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710.2753
Effects of anharmonic vibration on large-angle quasi-elastic scattering of 16O+144Sm
We study the effects of double octupole and quadrupole phonon excitations in the 144Sm nucleus on quasi-elastic 16O+144Sm scattering at backward angles. To this end, we use the coupled-channels framework, taking into account explicitly the anharmonicities of the vibrations. We use the same coupling scheme as that previously employed to explain the experimental data of sub-barrier fusion cross sections for the same system. We show that the experimental data for the quasi-elastic cross sections are well reproduced in this way, although the quasi-elastic barrier distribution has a distinct high energy peak which is somewhat smeared in the experimental barrier distribution. We also discuss the effects of proton transfer on the quasi-elastic barrier distribution. Our study indicates that the fusion and quasi-elastic barrier distributions for this system cannot be accounted for simultaneously with the standard coupled-channels approach.
nucl-th
we study the effects of double octupole and quadrupole phonon excitations in the 144sm nucleus on quasielastic 16o144sm scattering at backward angles to this end we use the coupledchannels framework taking into account explicitly the anharmonicities of the vibrations we use the same coupling scheme as that previously employed to explain the experimental data of subbarrier fusion cross sections for the same system we show that the experimental data for the quasielastic cross sections are well reproduced in this way although the quasielastic barrier distribution has a distinct high energy peak which is somewhat smeared in the experimental barrier distribution we also discuss the effects of proton transfer on the quasielastic barrier distribution our study indicates that the fusion and quasielastic barrier distributions for this system cannot be accounted for simultaneously with the standard coupledchannels approach
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710.2754
A comparison between detailed and configuration-averaged collisional-radiative codes applied to non-local thermal equilibrium plasma
A collisional-radiative model describing nonlocal-thermodynamic-equilibrium plasmas is developed. It is based on the HULLAC (Hebrew University Lawrence Livermore Atomic Code) suite for the transitions rates, in the zero-temperature radiation field hypothesis. Two variants of the model are presented: the first one is configuration averaged, while the second one is a detailed level version. Comparisons are made between them in the case of a carbon plasma; they show that the configuration-averaged code gives correct results for an electronic temperature Te=10 eV (or higher) but fails at lower temperatures such as Te=1 eV. The validity of the configuration-averaged approximation is discussed: the intuitive criterion requiring that the average configuration-energy dispersion must be less than the electron thermal energy turns out to be a necessary but far from sufficient condition. Another condition based on the resolution of a modified rate-equation system is proposed. Its efficiency is emphasized in the case of low-temperature plasmas. Finally, it is shown that near-threshold autoionization cascade processes may induce a severe failure of the configuration-average formalism.
physics.plasm-ph
a collisionalradiative model describing nonlocalthermodynamicequilibrium plasmas is developed it is based on the hullac hebrew university lawrence livermore atomic code suite for the transitions rates in the zerotemperature radiation field hypothesis two variants of the model are presented the first one is configuration averaged while the second one is a detailed level version comparisons are made between them in the case of a carbon plasma they show that the configurationaveraged code gives correct results for an electronic temperature te10 ev or higher but fails at lower temperatures such as te1 ev the validity of the configurationaveraged approximation is discussed the intuitive criterion requiring that the average configurationenergy dispersion must be less than the electron thermal energy turns out to be a necessary but far from sufficient condition another condition based on the resolution of a modified rateequation system is proposed its efficiency is emphasized in the case of lowtemperature plasmas finally it is shown that nearthreshold autoionization cascade processes may induce a severe failure of the configurationaverage formalism
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710.2755
Reduced branching processes with very heavy tails
The reduced Markov branching process is a stochastic model for the genealogy of an unstructured biological population. Its limit behavior in the critical case is well studied for the Zolotarev-Slack regularity parameter $\alpha\in(0,1]$. We turn to the case of very heavy tailed reproduction distribution $\alpha=0$ assuming Zubkov's regularity condition with parameter $\beta\in(0,\infty)$. Our main result gives a new asymptotic pattern for the reduced branching process conditioned on non-extinction during a long time interval.
math.PR
the reduced markov branching process is a stochastic model for the genealogy of an unstructured biological population its limit behavior in the critical case is well studied for the zolotarevslack regularity parameter alphain01 we turn to the case of very heavy tailed reproduction distribution alpha0 assuming zubkovs regularity condition with parameter betain0infty our main result gives a new asymptotic pattern for the reduced branching process conditioned on nonextinction during a long time interval
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710.2756
From Holonomy of the Ising Model Form Factors to n-Fold Integrals and the Theory of Elliptic Curve
We recall the form factors $ f^{(j)}_{N,N}$ corresponding to the $\lambda$-extension $C(N,N; \lambda)$ of the two-point diagonal correlation function of the Ising model on the square lattice and their associated linear differential equations which exhibit both a ``Russian-doll'' nesting, and a decomposition of the linear differential operators as a direct sum of operators (equivalent to symmetric powers of the differential operator of the complete elliptic integral $E$). The scaling limit of these differential operators breaks the direct sum structure but not the ``Russian doll'' structure, the ``scaled'' linear differential operators being no longer Fuchsian. We then introduce some multiple integrals of the Ising class expected to have the same singularities as the singularities of the $n$-particle contributions $\chi^{(n)}$ to the susceptibility of the square lattice Ising model. We find the Fuchsian linear differential equations satisfied by these multiple integrals for $n=1,2,3,4$ and, only modulo a prime, for $n=5$ and 6, thus providing a large set of (possible) new singularities of the $\chi^{(n)}$. ...
math-ph cond-mat.stat-mech hep-th math.CA math.MP
we recall the form factors fj_nn corresponding to the lambdaextension cnn lambda of the twopoint diagonal correlation function of the ising model on the square lattice and their associated linear differential equations which exhibit both a russiandoll nesting and a decomposition of the linear differential operators as a direct sum of operators equivalent to symmetric powers of the differential operator of the complete elliptic integral e the scaling limit of these differential operators breaks the direct sum structure but not the russian doll structure the scaled linear differential operators being no longer fuchsian we then introduce some multiple integrals of the ising class expected to have the same singularities as the singularities of the nparticle contributions chin to the susceptibility of the square lattice ising model we find the fuchsian linear differential equations satisfied by these multiple integrals for n1234 and only modulo a prime for n5 and 6 thus providing a large set of possible new singularities of the chin
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710.2757
Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : physics goal and overview
The Tibet air shower array, which has an effective area of 37,000 square meters and is located at 4300 m in altitude, has been observing air showers induced by cosmic rays with energies above a few TeV. We are planning to add a large muon detector array to it for the purpose of increasing its sensitivity to cosmic gamma rays in the 100 TeV (10 - 1000 TeV) energy region by discriminating them from cosmic-ray hadrons. We report on the possibility of detection of gamma rays in the 100 TeV energy region in our field of view, based on the improved sensitivity of our air shower array deduced from the full Monte Carlo simulation.
astro-ph
the tibet air shower array which has an effective area of 37000 square meters and is located at 4300 m in altitude has been observing air showers induced by cosmic rays with energies above a few tev we are planning to add a large muon detector array to it for the purpose of increasing its sensitivity to cosmic gamma rays in the 100 tev 10 1000 tev energy region by discriminating them from cosmicray hadrons we report on the possibility of detection of gamma rays in the 100 tev energy region in our field of view based on the improved sensitivity of our air shower array deduced from the full monte carlo simulation
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710.2758
The fundamental theorem of asset pricing under proportional transaction costs
We extend the fundamental theorem of asset pricing to a model where the risky stock is subject to proportional transaction costs in the form of bid-ask spreads and the bank account has different interest rates for borrowing and lending. We show that such a model is free of arbitrage if and only if one can embed in it a friction-free model that is itself free of arbitrage, in the sense that there exists an artificial friction-free price for the stock between its bid and ask prices and an artificial interest rate between the borrowing and lending interest rates such that, if one discounts this stock price by this interest rate, then the resulting process is a martingale under some non-degenerate probability measure. Restricting ourselves to the simple case of a finite number of time steps and a finite number of possible outcomes for the stock price, the proof follows by combining classical arguments based on finite-dimensional separation theorems with duality results from linear optimisation.
q-fin.PR math.PR
we extend the fundamental theorem of asset pricing to a model where the risky stock is subject to proportional transaction costs in the form of bidask spreads and the bank account has different interest rates for borrowing and lending we show that such a model is free of arbitrage if and only if one can embed in it a frictionfree model that is itself free of arbitrage in the sense that there exists an artificial frictionfree price for the stock between its bid and ask prices and an artificial interest rate between the borrowing and lending interest rates such that if one discounts this stock price by this interest rate then the resulting process is a martingale under some nondegenerate probability measure restricting ourselves to the simple case of a finite number of time steps and a finite number of possible outcomes for the stock price the proof follows by combining classical arguments based on finitedimensional separation theorems with duality results from linear optimisation
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710.2759
Structural anomalies, spin transitions and charge disproportionation in LnCoO3
The diamagnetic-paramagnetic and insulator-metal transitions in LnCoO3 perovskites (Ln = La, Y, rare earths) are reinterpreted and modeled as a two-level excitation process. In distinction to previous models, the present approach can be characterized as a LS-HS-IS (low-high-intermediate spin) scenario. The first level is the local excitation of HS Co3+ species in the LS ground state. The second excitation is based on the interatomic electron transfer between the LS/HS pairs, leading finally to a stabilization of the metallic phase based on IS Co3+. The model parameters have been quantified for Ln = La, Pr and Nd samples using the powder neutron diffraction on the thermal expansion of Co-O bonds, that is associated with the two successive spin transitions. The same model is applied to interpret the magnetic susceptibility of LaCoO3 and YCoO3.
cond-mat.mtrl-sci
the diamagneticparamagnetic and insulatormetal transitions in lncoo3 perovskites ln la y rare earths are reinterpreted and modeled as a twolevel excitation process in distinction to previous models the present approach can be characterized as a lshsis lowhighintermediate spin scenario the first level is the local excitation of hs co3 species in the ls ground state the second excitation is based on the interatomic electron transfer between the lshs pairs leading finally to a stabilization of the metallic phase based on is co3 the model parameters have been quantified for ln la pr and nd samples using the powder neutron diffraction on the thermal expansion of coo bonds that is associated with the two successive spin transitions the same model is applied to interpret the magnetic susceptibility of lacoo3 and ycoo3
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710.276
A quantitative study of quasiparticle traps using the single-Cooper-pair-transistor
We use radio-frequency reflectometry to measure quasiparticle tunneling rates in the single-Cooper-pair-transistor. Devices with and without quasiparticle traps in proximity to the island are studied. A $10^2$ to $10^3$-fold reduction in the quasiparticle tunneling rate onto the island is observed in the case of quasiparticle traps. In the quasiparticle trap samples we also measure a commensurate decrease in quasiparticle tunneling rate off the island.
cond-mat.supr-con cond-mat.mes-hall
we use radiofrequency reflectometry to measure quasiparticle tunneling rates in the singlecooperpairtransistor devices with and without quasiparticle traps in proximity to the island are studied a 102 to 103fold reduction in the quasiparticle tunneling rate onto the island is observed in the case of quasiparticle traps in the quasiparticle trap samples we also measure a commensurate decrease in quasiparticle tunneling rate off the island
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710.2761
VLT-VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies. I. The sample and first results
(Ultra)Luminous Infrared Galaxies [(U)LIRGs] are much more numerous at cosmological distances than locally, and are likely precursors of elliptical galaxies. Our goal is to carry out an integral field spectroscopic survey of a representative sample of low redshift (z < 0.26) (U)LIRGs, covering different morphologies from spirals to mergers over the entire infrared luminosity range. The present study is based on optical IFS obtained with the VIMOS instrument on the VLT. The first results of this survey are presented here with the study of two galaxies representative of the two major morphological types observed in (U)LIRGs, interacting pairs and morphologically- regular, weakly-interacting spirals, respectively. We have found that IRAS 06076-2139 consists of two low-intermediate mass (0.15 and 0.4 m*) galaxies with relative velocities of ~ 550 km/s and, therefore, it is unlikely that they will merge. The VIMOS IFS has also discovered the presence of a rapidly expanding and rotating ring of gas in the southern galaxy (Gs), likely due to a nearly central head-on passage of an intruder about 140 million years ago. IRASF 12115-4656 is a spiral for which we have found a mass of 1.2 m*. The neutral gas (traced by the NaI doublet) and ionized gas components are spatially and kinematically decoupled. The analysis presented here illustrates the full potential of IFS in two important aspects: (i) the study of the kinematics and ionization structure of complex interacting/merging systems, and (2i) the study of the kinematics of the different gas phases, neutral (cool) and ionized (warm), traced by the NaD and Halpha lines, respectively. (abbreviated)
astro-ph
ultraluminous infrared galaxies ulirgs are much more numerous at cosmological distances than locally and are likely precursors of elliptical galaxies our goal is to carry out an integral field spectroscopic survey of a representative sample of low redshift z 026 ulirgs covering different morphologies from spirals to mergers over the entire infrared luminosity range the present study is based on optical ifs obtained with the vimos instrument on the vlt the first results of this survey are presented here with the study of two galaxies representative of the two major morphological types observed in ulirgs interacting pairs and morphologically regular weaklyinteracting spirals respectively we have found that iras 060762139 consists of two lowintermediate mass 015 and 04 m galaxies with relative velocities of 550 kms and therefore it is unlikely that they will merge the vimos ifs has also discovered the presence of a rapidly expanding and rotating ring of gas in the southern galaxy gs likely due to a nearly central headon passage of an intruder about 140 million years ago irasf 121154656 is a spiral for which we have found a mass of 12 m the neutral gas traced by the nai doublet and ionized gas components are spatially and kinematically decoupled the analysis presented here illustrates the full potential of ifs in two important aspects i the study of the kinematics and ionization structure of complex interactingmerging systems and 2i the study of the kinematics of the different gas phases neutral cool and ionized warm traced by the nad and halpha lines respectively abbreviated
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710.2762
Valence and spin states in perovskites LaCo0.95M0.05O3 (M = Mg, Ga, Ti)
The samples LaCoO3 with dilute substitutions on cobalt sites have been studied using the resistivity, thermopower and magnetic susceptibility measurements over the temperature range up to ~900 K. The Co-site substitution does not affect the magnetic transition at ~100 K and the onset of massive population of hole carriers at ~500 K, characteristic for undoped LaCoO3. On the other hand, the low-temperature transport and magnetism is markedly distinct for samples with extra charge on cobalt ions introduced by the heterovalent dopants (Mg2+, Ti4+) compared to samples with minor non-stoichiometry (LaCoO3, Ga3+ doped sample). Magnetic properties suggest that these extra charges create thermally stable magnetic polarons of total S ~ 2-3. Common features of Co-site doped and La-site doped samples (La1-xSrxCoO3) are discussed
cond-mat.mtrl-sci
the samples lacoo3 with dilute substitutions on cobalt sites have been studied using the resistivity thermopower and magnetic susceptibility measurements over the temperature range up to 900 k the cosite substitution does not affect the magnetic transition at 100 k and the onset of massive population of hole carriers at 500 k characteristic for undoped lacoo3 on the other hand the lowtemperature transport and magnetism is markedly distinct for samples with extra charge on cobalt ions introduced by the heterovalent dopants mg2 ti4 compared to samples with minor nonstoichiometry lacoo3 ga3 doped sample magnetic properties suggest that these extra charges create thermally stable magnetic polarons of total s 23 common features of cosite doped and lasite doped samples la1xsrxcoo3 are discussed
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710.2763
Threefolds with big and nef anticanonical bundles II
In continuation of our paper in Math. Ann. 333 we classify smooth complex projective threefolds X with -K_X big and nef but not ample and Picard number 2, whose anticanonical map is small. We assume also that the Mori contraction of X and of its flop are not both birational.
