properties at zero magnetic field where the situation is clear and it should be not controversial i will present the various hypothesis at the basis of the theory and i will discuss their physical status
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711.037
Model-independent determination of the cosmic expansion rate. I. Application to type-Ia supernovae
Aims: In view of the substantial uncertainties regarding the possible dynamics of the dark energy, we aim at constraining the expansion rate of the universe without reference to a specific Friedmann model and its parameters. Methods: We show that cosmological observables integrating over the cosmic expansion rate can be converted into a Volterra integral equation which is known to have a unique solution in terms of a Neumann series. Expanding observables such as the luminosity distances to type-Ia supernovae into a series of orthonormal functions, the integral equation can be solved and the cosmic expansion rate recovered within the limits allowed by the accuracy of the data. Results: We demonstrate the performance of the method applying it to synthetic data sets of increasing complexity, and to the first-year SNLS data. In particular, we show that the method is capable of reproducing a hypothetical expansion function containing a sudden transition.
astro-ph
aims in view of the substantial uncertainties regarding the possible dynamics of the dark energy we aim at constraining the expansion rate of the universe without reference to a specific friedmann model and its parameters methods we show that cosmological observables integrating over the cosmic expansion rate can be converted into a volterra integral equation which is known to have a unique solution in terms of a neumann series expanding observables such as the luminosity distances to typeia supernovae into a series of orthonormal functions the integral equation can be solved and the cosmic expansion rate recovered within the limits allowed by the accuracy of the data results we demonstrate the performance of the method applying it to synthetic data sets of increasing complexity and to the firstyear snls data in particular we show that the method is capable of reproducing a hypothetical expansion function containing a sudden transition
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711.0371
Noncommutative fields and actions of twisted Poincare algebra
Within the context of the twisted Poincar\'e algebra, there exists no noncommutative analogue of the Minkowski space interpreted as the homogeneous space of the Poincar\'e group quotiented by the Lorentz group. The usual definition of commutative classical fields as sections of associated vector bundles on the homogeneous space does not generalise to the noncommutative setting, and the twisted Poincar\'e algebra does not act on noncommutative fields in a canonical way. We make a tentative proposal for the definition of noncommutative classical fields of any spin over the Moyal space, which has the desired representation theoretical properties. We also suggest a way to search for noncommutative Minkowski spaces suitable for studying noncommutative field theory with deformed Poincar\'e symmetries.
hep-th math-ph math.MP
within the context of the twisted poincare algebra there exists no noncommutative analogue of the minkowski space interpreted as the homogeneous space of the poincare group quotiented by the lorentz group the usual definition of commutative classical fields as sections of associated vector bundles on the homogeneous space does not generalise to the noncommutative setting and the twisted poincare algebra does not act on noncommutative fields in a canonical way we make a tentative proposal for the definition of noncommutative classical fields of any spin over the moyal space which has the desired representation theoretical properties we also suggest a way to search for noncommutative minkowski spaces suitable for studying noncommutative field theory with deformed poincare symmetries
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711.0372
Mixing Least-Squares Estimators when the Variance is Unknown
We propose a procedure to handle the problem of Gaussian regression when the variance is unknown. We mix least-squares estimators from various models according to a procedure inspired by that of Leung and Barron (2007). We show that in some cases the resulting estimator is a simple shrinkage estimator. We then apply this procedure in various statistical settings such as linear regression or adaptive estimation in Besov spaces. Our results provide non-asymptotic risk bounds for the Euclidean risk of the estimator.
math.ST stat.TH
we propose a procedure to handle the problem of gaussian regression when the variance is unknown we mix leastsquares estimators from various models according to a procedure inspired by that of leung and barron 2007 we show that in some cases the resulting estimator is a simple shrinkage estimator we then apply this procedure in various statistical settings such as linear regression or adaptive estimation in besov spaces our results provide nonasymptotic risk bounds for the euclidean risk of the estimator
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711.0373
Automorphisms in Loop Quantum Gravity
We investigate a certain distributional extension of the group of spatial diffeomorphisms in Loop Quantum Gravity. This extension, which is given by the automorphisms Aut(P) of the path groupoid P, was proposed by Velhinho and is inspired by category theory. This group is much larger than the group of piecewise analytic diffeomorphisms. In particular, we will show that graphs with the same combinatorics but different generalized knotting classes can be mapped into each other. We describe the automorphism-invariant Hilbert space and comment on how a combinatorial formulation of LQG might arise.
gr-qc
we investigate a certain distributional extension of the group of spatial diffeomorphisms in loop quantum gravity this extension which is given by the automorphisms autp of the path groupoid p was proposed by velhinho and is inspired by category theory this group is much larger than the group of piecewise analytic diffeomorphisms in particular we will show that graphs with the same combinatorics but different generalized knotting classes can be mapped into each other we describe the automorphisminvariant hilbert space and comment on how a combinatorial formulation of lqg might arise
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711.0374
Directed motion generated by heat bath nonlinearly driven by external noise
Based on the system heat bath approach where the bath is nonlinearly modulated by an external Gaussian random force, we propose a new microscopic model to study directed motion in the overdamped limit for a nonequilibrium open system. Making use of the coupling between the heat bath and the external modulation as a small perturbation we construct a Langevin equation with multiplicative noise and space dependent dissipation and the corresponding Fokker-Planck-Smoluchowski equation in the overdamped limit. We examine the thermodynamic consistency condition and explore the possibility of observing a phase induced current as a consequence of state dependent diffusion and, necessarily, nonlinear driving of the heat bath by the external noise.
cond-mat.stat-mech cond-mat.soft
based on the system heat bath approach where the bath is nonlinearly modulated by an external gaussian random force we propose a new microscopic model to study directed motion in the overdamped limit for a nonequilibrium open system making use of the coupling between the heat bath and the external modulation as a small perturbation we construct a langevin equation with multiplicative noise and space dependent dissipation and the corresponding fokkerplancksmoluchowski equation in the overdamped limit we examine the thermodynamic consistency condition and explore the possibility of observing a phase induced current as a consequence of state dependent diffusion and necessarily nonlinear driving of the heat bath by the external noise
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711.0375
Dynamics of Vortex Formation in Merging Bose-Einstein Condensate Fragments
We study the formation of vortices in a Bose-Einstein condensate (BEC) that has been prepared by allowing isolated and independent condensed fragments to merge together. We focus on the experimental setup of Scherer {\it et al.} [Phys. Rev. Lett. {\bf 98}, 110402 (2007)], where three BECs are created in a magnetic trap that is segmented into three regions by a repulsive optical potential; the BECs merge together as the optical potential is removed. First, we study the two-dimensional case, in particular we examine the effects of the relative phases of the different fragments and the removal rate of the optical potential on the vortex formation. We find that many vortices are created by instant removal of the optical potential regardless of relative phases, and that fewer vortices are created if the intensity of the optical potential is gradually ramped down and the condensed fragments gradually merge. In all cases, self-annihilation of vortices of opposite charge is observed. We also find that for sufficiently long barrier ramp times, the initial relative phases between the fragments leave a clear imprint on the resulting topological configuration. Finally, we study the three-dimensional system and the formation of vortex lines and vortex rings due to the merger of the BEC fragments; our results illustrate how the relevant vorticity is manifested for appropriate phase differences, as well as how it may be masked by the planar projections observed experimentally.
