Search results for "Exponent"

showing 10 items of 896 documents

A Study of Gravitational Lens Chromaticity using Ground-based Narrow Band Photometry

2011

We present observations of wavelength-dependent flux ratios for four gravitational lens systems (SDSS~J1650+4251, HE~0435$-$1223, FBQ 0951+2635, and Q~0142$-$100) obtained with the Nordic Optical Telescope. The use of narrowband photometry, as well as the excellent seeing conditions during the observations, allows us to study their chromatic behavior. For SDSS~J1650+4251, we determine the extinction curve of the dust in the $z_L=0.58$ lens galaxy and find that the 2175 \AA \ feature is absent. In the case of HE~0435$-$1223, we clearly detect chromatic microlensing. This allows us to estimate the wavelength-dependent size of the accretion disk. We find an R-band disk size of $r^{R}_s=13\pm5$…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGravitational microlensing01 natural sciencesNordic Optical TelescopeGalaxyPhotometry (astronomy)Gravitational lensThin diskSpace and Planetary Science0103 physical sciencesExponentChromatic scale010303 astronomy & astrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Whispers from the dark side: Confronting light new physics with NANOGrav data

2021

The NANOGrav collaboration has recently observed first evidence of a gravitational wave background (GWB) in pulsar timing data. Here we explore the possibility that this GWB is due to new physics, and show that the signal can be well fit also with peaked spectra like the ones expected from phase transitions (PTs) or from the dynamics of axion like particles (ALPs) in the early universe. We find that a good fit to the data is obtained for a very strong PT at temperatures around 1 MeV to 10 MeV. For the ALP explanation the best fit is obtained for a decay constant of $F \approx 5\times 10^{17}$ GeV and an axion mass of $2\times 10^{-13}$ eV. We also illustrate the ability of PTAs to constrain…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysicsQC1-999Physics beyond the Standard Modelmedia_common.quotation_subjectGeneral Physics and AstronomyFOS: Physical sciencesAstrophysicsParameter space01 natural sciencesSpectral lineUniverseGravitational wave backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Pulsar0103 physical sciencesExponential decay010306 general physicsAxionAstrophysics - Cosmology and Nongalactic Astrophysicsmedia_common
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Exponents of non-linear clustering in scale-free one-dimensional cosmological simulations

2012

One dimensional versions of cosmological N-body simulations have been shown to share many qualitative behaviours of the three dimensional problem. They can resolve a large range of time and length scales, and admit exact numerical integration. We use such models to study how non-linear clustering depends on initial conditions and cosmology. More specifically, we consider a family of models which, like the 3D EdS model, lead for power-law initial conditions to self-similar clustering characterized in the strongly non-linear regime by power-law behaviour of the two point correlation function. We study how the corresponding exponent \gamma depends on the initial conditions, characterized by th…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesSpectral densityAstronomy and AstrophysicsCosmologyNumerical integrationMetric expansion of spaceUniversality (dynamical systems)Nonlinear systemTheoretical physicsSpace and Planetary ScienceExponentStatistical physicsCluster analysisAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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Number of metastable states of a chain with competing and anharmonicΦ4−like interactions

1993

We investigate the number of metastable configurations of a Φ 4 -like model with competing and anharmonic interactions as a function of an effective coupling constant η. The model has piecewise harmonic nearest-neighbor and harmonic next-nearerst-neighbor interactions. The number M of metastable states in the configuration space increases exponentially with the number N of particles: M∞exp(vN). It is shown numerically that, outside the previously considered range |η|<1/3, v is approximately linearly decreasing with η for |η|<1 and that v=0 for η≥1. These findings can be understood by describing the metastable configurations as an arrangement of kink solitons whose width creases with η

PhysicsCoupling constantCondensed matter physicsExponential growthMetastabilityAnharmonicityPiecewiseConfiguration spaceMolecular physicsPhysical Review B
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CONSTRUCTION OF METASTABLE STATES IN QUANTUM ELECTRODYNAMICS

2004

In this paper, we construct metastable states of atoms interacting with the quantized radiation field. These states emerge from the excited bound states of the non-interacting system. We prove that these states obey an exponential time-decay law. In detail, we show that their decay is given by an exponential function in time, predicted by Fermi's Golden Rule, plus a small remainder term. The latter is proportional to the (4+β)th power of the coupling constant and decays algebraically in time. As a result, though it is small, it dominates the decay for large times. A central point of the paper is that our remainder term is significantly smaller than the one previously obtained in [1] and as…