math.AG
in continuation of our paper in math ann 333 we classify smooth complex projective threefolds x with k_x big and nef but not ample and picard number 2 whose anticanonical map is small we assume also that the mori contraction of x and of its flop are not both birational
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710.2764
On the Equivalent Theory of the Generalized \tau^{(2)}-model and the Chiral Potts Model with two Alternating Vertical Rapidities
By the Baxter's $Q_{72}$-operator method, we demonstrate the equivalent theory between the generalized $\tau^{(2)}$-model (other than two special cases with a pseudovacuum state) and the $N$-state chiral Potts model with two alternating vertical rapidities, where the degenerate models are included. As a consequence, the theory of the XXZ chain model associated to cyclic representations (with the parameter $\varsigma$) of $U_{\sf q}(sl_2)$ with ${\sf q}^N=1$ for odd $N$ is identified with either (for $\varsigma^N=1$) the chiral Potts model with two superintegrable vertical rapidities, or (for $\varsigma^N \neq 1$) the degenerate model for the selfdual solution of the star-triangle relation. In all these identifications, the transfer matrices $T, \hat{T}$ of the chiral Potts model (including the degenerate ones) serve as the $Q_R, Q_L$-operators of the corresponding $\tau^{(2)}$-model, so that the functional relations hold as in the solvable $N$-state chiral Potts model.
cond-mat.stat-mech hep-th math-ph math.AG math.MP nlin.SI
by the baxters q_72operator method we demonstrate the equivalent theory between the generalized tau2model other than two special cases with a pseudovacuum state and the nstate chiral potts model with two alternating vertical rapidities where the degenerate models are included as a consequence the theory of the xxz chain model associated to cyclic representations with the parameter varsigma of u_sf qsl_2 with sf qn1 for odd n is identified with either for varsigman1 the chiral potts model with two superintegrable vertical rapidities or for varsigman neq 1 the degenerate model for the selfdual solution of the startriangle relation in all these identifications the transfer matrices t hatt of the chiral potts model including the degenerate ones serve as the q_r q_loperators of the corresponding tau2model so that the functional relations hold as in the solvable nstate chiral potts model
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710.2765
Note on the existence theorem in ``Emergent Quantum Mechanics and Emergent Symmetries''
Recently 't Hooft demonstrated that ``For any quantum system there exists at least one deterministic model that reproduces all its dynamics after prequantization''. An extension is presented here which covers quantum systems that are characterized by a complete set of mutually commuting Hermitian operators (``beables''). We introduce the symmetry of beables: any complete set of beables is as good as any other one which is obtained through a real general linear group transformation. The quantum numbers of a specific set are related to symmetry breaking initial and boundary conditions in a deterministic model. The Hamiltonian, in particular, can be taken as the emergent beable which provides the best resolution of the evolution of the model universe.
quant-ph gr-qc hep-th
recently t hooft demonstrated that for any quantum system there exists at least one deterministic model that reproduces all its dynamics after prequantization an extension is presented here which covers quantum systems that are characterized by a complete set of mutually commuting hermitian operators beables we introduce the symmetry of beables any complete set of beables is as good as any other one which is obtained through a real general linear group transformation the quantum numbers of a specific set are related to symmetry breaking initial and boundary conditions in a deterministic model the hamiltonian in particular can be taken as the emergent beable which provides the best resolution of the evolution of the model universe
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710.2766
Thermodynamic properties of Holstein polarons and the effects of disorder
The ground state and finite temperature properties of polarons are studied considering a two-site and a four-site Holstein model by exact diagonalization of the Hamiltonian. The kinetic energy, Drude weight, correlation functions involving charge and lattice deformations, and the specific heat have been evaluated as a function of electron-phonon (e-ph) coupling strength and temperature. The effects of site diagonal disorder on the above properties have been investigated. The disorder is found to suppress the kinetic energy and the Drude weight, reduces the spatial extension of the polaron, and makes the large-to-small polaron crossover smoother. Increasing temperature also plays similar role. For strong coupling the kinetic energy arises mainly from the incoherent hopping processes owing to the motion of electrons within the polaron and is almost independent of the disorder strength. From the coherent and incoherent contributions to the kinetic energy, the temperature above which the incoherent part dominates is determined as a function of e-ph coupling strength.
cond-mat.str-el
the ground state and finite temperature properties of polarons are studied considering a twosite and a foursite holstein model by exact diagonalization of the hamiltonian the kinetic energy drude weight correlation functions involving charge and lattice deformations and the specific heat have been evaluated as a function of electronphonon eph coupling strength and temperature the effects of site diagonal disorder on the above properties have been investigated the disorder is found to suppress the kinetic energy and the drude weight reduces the spatial extension of the polaron and makes the largetosmall polaron crossover smoother increasing temperature also plays similar role for strong coupling the kinetic energy arises mainly from the incoherent hopping processes owing to the motion of electrons within the polaron and is almost independent of the disorder strength from the coherent and incoherent contributions to the kinetic energy the temperature above which the incoherent part dominates is determined as a function of eph coupling strength
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710.2767
Irreducible polynomials with prescribed trace and restricted norm
Let GF(q), q=p^r, be a finite field with a primitive element g. In this paper we use exponential sums and Jacobi sums to compute the number of the irreducible polynomials of degree m over GF(q) with trace fixed and norm restricted to a coset of a subgroup <g^s>, s|(q-1). We give the number explicitly for s=2, 3, 4 when q=p, and for s|(p^e+1) when r=2en. Finally, we give explicit formulae for the number when both trace and norm are fixed, p=2 and m =< 30.
math.NT
let gfq qpr be a finite field with a primitive element g in this paper we use exponential sums and jacobi sums to compute the number of the irreducible polynomials of degree m over gfq with trace fixed and norm restricted to a coset of a subgroup gs sq1 we give the number explicitly for s2 3 4 when qp and for spe1 when r2en finally we give explicit formulae for the number when both trace and norm are fixed p2 and m 30
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710.2768
On a problem of Juhasz and van Mill
A 27 years old and still open problem of Juhasz and van Mill asks whether there exists a cardinal kappa such that every regular dense in itself countably compact space has a dense in itself subset of cardinality at most kappa. We give a negative answer for the analogous question where_regular_ is weakened to_Hausdorff_, and_coutnably compact_ is strengthened to_sequentially compact_.
math.GN
a 27 years old and still open problem of juhasz and van mill asks whether there exists a cardinal kappa such that every regular dense in itself countably compact space has a dense in itself subset of cardinality at most kappa we give a negative answer for the analogous question where_regular_ is weakened to_hausdorff_ and_coutnably compact_ is strengthened to_sequentially compact_
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710.2769
Renormalization of the vacuum angle in quantum mechanics, Berry phase and continuous measurements
The vacuum angle $\theta$ renormalization is studied for a toy model of a quantum particle moving around a ring, threaded by a magnetic flux $\theta$. Different renormalization group (RG) procedures lead to the same generic RG flow diagram, similar to that of the quantum Hall effect. We argue that the renormalized value of the vacuum angle may be observed if the particle's position is measured with finite accuracy or coupled to additional slow variable, which can be viewed as a coordinate of a second (heavy) particle on the ring. In this case the renormalized $\theta$ appears as a magnetic flux this heavy particle sees, or the Berry phase, associated with its slow rotation.
hep-th cond-mat.mes-hall
the vacuum angle theta renormalization is studied for a toy model of a quantum particle moving around a ring threaded by a magnetic flux theta different renormalization group rg procedures lead to the same generic rg flow diagram similar to that of the quantum hall effect we argue that the renormalized value of the vacuum angle may be observed if the particles position is measured with finite accuracy or coupled to additional slow variable which can be viewed as a coordinate of a second heavy particle on the ring in this case the renormalized theta appears as a magnetic flux this heavy particle sees or the berry phase associated with its slow rotation
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710.277
Renormalizing the Schrodinger Equation for NN scattering
The renormalization of the Schr"odinger equation with regular One Boson Exchange and singular chiral potentials including One and Two-Pion exchanges is analyzed within the context of NN scattering.
nucl-th
the renormalization of the schrodinger equation with regular one boson exchange and singular chiral potentials including one and twopion exchanges is analyzed within the context of nn scattering
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710.2771
Hard exclusive scattering at Jlab
The various factorization schemes for hard exclusive processes and the status of their applications is briefly reviewed.
hep-ph
the various factorization schemes for hard exclusive processes and the status of their applications is briefly reviewed
[['the', 'various', 'factorization', 'schemes', 'for', 'hard', 'exclusive', 'processes', 'and', 'the', 'status', 'of', 'their', 'applications', 'is', 'briefly', 'reviewed']]
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710.2772
Significant g-factor values of a two-electron ground state in quantum dots with spin-orbit coupling
The magnetization of semiconductor quantum dots in the presence of spin-orbit coupling and interactions is investigated numerically. When the dot is occupied by two electrons we find that a level crossing between the two lowest many-body eigenstates may occur as a function of the spin-orbit coupling strength. This level crossing is accompanied by a non-vanishing magnetization of the ground-state. Using first order perturbation theory as well as exact numerical diagonalization of small clusters we show that the tendency of interactions to cause Stoner-like instability is enhanced by the SO coupling. The resulting g-factor can have a significant value, and thus may influence g-factor measurements. Finally we propose an experimental method by which the predicted phenomenon can be observed.
cond-mat.str-el cond-mat.mes-hall
the magnetization of semiconductor quantum dots in the presence of spinorbit coupling and interactions is investigated numerically when the dot is occupied by two electrons we find that a level crossing between the two lowest manybody eigenstates may occur as a function of the spinorbit coupling strength this level crossing is accompanied by a nonvanishing magnetization of the groundstate using first order perturbation theory as well as exact numerical diagonalization of small clusters we show that the tendency of interactions to cause stonerlike instability is enhanced by the so coupling the resulting gfactor can have a significant value and thus may influence gfactor measurements finally we propose an experimental method by which the predicted phenomenon can be observed
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710.2773
Ramond-Ramond Fields, Fractional Branes and Orbifold Differential K-Theory
We study D-branes and Ramond-Ramond fields on global orbifolds of Type II string theory with vanishing H-flux using methods of equivariant K-theory and K-homology. We illustrate how Bredon equivariant cohomology naturally realizes stringy orbifold cohomology. We emphasize its role as the correct cohomological tool which captures known features of the low-energy effective field theory, and which provides new consistency conditions for fractional D-branes and Ramond-Ramond fields on orbifolds. We use an equivariant Chern character from equivariant K-theory to Bredon cohomology to define new Ramond-Ramond couplings of D-branes which generalize previous examples. We propose a definition for groups of differential characters associated to equivariant K-theory. We derive a Dirac quantization rule for Ramond-Ramond fluxes, and study flat Ramond-Ramond potentials on orbifolds.
hep-th math.KT
we study dbranes and ramondramond fields on global orbifolds of type ii string theory with vanishing hflux using methods of equivariant ktheory and khomology we illustrate how bredon equivariant cohomology naturally realizes stringy orbifold cohomology we emphasize its role as the correct cohomological tool which captures known features of the lowenergy effective field theory and which provides new consistency conditions for fractional dbranes and ramondramond fields on orbifolds we use an equivariant chern character from equivariant ktheory to bredon cohomology to define new ramondramond couplings of dbranes which generalize previous examples we propose a definition for groups of differential characters associated to equivariant ktheory we derive a dirac quantization rule for ramondramond fluxes and study flat ramondramond potentials on orbifolds
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710.2774
Final state interaction and \Delta I=1/2 rule
Contrary to wide-spread opinion that the final state interaction (FSI) enhances the amplitude <2\pi;I=0|K^0>, we argue that FSI does not increase the absolute value of this amplitude.
hep-ph
contrary to widespread opinion that the final state interaction fsi enhances the amplitude 2pii0k0 we argue that fsi does not increase the absolute value of this amplitude
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710.2775
Dam Rain and Cumulative Gain
We consider a financial contract that delivers a single cash flow given by the terminal value of a cumulative gains process. The problem of modelling and pricing such an asset and associated derivatives is important, for example, in the determination of optimal insurance claims reserve policies, and in the pricing of reinsurance contracts. In the insurance setting, the aggregate claims play the role of the cumulative gains, and the terminal cash flow represents the totality of the claims payable for the given accounting period. A similar example arises when we consider the accumulation of losses in a credit portfolio, and value a contract that pays an amount equal to the totality of the losses over a given time interval. An explicit expression for the value process is obtained. The price of an Arrow-Debreu security on the cumulative gains process is determined, and is used to obtain a closed-form expression for the price of a European-style option on the value of the asset. The results obtained make use of various remarkable properties of the gamma bridge process, and are applicable to a wide variety of financial products based on cumulative gains processes such as aggregate claims, credit portfolio losses, defined-benefit pension schemes, emissions, and rainfall.
q-fin.PR math.PR
we consider a financial contract that delivers a single cash flow given by the terminal value of a cumulative gains process the problem of modelling and pricing such an asset and associated derivatives is important for example in the determination of optimal insurance claims reserve policies and in the pricing of reinsurance contracts in the insurance setting the aggregate claims play the role of the cumulative gains and the terminal cash flow represents the totality of the claims payable for the given accounting period a similar example arises when we consider the accumulation of losses in a credit portfolio and value a contract that pays an amount equal to the totality of the losses over a given time interval an explicit expression for the value process is obtained the price of an arrowdebreu security on the cumulative gains process is determined and is used to obtain a closedform expression for the price of a europeanstyle option on the value of the asset the results obtained make use of various remarkable properties of the gamma bridge process and are applicable to a wide variety of financial products based on cumulative gains processes such as aggregate claims credit portfolio losses definedbenefit pension schemes emissions and rainfall
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710.2776
New constraints on the membership of the T dwarf S Ori 70 in the sigma Orionis cluster
(Abridged) The nature of S Ori 70, a faint mid-T type object found towards the direction of the young sigma Orionis cluster, is still under debate. We intend to disentangle whether it is a field brown dwarf or a 3-Myr old planetary-mass member of the cluster. We report on near-infrared JHK_s and mid-infrared [3.6] and [4.5] IRAC/Spitzer photometry recently obtained for S Ori 70. The new near-infrared images (taken 3.82 yr after the discovery data) have allowed us to derive a very small proper motion (11.0 +/- 5.9 mas/yr) for this object, which is consistent with the proper motion of the cluster within 1.5 sigma the astrometric uncertainty. The colors (H-K_s), (J-K_s) and K_s-[3.6] appear discrepant when compared to T4-T7 dwarfs in the field. This behavior could be ascribed to a low-gravity atmosphere or alternatively to an atmosphere with a metallicity significantly different than solar. Taking into account the small proper motion of S Ori 70 and its new near- and mid-infrared colors, a low-gravity atmosphere remains as the most likely explanation to account for our observations. This supports S Ori 70's membership in sigma Orionis, with an estimated mass in the interval 2-7 Mjup, in agreement with our previous derivation.
astro-ph
abridged the nature of s ori 70 a faint midt type object found towards the direction of the young sigma orionis cluster is still under debate we intend to disentangle whether it is a field brown dwarf or a 3myr old planetarymass member of the cluster we report on nearinfrared jhk_s and midinfrared 36 and 45 iracspitzer photometry recently obtained for s ori 70 the new nearinfrared images taken 382 yr after the discovery data have allowed us to derive a very small proper motion 110 59 masyr for this object which is consistent with the proper motion of the cluster within 15 sigma the astrometric uncertainty the colors hk_s jk_s and k_s36 appear discrepant when compared to t4t7 dwarfs in the field this behavior could be ascribed to a lowgravity atmosphere or alternatively to an atmosphere with a metallicity significantly different than solar taking into account the small proper motion of s ori 70 and its new near and midinfrared colors a lowgravity atmosphere remains as the most likely explanation to account for our observations this supports s ori 70s membership in sigma orionis with an estimated mass in the interval 27 mjup in agreement with our previous derivation
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710.2777
Teleportation of two-mode squeezed states
We consider two-mode squeezed states which are parametrized by the squeezing parameter and the phase. We present a scheme for teleporting such entangled states of continuous variables from Alice to Bob. Our protocol is operationalized through the creation of a four-mode entangled state shared by Alice and Bob using linear amplifiers and beam splitters. Teleportation of the entangled state proceeds with local operations and the classical communication of four bits. We compute the fidelity of teleportation and find that it exhibits a trade-off with the magnitude of entanglement of the resultant teleported state.