cond-mat.other
we study the formation of vortices in a boseeinstein condensate bec that has been prepared by allowing isolated and independent condensed fragments to merge together we focus on the experimental setup of scherer it et al phys rev lett bf 98 110402 2007 where three becs are created in a magnetic trap that is segmented into three regions by a repulsive optical potential the becs merge together as the optical potential is removed first we study the twodimensional case in particular we examine the effects of the relative phases of the different fragments and the removal rate of the optical potential on the vortex formation we find that many vortices are created by instant removal of the optical potential regardless of relative phases and that fewer vortices are created if the intensity of the optical potential is gradually ramped down and the condensed fragments gradually merge in all cases selfannihilation of vortices of opposite charge is observed we also find that for sufficiently long barrier ramp times the initial relative phases between the fragments leave a clear imprint on the resulting topological configuration finally we study the threedimensional system and the formation of vortex lines and vortex rings due to the merger of the bec fragments our results illustrate how the relevant vorticity is manifested for appropriate phase differences as well as how it may be masked by the planar projections observed experimentally
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711.0376
Gauge k-vortices
We consider gauge vortices in symmetry breaking models with a non-canonical kinetic term. This work extends our previous study on global topological k-defects (hep-th/0608071), including a gauge field. The model consists of a scalar field with a non-canonical kinetic term, while for the gauge field the standard form of its kinetic term is preserved. Topological defects arising in such models, k-vortices, may have quite different properties as compared to ``standard'' vortices. This happens because an additional dimensional parameter enters the Lagrangian for the considered model -- a ``kinetic'' mass. We briefly discuss possible consequences for cosmology, in particular, the formation of cosmic strings during phase transitions in the early universe and their properties.
hep-th astro-ph hep-ph
we consider gauge vortices in symmetry breaking models with a noncanonical kinetic term this work extends our previous study on global topological kdefects hepth0608071 including a gauge field the model consists of a scalar field with a noncanonical kinetic term while for the gauge field the standard form of its kinetic term is preserved topological defects arising in such models kvortices may have quite different properties as compared to standard vortices this happens because an additional dimensional parameter enters the lagrangian for the considered model a kinetic mass we briefly discuss possible consequences for cosmology in particular the formation of cosmic strings during phase transitions in the early universe and their properties
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711.0377
Geodesible contact structures on 3--manifolds
In this paper, we study and almost completely classify contact structures on closed 3--manifolds which are totally geodesic for some Riemannian metric. Due to previously known results, this amounts to classifying contact structures on Seifert manifolds which are transverse to the fibers. Actually, we obtain the complete classification of contact structures with negative (maximal) twisting number (which includes the transverse ones) on Seifert manifolds whose base is not a sphere, as well as partial results in the spherical case.
math.GT math.SG
in this paper we study and almost completely classify contact structures on closed 3manifolds which are totally geodesic for some riemannian metric due to previously known results this amounts to classifying contact structures on seifert manifolds which are transverse to the fibers actually we obtain the complete classification of contact structures with negative maximal twisting number which includes the transverse ones on seifert manifolds whose base is not a sphere as well as partial results in the spherical case
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711.0378
M31N-2007-06b: A Nova in the M31 Globular Cluster Bol 111
We report spectroscopic observations of the nova M31N-2007-06b, which was found to be spatially coincident with the M31 globular cluster Bol 111. This nova is the first out of more than 700 discovered in M31 over the past century to be associated with one of the galaxy's globular clusters. A total of three spectra of the nova were obtained 3, 6, and 36 days post discovery. The data reveal broad (FWHM ~3000 km/s) Balmer, NII, and NIII emission lines, and show that the nova belongs to the He/N spectroscopic class. The He/N class of novae are relatively rare, making up roughly 15% of the novae with measured spectra in M31, and roughly 20-25% of the Galactic novae for which spectroscopic data are available. The implications of a nova, particularly an He/N nova, occurring in a globular cluster are discussed.
astro-ph
we report spectroscopic observations of the nova m31n200706b which was found to be spatially coincident with the m31 globular cluster bol 111 this nova is the first out of more than 700 discovered in m31 over the past century to be associated with one of the galaxys globular clusters a total of three spectra of the nova were obtained 3 6 and 36 days post discovery the data reveal broad fwhm 3000 kms balmer nii and niii emission lines and show that the nova belongs to the hen spectroscopic class the hen class of novae are relatively rare making up roughly 15 of the novae with measured spectra in m31 and roughly 2025 of the galactic novae for which spectroscopic data are available the implications of a nova particularly an hen nova occurring in a globular cluster are discussed
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711.0379
Time-Domain Measurement of Spontaneous Vibrational Decay of Magnetically Trapped NH
The v = 1 -> 0 radiative lifetime of NH (X triplet-Sigma-, v=1,N=0) is determined to be tau_rad,exp. = 37.0 +/- 0.5 stat +2.0 / -0.8 sys miliseconds, corresponding to a transition dipole moment of |mu_10| = 0.0540 + 0.0009 / -0.0018 Debye. To achieve the long observation times necessary for direct time-domain measurement, vibrationally excited NH (X triplet-Sigma-, v=1,N=0) radicals are magnetically trapped using helium buffer-gas loading. Simultaneous trapping and lifetime measurement of both the NH(v=1, N=0) and NH(v=0,N=0) populations allows for accurate extraction of tau_rad,exp. Background helium atoms are present during our measurement of tau_rad,exp., and the rate constant for helium atom induced collisional quenching of NH(v=1,N=0) was determined to be k_q < 3.9 * 10^-15 cm^3/s. This bound on k_q yields the quoted systematic uncertainty on tau_rad,exp. Using an ab initio dipole moment function and an RKR potential, we also determine a theoretical value of 36.99 ms for this lifetime, in agreement with our experimental value. Our results provide an independent determination of tau_rad,10, test molecular theory, and furthermore demonstrate the efficacy of buffer-gas loading and trapping in determining metastable radiative and collisional lifetimes.
physics.atom-ph physics.ao-ph
the v 1 0 radiative lifetime of nh x tripletsigma v1n0 is determined to be tau_radexp 370 05 stat 20 08 sys miliseconds corresponding to a transition dipole moment of mu_10 00540 00009 00018 debye to achieve the long observation times necessary for direct timedomain measurement vibrationally excited nh x tripletsigma v1n0 radicals are magnetically trapped using helium buffergas loading simultaneous trapping and lifetime measurement of both the nhv1 n0 and nhv0n0 populations allows for accurate extraction of tau_radexp background helium atoms are present during our measurement of tau_radexp and the rate constant for helium atom induced collisional quenching of nhv1n0 was determined to be k_q 39 1015 cm3s this bound on k_q yields the quoted systematic uncertainty on tau_radexp using an ab initio dipole moment function and an rkr potential we also determine a theoretical value of 3699 ms for this lifetime in agreement with our experimental value our results provide an independent determination of tau_rad10 test molecular theory and furthermore demonstrate the efficacy of buffergas loading and trapping in determining metastable radiative and collisional lifetimes
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711.038
Kinematics of NGC 2264: signs of cluster formation
We present results from 1078 high resolution spectra of 990 stars in the young open cluster NGC 2264, obtained with the Hectochelle multiobject echelle spectrograph on the 6.5m MMT. We confirm 471 stars as members, based on their radial velocity and/or H-alpha emission. The radial velocity distribution of cluster members is non-Gaussian with a dispersion of approx 3.5 km/s. We find a substantial north-south velocity gradient and spatially coherent structure inthe radial velocity distribution, similar to that seen in the molecular gas in the region. Our results suggest that there are at least three distinguishable subclusters in NGC 2264, correlated with similar structure seen in 13CO emission, which is likely to be a remnant of initial structure in this very young cluster. We propose that this substructure is the result of gravitational amplification of initial inhomogeneities during overall collapse to a filamentary distribution of gas and stars, as found in simulations by Burkert & Hartman (2004).