PhysicsCoupling constantStatistical and Nonlinear PhysicsExponential functionsymbols.namesakeQuantum mechanicsQuantum electrodynamicsMetastabilityExcited stateBound statesymbolsFermi's golden ruleRemainderMathematical PhysicsFermi Gamma-ray Space TelescopeReviews in Mathematical Physics
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Critical Attractor and Universality in a Renormalization Scheme for Three Frequency Hamiltonian Systems

1998

We study an approximate renormalization-group transformation to analyze the breakup of invariant tori for three degrees of freedom Hamiltonian systems. The scheme is implemented for the spiral mean torus. We find numerically that the critical surface is the stable manifold of a critical nonperiodic attractor. We compute scaling exponents associated with this fixed set, and find that they can be expected to be universal.

PhysicsCritical phenomenaGeneral Physics and AstronomyFOS: Physical sciencesTorusNonlinear Sciences - Chaotic DynamicsStable manifoldUniversality (dynamical systems)Hamiltonian systemRenormalizationAttractorChaotic Dynamics (nlin.CD)Critical exponentMathematics::Symplectic GeometryMathematical physics
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Single-cluster Monte Carlo study of the Ising model on two-dimensional random lattices.

1994

We use the single-cluster Monte Carlo update algorithm to simulate the Ising model on two-dimensional Poissonian random lattices with up to 80,000 sites which are linked together according to the Voronoi/Delaunay prescription. In one set of simulations we use reweighting techniques and finite-size scaling analysis to investigate the critical properties of the model in the very vicinity of the phase transition. In the other set of simulations we study the approach to criticality in the disordered phase, making use of improved estimators for measurements. From both sets of simulations we obtain clear evidence that the critical exponents agree with the exactly known exponents for regular latti…

PhysicsCritical phenomenaQuantum Monte CarloHigh Energy Physics - Lattice (hep-lat)Condensed Matter (cond-mat)FOS: Physical sciencesSquare-lattice Ising modelCondensed MatterHybrid Monte CarloHigh Energy Physics - LatticeIsing modelMonte Carlo method in statistical physicsStatistical physicsCritical exponentMonte Carlo molecular modelingPhysical review. B, Condensed matter
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Application of the Monte Carlo coherent-anomaly method to two-dimensional lattice-gas systems with further-neighbor interactions

1990

A Monte Carlo version of the coherent-anomaly method has been used to determine critical properties of a two-dimensional Ising ferromagnet with nearest- and next-nearest-neighbor interactions and of a series of two-dimensional lattice-gas systems of particles interacting via 6-12 Lennard-Jones potential. It has demonstrated that the method leads to quite accurate determination of critical temperature but is less successful when used to determine the values of critical exponents \ensuremath{\gamma} and \ensuremath{\nu}.

PhysicsCritical point (thermodynamics)Monte Carlo methodDynamic Monte Carlo methodIsing modelMonte Carlo method in statistical physicsStatistical physicsCritical exponentSquare latticeMonte Carlo molecular modelingPhysical Review B
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Ising Spins on 3D Random Lattices

1999

We perform single-cluster Monte Carlo simulations of the Ising model on three-dimensional Poissonian random lattices of Voronoi/Delaunay type with up to 128 000 sites. For each lattice size quenched averages are computed over 96 realizations. From a finite-size scaling analysis we obtain strong evidence that the critical exponents coincide with those on regular cubic lattices.

PhysicsDelaunay triangulationLattice sizeHigh Energy Physics::LatticeMonte Carlo methodIsing modelStatistical physicsType (model theory)Voronoi diagramCritical exponentScaling
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On the theory of domain switching kinetics in ferroelectrics

2011

Abstract We investigate theoretically the polarization switching kinetics in ferroelectrics, both bulk and thin films samples. In such substances, the domain walls are pinned by (usually dipole) defects, which are present also in ordered samples as technologically unavoidable impurities. This random interaction with dipole pinning centers results, in particular, in exponentially broad distribution of switching times. Under supposition of low pinning centers concentration, we derive the distribution function of switching times showing that it is not simply Lorentzian (as it was first suggested by Tagantsev et al. [Phys. Rev. B 66 (2002) 214109]), but is a “square of Lorentzian”, which is due…

PhysicsDipoleDistribution functionCondensed matter physicsExponential growthImpurityElectric fieldKineticsGeneral Physics and AstronomyThin filmPolarization (waves)Physics Letters A
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