quant-ph
we consider twomode squeezed states which are parametrized by the squeezing parameter and the phase we present a scheme for teleporting such entangled states of continuous variables from alice to bob our protocol is operationalized through the creation of a fourmode entangled state shared by alice and bob using linear amplifiers and beam splitters teleportation of the entangled state proceeds with local operations and the classical communication of four bits we compute the fidelity of teleportation and find that it exhibits a tradeoff with the magnitude of entanglement of the resultant teleported state
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710.2778
Determining the crystal-field ground state in rare earth Heavy Fermion materials using soft-x-ray absorption spectroscopy
We infer that soft-x-ray absorption spectroscopy is a versatile method for the determination of the crystal-field ground state symmetry of rare earth Heavy Fermion systems, complementing neutron scattering. Using realistic and universal parameters, we provide a theoretical mapping between the polarization dependence of Ce $M_{4,5}$ spectra and the charge distribution of the Ce $4f$ states. The experimental resolution can be orders of magnitude larger than the $4f$ crystal field splitting itself. To demonstrate the experimental feasibility of the method, we investigated CePd$_2$Si$_2$, thereby settling an existing disagreement about its crystal-field ground state.
cond-mat.str-el
we infer that softxray absorption spectroscopy is a versatile method for the determination of the crystalfield ground state symmetry of rare earth heavy fermion systems complementing neutron scattering using realistic and universal parameters we provide a theoretical mapping between the polarization dependence of ce m_45 spectra and the charge distribution of the ce 4f states the experimental resolution can be orders of magnitude larger than the 4f crystal field splitting itself to demonstrate the experimental feasibility of the method we investigated cepd_2si_2 thereby settling an existing disagreement about its crystalfield ground state
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710.2779
Quantum degenerate two-species Fermi-Fermi mixture coexisting with a Bose-Einstein condensate
We report on the generation of a quantum degenerate Fermi-Fermi mixture of two different atomic species. The quantum degenerate mixture is realized employing sympathetic cooling of fermionic Li-6 and K-40 gases by an evaporatively cooled bosonic Rb-87 gas. We describe the combination of trapping and cooling methods that proved crucial to successfully cool the mixture. In particular, we study the last part of the cooling process and show that the efficiency of sympathetic cooling of the Li-6 gas by Rb-87 is increased by the presence of K-40 through catalytic cooling. Due to the differing physical properties of the two components, the quantum degenerate Li-6 K-40 Fermi-Fermi mixture is an excellent candidate for a stable, heteronuclear system allowing to study several so far unexplored types of quantum matter.
cond-mat.other
we report on the generation of a quantum degenerate fermifermi mixture of two different atomic species the quantum degenerate mixture is realized employing sympathetic cooling of fermionic li6 and k40 gases by an evaporatively cooled bosonic rb87 gas we describe the combination of trapping and cooling methods that proved crucial to successfully cool the mixture in particular we study the last part of the cooling process and show that the efficiency of sympathetic cooling of the li6 gas by rb87 is increased by the presence of k40 through catalytic cooling due to the differing physical properties of the two components the quantum degenerate li6 k40 fermifermi mixture is an excellent candidate for a stable heteronuclear system allowing to study several so far unexplored types of quantum matter
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710.278
The Optical Gravitational Lensing Experiment. Period-Luminosity Relations of Variable Red Giant Stars
Period-luminosity (PL) relations of variable red giants in the Large (LMC) and Small Magellanic Clouds (SMC) are presented. The PL diagrams are plotted in three planes: logP-K_S, logP-W_{JK}, and logP-W_I. Fourteen PL sequences are distinguishable, and some of them consist of three closely spaced ridges. Each of the sequences is fitted with a linear or quadratic function. The similarities and differences between the PL relations in both galaxies are discussed for four types of red giant variability: OGLE Small Amplitude Red Giants (OSARGs), Miras and Semiregular Variables (SRVs), Long Secondary Periods (LSPs) and ellipsoidal variables. We propose a new method of separating OSARGs from non-variable stars and SRVs. The method employs the position in the reddening-free PL diagrams and the characteristic period ratios of these multiperiodic variables. The PL relations for the LMC OSARG are compared with the calculated relations for RGB models along isochrones of relevant ages and metallicities. We also compare measured periods and amplitudes of the OSARGs with predictions based on the relations valid for less luminous solar-like pulsators. Miras and SRVs seem to follow PL relation of the same slopes in the LMC and SMC, while for LSP and ellipsoidal variables slopes in both galaxies are different. The PL sequences defined by LSP variables and binary systems overlap in the whole range of analyzed wavebands. We put forward new arguments for the binary star scenario as an explanation of the LSP variability and elaborate on it further. The measured pulsation to orbital period ratio implies nearly constant ratio of the star radius to orbital distance, R/A=0.4, as we find. Combined effect of tidal friction and mass loss enhanced by the low-mass companion may explain why such a value is preferred.
astro-ph
periodluminosity pl relations of variable red giants in the large lmc and small magellanic clouds smc are presented the pl diagrams are plotted in three planes logpk_s logpw_jk and logpw_i fourteen pl sequences are distinguishable and some of them consist of three closely spaced ridges each of the sequences is fitted with a linear or quadratic function the similarities and differences between the pl relations in both galaxies are discussed for four types of red giant variability ogle small amplitude red giants osargs miras and semiregular variables srvs long secondary periods lsps and ellipsoidal variables we propose a new method of separating osargs from nonvariable stars and srvs the method employs the position in the reddeningfree pl diagrams and the characteristic period ratios of these multiperiodic variables the pl relations for the lmc osarg are compared with the calculated relations for rgb models along isochrones of relevant ages and metallicities we also compare measured periods and amplitudes of the osargs with predictions based on the relations valid for less luminous solarlike pulsators miras and srvs seem to follow pl relation of the same slopes in the lmc and smc while for lsp and ellipsoidal variables slopes in both galaxies are different the pl sequences defined by lsp variables and binary systems overlap in the whole range of analyzed wavebands we put forward new arguments for the binary star scenario as an explanation of the lsp variability and elaborate on it further the measured pulsation to orbital period ratio implies nearly constant ratio of the star radius to orbital distance ra04 as we find combined effect of tidal friction and mass loss enhanced by the lowmass companion may explain why such a value is preferred
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710.2781
Rhombus Filtrations and Rauzy Algebras
Peach introduced rhombal algebras associated to quivers given by tilings of the plane by rhombi. We develop general techniques to analyse rhombal algebras, including a filtration by what we call rhombus modules. We introduce a way to relate the infinite-dimensional rhombal algebra corresponding to a complete tiling of the plane to finite-dimensional algebras corresponding to finite portions of the tiling. Throughout, we apply our general techniques to the special case of the Rauzy tiling, which is built in stages reflecting an underlying self-similarity. Exploiting this self-similar structure allows us to uncover interesting features of the associated finite-dimensional algebras, including some of the tree classes in the stable Auslander-Reiten quiver.
math.RT math.DS
peach introduced rhombal algebras associated to quivers given by tilings of the plane by rhombi we develop general techniques to analyse rhombal algebras including a filtration by what we call rhombus modules we introduce a way to relate the infinitedimensional rhombal algebra corresponding to a complete tiling of the plane to finitedimensional algebras corresponding to finite portions of the tiling throughout we apply our general techniques to the special case of the rauzy tiling which is built in stages reflecting an underlying selfsimilarity exploiting this selfsimilar structure allows us to uncover interesting features of the associated finitedimensional algebras including some of the tree classes in the stable auslanderreiten quiver
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710.2782
Effective linkage learning using low-order statistics and clustering
The adoption of probabilistic models for the best individuals found so far is a powerful approach for evolutionary computation. Increasingly more complex models have been used by estimation of distribution algorithms (EDAs), which often result better effectiveness on finding the global optima for hard optimization problems. Supervised and unsupervised learning of Bayesian networks are very effective options, since those models are able to capture interactions of high order among the variables of a problem. Diversity preservation, through niching techniques, has also shown to be very important to allow the identification of the problem structure as much as for keeping several global optima. Recently, clustering was evaluated as an effective niching technique for EDAs, but the performance of simpler low-order EDAs was not shown to be much improved by clustering, except for some simple multimodal problems. This work proposes and evaluates a combination operator guided by a measure from information theory which allows a clustered low-order EDA to effectively solve a comprehensive range of benchmark optimization problems.
cs.NE cs.AI
the adoption of probabilistic models for the best individuals found so far is a powerful approach for evolutionary computation increasingly more complex models have been used by estimation of distribution algorithms edas which often result better effectiveness on finding the global optima for hard optimization problems supervised and unsupervised learning of bayesian networks are very effective options since those models are able to capture interactions of high order among the variables of a problem diversity preservation through niching techniques has also shown to be very important to allow the identification of the problem structure as much as for keeping several global optima recently clustering was evaluated as an effective niching technique for edas but the performance of simpler loworder edas was not shown to be much improved by clustering except for some simple multimodal problems this work proposes and evaluates a combination operator guided by a measure from information theory which allows a clustered loworder eda to effectively solve a comprehensive range of benchmark optimization problems
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710.2783
Void Statistics and Void Galaxies in the 2dFGRS
For the 2dFGRS we study the properties of voids and of fainter galaxies within voids that are defined by brighter galaxies. Our results are compared with simulated galaxy catalogues from the Millenium simulation coupled with a semianalytical galaxy formation recipe. We derive the void size distribution and discuss its dependence on the faint magnitude limit of the galaxies defining the voids. While voids among faint galaxies are typically smaller than those among bright galaxies, the ratio of the void sizes to the mean galaxy separation reaches larger values. This is well reproduced in the mock galaxy samples studied. We provide analytic fitting functions for the void size distribution. Furthermore, we study the galaxy population inside voids defined by objects with $B_J -5\log{h}< -20$ and diameter larger than 10 \hMpc. We find a clear bimodality of the void galaxies similar to the average comparison sample. We confirm the enhanced abundance of galaxies in the blue cloud and a depression of the number of red sequence galaxies. There is an indication of a slight blue shift of the blue cloud. Furthermore, we find that galaxies in void centers have higher specific star formation rates as measured by the $\eta$ parameter. We determine the radial distribution of the ratio of early and late type galaxies through the voids. We find and discuss some differences between observations and the Millenium catalogues.
astro-ph
for the 2dfgrs we study the properties of voids and of fainter galaxies within voids that are defined by brighter galaxies our results are compared with simulated galaxy catalogues from the millenium simulation coupled with a semianalytical galaxy formation recipe we derive the void size distribution and discuss its dependence on the faint magnitude limit of the galaxies defining the voids while voids among faint galaxies are typically smaller than those among bright galaxies the ratio of the void sizes to the mean galaxy separation reaches larger values this is well reproduced in the mock galaxy samples studied we provide analytic fitting functions for the void size distribution furthermore we study the galaxy population inside voids defined by objects with b_j 5logh 20 and diameter larger than 10 hmpc we find a clear bimodality of the void galaxies similar to the average comparison sample we confirm the enhanced abundance of galaxies in the blue cloud and a depression of the number of red sequence galaxies there is an indication of a slight blue shift of the blue cloud furthermore we find that galaxies in void centers have higher specific star formation rates as measured by the eta parameter we determine the radial distribution of the ratio of early and late type galaxies through the voids we find and discuss some differences between observations and the millenium catalogues
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710.2784
Routes to thermodynamic limit on scale-free networks
We show that there are two classes of finite size effects for dynamic models taking place on a scale-free topology. Some models in finite networks show a behavior that depends only on the system size N. Others present an additional distinct dependence on the upper cutoff k_c of the degree distribution. Since the infinite network limit can be obtained by allowing k_c to diverge with the system size in an arbitrary way, this result implies that there are different routes to the thermodynamic limit in scale-free networks. The contact process (in its mean-field version) belongs to this second class and thus our results clarify the recent discrepancy between theory and simulations with different scaling of k_c reported in the literature.
cond-mat.stat-mech
we show that there are two classes of finite size effects for dynamic models taking place on a scalefree topology some models in finite networks show a behavior that depends only on the system size n others present an additional distinct dependence on the upper cutoff k_c of the degree distribution since the infinite network limit can be obtained by allowing k_c to diverge with the system size in an arbitrary way this result implies that there are different routes to the thermodynamic limit in scalefree networks the contact process in its meanfield version belongs to this second class and thus our results clarify the recent discrepancy between theory and simulations with different scaling of k_c reported in the literature
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710.2785
Monte Carlo Generators for the LHC
The status of two Monte Carlo generators, HELAC-PHEGAS, a program for multi-jet processes and VBFNLO, a parton level program for vector boson fusion processes at NLO QCD, is briefly presented. The aim of these tools is the simulation of events within the Standard Model at current and future high energy experiments, in particular the LHC. Some results related to the production of multi-jet final states at the LHC are also shown.
hep-ph
the status of two monte carlo generators helacphegas a program for multijet processes and vbfnlo a parton level program for vector boson fusion processes at nlo qcd is briefly presented the aim of these tools is the simulation of events within the standard model at current and future high energy experiments in particular the lhc some results related to the production of multijet final states at the lhc are also shown
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710.2786
Higgsless electroweak symmetry breaking at the LHC
While the Higgs model is the best studied scenario of electroweak symmetry breaking, a number strongly-coupled models exist, predicting new signatures. Recent studies of WW and WZ final states at the ATLAS and CMS experiments are summarized and expected sensitivities are presented within the frameworks of the technicolor straw-man model and the electroweak chiral Lagrangian.
hep-ex
while the higgs model is the best studied scenario of electroweak symmetry breaking a number stronglycoupled models exist predicting new signatures recent studies of ww and wz final states at the atlas and cms experiments are summarized and expected sensitivities are presented within the frameworks of the technicolor strawman model and the electroweak chiral lagrangian
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710.2787
The shuffle Hopf algebra and quasiplanar Wick products
The operator valued distributions which arise in quantum field theory on the noncommutative Minkowski space can be symbolized by a generalization of chord diagrams, the dotted chord diagrams. In this framework, the combinatorial aspects of quasiplanar Wick products are understood in terms of the shuffle Hopf algebra of dotted chord diagrams, leading to an algebraic characterization of quasiplanar Wick products as a convolution. Moreover, it is shown that the distributions do not provide a weight system for universal knot invariants.
math.QA hep-th
the operator valued distributions which arise in quantum field theory on the noncommutative minkowski space can be symbolized by a generalization of chord diagrams the dotted chord diagrams in this framework the combinatorial aspects of quasiplanar wick products are understood in terms of the shuffle hopf algebra of dotted chord diagrams leading to an algebraic characterization of quasiplanar wick products as a convolution moreover it is shown that the distributions do not provide a weight system for universal knot invariants
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710.2788
Exploring the QCD vacuum - (some) recent developments in confinement and topology
I start by giving a brief overview over new developments in the area of confinement and topology. As an example for the interrelations between topological objects, instantons at finite temperature are discussed. Then I focus on new insights into the structure of the QCD vacuum obtained through filtering methods, in particular those based on decompositions w.r.t. fermionic eigenmodes.