astro-ph
we present results from 1078 high resolution spectra of 990 stars in the young open cluster ngc 2264 obtained with the hectochelle multiobject echelle spectrograph on the 65m mmt we confirm 471 stars as members based on their radial velocity andor halpha emission the radial velocity distribution of cluster members is nongaussian with a dispersion of approx 35 kms we find a substantial northsouth velocity gradient and spatially coherent structure inthe radial velocity distribution similar to that seen in the molecular gas in the region our results suggest that there are at least three distinguishable subclusters in ngc 2264 correlated with similar structure seen in 13co emission which is likely to be a remnant of initial structure in this very young cluster we propose that this substructure is the result of gravitational amplification of initial inhomogeneities during overall collapse to a filamentary distribution of gas and stars as found in simulations by burkert hartman 2004
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711.0381
Effects of carbon nanotubes on grain boundary sliding in zirconia polycrystals
Mechanical properties of zirconia polycrystals decrease drastically at high temperature due to thermally activated grain boundary (GB) sliding, leading to plastic or even super-plastic deformation. As GB sliding is a source of energy dissipation in the material, mechanical loss measurements are well suited to study such a mechanism. They reveal, in general, a mechanical loss peak, which evolves into an exponential increase at higher temperature. When intergranular glassy films or/and amorphous pockets are presented in polycrystalline ceramics, the mechanical loss is globally higher and so is the creep rate. Here we show that introducing carbon nanotubes in zirconia, in particular, reduces drastically GB sliding and consequently the mechanical loss at high temperature. The nanotubes were observed at the grain boundaries by high-resolution transmission electron microscopy and were related to the reduction of superplasic flow through the boundaries, which should improve the material creep resistance.
cond-mat.mtrl-sci
mechanical properties of zirconia polycrystals decrease drastically at high temperature due to thermally activated grain boundary gb sliding leading to plastic or even superplastic deformation as gb sliding is a source of energy dissipation in the material mechanical loss measurements are well suited to study such a mechanism they reveal in general a mechanical loss peak which evolves into an exponential increase at higher temperature when intergranular glassy films orand amorphous pockets are presented in polycrystalline ceramics the mechanical loss is globally higher and so is the creep rate here we show that introducing carbon nanotubes in zirconia in particular reduces drastically gb sliding and consequently the mechanical loss at high temperature the nanotubes were observed at the grain boundaries by highresolution transmission electron microscopy and were related to the reduction of superplasic flow through the boundaries which should improve the material creep resistance
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711.0382
An extension of the Linear Delta Expansion to Superspace
We introduce and discuss the method of Linear Delta Expansion for the calculation of effective potentials in superspace, by adopting the improved version of the super-Feynman rules. Calculations are carried out up to two-loops and an expression for the optimized K\"{a}hler potential is worked out.
hep-th
we introduce and discuss the method of linear delta expansion for the calculation of effective potentials in superspace by adopting the improved version of the superfeynman rules calculations are carried out up to twoloops and an expression for the optimized kahler potential is worked out
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711.0383
Lawson homology, morphic cohomology and Chow motives
In this paper, the Lawson homology and morphic cohomology are defined on the Chow motives. We also define the rational coefficient Lawson homology and morphic cohomology of the Chow motives of finite quotient projective varieties. As a consequence, we obtain a formula for the Hilbert scheme of points on a smooth complex projective surface. Further discussion concerning generic finite maps is given. As a result, we give examples of self-product of smooth projective curves with nontrivial Griffiths groups by using a result of Ceresa.
math.AG math.KT
in this paper the lawson homology and morphic cohomology are defined on the chow motives we also define the rational coefficient lawson homology and morphic cohomology of the chow motives of finite quotient projective varieties as a consequence we obtain a formula for the hilbert scheme of points on a smooth complex projective surface further discussion concerning generic finite maps is given as a result we give examples of selfproduct of smooth projective curves with nontrivial griffiths groups by using a result of ceresa
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711.0384
The impact of Spitzer infrared data on stellar mass estimates - and a revised galaxy stellar mass function at 0 < z < 5
Aims: We estimate stellar masses of galaxies in the high redshift universe with the intention of determining the influence of newly available Spitzer/IRAC infrared data on the analysis. Based on the results, we probe the mass assembly history of the universe. Methods: We use the GOODS-MUSIC catalog, which provides multiband photometry from the U--filter to the 8 mum Spitzer band for almost 15,000 galaxies with either spectroscopic (for ~7 % of the sample) or photometric redshifts, and apply a standard model fitting technique to estimate stellar masses. We then repeat our calculations with fixed photometric redshifts excluding Spitzer photometry and directly compare the outcomes to look for systematic deviations. Finally we use our results to compute stellar mass functions and mass densities up to redshift z = 5. Results: We find that stellar masses tend to be overestimated on average if further constraining Spitzer data are not included into the analysis. Whilst this trend is small up to intermediate redshifts z < 2.5 and falls within the typical error in mass, the deviation increases strongly for higher redshifts and reaches a maximum of a factor of three at redshift z = 3.5. Thus, up to intermediate redshifts, results for stellar mass density are in good agreement with values taken from literature calculated without additional Spitzer photometry. At higher redshifts, however, we find a systematic trend towards lower mass densities if Spitzer/IRAC data are included.
astro-ph
aims we estimate stellar masses of galaxies in the high redshift universe with the intention of determining the influence of newly available spitzerirac infrared data on the analysis based on the results we probe the mass assembly history of the universe methods we use the goodsmusic catalog which provides multiband photometry from the ufilter to the 8 mum spitzer band for almost 15000 galaxies with either spectroscopic for 7 of the sample or photometric redshifts and apply a standard model fitting technique to estimate stellar masses we then repeat our calculations with fixed photometric redshifts excluding spitzer photometry and directly compare the outcomes to look for systematic deviations finally we use our results to compute stellar mass functions and mass densities up to redshift z 5 results we find that stellar masses tend to be overestimated on average if further constraining spitzer data are not included into the analysis whilst this trend is small up to intermediate redshifts z 25 and falls within the typical error in mass the deviation increases strongly for higher redshifts and reaches a maximum of a factor of three at redshift z 35 thus up to intermediate redshifts results for stellar mass density are in good agreement with values taken from literature calculated without additional spitzer photometry at higher redshifts however we find a systematic trend towards lower mass densities if spitzerirac data are included
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711.0385
Geometric Transitions and D-Term SUSY Breaking
We propose a new way of using geometric transitions to study metastable vacua in string theory and certain confining gauge theories. The gauge theories in question are N=2 supersymmetric theories deformed to N=1 by superpotential terms. We first geometrically engineer supersymmetry-breaking vacua by wrapping D5 branes on rigid 2-cycles in noncompact Calabi-Yau geometries, such that the central charges of the branes are misaligned. In a limit of slightly misaligned charges, this has a gauge theory description, where supersymmetry is broken by Fayet-Iliopoulos D-terms. Geometric transitions relate these configurations to dual Calabi-Yaus with fluxes, where H_RR, H_NS and dJ are all nonvanishing. We argue that the dual geometry can be effectively used to study the resulting non-supersymmetric, confining vacua.