hep-lat hep-ph hep-th
i start by giving a brief overview over new developments in the area of confinement and topology as an example for the interrelations between topological objects instantons at finite temperature are discussed then i focus on new insights into the structure of the qcd vacuum obtained through filtering methods in particular those based on decompositions wrt fermionic eigenmodes
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710.2789
SGR 1806-20 about two years after the giant flare: Suzaku, XMM-Newton and INTEGRAL observations
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever observed. This probably involved a large-scale rearrangement of the magnetosphere leading to observable variations in the properties of its X-ray emission. Here we present the results of the first Suzaku observation of SGR 1806-20, together with almost simultaneous observations with XMM-Newton and INTEGRAL. The source seems to have reached a state characterized by a flux close to the pre-flare level and by a relatively soft spectrum. Despite this, SGR 1806-20 remained quite active also after the giant flare, allowing us to study several short bursts observed by Suzaku in the 1-100 keV range. We discuss the broad-band spectral properties of SGR 1806-20, covering both persistent and bursting emission, in the context of the magnetar model, and consider its recent theoretical developments.
astro-ph
in december 2004 the soft gammaray repeater sgr 180620 emitted the most powerful giant flare ever observed this probably involved a largescale rearrangement of the magnetosphere leading to observable variations in the properties of its xray emission here we present the results of the first suzaku observation of sgr 180620 together with almost simultaneous observations with xmmnewton and integral the source seems to have reached a state characterized by a flux close to the preflare level and by a relatively soft spectrum despite this sgr 180620 remained quite active also after the giant flare allowing us to study several short bursts observed by suzaku in the 1100 kev range we discuss the broadband spectral properties of sgr 180620 covering both persistent and bursting emission in the context of the magnetar model and consider its recent theoretical developments
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710.279
PNJL model with a Van der Monde term
We extend the Polyakov-Nambu-Jona-Lasinio (PNJL) model for two degenerate flavours by including the effect of the SU(3) measure with a Van der Monde (VdM) term. This ensures that the Polyakov loop always remains in the domain [0,1]. The pressure, energy density, specific heat, speed of sound and conformal measure show small or negligible effects from this term. However various quark number and isospin susceptibilities are all found to approach their respective ideal gas limits around 2 $T_c$. We compare our methods with other similar approaches in PNJL model and also present a quantitative comparison with Lattice QCD data.
hep-ph hep-lat nucl-th
we extend the polyakovnambujonalasinio pnjl model for two degenerate flavours by including the effect of the su3 measure with a van der monde vdm term this ensures that the polyakov loop always remains in the domain 01 the pressure energy density specific heat speed of sound and conformal measure show small or negligible effects from this term however various quark number and isospin susceptibilities are all found to approach their respective ideal gas limits around 2 t_c we compare our methods with other similar approaches in pnjl model and also present a quantitative comparison with lattice qcd data
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710.2791
Drift instability and tunneling of lattice solitons
We derive an analytic formula for the lateral dynamics of solitons in a general inhomogeneous nonlinear media, and show that it can be valid over tens of diffraction lengths. In particular, we show that solitons centered at a lattice maximum can be ``mathematically unstable'' but ``physically stable''. We also derive an analytic upper bound for the critical velocity for tunneling, which is valid even when the standard Peierls-Nabarro potential approach fails.
nlin.PS
we derive an analytic formula for the lateral dynamics of solitons in a general inhomogeneous nonlinear media and show that it can be valid over tens of diffraction lengths in particular we show that solitons centered at a lattice maximum can be mathematically unstable but physically stable we also derive an analytic upper bound for the critical velocity for tunneling which is valid even when the standard peierlsnabarro potential approach fails
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710.2792
Market completion using options
Mathematical models for financial asset prices which include, for example, stochastic volatility or jumps are incomplete in that derivative securities are generally not replicable by trading in the underlying. In earlier work (2004) the first author provided a geometric condition under which trading in the underlying and a finite number of vanilla options completes the market. We complement this result in several ways. First, we show that the geometric condition is not necessary and a weaker, necessary and sufficient, condition is presented. While this condition is generally not directly verifiable, we show that it simplifies to matrix non-degeneracy in a single point when the pricing functions are real analytic functions. In particular, any stochastic volatility model is then completed with an arbitrary European type option. Further, we show that adding path-dependent options such as a variance swap to the set of primary assets, instead of plain vanilla options, also completes the market.
q-fin.PR math.PR
mathematical models for financial asset prices which include for example stochastic volatility or jumps are incomplete in that derivative securities are generally not replicable by trading in the underlying in earlier work 2004 the first author provided a geometric condition under which trading in the underlying and a finite number of vanilla options completes the market we complement this result in several ways first we show that the geometric condition is not necessary and a weaker necessary and sufficient condition is presented while this condition is generally not directly verifiable we show that it simplifies to matrix nondegeneracy in a single point when the pricing functions are real analytic functions in particular any stochastic volatility model is then completed with an arbitrary european type option further we show that adding pathdependent options such as a variance swap to the set of primary assets instead of plain vanilla options also completes the market
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710.2793
The SGR 1806-20 magnetar signature on the Earth's magnetic field
SGRs denote ``soft $\gamma$-ray repeaters'', a small class of slowly spinning neutron stars with strong magnetic fields. On 27 December 2004, a giant flare was detected from magnetar SGR 1806-20. The initial spike was followed by a hard-X-ray tail persisting for 380 s with a modulation period of 7.56 s. This event has received considerable attention, particularly in the astrophysics area. Its relevance to the geophysics community lies in the importance of investigating the effects of such an event on the near-earth electromagnetic environment. However, the signature of a magnetar flare on the geomagnetic field has not previously been investigated. Here, by applying wavelet analysis to the high-resolution magnetic data provided by the CHAMP satellite, a modulated signal with a period of 7.5 s over the duration of the giant flare appears in the observed data. Moreover, this event was detected by the energetic ion counters onboard the DEMETER satellite.
astro-ph
sgrs denote soft gammaray repeaters a small class of slowly spinning neutron stars with strong magnetic fields on 27 december 2004 a giant flare was detected from magnetar sgr 180620 the initial spike was followed by a hardxray tail persisting for 380 s with a modulation period of 756 s this event has received considerable attention particularly in the astrophysics area its relevance to the geophysics community lies in the importance of investigating the effects of such an event on the nearearth electromagnetic environment however the signature of a magnetar flare on the geomagnetic field has not previously been investigated here by applying wavelet analysis to the highresolution magnetic data provided by the champ satellite a modulated signal with a period of 75 s over the duration of the giant flare appears in the observed data moreover this event was detected by the energetic ion counters onboard the demeter satellite
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710.2794
Fermion loop simulations in 2--d lattice theories -- results and limitations
We review our results for the simulation of the 2--d lattice Gross--Neveu model in a fermion loop representation. Possible extensions of our techniques to other models and higher dimensions are discussed, as well as the limitations of loop--type representations.
hep-lat
we review our results for the simulation of the 2d lattice grossneveu model in a fermion loop representation possible extensions of our techniques to other models and higher dimensions are discussed as well as the limitations of looptype representations
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710.2795
Charmonium properties in the quark-gluon plasma
We present results for charmonium correlators and spectral functions in 2-flavour CD on anisotropic lattices. Our results indicate that the S-waves (J/psi and eta_c) survive up to temperatures close to 2T_c, while the P-waves (chi_c0 and chi_c1) melt away below 1.2T_c.
hep-lat
we present results for charmonium correlators and spectral functions in 2flavour cd on anisotropic lattices our results indicate that the swaves jpsi and eta_c survive up to temperatures close to 2t_c while the pwaves chi_c0 and chi_c1 melt away below 12t_c
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710.2796
On the Limitations of the Color Dipole Picture
We discuss two aspects of the color dipole picture of high energy photon-proton scattering. First we present bounds on various ratios of deep inelastic structure functions resulting from the dipole picture that, together with the measured data, can be used to restrict the kinematical range of its applicability. The second issue that we address is the choice of energy variable in the dipole-proton cross section.
hep-ph
we discuss two aspects of the color dipole picture of high energy photonproton scattering first we present bounds on various ratios of deep inelastic structure functions resulting from the dipole picture that together with the measured data can be used to restrict the kinematical range of its applicability the second issue that we address is the choice of energy variable in the dipoleproton cross section
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710.2797
Unparticles and holography
We construct the holographic dual theory of unparticles. The Randall-Sundrum type hard wall model is shown to produce deconstructing particles, whose spectrum has a finite mass gap proportional to the inverse of the fifth direction segment. The introduction of new scale corresponds to setting a brane in ${\rm AdS}_5$. The broken conformal symmetry due to this brane is restored when it is moved to infinity. Unparticles then emerge as an infinite tower of massless particles.
hep-ph astro-ph hep-th
we construct the holographic dual theory of unparticles the randallsundrum type hard wall model is shown to produce deconstructing particles whose spectrum has a finite mass gap proportional to the inverse of the fifth direction segment the introduction of new scale corresponds to setting a brane in rm ads_5 the broken conformal symmetry due to this brane is restored when it is moved to infinity unparticles then emerge as an infinite tower of massless particles
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710.2798
A common integrable structure in the hermitian matrix model and Hele-Shaw flows
It is proved that the system of string equations of the dispersionless 2-Toda hierarchy which arises in the planar limit of the hermitian matrix model also underlies certain processes in Hele-Shaw flows.
nlin.SI
it is proved that the system of string equations of the dispersionless 2toda hierarchy which arises in the planar limit of the hermitian matrix model also underlies certain processes in heleshaw flows
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710.2799
Study of the topological vacuum structure of SU(2) gluodynamics at T > 0 with overlap fermions and improved action
We study SU(2) gluodynamics at finite temperature near the deconfining phase transition. We create the lattice ensembles using the tadpole improved Luscher-Weisz action. The overlap Dirac operator is used to determine the following three aspects of vacuum structure: (i) The topological susceptibility is evaluated at various temperatures across the phase transition, (ii) the overlap fermion spectral density is determined and found to depend on the Polyakov loop above the phase transition and (iii) the corresponding localization properties of low lying eigenmodes are investigated.
hep-lat
we study su2 gluodynamics at finite temperature near the deconfining phase transition we create the lattice ensembles using the tadpole improved luscherweisz action the overlap dirac operator is used to determine the following three aspects of vacuum structure i the topological susceptibility is evaluated at various temperatures across the phase transition ii the overlap fermion spectral density is determined and found to depend on the polyakov loop above the phase transition and iii the corresponding localization properties of low lying eigenmodes are investigated
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710.28
A weight two phenomenon for the moduli of rank one local systems on open varieties
The twistor space of representations on an open variety maps to a weight two space of local monodromy transformations around a divisor component at infinty. The space of $\sigma$-invariant sections of this slope-two bundle over the twistor line is a real 3 dimensional space whose parameters correspond to the complex residue of the Higgs field, and the real parabolic weight of a harmonic bundle.
math.AG
the twistor space of representations on an open variety maps to a weight two space of local monodromy transformations around a divisor component at infinty the space of sigmainvariant sections of this slopetwo bundle over the twistor line is a real 3 dimensional space whose parameters correspond to the complex residue of the higgs field and the real parabolic weight of a harmonic bundle
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710.2801
Multi-Gap Superconductivity in MgB2: Magneto-Raman Spectroscopy
Electronic Raman scattering studies on MgB2 single crystals as a function of excitation and polarization have revealed three distinct superconducting features: a clean gap below 37 cm-1 and two coherence peaks at 109 cm-1 and 78 cm-1 which we identify as the superconducting gaps in \pi- and \sigma-bands and as the Leggett's collective mode arising from the fluctuation in the relative phase between two superconducting condensates residing on corresponding bands. The temperature and field dependencies of the superconducting features have been established. A phononic Raman scattering study of the E2g boron stretching mode anharmonicity and of superconductivity induced self-energy effects is presented. We show that anharmonic two phonon decay is mainly responsible for the unusually large linewidth of the E2g mode. We observe ~2.5% hardening of the E2g phonon frequency upon cooling into the superconducting state and estimate the electron-phonon coupling strength associated with this renormalization.
cond-mat.supr-con
electronic raman scattering studies on mgb2 single crystals as a function of excitation and polarization have revealed three distinct superconducting features a clean gap below 37 cm1 and two coherence peaks at 109 cm1 and 78 cm1 which we identify as the superconducting gaps in pi and sigmabands and as the leggetts collective mode arising from the fluctuation in the relative phase between two superconducting condensates residing on corresponding bands the temperature and field dependencies of the superconducting features have been established a phononic raman scattering study of the e2g boron stretching mode anharmonicity and of superconductivity induced selfenergy effects is presented we show that anharmonic two phonon decay is mainly responsible for the unusually large linewidth of the e2g mode we observe 25 hardening of the e2g phonon frequency upon cooling into the superconducting state and estimate the electronphonon coupling strength associated with this renormalization
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710.2802
Investigation of Strongly Correlated Electron Systems with Cellular Dynamical Mean Field Theory
In this thesis we study the strongly-correlated-electron physics of the longstanding H-Tc-superconductivity problem using a non-perturbative method, the Dynamical Mean Field Theory (DMFT), capable to go beyond standard perturbation-theory techniques. DMFT is by construction a local theory which neglects spatial correlation. Experiments have however shown that the latter is a fundamental property of cuprate materials. In a first step, we approach the problem of spatial correlation in the normal state of cuprate materials using a phenomenological Fermi-Liquid-Boltzmann model. We then introduce and develop in detail an extension to DMFT, the Cellular Dynamical Mean Field Theory (CDMFT), capable of considering short-ranged spatial correlation in a system, and we implement it using the exact diagonalization algorithm . After benchmarking CDMFT with the exact one-dimensional solution of the Hubbard Model, we employ it to study the density-driven Mott metal-insulator transition in the two-dimensional Hubbard Model, focusing in particular on the anomalous properties of the doped normal state close to the Mott insulator. We finally study the superconducting state. We show that within CDMFT the one-band Hubbard Model supports a d-wave superconductive state, which strongly departs from the standard BCS theory. We conjecture a link between the instabilities found in the normal state and the onset of superconductivity.
cond-mat.str-el
in this thesis we study the stronglycorrelatedelectron physics of the longstanding htcsuperconductivity problem using a nonperturbative method the dynamical mean field theory dmft capable to go beyond standard perturbationtheory techniques dmft is by construction a local theory which neglects spatial correlation experiments have however shown that the latter is a fundamental property of cuprate materials in a first step we approach the problem of spatial correlation in the normal state of cuprate materials using a phenomenological fermiliquidboltzmann model we then introduce and develop in detail an extension to dmft the cellular dynamical mean field theory cdmft capable of considering shortranged spatial correlation in a system and we implement it using the exact diagonalization algorithm after benchmarking cdmft with the exact onedimensional solution of the hubbard model we employ it to study the densitydriven mott metalinsulator transition in the twodimensional hubbard model focusing in particular on the anomalous properties of the doped normal state close to the mott insulator we finally study the superconducting state we show that within cdmft the oneband hubbard model supports a dwave superconductive state which strongly departs from the standard bcs theory we conjecture a link between the instabilities found in the normal state and the onset of superconductivity
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710.2803
Observation of Leggett's collective mode in a multi-band MgB2 superconductor
We report observation of Leggett's collective mode in a multi-band MgB2 superconductor with T_c=39K arising from the fluctuations in the relative phase between two superconducting condensates. The novel mode is observed by Raman spectroscopy at 9.4 meV in the fully symmetric scattering channel. The observed mode frequency is consistent with theoretical considerations based on the first principle computations.
cond-mat.supr-con
we report observation of leggetts collective mode in a multiband mgb2 superconductor with t_c39k arising from the fluctuations in the relative phase between two superconducting condensates the novel mode is observed by raman spectroscopy at 94 mev in the fully symmetric scattering channel the observed mode frequency is consistent with theoretical considerations based on the first principle computations
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710.2804
Inelastic soliton processes generated by the perturbed KdV equation
Perturbations commonly added to the KdV equation contain terms that represent inelastic interac-tions among KdV solitons in multiple-soliton solutions. These terms trigger the emergence of new waves in the first-order correction to the solution of the perturbed equation. The new waves can represent soliton-anti-soliton creation, annihilation and scattering. Other possible waves represent soliton decay and production.
nlin.PS
perturbations commonly added to the kdv equation contain terms that represent inelastic interactions among kdv solitons in multiplesoliton solutions these terms trigger the emergence of new waves in the firstorder correction to the solution of the perturbed equation the new waves can represent solitonantisoliton creation annihilation and scattering other possible waves represent soliton decay and production
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710.2805
Nouvelle analyse des ph\'enom\`enes vibratoires en tournage
In the cutting process, machine-tools vibrations are generally a real problem when the amplitude crosses the limits of dimensional or surface quality workpiece precision required. It is necessary to develop models taking into account the three-dimensional vibratory approach to control the vibrations phenomena. An experimental study has been realized to understand the behavior of the cutting system and to identify its vibrations properties. The displacement's localization of the tool in a spatial plan, showed by the experimental results, allows us to simplify the three-dimensional dynamical model. In this study, the experimental approach is completely presented and the first points of the three dimensional vibratory model are proposed according to the experimental results.
physics.class-ph
in the cutting process machinetools vibrations are generally a real problem when the amplitude crosses the limits of dimensional or surface quality workpiece precision required it is necessary to develop models taking into account the threedimensional vibratory approach to control the vibrations phenomena an experimental study has been realized to understand the behavior of the cutting system and to identify its vibrations properties the displacements localization of the tool in a spatial plan showed by the experimental results allows us to simplify the threedimensional dynamical model in this study the experimental approach is completely presented and the first points of the three dimensional vibratory model are proposed according to the experimental results
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710.2806
Direct measurement of the coherence length of edge states in the Integer Quantum Hall Regime
We have determined the finite temperature coherence length of edge states in the Integer Quantum Hall Effect (IQHE) regime. This was realized by measuring the visibility of electronic Mach-Zehnder interferometers of different sizes, at filling factor 2. The visibility shows an exponential decay with the temperature. The characteristic temperature scale is found inversely proportional to the length of the interferometer arm, allowing to define a coherence length $\l_\phi$. The variations of $\l_\phi$ with magnetic field are the same for all samples, with a maximum located at the upper end of the quantum hall plateau. Our results provide the first accurate determination of $\l_\phi$ in the quantum Hall regime.
cond-mat.mes-hall
we have determined the finite temperature coherence length of edge states in the integer quantum hall effect iqhe regime this was realized by measuring the visibility of electronic machzehnder interferometers of different sizes at filling factor 2 the visibility shows an exponential decay with the temperature the characteristic temperature scale is found inversely proportional to the length of the interferometer arm allowing to define a coherence length l_phi the variations of l_phi with magnetic field are the same for all samples with a maximum located at the upper end of the quantum hall plateau our results provide the first accurate determination of l_phi in the quantum hall regime
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710.2807
Metal-rich debris discs around white dwarfs
We have identified two moderately hot (~18000-22000K) white dwarfs, SDSSJ1228+1040 and SDSSJ1043+0855, which exhibit double-peaked emission lines in the CaII 8600A triplet. These line profiles are unambiguous signatures of gaseous discs with outer radii of ~1Rsun orbiting the two white dwarfs. Both stars accrete from the circumstellar material, resulting in large photospheric Mg abundances. The absence of hydrogen emission from the discs, and helium absorption in the white dwarf photospheres demonstrates that the circumstellar material is depleted in volatile elements, and the most likely origin of these gaseous rings are tidally disrupted rocky asteroids. The relatively high mass of SDSSJ1228+1040 implies that planetary systems can not only form around 4-5Msun stars, but may also survive their post main-sequence evolution.
astro-ph
we have identified two moderately hot 1800022000k white dwarfs sdssj12281040 and sdssj10430855 which exhibit doublepeaked emission lines in the caii 8600a triplet these line profiles are unambiguous signatures of gaseous discs with outer radii of 1rsun orbiting the two white dwarfs both stars accrete from the circumstellar material resulting in large photospheric mg abundances the absence of hydrogen emission from the discs and helium absorption in the white dwarf photospheres demonstrates that the circumstellar material is depleted in volatile elements and the most likely origin of these gaseous rings are tidally disrupted rocky asteroids the relatively high mass of sdssj12281040 implies that planetary systems can not only form around 45msun stars but may also survive their post mainsequence evolution
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710.2808
Identification of specificity determining residues in enzymes using environment specific substitution tables
Environment specific substitution tables have been used effectively for distinguishing structural and functional constraints on proteins and thereby identify their active sites (Chelliah et al. (2004)). This work explores whether a similar approach can be used to identify specificity determining residues (SDRs) responsible for cofactor dependence, substrate specificity or subtle catalytic variations. We combine structure-sequence information and functional annotation from various data sources to create structural alignments for homologous enzymes and functional partitions therein. We develop a scoring procedure to predict SDRs and assess their accuracy using information from bound specific ligands and published literature.
q-bio.QM
environment specific substitution tables have been used effectively for distinguishing structural and functional constraints on proteins and thereby identify their active sites chelliah et al 2004 this work explores whether a similar approach can be used to identify specificity determining residues sdrs responsible for cofactor dependence substrate specificity or subtle catalytic variations we combine structuresequence information and functional annotation from various data sources to create structural alignments for homologous enzymes and functional partitions therein we develop a scoring procedure to predict sdrs and assess their accuracy using information from bound specific ligands and published literature
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710.2809
Rescuing H -> bb in VBF at the LHC by requiring a central photon
The LHC potential for a measurement of the Higgs boson coupling to the b quark in the standard model is not well established yet. We show that requiring a large transverse momentum photon in the light Higgs boson production via vector-boson fusion (with subsequent H->bb decay) could provide a further handle on the Hbb coupling determination, and on the measurement of the HWW coupling as well.
hep-ph
the lhc potential for a measurement of the higgs boson coupling to the b quark in the standard model is not well established yet we show that requiring a large transverse momentum photon in the light higgs boson production via vectorboson fusion with subsequent hbb decay could provide a further handle on the hbb coupling determination and on the measurement of the hww coupling as well
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710.281
A note on the mass splitting of K*(892)
Belle Collaboration reported a new observed value of K*-(892) mass by studying tau --> K_S pi nu_tau decay, which is significantly different from the current world average value given by Particle Data Group 2006. Motivated by this new data, we revisit the issue on the K*0(892)-K*+(892) mass splitting. Our theoretical estimation favors the new measurement by Belle Collaboration. Therefore further experimental efforts are urgently needed to improve our understanding of these issues.
hep-ph hep-ex
belle collaboration reported a new observed value of k892 mass by studying tau k_s pi nu_tau decay which is significantly different from the current world average value given by particle data group 2006 motivated by this new data we revisit the issue on the k0892k892 mass splitting our theoretical estimation favors the new measurement by belle collaboration therefore further experimental efforts are urgently needed to improve our understanding of these issues
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710.2811
Charge disproportionation and collinear magnetic order in the frustrated triangular antiferromagnet AgNiO2
We report a high-resolution neutron diffraction study of the crystal and magnetic structure of the orbitally-degenerate frustrated metallic magnet AgNiO2. At high temperatures the structure is hexagonal with a single crystallographic Ni site, low-spin Ni3+ with spin-1/2 and two-fold orbital degeneracy, arranged in an antiferromagnetic triangular lattice with frustrated spin and orbital order. A structural transition occurs upon cooling below 365 K to a tripled hexagonal unit cell containing three crystallographically-distinct Ni sites with expanded and contracted NiO6 octahedra, naturally explained by spontaneous charge order on the Ni triangular layers. No Jahn-Teller distortions occur, suggesting that charge order occurs in order to lift the orbital degeneracy. Symmetry analysis of the inferred Ni charge order pattern and the observed oxygen displacement pattern suggests that the transition could be mediated by charge fluctuations at the Ni sites coupled to a soft oxygen optical phonon breathing mode. At low temperatures the electron-rich Ni sublattice (assigned to a valence close to Ni2+ with S = 1) orders magnetically into a collinear stripe structure of ferromagnetic rows ordered antiferromagnetically in the triangular planes. We discuss the stability of this uncommon spin order pattern in the context of an easy-axis triangular antiferromagnet with additional weak second neighbor interactions and interlayer couplings.
cond-mat.str-el
we report a highresolution neutron diffraction study of the crystal and magnetic structure of the orbitallydegenerate frustrated metallic magnet agnio2 at high temperatures the structure is hexagonal with a single crystallographic ni site lowspin ni3 with spin12 and twofold orbital degeneracy arranged in an antiferromagnetic triangular lattice with frustrated spin and orbital order a structural transition occurs upon cooling below 365 k to a tripled hexagonal unit cell containing three crystallographicallydistinct ni sites with expanded and contracted nio6 octahedra naturally explained by spontaneous charge order on the ni triangular layers no jahnteller distortions occur suggesting that charge order occurs in order to lift the orbital degeneracy symmetry analysis of the inferred ni charge order pattern and the observed oxygen displacement pattern suggests that the transition could be mediated by charge fluctuations at the ni sites coupled to a soft oxygen optical phonon breathing mode at low temperatures the electronrich ni sublattice assigned to a valence close to ni2 with s 1 orders magnetically into a collinear stripe structure of ferromagnetic rows ordered antiferromagnetically in the triangular planes we discuss the stability of this uncommon spin order pattern in the context of an easyaxis triangular antiferromagnet with additional weak second neighbor interactions and interlayer couplings
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710.2812
Ultra-Broadband Radial Polarization Conversion based on Goos-Hanchen Shift
We demonstrate, for the first time, a scheme that generates radially-polarized light using Goos-Hanchen shift of a cylindrically symmetric Total Internal Reflection. It allows ultra-broadband radial polarization conversion for wavelengths differing >1 micron.
physics.optics
we demonstrate for the first time a scheme that generates radiallypolarized light using gooshanchen shift of a cylindrically symmetric total internal reflection it allows ultrabroadband radial polarization conversion for wavelengths differing 1 micron
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710.2813
A Search for Mid-Infrared Molecular Hydrogen Emission from Protoplanetary Disks
We observed the Herbig Ae/Be stars UX Ori, HD 34282, HD 100453, HD 101412, HD 104237 and HD 142666, and the T Tauri star HD 319139 and searched for H2 0-0 S(2) emission at 12.278 micron and H2 0-0 S(1) emission at 17.035 micron with VISIR, ESO-VLT's high-resolution MIR spectrograph. None of the sources present evidence for H2 emission. Stringent 3sigma upper limits to the integrated line fluxes and the mass of optically thin warm gas in the disks are derived. The disks contain less than a few tenths of Jupiter mass of optically thin H2 gas at 150 K at most, and less than a few Earth masses of optically thin H2 gas at 300 K and higher temperatures. We compare our results to a Chiang and Goldreich (1997, CG97) two-layer disk model. The upper limits to the disk's optically thin warm gas mass are smaller than the amount of warm gas in the interior layer of the disk, but they are much larger than the amount of molecular gas in the surface layer. We present a calculation of the expected thermal H2 emission from optically thick disks, assuming a CG97 disk structure, a gas-to-dust ratio of 100 and Tgas = Tdust. The expected H2 thermal emission fluxes from typical disks around Herbig Ae/Be stars (10^-16 to 10^-17 erg/s/cm2 at 140 pc) are much lower than the detection limits of our observations (5*10^-15 erg/s/cm2). H2 emission levels are very sensitive to departures from the thermal coupling between the molecular gas and dust. Additional sources of heating of gas in the disk's surface layer could have a major impact on the expected H2 disk emission. In the observed sources the molecular gas and dust in the surface layer have not significantly departed from thermal coupling (Tgas/Tdust< 2) and that the gas-to-dust ratio in the surface layer is very likely lower than 1000.
astro-ph
we observed the herbig aebe stars ux ori hd 34282 hd 100453 hd 101412 hd 104237 and hd 142666 and the t tauri star hd 319139 and searched for h2 00 s2 emission at 12278 micron and h2 00 s1 emission at 17035 micron with visir esovlts highresolution mir spectrograph none of the sources present evidence for h2 emission stringent 3sigma upper limits to the integrated line fluxes and the mass of optically thin warm gas in the disks are derived the disks contain less than a few tenths of jupiter mass of optically thin h2 gas at 150 k at most and less than a few earth masses of optically thin h2 gas at 300 k and higher temperatures we compare our results to a chiang and goldreich 1997 cg97 twolayer disk model the upper limits to the disks optically thin warm gas mass are smaller than the amount of warm gas in the interior layer of the disk but they are much larger than the amount of molecular gas in the surface layer we present a calculation of the expected thermal h2 emission from optically thick disks assuming a cg97 disk structure a gastodust ratio of 100 and tgas tdust the expected h2 thermal emission fluxes from typical disks around herbig aebe stars 1016 to 1017 ergscm2 at 140 pc are much lower than the detection limits of our observations 51015 ergscm2 h2 emission levels are very sensitive to departures from the thermal coupling between the molecular gas and dust additional sources of heating of gas in the disks surface layer could have a major impact on the expected h2 disk emission in the observed sources the molecular gas and dust in the surface layer have not significantly departed from thermal coupling tgastdust 2 and that the gastodust ratio in the surface layer is very likely lower than 1000
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710.2814
CO abundances in a protostellar cloud: freeze-out and desorption in the envelope and outflow of L483
CO isotopes are able to probe the different components in protostellar clouds. These components, core, envelope and outflow have distinct physical conditions and sometimes more than one component contributes to the observed line profile. In this study we determine how CO isotope abundances are altered by the physical conditions in the different components. We use a 3D molecular line transport code to simulate the emission of four CO isotopomers, 12CO J=2-1, 13CO J=2-1, C18O J=2-1 and C17O J=2-1 from the Class 0/1 object L483, which contains a cold quiescent core, an infalling envelope and a clear outflow. Our models replicate JCMT (James Clerk Maxwell Telescope) line observations with the inclusion of freeze-out, a density profile and infall. Our model profiles of 12CO and 13CO have a large linewidth due to a high velocity jet. These profiles replicate the process of more abundant material being susceptible to a jet. C18O and C17O do not display such a large linewidth as they trace denser quiescent material deep in the cloud.
astro-ph
co isotopes are able to probe the different components in protostellar clouds these components core envelope and outflow have distinct physical conditions and sometimes more than one component contributes to the observed line profile in this study we determine how co isotope abundances are altered by the physical conditions in the different components we use a 3d molecular line transport code to simulate the emission of four co isotopomers 12co j21 13co j21 c18o j21 and c17o j21 from the class 01 object l483 which contains a cold quiescent core an infalling envelope and a clear outflow our models replicate jcmt james clerk maxwell telescope line observations with the inclusion of freezeout a density profile and infall our model profiles of 12co and 13co have a large linewidth due to a high velocity jet these profiles replicate the process of more abundant material being susceptible to a jet c18o and c17o do not display such a large linewidth as they trace denser quiescent material deep in the cloud
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710.2815
Optical emission from massive donors in ULX binary systems
We present evolutionary tracks of binary systems with high mass companion stars and stellar-through-intermediate mass BHs. Using Eggleton's stellar evolution code, we compute the luminosity produced by accretion from the donor during its entire evolution. We compute also the evolution of the optical spectrum of the binary system taking the disc contribution and irradiation effects into account. The calculations presented here can be used to constrain the properties of the donor stars in Ultraluminous X-ray Sources by comparing their position on the HR or color-magnitude diagrams with the evolutionary tracks of massive BH binaries. This approach may actually provide interesting clues also on the properties of the binary system itself, including the BH mass. We found that, on the basis of their position on the color-magnitude diagram, some of the candidate counterparts considered can be ruled out and more stringent constraints can be applied to the donor masses.