hep-th
we propose a new way of using geometric transitions to study metastable vacua in string theory and certain confining gauge theories the gauge theories in question are n2 supersymmetric theories deformed to n1 by superpotential terms we first geometrically engineer supersymmetrybreaking vacua by wrapping d5 branes on rigid 2cycles in noncompact calabiyau geometries such that the central charges of the branes are misaligned in a limit of slightly misaligned charges this has a gauge theory description where supersymmetry is broken by fayetiliopoulos dterms geometric transitions relate these configurations to dual calabiyaus with fluxes where h_rr h_ns and dj are all nonvanishing we argue that the dual geometry can be effectively used to study the resulting nonsupersymmetric confining vacua
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711.0386
Massless Limit of Gravitational Higgs Mechanism
In gravitational Higgs mechanism graviton components acquire mass via spontaneous diffeomorphism breaking by scalar vacuum expectation values. We point out that in the massless limit the resulting theory is not Einstein-Hilbert gravity (EHG) but constrained gravity (CG). Consequently, massive solutions in the massless limit must be compared to those in CG (as opposed to EHG). We discuss spherically symmetric solutions in this context. The Schwarzschild solution in EHG can be coordinate-transformed such that it is also a solution in CG. The resulting solutions are non-perturbative in the asymptotic regime, and are reproduced in the massless limit of asymptotic massive solutions, hence no van Dam-Veltman-Zakharov discontinuity. We point out that higher curvature terms must be included to obtain non-singular spherically symmetric massive solutions and discuss a suitable framework.
hep-th gr-qc
in gravitational higgs mechanism graviton components acquire mass via spontaneous diffeomorphism breaking by scalar vacuum expectation values we point out that in the massless limit the resulting theory is not einsteinhilbert gravity ehg but constrained gravity cg consequently massive solutions in the massless limit must be compared to those in cg as opposed to ehg we discuss spherically symmetric solutions in this context the schwarzschild solution in ehg can be coordinatetransformed such that it is also a solution in cg the resulting solutions are nonperturbative in the asymptotic regime and are reproduced in the massless limit of asymptotic massive solutions hence no van damveltmanzakharov discontinuity we point out that higher curvature terms must be included to obtain nonsingular spherically symmetric massive solutions and discuss a suitable framework
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711.0387
Cascading to the MSSM
The MSSM can arise as an orientifold of a pyramid-like quiver in the context of intersecting D-branes. Here we consider quiver realizations of the MSSM which can emerge at the bottom of a duality cascade. We classify all possible minimal ways this can be done by allowing only one extra node. It turns out that this requires extending the geometry of the pyramid to an octahedron. The MSSM at the bottom of the cascade arises in one of two possible ways, with the extra node disappearing either via Higgsing or confinement. Remarkably, the quiver of the Higgsing scenario turns out to be nothing but the quiver version of the left-right symmetric extension of the MSSM. In the minimal confining scenario the duality cascade can proceed if and only if there is exactly one up/down Higgs pair. Moreover, the symmetries of the octahedron naturally admit an automorphism of the quiver which solves a version of the mu problem precisely when there are an odd number of generations.
hep-ph hep-th
the mssm can arise as an orientifold of a pyramidlike quiver in the context of intersecting dbranes here we consider quiver realizations of the mssm which can emerge at the bottom of a duality cascade we classify all possible minimal ways this can be done by allowing only one extra node it turns out that this requires extending the geometry of the pyramid to an octahedron the mssm at the bottom of the cascade arises in one of two possible ways with the extra node disappearing either via higgsing or confinement remarkably the quiver of the higgsing scenario turns out to be nothing but the quiver version of the leftright symmetric extension of the mssm in the minimal confining scenario the duality cascade can proceed if and only if there is exactly one updown higgs pair moreover the symmetries of the octahedron naturally admit an automorphism of the quiver which solves a version of the mu problem precisely when there are an odd number of generations
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711.0388
An elasto-visco-plastic model for immortal foams or emulsions
A variety of complex fluids consist in soft, round objects (foams, emulsions, assemblies of copolymer micelles or of multilamellar vesicles -- also known as onions). Their dense packing induces a slight deviation from their prefered circular or spherical shape. As a frustrated assembly of interacting bodies, such a material evolves from one conformation to another through a succession of discrete, topological events driven by finite external forces. As a result, the material exhibits a finite yield threshold. The individual objects usually evolve spontaneously (colloidal diffusion, object coalescence, molecular diffusion), and the material properties under low or vanishing stress may alter with time, a phenomenon known as aging. We neglect such effects to address the simpler behaviour of (uncommon) immortal fluids: we construct a minimal, fully tensorial, rheological model, equivalent to the (scalar) Bingham model. Importantly, the model consistently describes the ability of such soft materials to deform substantially in the elastic regime (be it compressible or not) before they undergo (incompressible) plastic creep -- or viscous flow under even higher stresses.
cond-mat.soft physics.class-ph
a variety of complex fluids consist in soft round objects foams emulsions assemblies of copolymer micelles or of multilamellar vesicles also known as onions their dense packing induces a slight deviation from their prefered circular or spherical shape as a frustrated assembly of interacting bodies such a material evolves from one conformation to another through a succession of discrete topological events driven by finite external forces as a result the material exhibits a finite yield threshold the individual objects usually evolve spontaneously colloidal diffusion object coalescence molecular diffusion and the material properties under low or vanishing stress may alter with time a phenomenon known as aging we neglect such effects to address the simpler behaviour of uncommon immortal fluids we construct a minimal fully tensorial rheological model equivalent to the scalar bingham model importantly the model consistently describes the ability of such soft materials to deform substantially in the elastic regime be it compressible or not before they undergo incompressible plastic creep or viscous flow under even higher stresses
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711.0389
Spin dependent parton distributions and structure functions
Nuclear parton distributions and structure functions are determined in an effective chiral quark theory. We also discuss an extension of our model to fragmentation functions.
nucl-th
nuclear parton distributions and structure functions are determined in an effective chiral quark theory we also discuss an extension of our model to fragmentation functions
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711.039
On the Asymptotic Representation for Transverse Magnetic Multiple Scattering of Radiation by an Infinite Grating of Dielectric Circular Cylinders at Oblique Incidence
In this article, we present the derivation of the asymptotic forms of the equations corresponding to the scattering coefficients of the exterior electric and magnetic fields of an infinite grating of insulating dielectric circular cylinders for vertically polarized and obliquely incident plane electromagnetic waves. Exploiting the generalized forms of the Twersky's elementary function representations for Schloemilch series, we have deducted an Ansatz describing the behavior of the scattering coefficients of the electric and magnetic fields for obliquely incident waves when the grating spacing is much smaller than the wavelength of the incident electromagnetic radiation. Introducing the statement of this Ansatz into the equations of the scattering coefficients of the infinite grating at oblique incidence, and expanding the scattering coefficients in the form of an asymptotic series as a function of the ratio of the radius of the cylinders to the grating spacing, we have acquired two new infinite sets of algebraic equations associated with the scattering coefficients of the exterior electric and magnetic fields of the grating for vertically polarized and obliquely incident plane waves.