astro-ph
we present evolutionary tracks of binary systems with high mass companion stars and stellarthroughintermediate mass bhs using eggletons stellar evolution code we compute the luminosity produced by accretion from the donor during its entire evolution we compute also the evolution of the optical spectrum of the binary system taking the disc contribution and irradiation effects into account the calculations presented here can be used to constrain the properties of the donor stars in ultraluminous xray sources by comparing their position on the hr or colormagnitude diagrams with the evolutionary tracks of massive bh binaries this approach may actually provide interesting clues also on the properties of the binary system itself including the bh mass we found that on the basis of their position on the colormagnitude diagram some of the candidate counterparts considered can be ruled out and more stringent constraints can be applied to the donor masses
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710.2816
A classification of some Finsler connections and their applications
Some general Finsler connections are defined. Emphasis is being made on the Cartan tensor and its derivatives. Vanishing of the hv-curvature tensors of these connections characterizes Landsbergian, Berwaldian as well as Riemannian structures. This view point makes it possible to give a smart representation of connection theory in Finsler geometry and yields to a classification of Finsler connections. Some practical applications of these connections are also considered.
math.DG
some general finsler connections are defined emphasis is being made on the cartan tensor and its derivatives vanishing of the hvcurvature tensors of these connections characterizes landsbergian berwaldian as well as riemannian structures this view point makes it possible to give a smart representation of connection theory in finsler geometry and yields to a classification of finsler connections some practical applications of these connections are also considered
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710.2817
Progress in the evaluation of the anti-B -> X_s gamma decay rate at NNLO
The theoretical status of NNLO QCD corrections to the inclusive radiative anti-B -> X_s gamma decay in the standard model is briefly overviewed. Emphasis is put on recent results for three-loop fermionic corrections to matrix elements of the most relevant four-quark operators.
hep-ph
the theoretical status of nnlo qcd corrections to the inclusive radiative antib x_s gamma decay in the standard model is briefly overviewed emphasis is put on recent results for threeloop fermionic corrections to matrix elements of the most relevant fourquark operators
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710.2818
Track finding in gamma conversions in CMS
A track finding algorithm has been developed for reconstruction of e+e- pairs. It combines the information of the electromagnetic calorimeter with the information provided by the Tracker. Results on reconstruction efficiency of converted photons, as well as on fake rate are shown for single isolated photons and for photons from H->gamma gamma events with pile-up events at 10^33 cm^-2 s^-1 LHC luminosity.
physics.data-an hep-ex
a track finding algorithm has been developed for reconstruction of ee pairs it combines the information of the electromagnetic calorimeter with the information provided by the tracker results on reconstruction efficiency of converted photons as well as on fake rate are shown for single isolated photons and for photons from hgamma gamma events with pileup events at 1033 cm2 s1 lhc luminosity
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710.2819
Fractional diffusion equation for aging and equilibrated random walks
We consider continuous time random walks (CTRW) and discuss situations pertinent to aging. These correspond to the case when the initial state of the system is known not at preparation (at $t=0$) but at the later instant of time $t_1>0$ (intermediate-time initial condition). We derive the generalized aging diffusion equation for this case and express it through a single memory kernel. The results obtained are applied to the practically relevant case of the equilibrated random walks. We moreover discuss some subtleties in the setup of the aging subdiffusion problem and show that the behavior of the system depends on what was taken as the intermediate-time initial condition: whether it was coordinate of one particle given by measurement or the whole probability distribution. The two setups lead to different predictions for the evolution of a system. This fact stresses the necessity of a precise definition of aging statistical ensembles.
cond-mat.stat-mech
we consider continuous time random walks ctrw and discuss situations pertinent to aging these correspond to the case when the initial state of the system is known not at preparation at t0 but at the later instant of time t_10 intermediatetime initial condition we derive the generalized aging diffusion equation for this case and express it through a single memory kernel the results obtained are applied to the practically relevant case of the equilibrated random walks we moreover discuss some subtleties in the setup of the aging subdiffusion problem and show that the behavior of the system depends on what was taken as the intermediatetime initial condition whether it was coordinate of one particle given by measurement or the whole probability distribution the two setups lead to different predictions for the evolution of a system this fact stresses the necessity of a precise definition of aging statistical ensembles
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710.282
Resonant mode flopping in modulated waveguiding structures
We put forward the concept of resonant, Rabi-like flopping and adiabatic transitions between confined light modes in properly modulated multimode waveguides. The phenomenon is shown to take place in both, the linear and the nonlinear regimes. In addition, we find that the mode transitions occur not only in simple geometries, but also in complex confining multimode structures. The phenomenon is analogous to the familiar stimulated state transitions that occur in multilevel quantum systems.
physics.optics nlin.PS
we put forward the concept of resonant rabilike flopping and adiabatic transitions between confined light modes in properly modulated multimode waveguides the phenomenon is shown to take place in both the linear and the nonlinear regimes in addition we find that the mode transitions occur not only in simple geometries but also in complex confining multimode structures the phenomenon is analogous to the familiar stimulated state transitions that occur in multilevel quantum systems
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710.2821
First Stiefel-Whitney class of real moduli spaces of stable maps to a convex surface
Let $(X,c_X)$ be a convex projective surface equipped with a real structure. The space of stable maps $\bar{\mathcal{M}}_{0,k}(X,d)$ carries different real structures induced by $c_X$ and any order two element $\tau$ of permutation group $S_k$ acting on marked points. Each corresponding real part $\R_{\tau}\bar{\mathcal{M}}_{0,k}(X,d)$ is a real normal projective variety. As the singular locus is of codimension bigger than two, these spaces thus carry a first Stiefel-Whitney class for which we determine a representative in the case $k=c_1(X)d-1$ where $c_1(X)$ is the first Chern class of $X$. Namely, we give a homological description of these classes in term of the real part of boundary divisors of the space of stable maps.
math.AG math.AT
let xc_x be a convex projective surface equipped with a real structure the space of stable maps barmathcalm_0kxd carries different real structures induced by c_x and any order two element tau of permutation group s_k acting on marked points each corresponding real part r_taubarmathcalm_0kxd is a real normal projective variety as the singular locus is of codimension bigger than two these spaces thus carry a first stiefelwhitney class for which we determine a representative in the case kc_1xd1 where c_1x is the first chern class of x namely we give a homological description of these classes in term of the real part of boundary divisors of the space of stable maps
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710.2822
SFitter: Reconstructing the MSSM Lagrangian from LHC data
Once supersymmetry is found at the LHC, the question arises what are the fundamental parameters of the Lagrangian. The answer to this question should thereby not be biased by assumptions on high-scale models. SFitter is a tool designed for this task. Taking LHC (and possibly ILC) data as input it scans the TeV-scale MSSM parameter space using its new weighted Markov chain technique. Using this scan it determines a list of best-fitting parameter points. Additionally a log-likelihood map is calculated, which can be reduced to lower-dimensional Frequentist's profile likelihoods or Bayesian probability maps.
hep-ph
once supersymmetry is found at the lhc the question arises what are the fundamental parameters of the lagrangian the answer to this question should thereby not be biased by assumptions on highscale models sfitter is a tool designed for this task taking lhc and possibly ilc data as input it scans the tevscale mssm parameter space using its new weighted markov chain technique using this scan it determines a list of bestfitting parameter points additionally a loglikelihood map is calculated which can be reduced to lowerdimensional frequentists profile likelihoods or bayesian probability maps
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710.2823
On the Whitehead spectrum of the circle
The seminal work of Waldhausen, Farrell and Jones, Igusa, and Weiss and Williams shows that the homotopy groups in low degrees of the space of homeomorphisms of a closed Riemannian manifold of negative sectional curvature can be expressed as a functor of the fundamental group of the manifold. To determine this functor, however, it remains to determine the homotopy groups of the topological Whitehead spectrum of the circle. The cyclotomic trace of B okstedt, Hsiang, and Madsen and a theorem of Dundas, in turn, lead to an expression for these homotopy groups in terms of the equivariant homotopy groups of the homotopy fiber of the map from the topological Hochschild T-spectrum of the sphere spectrum to that of the ring of integers induced by the Hurewicz map. We evaluate the latter homotopy groups, and hence, the homotopy groups of the topological Whitehead spectrum of the circle in low degrees. The result extends earlier work by Anderson and Hsiang and by Igusa and complements recent work by Grunewald, Klein, and Macko.
math.AT math.KT
the seminal work of waldhausen farrell and jones igusa and weiss and williams shows that the homotopy groups in low degrees of the space of homeomorphisms of a closed riemannian manifold of negative sectional curvature can be expressed as a functor of the fundamental group of the manifold to determine this functor however it remains to determine the homotopy groups of the topological whitehead spectrum of the circle the cyclotomic trace of b okstedt hsiang and madsen and a theorem of dundas in turn lead to an expression for these homotopy groups in terms of the equivariant homotopy groups of the homotopy fiber of the map from the topological hochschild tspectrum of the sphere spectrum to that of the ring of integers induced by the hurewicz map we evaluate the latter homotopy groups and hence the homotopy groups of the topological whitehead spectrum of the circle in low degrees the result extends earlier work by anderson and hsiang and by igusa and complements recent work by grunewald klein and macko
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710.2824
Polarization Retarder with Cylindrical-Symmetry for Radially Polarized Light
We demonstrate a cylindrically-symmetric polarization retarder for generating exact radially polarized light. It involves an uni-axial crystal whose crystallographic optics axis is aligned to its optical axis. This method offers high power-handling capability
physics.optics
we demonstrate a cylindricallysymmetric polarization retarder for generating exact radially polarized light it involves an uniaxial crystal whose crystallographic optics axis is aligned to its optical axis this method offers high powerhandling capability
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710.2825
Spatially extended PAHs in circumstellar disks around T Tauri and Herbig Ae stars
Our aim is to determine the presence and location of the emission from polycyclic aromatic hydrocarbons (PAHs) towards low and intermediate mass young stars with disks using large aperture telescopes. VLT-VISIR N-band spectra and VLT-ISAAC and VLT-NACO L-band spectra of 29 sources are presented, spectrally resolving the 3.3, 8.6, 11.2, and 12.6 micron PAH features. Spatial-extent profiles of the features and the continuum emission are derived and used to associate the PAH emission with the disks. The results are discussed in the context of recent PAH-emission disk models. The 3.3, 8.6, and 11.2 micron PAH features are detected toward a small fraction of the T Tauri stars, with typical upper limits between 1E-15 and 5E-17 W/m^2. All 11.2 micron detections from a previous Spitzer survey are confirmed with (tentative) 3.3 micron detections, and both the 8.6 and the 11.2 micron features are detected in all PAH sources. For 6 detections, the spatial extent of the PAH features is confined to scales typically smaller than 0.12-0.34'', consistent with the radii of 12-60 AU disks at their distances (typically 150 pc). For 3 additional sources, WL 16, HD 100546, and TY CrA, one or more of the PAH features are more extended than the hot dust continuum of the disk, whereas for Oph IRS 48, the size of the resolved PAH emission is confirmed as smaller than for the large grains. For HD 100546, the 3.3 micron emission is confined to a small radial extent of 12 +- 3 AU, most likely associated with the outer rim of the gap in this disk. Gaps with radii out to 10-30 AU may also affect the observed PAH extent for other sources. For both Herbig Ae and T Tauri stars, the small measured extents of the 8.6 and 11.2 micron features are consistent with larger (>= 100 carbon atoms) PAHs.
astro-ph
our aim is to determine the presence and location of the emission from polycyclic aromatic hydrocarbons pahs towards low and intermediate mass young stars with disks using large aperture telescopes vltvisir nband spectra and vltisaac and vltnaco lband spectra of 29 sources are presented spectrally resolving the 33 86 112 and 126 micron pah features spatialextent profiles of the features and the continuum emission are derived and used to associate the pah emission with the disks the results are discussed in the context of recent pahemission disk models the 33 86 and 112 micron pah features are detected toward a small fraction of the t tauri stars with typical upper limits between 1e15 and 5e17 wm2 all 112 micron detections from a previous spitzer survey are confirmed with tentative 33 micron detections and both the 86 and the 112 micron features are detected in all pah sources for 6 detections the spatial extent of the pah features is confined to scales typically smaller than 012034 consistent with the radii of 1260 au disks at their distances typically 150 pc for 3 additional sources wl 16 hd 100546 and ty cra one or more of the pah features are more extended than the hot dust continuum of the disk whereas for oph irs 48 the size of the resolved pah emission is confirmed as smaller than for the large grains for hd 100546 the 33 micron emission is confined to a small radial extent of 12 3 au most likely associated with the outer rim of the gap in this disk gaps with radii out to 1030 au may also affect the observed pah extent for other sources for both herbig ae and t tauri stars the small measured extents of the 86 and 112 micron features are consistent with larger 100 carbon atoms pahs
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710.2826
Ferromagnetic resonance study of polycrystalline Fe_{1-x}V_x alloy thin films
Ferromagnetic resonance has been used to study the magnetic properties and magnetization dynamics of polycrystalline Fe$_{1-x}$V$_{x}$ alloy films with $0\leq x < 0.7$. Films were produced by co-sputtering from separate Fe and V targets, leading to a composition gradient across a Si substrate. FMR studies were conducted at room temperature with a broadband coplanar waveguide at frequencies up to 50 GHz using the flip-chip method. The effective demagnetization field $4 \pi M_{\mathrm{eff}}$ and the Gilbert damping parameter $\alpha$ have been determined as a function of V concentration. The results are compared to those of epitaxial FeV films.
cond-mat.mes-hall cond-mat.mtrl-sci
ferromagnetic resonance has been used to study the magnetic properties and magnetization dynamics of polycrystalline fe_1xv_x alloy films with 0leq x 07 films were produced by cosputtering from separate fe and v targets leading to a composition gradient across a si substrate fmr studies were conducted at room temperature with a broadband coplanar waveguide at frequencies up to 50 ghz using the flipchip method the effective demagnetization field 4 pi m_mathrmeff and the gilbert damping parameter alpha have been determined as a function of v concentration the results are compared to those of epitaxial fev films
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710.2827
A high fidelity approximation of radial polarization conversion
We report a high fidelity (>90%) approximation of radial polarization conversion using a birefringent lens. It offers the advantages of low-cost, easy fabrication, alignment robustness and high laser power handling capability.
physics.optics
we report a high fidelity 90 approximation of radial polarization conversion using a birefringent lens it offers the advantages of lowcost easy fabrication alignment robustness and high laser power handling capability
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710.2828
Fermionic representation for the ferromagnetic Kondo lattice model -- diagrammatic study of spin-charge coupling effects on magnon excitations
A purely fermionic representation is introduced for the ferromagnetic Kondo lattice model which allows conventional diagrammatic tools to be employed to study correlation effects. Quantum 1/S corrections to magnon excitations are investigated using a systematic inverse-degeneracy expansion scheme which incorporates correlation effects in the form of self-energy and vertex corrections, while explicitly preserving the continuous spin-rotation symmetry. Magnon self-energy is studied in the full range of interaction strength, and shown to result in strong magnon damping and anomalous softening for zone boundary modes, which accounts for several zone-boundary anomalies observed in recent spin-wave measurements of ferromagnetic manganites.