math-ph math.MP
in this article we present the derivation of the asymptotic forms of the equations corresponding to the scattering coefficients of the exterior electric and magnetic fields of an infinite grating of insulating dielectric circular cylinders for vertically polarized and obliquely incident plane electromagnetic waves exploiting the generalized forms of the twerskys elementary function representations for schloemilch series we have deducted an ansatz describing the behavior of the scattering coefficients of the electric and magnetic fields for obliquely incident waves when the grating spacing is much smaller than the wavelength of the incident electromagnetic radiation introducing the statement of this ansatz into the equations of the scattering coefficients of the infinite grating at oblique incidence and expanding the scattering coefficients in the form of an asymptotic series as a function of the ratio of the radius of the cylinders to the grating spacing we have acquired two new infinite sets of algebraic equations associated with the scattering coefficients of the exterior electric and magnetic fields of the grating for vertically polarized and obliquely incident plane waves
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711.0391
Kinematic Structure of the Orion Nebula Cluster and its Surroundings
We present results from 1351 high resolution spectra of 1215 stars in the Orion Nebula Cluster (ONC) and the surrounding Orion 1c association, obtained with the Hectochelle multiobject echelle spectrograph on the 6.5m MMT. We confirmed 1111 stars as members, based on their radial velocity and/or H-alpha emission. The radial velocity distribution of members shows a dispersion of 3.1 km/s. We found a substantial north-south velocity gradient and spatially coherent structure in the radial velocity distribution, similar to that seen in the molecular gas in the region. We also identified several binary and high velocity stars, a region exhibiting signs of triggered star formation, and a possible foreground population of stars somewhat older than the ONC. Stars without infrared excesses (as detected with the IRAC instrument on the Spitzer Space Telescope) exhibit a wider spread in radial velocity than the infrared excess stars; this spread is mostly due to a blue-shifted population of stars that may constitute a foreground population. We also identify some accreting stars, based on H-alpha, that do not have detectable infrared excesses with IRAC, and thus are potential transitional disk systems (objects with inner disk holes). We propose that the substructure seen both in stellar and gaseous component is the result of non-uniform gravitational collapse to a filamentary distribution of gas. The spatial and kinematic correlation between the stellar and gaseous components suggests the region is very young, probably only ~1 crossing time old or less to avoid shock dissipation and gravitational interactions which would tend to destroy the correlation between stars and gas.
astro-ph
we present results from 1351 high resolution spectra of 1215 stars in the orion nebula cluster onc and the surrounding orion 1c association obtained with the hectochelle multiobject echelle spectrograph on the 65m mmt we confirmed 1111 stars as members based on their radial velocity andor halpha emission the radial velocity distribution of members shows a dispersion of 31 kms we found a substantial northsouth velocity gradient and spatially coherent structure in the radial velocity distribution similar to that seen in the molecular gas in the region we also identified several binary and high velocity stars a region exhibiting signs of triggered star formation and a possible foreground population of stars somewhat older than the onc stars without infrared excesses as detected with the irac instrument on the spitzer space telescope exhibit a wider spread in radial velocity than the infrared excess stars this spread is mostly due to a blueshifted population of stars that may constitute a foreground population we also identify some accreting stars based on halpha that do not have detectable infrared excesses with irac and thus are potential transitional disk systems objects with inner disk holes we propose that the substructure seen both in stellar and gaseous component is the result of nonuniform gravitational collapse to a filamentary distribution of gas the spatial and kinematic correlation between the stellar and gaseous components suggests the region is very young probably only 1 crossing time old or less to avoid shock dissipation and gravitational interactions which would tend to destroy the correlation between stars and gas
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711.0392
Polarized structure functions of nucleons and nuclei
We determine the quark distributions and structure functions for both unpolarized and polarized DIS of leptons on nucleons and nuclei. The scalar and vector mean fields in the nucleus modify the motion of the quarks inside the nucleons. By taking into account this medium modification, we are able to reproduce the experimental data on the unpolarized EMC effect, and to make predictions for the polarized EMC effect. We discuss examples of nuclei where the polarized EMC effect could be measured. We finally present an extension of our model to describe fragmentation functions.
nucl-th
we determine the quark distributions and structure functions for both unpolarized and polarized dis of leptons on nucleons and nuclei the scalar and vector mean fields in the nucleus modify the motion of the quarks inside the nucleons by taking into account this medium modification we are able to reproduce the experimental data on the unpolarized emc effect and to make predictions for the polarized emc effect we discuss examples of nuclei where the polarized emc effect could be measured we finally present an extension of our model to describe fragmentation functions
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711.0393
Uniform non-amenability, cost, and the first l^2-Betti number
It is shown that $2\beta_1(\G)\leq h(\G)$ for any countable group $\G$, where $\beta_1(\G)$ is the first $\ell^2$-Betti number and $h(\G)$ the uniform isoperimetric constant. In particular, a countable group with non-vanishing first $\ell^2$-Betti number is uniformly non-amenable. We then define isoperimetric constants in the framework of measured equivalence relations. For an ergodic measured equivalence relation $R$ of type $\IIi$, the uniform isoperimetric constant $h(R)$ of $R$ is invariant under orbit equivalence and satisfies $$ 2\beta_1(R)\leq 2C(R)-2\leq h(R), $$ where $\beta_1(\R)$ is the first $\ell^2$-Betti number and $C(R)$ the cost of $R$ in the sense of Levitt (in particular $h(R)$ is a non-trivial invariant). In contrast with the group case, uniformly non-amenable measured equivalence relations of type $\IIi$ always contain non-amenable subtreeings. An ergodic version $h_e(\G)$ of the uniform isoperimetric constant $h(\G)$ is defined as the infimum over all essentially free ergodic and measure preserving actions $\alpha$ of $\G$ of the uniform isoperimetric constant $h(\R_\alpha)$ of the equivalence relation $R_\alpha$ associated to $\alpha$. By establishing a connection with the cost of measure-preserving equivalence relations, we prove that $h_e(\G)=0$ for any lattice $\G$ in a semi-simple Lie group of real rank at least 2 (while $h_e(\G)$ does not vanish in general).
math.GR math.DS
it is shown that 2beta_1gleq hg for any countable group g where beta_1g is the first ell2betti number and hg the uniform isoperimetric constant in particular a countable group with nonvanishing first ell2betti number is uniformly nonamenable we then define isoperimetric constants in the framework of measured equivalence relations for an ergodic measured equivalence relation r of type iii the uniform isoperimetric constant hr of r is invariant under orbit equivalence and satisfies 2beta_1rleq 2cr2leq hr where beta_1r is the first ell2betti number and cr the cost of r in the sense of levitt in particular hr is a nontrivial invariant in contrast with the group case uniformly nonamenable measured equivalence relations of type iii always contain nonamenable subtreeings an ergodic version h_eg of the uniform isoperimetric constant hg is defined as the infimum over all essentially free ergodic and measure preserving actions alpha of g of the uniform isoperimetric constant hr_alpha of the equivalence relation r_alpha associated to alpha by establishing a connection with the cost of measurepreserving equivalence relations we prove that h_eg0 for any lattice g in a semisimple lie group of real rank at least 2 while h_eg does not vanish in general
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711.0394
Electronic Transport through Magnetic Molecules with Soft Vibrating Modes
The low-temperature transport properties of a molecule are studied in the field-effect transitor geometry. The molecule has an internal mechanical mode that modulates its electronic levels and renormalizes both the interactions and the coupling to the electrodes. For a soft mechanical mode the spin fluctuations in the molecule are dominated by the bare couplings while the valence changes are determined by the dressed energies. In this case, the transport properties present an anomalous behavior and the Kondo temperature has a weak gate voltage dependence. These observations are in agreement with recent experimental data.
cond-mat.str-el cond-mat.mes-hall
the lowtemperature transport properties of a molecule are studied in the fieldeffect transitor geometry the molecule has an internal mechanical mode that modulates its electronic levels and renormalizes both the interactions and the coupling to the electrodes for a soft mechanical mode the spin fluctuations in the molecule are dominated by the bare couplings while the valence changes are determined by the dressed energies in this case the transport properties present an anomalous behavior and the kondo temperature has a weak gate voltage dependence these observations are in agreement with recent experimental data
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711.0395
Chandra Observations of Early-type Galaxies
We have performed uniform analysis of a sample of 54 nearby, early-type galaxies observed with \emph{Chandra}. In this work we present the spectral results for both the diffuse Interstellar Medium, ISM, and low-mass X-ray binaries, LMXBs. We determine the metallicity of the hot ISM in the 22 brightest galaxies and find a narrow range of abundance ratios relative to iron. The average iron metallicity of these bright galaxies is $0.96\pm0.33$ relative to solar. By assuming these enrichment patterns continue to fainter galaxies, we are able to extend accurate ISM modeling down to the faintest galaxies in the sample. The sample of galaxies span 4.5 orders of magnitude in X-ray luminosity starting at $L_X=10^{38} erg \cdot s^{-1}$ and the average gas temperature in the sample is $0.58\pm0.24 keV$. We present the X-ray properties of these galaxies scaled to one effective radius as well as radial variations of gas and stellar binary luminosities, and radial variations of gas temperature, metallicity, mass, entropy and density.
astro-ph
we have performed uniform analysis of a sample of 54 nearby earlytype galaxies observed with emphchandra in this work we present the spectral results for both the diffuse interstellar medium ism and lowmass xray binaries lmxbs we determine the metallicity of the hot ism in the 22 brightest galaxies and find a narrow range of abundance ratios relative to iron the average iron metallicity of these bright galaxies is 096pm033 relative to solar by assuming these enrichment patterns continue to fainter galaxies we are able to extend accurate ism modeling down to the faintest galaxies in the sample the sample of galaxies span 45 orders of magnitude in xray luminosity starting at l_x1038 erg cdot s1 and the average gas temperature in the sample is 058pm024 kev we present the xray properties of these galaxies scaled to one effective radius as well as radial variations of gas and stellar binary luminosities and radial variations of gas temperature metallicity mass entropy and density
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711.0396
Realistic Yukawa Textures and SUSY Spectra from Intersecting Branes
We study the possible phenomenology of a three-family Pati-Salam model constructed from intersecting D6-branes in Type IIA string theory on the T^6/(Z2 x Z2) orientifold with some desirable semi-realistic features. In the model, tree-level gauge coupling unification is achieved automatically at the string scale, and the gauge symmetry may be broken to the Standard Model (SM) close to the string scale. The small number of extra chiral exotic states in the model may be decoupled via the Higgs mechanism and strong dynamics. We calculate the possible supersymmetry breaking soft terms and the corresponding low-energy supersymmetric particle spectra which may potentially be tested at the Large Hadron Collider (LHC). We find that for the viable regions of the parameter space the lightest CP-even Higgs boson mass usually satisfies m_H < 120 GeV, and the observed dark matter density may be generated. Finally, we find that it is possible to obtain correct SM quark masses and mixings, and the tau lepton mass at the unification scale. Additionally, neutrino masses and mixings may be generated via the seesaw mechanism. Mechanisms to stabilize the open and closed-string moduli, which are necessary for the model to be truly viable and to make definite predictions are discussed.
hep-ph astro-ph hep-th
we study the possible phenomenology of a threefamily patisalam model constructed from intersecting d6branes in type iia string theory on the t6z2 x z2 orientifold with some desirable semirealistic features in the model treelevel gauge coupling unification is achieved automatically at the string scale and the gauge symmetry may be broken to the standard model sm close to the string scale the small number of extra chiral exotic states in the model may be decoupled via the higgs mechanism and strong dynamics we calculate the possible supersymmetry breaking soft terms and the corresponding lowenergy supersymmetric particle spectra which may potentially be tested at the large hadron collider lhc we find that for the viable regions of the parameter space the lightest cpeven higgs boson mass usually satisfies m_h 120 gev and the observed dark matter density may be generated finally we find that it is possible to obtain correct sm quark masses and mixings and the tau lepton mass at the unification scale additionally neutrino masses and mixings may be generated via the seesaw mechanism mechanisms to stabilize the open and closedstring moduli which are necessary for the model to be truly viable and to make definite predictions are discussed
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711.0397
Coherent, adiabatic and dissociation regimes in coupled atomic-molecular Bose-Einstein condensates
We discuss the dynamics of a Bose-Einstein condensate of atoms which is suddenly coupled to a condensate of molecules by an optical or magnetic Feshbach resonance. Three limiting regimes are found and can be understood from the transient dynamics occuring for each pair of atoms. This transient dynamics can be summarised into a time-dependent shift and broadening of the molecular state. A simple Gross-Pitaevskii picture including this shift and broadening is proposed to describe the system in the three regimes. Finally, we suggest how to explore these regimes experimentally.
cond-mat.other
we discuss the dynamics of a boseeinstein condensate of atoms which is suddenly coupled to a condensate of molecules by an optical or magnetic feshbach resonance three limiting regimes are found and can be understood from the transient dynamics occuring for each pair of atoms this transient dynamics can be summarised into a timedependent shift and broadening of the molecular state a simple grosspitaevskii picture including this shift and broadening is proposed to describe the system in the three regimes finally we suggest how to explore these regimes experimentally
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711.0398
Redox Entropy of Plastocyanin: Developing a Microscopic View of Mesoscopic Polar Solvation
We report applications of analytical formalisms and Molecular Dynamics (MD) simulations to the calculation of redox entropy of plastocyanin metalloprotein in aqueous solution. The goal of our analysis is to establish critical components of the theory required to describe polar solvation at the mesoscopic scale. The analytical techniques include a microscopic formalism based on structure factors of the solvent dipolar orientations and density and continuum dielectric theories. The microscopic theory employs the atomistic structure of the protein with force-field atomic charges and solvent structure factors obtained from separate MD simulations of the homogeneous solvent. The MD simulations provide linear response solvation free energies and reorganization energies of electron transfer in the temperature range 280--310 K. We found that continuum models universally underestimate solvation entropies, and a more favorable agreement is reported between the microscopic calculations and MD simulations. The analysis of simulations also suggests that difficulties of extending standard formalisms to protein solvation are related to the inhomogeneous structure of the solvation shell at the protein-water interface combining islands of highly structured water around ionized residues along with partial dewetting of hydrophobic patches. Quantitative theories of electrostatic protein hydration need to incorporate realistic density profile of water at the protein-water interface.