cond-mat.str-el
a purely fermionic representation is introduced for the ferromagnetic kondo lattice model which allows conventional diagrammatic tools to be employed to study correlation effects quantum 1s corrections to magnon excitations are investigated using a systematic inversedegeneracy expansion scheme which incorporates correlation effects in the form of selfenergy and vertex corrections while explicitly preserving the continuous spinrotation symmetry magnon selfenergy is studied in the full range of interaction strength and shown to result in strong magnon damping and anomalous softening for zone boundary modes which accounts for several zoneboundary anomalies observed in recent spinwave measurements of ferromagnetic manganites
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710.2829
Nonequilibrium critical dynamics of the two-dimensional Ising model quenched from a correlated initial state
The universality class, even the order of the transition, of the two-dimensional Ising model depends on the range and the symmetry of the interactions (Onsager model, Baxter-Wu model, Turban model, etc.), but the critical temperature is generally the same due to self-duality. Here we consider a sudden change in the form of the interaction and study the nonequilibrium critical dynamical properties of the nearest-neighbor model. The relaxation of the magnetization and the decay of the autocorrelation function are found to display a power law behavior with characteristic exponents that depend on the universality class of the initial state.
cond-mat.stat-mech
the universality class even the order of the transition of the twodimensional ising model depends on the range and the symmetry of the interactions onsager model baxterwu model turban model etc but the critical temperature is generally the same due to selfduality here we consider a sudden change in the form of the interaction and study the nonequilibrium critical dynamical properties of the nearestneighbor model the relaxation of the magnetization and the decay of the autocorrelation function are found to display a power law behavior with characteristic exponents that depend on the universality class of the initial state
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710.283
Precision extraction of a_nn from pi- d --> n n gamma using chiral perturbation theory
The neutron-neutron scattering length a_nn provides a sensitive probe of charge-symmetry breaking in the strong interaction. Here we summarize our recent efforts to use chiral perturbation theory in order to systematically relate a_nn to the shape of the neutron spectrum in the reaction pi- d --> n n gamma. In particular we show how the chiral symmetry of QCD relates this process to low-energy electroweak reactions such as p p --> d e+ nu_e. This allows us to reduce the uncertainty in the extracted a_nn (mainly due to short-distance physics in the two-nucleon system) by a factor of more than three, to <0.05 fm. We also report first results on the impact that two-nucleon mechanisms of chiral order P^4 have on the pi- d --> n n gamma neutron spectrum.
nucl-th hep-ph
the neutronneutron scattering length a_nn provides a sensitive probe of chargesymmetry breaking in the strong interaction here we summarize our recent efforts to use chiral perturbation theory in order to systematically relate a_nn to the shape of the neutron spectrum in the reaction pi d n n gamma in particular we show how the chiral symmetry of qcd relates this process to lowenergy electroweak reactions such as p p d e nu_e this allows us to reduce the uncertainty in the extracted a_nn mainly due to shortdistance physics in the twonucleon system by a factor of more than three to 005 fm we also report first results on the impact that twonucleon mechanisms of chiral order p4 have on the pi d n n gamma neutron spectrum
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710.2831
Quantum dynamics in phase space: From coherent states to the Gaussian representation
We give an outlook on the future of coherence theory and many-body quantum dynamics as experiments develop in the arena of ultra-cold atoms. Novel results on quantum heating of center-of-mass temperature in evaporative cooling and simulation methods for long-range interactions are obtained, using positive-P phase-space techniques.
cond-mat.other cond-mat.stat-mech
we give an outlook on the future of coherence theory and manybody quantum dynamics as experiments develop in the arena of ultracold atoms novel results on quantum heating of centerofmass temperature in evaporative cooling and simulation methods for longrange interactions are obtained using positivep phasespace techniques
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710.2832
Schr\"odinger operator with periodic plus compactly supported potentials on the half-line
We consider the Schr\"odinger operator $H$ with a periodic potential $p$ plus a compactly supported potential $q$ on the half-line. We prove the following results: 1) a forbidden domain for the resonances is specified, 2) asymptotics of the resonance-counting function is determined, 3) in each nondegenerate gap $\g_n$ for $n$ large enough there is exactly an eigenvalue or an antibound state, 4) the asymptotics of eigenvalues and antibound states are determined at high energy, 5) the number of eigenvalues plus antibound states is odd $\ge 1$ in each gap, 6) between any two eigenvalues there is an odd number $\ge 1$ of antibound states, 7) for any potential $q$ and for any sequences $(\s_n)_{1}^\iy, \s_n\in \{0,1\}$ and $(\vk_n)_1^\iy\in \ell^2, \vk_n\ge 0$, there exists a potential $p$ such that each gap length $|\g_n|=\vk_n, n\ge 1$ and $H$ has exactly $\s_n$ eigenvalues and $1-\s_n$ antibound state in each gap $\g_n\ne \es$ for $n$ large enough, 8) if unperturbed operator (at $q=0$) has infinitely many virtual states, then for any sequence $(\s)_1^\iy, \s_n\in \{0,1\}$, there exists a potential $q$ such that $H$ has $\s_n$ bound states and $1-\s_n$ antibound states in each gap open $\g_n$ for $n$ large enough.
math-ph math.MP
we consider the schrodinger operator h with a periodic potential p plus a compactly supported potential q on the halfline we prove the following results 1 a forbidden domain for the resonances is specified 2 asymptotics of the resonancecounting function is determined 3 in each nondegenerate gap g_n for n large enough there is exactly an eigenvalue or an antibound state 4 the asymptotics of eigenvalues and antibound states are determined at high energy 5 the number of eigenvalues plus antibound states is odd ge 1 in each gap 6 between any two eigenvalues there is an odd number ge 1 of antibound states 7 for any potential q and for any sequences s_n_1iy s_nin 01 and vk_n_1iyin ell2 vk_nge 0 there exists a potential p such that each gap length g_nvk_n nge 1 and h has exactly s_n eigenvalues and 1s_n antibound state in each gap g_nne es for n large enough 8 if unperturbed operator at q0 has infinitely many virtual states then for any sequence s_1iy s_nin 01 there exists a potential q such that h has s_n bound states and 1s_n antibound states in each gap open g_n for n large enough
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710.2833
Marchenko-Ostrovski mappings for periodic Jacobi matrices
We consider the 1D periodic Jacobi matrices. The spectrum of this operator is purely absolutely continuous and consists of intervals separated by gaps. We solve the inverse problem (including characterization) in terms of vertical slits on the quasimomentum domain . Furthermore, we obtain a priori two-sided estimates for vertical slits in terms of Jacoby matrices.
math-ph math.MP math.SP
we consider the 1d periodic jacobi matrices the spectrum of this operator is purely absolutely continuous and consists of intervals separated by gaps we solve the inverse problem including characterization in terms of vertical slits on the quasimomentum domain furthermore we obtain a priori twosided estimates for vertical slits in terms of jacoby matrices
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710.2834
Fermion masses and neutrino mixing in an U(1)_H flavor symmetry model with hierarchical radiative generation for light charged fermion masses
I report the analysis performed on fermion masses and mixing, including neutrino mixing, within the context of a model with hierarchical radiative mass generation mechanism for light charged fermions, mediated by exotic scalar particles at one and two loops, respectively, meanwhile the neutrinos get Majorana mass terms at tree level through the Yukawa couplings with two SU(2)_L Higgs triplets. All the resulting mass matrices in the model, for the u, d, and e fermion charged sectors, the neutrinos and the exotic scalar particles, are diagonalized in exact analytical form. Quantitative analysis shows that this model is successful to accommodate the hierarchical spectrum of masses and mixing in the quark sector as well as the charged lepton masses. The lepton mixing matrix, V_{PMNS}, is written completely in terms of the neutrino masses m_1, m_2, and m_3. Large lepton mixing for \theta_{12} and \theta_{23} is predicted in the range of values 0.7 \lesssim \sin^22\theta_{12}\lesssim 0.7772 and 0.87 \lesssim \sin^22\theta_{23} \lesssim 0.9023 by using 0.033 \lesssim s_{13}^2 \lesssim 0.04. These values for lepton mixing are consistent with 3 \sigma allowed ranges provided by recent global analysis of neutrino data oscillation. From \Delta m_{\text{sol}}^2 bounds, neutrino masses are predicted in the range of values m_1 \thickapprox (1.706 - 2.494) x 10^{- 3} eV, m_2 \thickapprox (6.675 - 12.56) x 10^{- 3} eV, and m_3 \thickapprox (1.215 - 2.188) x 10^{- 2} eV, respectively. The above allowed lepton mixing leads to the quak-lepton complementary relations \theta_{12}^{CKM} + \theta_{12}^{PMNS} \thickapprox 41.543^{\circ} - 44.066^{\circ} and \theta_{23}^{CKM}+\theta_{23}^{PMNS}\thickapprox 36.835^{\circ} - 38.295^{\circ}.
hep-ph
i report the analysis performed on fermion masses and mixing including neutrino mixing within the context of a model with hierarchical radiative mass generation mechanism for light charged fermions mediated by exotic scalar particles at one and two loops respectively meanwhile the neutrinos get majorana mass terms at tree level through the yukawa couplings with two su2_l higgs triplets all the resulting mass matrices in the model for the u d and e fermion charged sectors the neutrinos and the exotic scalar particles are diagonalized in exact analytical form quantitative analysis shows that this model is successful to accommodate the hierarchical spectrum of masses and mixing in the quark sector as well as the charged lepton masses the lepton mixing matrix v_pmns is written completely in terms of the neutrino masses m_1 m_2 and m_3 large lepton mixing for theta_12 and theta_23 is predicted in the range of values 07 lesssim sin22theta_12lesssim 07772 and 087 lesssim sin22theta_23 lesssim 09023 by using 0033 lesssim s_132 lesssim 004 these values for lepton mixing are consistent with 3 sigma allowed ranges provided by recent global analysis of neutrino data oscillation from delta m_textsol2 bounds neutrino masses are predicted in the range of values m_1 thickapprox 1706 2494 x 10 3 ev m_2 thickapprox 6675 1256 x 10 3 ev and m_3 thickapprox 1215 2188 x 10 2 ev respectively the above allowed lepton mixing leads to the quaklepton complementary relations theta_12ckm theta_12pmns thickapprox 41543circ 44066circ and theta_23ckmtheta_23pmnsthickapprox 36835circ 38295circ
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710.2835
Folksonomies and clustering in the collaborative system CiteULike
We analyze CiteULike, an online collaborative tagging system where users bookmark and annotate scientific papers. Such a system can be naturally represented as a tripartite graph whose nodes represent papers, users and tags connected by individual tag assignments. The semantics of tags is studied here, in order to uncover the hidden relationships between tags. We find that the clustering coefficient reflects the semantical patterns among tags, providing useful ideas for the designing of more efficient methods of data classification and spam detection.
physics.soc-ph physics.data-an
we analyze citeulike an online collaborative tagging system where users bookmark and annotate scientific papers such a system can be naturally represented as a tripartite graph whose nodes represent papers users and tags connected by individual tag assignments the semantics of tags is studied here in order to uncover the hidden relationships between tags we find that the clustering coefficient reflects the semantical patterns among tags providing useful ideas for the designing of more efficient methods of data classification and spam detection
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710.2836
Topological entropies of equivalent smooth flows
Two flows defined on a smooth manifold are equivalent if there exists a homeomorphism of the manifold that sends each orbit of one flow onto an orbit of the other flow while preserving the time orientation. The topological entropy of a flow is defined as the entropy of its time-1 map. While topological entropy is an invariant for equivalent homeomorphisms, finite non-zero topological entropy for a flow cannot be an invariant because its value is affected by time reparameterization. However, 0 and $\infty$ topological entropy are invariants for equivalent flows without fixed points. In equivalent flows with fixed points there exists a counterexample, constructed by Ohno, showing that neither 0 nor $\infty$ topological entropy is preserved by equivalence. The two flows constructed by Ohno are suspensions of a transitive subshift and thus are not differentiable. Note that a differentiable flow on a compact manifold cannot have $\infty$ entropy. These facts led Ohno in 1980 to ask the following: "Is 0 topological entropy an invariant for equivalent differentiable flows?" In this paper, we construct two equivalent $C^\infty$ smooth flows with a singularity, one of which has positive topological entropy while the other has zero topological entropy. This gives a negative answer to Ohno's question in the class $C^\infty$.
math.DS
two flows defined on a smooth manifold are equivalent if there exists a homeomorphism of the manifold that sends each orbit of one flow onto an orbit of the other flow while preserving the time orientation the topological entropy of a flow is defined as the entropy of its time1 map while topological entropy is an invariant for equivalent homeomorphisms finite nonzero topological entropy for a flow cannot be an invariant because its value is affected by time reparameterization however 0 and infty topological entropy are invariants for equivalent flows without fixed points in equivalent flows with fixed points there exists a counterexample constructed by ohno showing that neither 0 nor infty topological entropy is preserved by equivalence the two flows constructed by ohno are suspensions of a transitive subshift and thus are not differentiable note that a differentiable flow on a compact manifold cannot have infty entropy these facts led ohno in 1980 to ask the following is 0 topological entropy an invariant for equivalent differentiable flows in this paper we construct two equivalent cinfty smooth flows with a singularity one of which has positive topological entropy while the other has zero topological entropy this gives a negative answer to ohnos question in the class cinfty
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710.2837
Overhauser effect in individual InP/GaInP dots
Sizable nuclear spin polarization is pumped in individual InP/GaInP dots in a wide range of external magnetic fields B_ext=0-5T by circularly polarized optical excitation. We observe nuclear polarization of up to ~40% at Bext=1.5T and corresponding to an Overhauser field of ~1.2T. We find a strong feedback of the nuclear spin on the spin pumping efficiency. This feedback, produced by the Overhauser field, leads to nuclear spin bi-stability at low magnetic fields of Bext=0.5-1.5T. We find that the exciton Zeeman energy increases markedly, when the Overhauser field cancels the external field. This counter-intuitive result is shown to arise from the opposite contribution of the electron and hole Zeeman splittings to the total exciton Zeeman energy.
cond-mat.mes-hall cond-mat.mtrl-sci
sizable nuclear spin polarization is pumped in individual inpgainp dots in a wide range of external magnetic fields b_ext05t by circularly polarized optical excitation we observe nuclear polarization of up to 40 at bext15t and corresponding to an overhauser field of 12t we find a strong feedback of the nuclear spin on the spin pumping efficiency this feedback produced by the overhauser field leads to nuclear spin bistability at low magnetic fields of bext0515t we find that the exciton zeeman energy increases markedly when the overhauser field cancels the external field this counterintuitive result is shown to arise from the opposite contribution of the electron and hole zeeman splittings to the total exciton zeeman energy
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710.2838
Experimental Precision Tests for the Electroweak Standard Model
This paper contains a review of recent precision measurements of electroweak observables and resulting tests of the electroweak Standard Model.
hep-ex
this paper contains a review of recent precision measurements of electroweak observables and resulting tests of the electroweak standard model
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710.2839
Magnetic field evolution in neutron stars
Neutron stars contain persistent, ordered magnetic fields that are the strongest known in the Universe. However, their magnetic fluxes are similar to those in magnetic A and B stars and white dwarfs, suggesting that flux conservation during gravitational collapse may play an important role in establishing the field, although it might also be modified substantially by early convection, differential rotation, and magnetic instabilities. The equilibrium field configuration, established within hours (at most) of the formation of the star, is likely to be roughly axisymmetric, involving both poloidal and toroidal components. The stable stratification of the neutron star matter (due to its radial composition gradient) probably plays a crucial role in holding this magnetic structure inside the star. The field can evolve on long time scales by processes that overcome the stable stratification, such as weak interactions changing the relative abundances and ambipolar diffusion of charged particles with respect to neutrons. These processes become more effective for stronger magnetic fields, thus naturally explaining the magnetic energy dissipation expected in magnetars, at the same time as the longer-lived, weaker fields in classical and millisecond pulsars.