physics.bio-ph physics.chem-ph
we report applications of analytical formalisms and molecular dynamics md simulations to the calculation of redox entropy of plastocyanin metalloprotein in aqueous solution the goal of our analysis is to establish critical components of the theory required to describe polar solvation at the mesoscopic scale the analytical techniques include a microscopic formalism based on structure factors of the solvent dipolar orientations and density and continuum dielectric theories the microscopic theory employs the atomistic structure of the protein with forcefield atomic charges and solvent structure factors obtained from separate md simulations of the homogeneous solvent the md simulations provide linear response solvation free energies and reorganization energies of electron transfer in the temperature range 280310 k we found that continuum models universally underestimate solvation entropies and a more favorable agreement is reported between the microscopic calculations and md simulations the analysis of simulations also suggests that difficulties of extending standard formalisms to protein solvation are related to the inhomogeneous structure of the solvation shell at the proteinwater interface combining islands of highly structured water around ionized residues along with partial dewetting of hydrophobic patches quantitative theories of electrostatic protein hydration need to incorporate realistic density profile of water at the proteinwater interface
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711.0399
Slow failure of quasi-brittle solids
A new mesoscopic non-equilibrium thermodynamic approach is developed. The approach is based on the thermodynamic identity associated the first and second law of thermodynamics. In the framework of the approach different internal dissipative channels of energy are taken in account in an explicit form, namely, the thermal channel and channels of defect subsystems. The identity has a perfect differential form what permits to introduce an extended non-equilibrium state and use the good developed mathematical formalism of equilibrium and non-equilibrium thermodynamics. The evolution of non-equilibrium variables of a physical system are described by a Landau-based equation set expressed through internal or different kinds of free energy connected by means of the Legendre transforms. The accordance between the different kinds of energy is possible owing to introduction of some trends into the equation subset described the defect subsystems and having a nature of structural viscosity. The possibilities of the approach are illustrated on the example of quasibrittle solid damage and failure. Taking into account only one type of defects (viz., microcracks) and mechanical parameters in an expansion of free energy down to third powers in relative to average energy per microcrack, the description of destruction of quasi-brittle solids during long-term loading is considered. The consideration allows to find equilibrium and non-equilibrium values of the free energy. A qualitative behavior of the system on parameters of the theory is analyzed. The destruction of material is described from the uniform positions, both at uniform tension and uniaxial compression. Origins of the high stability of mine workings at small depths and their instability at large depths are explained.
cond-mat.mtrl-sci
a new mesoscopic nonequilibrium thermodynamic approach is developed the approach is based on the thermodynamic identity associated the first and second law of thermodynamics in the framework of the approach different internal dissipative channels of energy are taken in account in an explicit form namely the thermal channel and channels of defect subsystems the identity has a perfect differential form what permits to introduce an extended nonequilibrium state and use the good developed mathematical formalism of equilibrium and nonequilibrium thermodynamics the evolution of nonequilibrium variables of a physical system are described by a landaubased equation set expressed through internal or different kinds of free energy connected by means of the legendre transforms the accordance between the different kinds of energy is possible owing to introduction of some trends into the equation subset described the defect subsystems and having a nature of structural viscosity the possibilities of the approach are illustrated on the example of quasibrittle solid damage and failure taking into account only one type of defects viz microcracks and mechanical parameters in an expansion of free energy down to third powers in relative to average energy per microcrack the description of destruction of quasibrittle solids during longterm loading is considered the consideration allows to find equilibrium and nonequilibrium values of the free energy a qualitative behavior of the system on parameters of the theory is analyzed the destruction of material is described from the uniform positions both at uniform tension and uniaxial compression origins of the high stability of mine workings at small depths and their instability at large depths are explained
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711.04
Infinite-Dimensional Symmetries of Two-Dimensional Coset Models
It has long been appreciated that the toroidal reduction of any gravity or supergravity to two dimensions gives rise to a scalar coset theory exhibiting an infinite-dimensional global symmetry. This symmetry is an extension of the finite-dimensional symmetry G in three dimensions, after performing a further circle reduction. There has not been universal agreement as to exactly what the extended symmetry algebra is, with different arguments seemingly concluding either that it is $\hat G$, the affine Kac-Moody extension of G, or else a subalgebra thereof. Exceptional in the literature for its explicit and transparent exposition is the extremely lucid discussion by Schwarz, which we take as our starting point for studying the simpler situation of two-dimensional flat-space sigma models, which nonetheless capture all the essential details. We arrive at the conclusion that the full symmetry is described by the Kac-Moody algebra G, although truncations to subalgebras, such as the one obtained by Schwarz, can be considered too. We then consider the explicit example of the SL(2,R)/O(2) coset, and relate Schwarz's approach to an earlier discussion that goes back to the work of Geroch.
hep-th
it has long been appreciated that the toroidal reduction of any gravity or supergravity to two dimensions gives rise to a scalar coset theory exhibiting an infinitedimensional global symmetry this symmetry is an extension of the finitedimensional symmetry g in three dimensions after performing a further circle reduction there has not been universal agreement as to exactly what the extended symmetry algebra is with different arguments seemingly concluding either that it is hat g the affine kacmoody extension of g or else a subalgebra thereof exceptional in the literature for its explicit and transparent exposition is the extremely lucid discussion by schwarz which we take as our starting point for studying the simpler situation of twodimensional flatspace sigma models which nonetheless capture all the essential details we arrive at the conclusion that the full symmetry is described by the kacmoody algebra g although truncations to subalgebras such as the one obtained by schwarz can be considered too we then consider the explicit example of the sl2ro2 coset and relate schwarzs approach to an earlier discussion that goes back to the work of geroch
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711.0401
Rabi flopping between ground and Rydberg states with dipole-dipole atomic interactions
We demonstrate Rabi flopping of small numbers of $\rm{^{87}Rb}$ atoms between ground and Rydberg states with $n\le 43$. Coherent population oscillations are observed for single atom flopping, while the presence of two or more atoms decoheres the oscillations. We show that these observations are consistent with van der Waals interactions of Rydberg atoms.
quant-ph
we demonstrate rabi flopping of small numbers of rm87rb atoms between ground and rydberg states with nle 43 coherent population oscillations are observed for single atom flopping while the presence of two or more atoms decoheres the oscillations we show that these observations are consistent with van der waals interactions of rydberg atoms
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711.0402
Vortex core size in interacting cylindrical nanodot arrays
The effect of dipolar interactions among cylindrical nanodots, with a vortex-core magnetic configuration, is analyzed by means of analytical calculations. The cylinders are placed in a N x N square array in two configurations - core oriented parallel to each other and with antiparallel alignment between nearest neighbors. Results comprise the variation in the core radius with the number of interacting dots, the distance between them and dot height. The dipolar interdot coupling leads to a decrease (increase) of the core radius for parallel (antiparallel) arrays.