astro-ph
neutron stars contain persistent ordered magnetic fields that are the strongest known in the universe however their magnetic fluxes are similar to those in magnetic a and b stars and white dwarfs suggesting that flux conservation during gravitational collapse may play an important role in establishing the field although it might also be modified substantially by early convection differential rotation and magnetic instabilities the equilibrium field configuration established within hours at most of the formation of the star is likely to be roughly axisymmetric involving both poloidal and toroidal components the stable stratification of the neutron star matter due to its radial composition gradient probably plays a crucial role in holding this magnetic structure inside the star the field can evolve on long time scales by processes that overcome the stable stratification such as weak interactions changing the relative abundances and ambipolar diffusion of charged particles with respect to neutrons these processes become more effective for stronger magnetic fields thus naturally explaining the magnetic energy dissipation expected in magnetars at the same time as the longerlived weaker fields in classical and millisecond pulsars
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710.284
Effective Action, Conformal Anomaly and the Issue of Quadratic Divergences
For massless $\phi^4$ theory, we explicitly compute the lowest order non-local contributions to the one-loop effective action required for the determination of the trace anomaly. Imposing exact conformal invariance of the local part of the effective action, we argue that the issue of quadratic divergences does not arise in a theory where exact conformal symmetry is only broken by quantum effects. Conformal symmetry can thus replace low energy supersymmetry as a possible guide towards stabilizing the weak scale and solving the hierarchy problem, if (i) there are no intermediate scales between the weak scale and the Planck scale, and (ii) the running couplings exhibit neither Landau poles nor instabilities over this whole range of energies.
hep-th
for massless phi4 theory we explicitly compute the lowest order nonlocal contributions to the oneloop effective action required for the determination of the trace anomaly imposing exact conformal invariance of the local part of the effective action we argue that the issue of quadratic divergences does not arise in a theory where exact conformal symmetry is only broken by quantum effects conformal symmetry can thus replace low energy supersymmetry as a possible guide towards stabilizing the weak scale and solving the hierarchy problem if i there are no intermediate scales between the weak scale and the planck scale and ii the running couplings exhibit neither landau poles nor instabilities over this whole range of energies
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710.2841
Interplay of causticity and vorticality within the complex quantum Hamilton-Jacobi formalism
Interference dynamics is analyzed in the light of the complex quantum Hamilton-Jacobi formalism, using as a working model the collision of two Gaussian wave packets. Though simple, this model nicely shows that interference in quantum scattering processes gives rise to rich dynamics and trajectory topologies in the complex plane, both ruled by two types of singularities: caustics and vortices, where the former are associated with the regime of free wave-packet propagation, and the latter with the collision (interference) process. Furthermore, an unambiguous picture connecting the complex and real frameworks is also provided and discussed.
quant-ph
interference dynamics is analyzed in the light of the complex quantum hamiltonjacobi formalism using as a working model the collision of two gaussian wave packets though simple this model nicely shows that interference in quantum scattering processes gives rise to rich dynamics and trajectory topologies in the complex plane both ruled by two types of singularities caustics and vortices where the former are associated with the regime of free wavepacket propagation and the latter with the collision interference process furthermore an unambiguous picture connecting the complex and real frameworks is also provided and discussed
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710.2842
Coherence and Correlations in Atom Lasers
We review and characterize the quantum coherence measures that are most useful for quantum gases, including Bose-Einstein condensates (BEC) and ultra-cold fermions, and outline how to calculate these in the typically dynamical environment of an interacting multi-mode quantum gas.
cond-mat.other cond-mat.stat-mech
we review and characterize the quantum coherence measures that are most useful for quantum gases including boseeinstein condensates bec and ultracold fermions and outline how to calculate these in the typically dynamical environment of an interacting multimode quantum gas
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710.2843
Relativistic time dilatation and the spectrum of electrons emitted by 33 TeV lead ions penetrating thin foils
We study the energy distribution of ultrarelativistic electrons produced when a beam of 33 TeV Pb$^{81+}$(1s) ions penetrates a thin Al foil. We show that, because of a prominent role of the excitations of the ions inside the foil which becomes possible due to the relativistic time dilatation, the width of this distribution can be much narrower compared to the case when the ions interact with rarefied gaseous targets. We also show that a very similar shape of the energy distribution may arise when 33 TeV Pb$^{82+}$ ions penetrate a thin Au foil. These results shed some light on the origin of the very narrow electron energy distributions observed experimentally about a decade ago.
physics.atom-ph physics.acc-ph
we study the energy distribution of ultrarelativistic electrons produced when a beam of 33 tev pb811s ions penetrates a thin al foil we show that because of a prominent role of the excitations of the ions inside the foil which becomes possible due to the relativistic time dilatation the width of this distribution can be much narrower compared to the case when the ions interact with rarefied gaseous targets we also show that a very similar shape of the energy distribution may arise when 33 tev pb82 ions penetrate a thin au foil these results shed some light on the origin of the very narrow electron energy distributions observed experimentally about a decade ago
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710.2844
Does a particle swept by a turbulent liquid diffuse?
Since the famous 1926 paper by Richardson, the relative diffusion of two particles in a turbulent liquid has attracted a lot of interest. The motion of a single particle on the other hand is usually considered not to be especially interesting. The widely accepted picture is that the velocity of the particle has short-range correlations in time, resulting in motion that is diffusive on time scales large compared to the correlation time. We find, however, that the correlation time is infinite and that the square displacement, F, is not linear in the traversed time, T, which would correspond to diffusion, but rather F is proportional to T^6/5. Namely, the motion is slightly super diffusive.
cond-mat.stat-mech
since the famous 1926 paper by richardson the relative diffusion of two particles in a turbulent liquid has attracted a lot of interest the motion of a single particle on the other hand is usually considered not to be especially interesting the widely accepted picture is that the velocity of the particle has shortrange correlations in time resulting in motion that is diffusive on time scales large compared to the correlation time we find however that the correlation time is infinite and that the square displacement f is not linear in the traversed time t which would correspond to diffusion but rather f is proportional to t65 namely the motion is slightly super diffusive
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710.2845
Current saturation and Coulomb interactions in organic single-crystal transistors
Electronic transport through rubrene single-crystal field effect transistors (FETs) is investigated experimentally in the high carrier density regime (n ~ 0.1 carrier/molecule). In this regime, we find that the current does not increase linearly with the density of charge carriers, and tends to saturate. At the same time, the activation energy for transport unexpectedly increases with increasing n. We perform a theoretical analysis in terms of a well-defined microscopic model for interacting Frohlich polarons, that quantitatively accounts for our experimental observations. This work is particularly significant for our understanding of electronic transport through organic FETs.
cond-mat.str-el cond-mat.mtrl-sci
electronic transport through rubrene singlecrystal field effect transistors fets is investigated experimentally in the high carrier density regime n 01 carriermolecule in this regime we find that the current does not increase linearly with the density of charge carriers and tends to saturate at the same time the activation energy for transport unexpectedly increases with increasing n we perform a theoretical analysis in terms of a welldefined microscopic model for interacting frohlich polarons that quantitatively accounts for our experimental observations this work is particularly significant for our understanding of electronic transport through organic fets
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710.2846
Two-photon decay of heavy quarkonium from heavy-quark spin symmetry
With the recent measurements on $\eta_{c}$ and $\eta_{c}^{\prime}$ at CLEO, Babar and Belle, and with the prospect of finding the $\eta_{b}$ at the Tevatron, it seems appropriate to have another look at the two-photon decay of heavy quarkonium from the standpoint of an effective Lagrangian based on local operator expansion and heavy-quark spin symmetry. In this talk, I would like to discuss a recent work on the two-photon decay rates of ground states and excited states of $\eta_c$ and $\eta_b$ using the local operator expansion approach and heavy-quark spin symmetry and taking into account the binding-energy. We find that the predicted two-photon width for $\eta_c$ agrees well with experiment, but the predicted value for $\eta_c(2S)$ is twice larger than the CLEO estimation. We point out that the essentially model-independent ratio of $\eta_b$ two-photon width to the $\Upsilon$ leptonic width and the $\eta_b $ two-photon width could be used to extract the strong coupling constant $\alpha_s$ .
hep-ph
with the recent measurements on eta_c and eta_cprime at cleo babar and belle and with the prospect of finding the eta_b at the tevatron it seems appropriate to have another look at the twophoton decay of heavy quarkonium from the standpoint of an effective lagrangian based on local operator expansion and heavyquark spin symmetry in this talk i would like to discuss a recent work on the twophoton decay rates of ground states and excited states of eta_c and eta_b using the local operator expansion approach and heavyquark spin symmetry and taking into account the bindingenergy we find that the predicted twophoton width for eta_c agrees well with experiment but the predicted value for eta_c2s is twice larger than the cleo estimation we point out that the essentially modelindependent ratio of eta_b twophoton width to the upsilon leptonic width and the eta_b twophoton width could be used to extract the strong coupling constant alpha_s
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710.2847
A synchrotron self-Compton scenario for the very high energy gamma-ray emission of the radiogalaxy M87
M87 is the first extragalactic source detected in the TeV range that is not a blazar. With the increasing performances of ground-based Cherenkov telescopes, we can now probe the variability in the gamma-ray flux at small timescales, thus putting strong constraints on the size of the emitting zone. A modification of standard emission models of TeV blazars appears necessary to account for the gamma-ray observations despite this misalignment. We explain TeV gamma-ray spectra and fast variability of M87 by invoking an emission zone close to the central supermassive black hole, which is filled with several plasma blobs moving in the large opening angle of the jet formation zone. We develop a new multi-blob synchrotron self-Compton (SSC) model with emitting blobs beyond the Alfven surface in the jet, at a distance of about 100 r_g from the central engine. This model is explicitly adapted to deal with large viewing angles and moderate values of the Lorentz factor inferred from (general relativistic) magnetohydrodynamic models of jet formation. This scenario can account for the recent gamma-ray observations of M87 made by the High Energy Stereoscopic System (H.E.S.S.) telescope array. We find individual blob radii of about 10^{14} cm, which is compatible with the variability on timescales of days recently reported by the H.E.S.S. collaboration and is of the order of the black hole gravitational radius. Predictions of the very high energy emission for three other sources with extended optical or X-ray jet which could be misaligned blazars still with moderate beaming are presented for one Seyfert 2 radiogalaxy, namely Cen A, one peculiar BL Lac, PKS 0521-36, and one quasar, 3C 273.
astro-ph
m87 is the first extragalactic source detected in the tev range that is not a blazar with the increasing performances of groundbased cherenkov telescopes we can now probe the variability in the gammaray flux at small timescales thus putting strong constraints on the size of the emitting zone a modification of standard emission models of tev blazars appears necessary to account for the gammaray observations despite this misalignment we explain tev gammaray spectra and fast variability of m87 by invoking an emission zone close to the central supermassive black hole which is filled with several plasma blobs moving in the large opening angle of the jet formation zone we develop a new multiblob synchrotron selfcompton ssc model with emitting blobs beyond the alfven surface in the jet at a distance of about 100 r_g from the central engine this model is explicitly adapted to deal with large viewing angles and moderate values of the lorentz factor inferred from general relativistic magnetohydrodynamic models of jet formation this scenario can account for the recent gammaray observations of m87 made by the high energy stereoscopic system hess telescope array we find individual blob radii of about 1014 cm which is compatible with the variability on timescales of days recently reported by the hess collaboration and is of the order of the black hole gravitational radius predictions of the very high energy emission for three other sources with extended optical or xray jet which could be misaligned blazars still with moderate beaming are presented for one seyfert 2 radiogalaxy namely cen a one peculiar bl lac pks 052136 and one quasar 3c 273
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710.2848
Consistency of trace norm minimization
Regularization by the sum of singular values, also referred to as the trace norm, is a popular technique for estimating low rank rectangular matrices. In this paper, we extend some of the consistency results of the Lasso to provide necessary and sufficient conditions for rank consistency of trace norm minimization with the square loss. We also provide an adaptive version that is rank consistent even when the necessary condition for the non adaptive version is not fulfilled.
cs.LG
regularization by the sum of singular values also referred to as the trace norm is a popular technique for estimating low rank rectangular matrices in this paper we extend some of the consistency results of the lasso to provide necessary and sufficient conditions for rank consistency of trace norm minimization with the square loss we also provide an adaptive version that is rank consistent even when the necessary condition for the non adaptive version is not fulfilled
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710.2849
NA57 main results
The CERN NA57 experiment was designed to study the production of strange and multi-strange particles in heavy ion collisions at SPS energies; its physics programme is essentially completed. A review of the main results is presented.
nucl-ex
the cern na57 experiment was designed to study the production of strange and multistrange particles in heavy ion collisions at sps energies its physics programme is essentially completed a review of the main results is presented
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710.285
Local SU(5) Unification in 6D from the Heterotic String
We present a six-dimensional T^2/Z_2 orbifold model which arises as an intermediate step in the compactification of the heterotic string to the MSSM. The orbifold contains two pairs of inequivalent fixed points, with unbroken local gauge groups SU(5) and SU(2)xSU(4), respectively, the intersection of which gives the standard model gauge group. All bulk and brane anomalies are cancelled by the Green--Schwarz mechanism. At each SU(5) fixed point, there is a localised \bar{5}+10 standard model generation, while the third generation and the Higgs fields come in split bulk multiplets due to the breaking of SU(5) at the other fixed point.
hep-ph
we present a sixdimensional t2z_2 orbifold model which arises as an intermediate step in the compactification of the heterotic string to the mssm the orbifold contains two pairs of inequivalent fixed points with unbroken local gauge groups su5 and su2xsu4 respectively the intersection of which gives the standard model gauge group all bulk and brane anomalies are cancelled by the greenschwarz mechanism at each su5 fixed point there is a localised bar510 standard model generation while the third generation and the higgs fields come in split bulk multiplets due to the breaking of su5 at the other fixed point
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710.2851
CP asymmetries at D0
Using two independent measurements of the semileptonic CP asymmetry in the $B_s$ system, we constrain the CP violating phase of the $B_s$ system to be $\phi_s = -0.70^{+0.47}_{-0.39}$. The data sample corresponds to an integrated luminosity of 1.1 fb$^{-1}$ accumulated with D0 detector at the Fermilab Tevatron collider. We also measure the direct CP violating asymmetry in the decay $B^+ \to J/\psi K^+$ to be $A_{CP}(B^+ \to J/\psi K^+) = +0.0067 \pm 0.0074$(stat)$\pm0.0026$(syst). The data corresponds to an integrated luminosity of 1.6 fb$^{-1}$.
hep-ex
using two independent measurements of the semileptonic cp asymmetry in the b_s system we constrain the cp violating phase of the b_s system to be phi_s 070047_039 the data sample corresponds to an integrated luminosity of 11 fb1 accumulated with d0 detector at the fermilab tevatron collider we also measure the direct cp violating asymmetry in the decay b to jpsi k to be a_cpb to jpsi k 00067 pm 00074statpm00026syst the data corresponds to an integrated luminosity of 16 fb1
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710.2852
Generating models for temporal representations
We discuss the use of model building for temporal representations. We chose Polish to illustrate our discussion because it has an interesting aspectual system, but the points we wish to make are not language specific. Rather, our goal is to develop theoretical and computational tools for temporal model building tasks in computational semantics. To this end, we present a first-order theory of time and events which is rich enough to capture interesting semantic distinctions, and an algorithm which takes minimal models for first-order theories and systematically attempts to ``perturb'' their temporal component to provide non-minimal, but semantically significant, models.
cs.CL
we discuss the use of model building for temporal representations we chose polish to illustrate our discussion because it has an interesting aspectual system but the points we wish to make are not language specific rather our goal is to develop theoretical and computational tools for temporal model building tasks in computational semantics to this end we present a firstorder theory of time and events which is rich enough to capture interesting semantic distinctions and an algorithm which takes minimal models for firstorder theories and systematically attempts to perturb their temporal component to provide nonminimal but semantically significant models
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