cond-mat.mtrl-sci
the effect of dipolar interactions among cylindrical nanodots with a vortexcore magnetic configuration is analyzed by means of analytical calculations the cylinders are placed in a n x n square array in two configurations core oriented parallel to each other and with antiparallel alignment between nearest neighbors results comprise the variation in the core radius with the number of interacting dots the distance between them and dot height the dipolar interdot coupling leads to a decrease increase of the core radius for parallel antiparallel arrays
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711.0403
Hyperbolic conservation laws and spacetimes with limited regularity
Hyperbolic conservation laws posed on manifolds arise in many applications to geophysical flows and general relativity. Recent work by the author and his collaborators attempts to set the foundations for a study of weak solutions defined on Riemannian or Lorentzian manifolds and includes an investigation of the existence and qualitative behavior of solutions. The metric on the manifold may either be fixed (shallow water equations on the sphere, for instance) or be one of the unknowns of the theory (Einstein-Euler equations of general relativity).
math.AP math.DG
hyperbolic conservation laws posed on manifolds arise in many applications to geophysical flows and general relativity recent work by the author and his collaborators attempts to set the foundations for a study of weak solutions defined on riemannian or lorentzian manifolds and includes an investigation of the existence and qualitative behavior of solutions the metric on the manifold may either be fixed shallow water equations on the sphere for instance or be one of the unknowns of the theory einsteineuler equations of general relativity
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711.0404
Generalizations of Nonlinear and Supersymmetric Classical Electrodynamics
We first write down a very general description of nonlinear classical electrodynamics, making use of generalized constitutive equations and constitutive tensors. Our approach includes non-Lagrangian as well as Lagrangian theories, allows for electromagnetic fields in the widest possible variety of media (anisotropic, piroelectric, chiral and ferromagnetic), and accommodates the incorporation of nonlocal effects. We formulate electric-magnetic duality in terms of the constitutive tensors. We then propose a supersymmetric version of the general constitutive equations, in a superfield approach.
hep-th hep-ph math-ph math.MP physics.class-ph
we first write down a very general description of nonlinear classical electrodynamics making use of generalized constitutive equations and constitutive tensors our approach includes nonlagrangian as well as lagrangian theories allows for electromagnetic fields in the widest possible variety of media anisotropic piroelectric chiral and ferromagnetic and accommodates the incorporation of nonlocal effects we formulate electricmagnetic duality in terms of the constitutive tensors we then propose a supersymmetric version of the general constitutive equations in a superfield approach
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711.0405
Spin-torque driven ferromagnetic resonance of Co/Ni synthetic layers in spin valves
Spin-torque driven ferromagnetic resonance (ST-FMR) is used to study thin Co/Ni synthetic layers with perpendicular anisotropy confined in spin-valve based nanojunctions. Field swept ST-FMR measurements were conducted with a magnetic field applied perpendicular to the layer surface. The resonance lines were measured under low amplitude rf excitation, from 1 to 20 GHz. These results are compared with those obtained using conventional rf field driven FMR on extended films with the same Co/Ni layer structure. The layers confined in spin valves have a lower resonance field, a narrower resonance linewidth and approximately the same linewidth vs frequency slope, implying the same damping parameter. The critical current for magnetic excitations is determined from measurements of the resonance linewidth vs dc current and is in accord with the one determined from I-V measurements.
cond-mat.mes-hall cond-mat.mtrl-sci
spintorque driven ferromagnetic resonance stfmr is used to study thin coni synthetic layers with perpendicular anisotropy confined in spinvalve based nanojunctions field swept stfmr measurements were conducted with a magnetic field applied perpendicular to the layer surface the resonance lines were measured under low amplitude rf excitation from 1 to 20 ghz these results are compared with those obtained using conventional rf field driven fmr on extended films with the same coni layer structure the layers confined in spin valves have a lower resonance field a narrower resonance linewidth and approximately the same linewidth vs frequency slope implying the same damping parameter the critical current for magnetic excitations is determined from measurements of the resonance linewidth vs dc current and is in accord with the one determined from iv measurements
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711.0406
Generalized monotone schemes, discrete paths of extrema, and discrete entropy conditions
Solutions to conservation laws satisfy the monotonicity property: the number of local extrema is a non-increasing function of time, and local maximum/minimum values decrease/increase monotonically in time. This paper investigates this property from a numerical standpoint. We introduce a class of fully discrete in space and time, high order accurate, difference schemes, called generalized monotone schemes. Convergence toward the entropy solution is proven via a new technique of proof, assuming that the initial data has a finite number of extremum values only, and the flux-function is strictly convex. We define discrete paths of extrema by tracking local extremum values in the approximate solution. In the course of the analysis we establish the pointwise convergence of the trace of the solution along a path of extremum. As a corollary, we obtain a proof of convergence for a MUSCL-type scheme being second order accurate away from sonic points and extrema.
math.NA math.AP
solutions to conservation laws satisfy the monotonicity property the number of local extrema is a nonincreasing function of time and local maximumminimum values decreaseincrease monotonically in time this paper investigates this property from a numerical standpoint we introduce a class of fully discrete in space and time high order accurate difference schemes called generalized monotone schemes convergence toward the entropy solution is proven via a new technique of proof assuming that the initial data has a finite number of extremum values only and the fluxfunction is strictly convex we define discrete paths of extrema by tracking local extremum values in the approximate solution in the course of the analysis we establish the pointwise convergence of the trace of the solution along a path of extremum as a corollary we obtain a proof of convergence for a muscltype scheme being second order accurate away from sonic points and extrema
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711.0407
On holographic phase transitions at finite chemical potential
Recent Holographic studies have shown that N=4 super Yang-Mills theory coupled to fundamental matter with finite chemical potential undergoes a first order phase transition. In this paper, we study Nf D6 probe branes with or without electric field on it in the black D4 brane background compactified on a circle with supersymmetry breaking boundary condition. At energy scales much lower than the compactification scale, the dual gauge theory is effectively four dimensional non-supersymmetric SU(Nc) Yang-Mills theory coupled to fundamental matter with or without baryon number charge. Within the supergravity approximation, the decoupling of the Kaluza-Klein modes is not fully realized. For chemical potential mu<NcMq there is a line of first order phase transitions from stable meson phase to unstable meson phase. On the other hand for mu>NcMq there is no phase transition and mesons are unstable. A peculiar and interesting property of this system is that for a certain range of chemical potential mu<NcMq, a new phase transition appears in the unstable meson phase. This phase transition is characterized by a discontinuous change of unstable meson lifetime.
hep-th
recent holographic studies have shown that n4 super yangmills theory coupled to fundamental matter with finite chemical potential undergoes a first order phase transition in this paper we study nf d6 probe branes with or without electric field on it in the black d4 brane background compactified on a circle with supersymmetry breaking boundary condition at energy scales much lower than the compactification scale the dual gauge theory is effectively four dimensional nonsupersymmetric sunc yangmills theory coupled to fundamental matter with or without baryon number charge within the supergravity approximation the decoupling of the kaluzaklein modes is not fully realized for chemical potential muncmq there is a line of first order phase transitions from stable meson phase to unstable meson phase on the other hand for muncmq there is no phase transition and mesons are unstable a peculiar and interesting property of this system is that for a certain range of chemical potential muncmq a new phase transition appears in the unstable meson phase this phase transition is characterized by a discontinuous change of unstable meson lifetime
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