Search results for "Relativity"

showing 10 items of 1213 documents

A note on static metrics: the degenerate case

2013

We give the necessary and sufficient conditions for a 3-metric to be the adapted spatial metric of a static vacuum solution. This work accomplishes for the degenerate cases the already known study for the regular ones (Bartnik and Tod 2006 {\it Class. Quantum Grav.} {\bf 23} 569-571).

PhysicsClass (set theory)Theoretical physicsWork (thermodynamics)Physics and Astronomy (miscellaneous)Metric (mathematics)Degenerate energy levelsFOS: Physical sciencesVacuum solutionGeneral Relativity and Quantum Cosmology (gr-qc)QuantumGeneral Relativity and Quantum CosmologyClassical and Quantum Gravity
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General-relativistic approach to the nonlinear evolution of collisionless matter.

1993

A new general-relativistic algorithm is developed to study the nonlinear evolution of scalar (density) perturbations of an irrotational collisionless fluid up to shell crossing, under the approximation of neglecting the interaction with tensor (gravitational-wave) perturbations. The dynamics of each fluid element is separately followed in its own inertial rest frame by a system of twelve coupled first-order ordinary differential equations, which can be further reduced to six under very general conditions. Initial conditions are obtained in a cosmological framework, from linear theory, in terms of a single gauge-invariant potential. Physical observables, which are expressed in the Lagrangian…

PhysicsClassical mechanicsExact solutions in general relativityGeneral relativityDifferential equationOrdinary differential equationEinstein field equationsLinear systemInitial value problemPerfect fluidAstrophysics::Cosmology and Extragalactic AstrophysicsPhysical review. D, Particles and fields
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Constraining Unmodeled Physics with Compact Binary Mergers from GWTC-1

2020

We present a flexible model to describe the effects of generic deviations of observed gravitational wave signals from modeled waveforms in the LIGO and Virgo gravitational wave detectors. With the detection of 11 gravitational wave events from the GWTC-1 catalog, we are able to constrain possible deviations from our modeled waveforms. In this paper we present our coherent spline model that describes the deviations, then choose to validate our model on an example phenomenological and astrophysically motivated departure in waveforms based on extreme spontaneous scalarization. We find that the model is capable of recovering the simulated deviations. By performing model comparisons we observe t…

PhysicsCoalescence (physics)010308 nuclear & particles physicsDetectorBinary numberFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesLIGOGeneral Relativity and Quantum CosmologyGravitationSpline (mathematics)0103 physical sciencesWaveformStatistical physics010306 general physics
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Toward early-warning detection of gravitational waves from compact binary coalescence

2012

Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave detectors will offer a unique opportunity for multi-messenger astronomy. Prompt detection alerts for the astronomical community might make it possible to observe the onset of electromagnetic emission from (CBC). We demonstrate a computationally practical filtering strategy that could produce early-warning triggers before gravitational radiation from the final merger has arrived at the detectors.

PhysicsCoalescence (physics)Warning system010308 nuclear & particles physicsGravitational waveDetectorAstronomyBinary numberFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Electromagnetic emission01 natural sciencesRapid detectionGeneral Relativity and Quantum CosmologySpace and Planetary Science0103 physical sciencesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Computer Science::Cryptography and Security
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The nonadiabatic general-relativistic stellar oscillations

1990

We have derived the equations which govern the linear nonadiabatic general-relativistic radial oscillations. The perturbation produces a heat flux that is coupled with the geometry, through the Einstein field equations of a stellar configuration. The classical limit is recovered. The stability conditions are examined by means of a simplified one-zone model.

PhysicsComputational astrophysicsClassical mechanicsHeat fluxSpace and Planetary ScienceGeneral relativityEinstein field equationsPerturbation (astronomy)Astronomy and AstrophysicsAstrophysics::Earth and Planetary AstrophysicsRelativistic quantum chemistryClassical limitStellar pulsationAstrophysics and Space Science
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The exact solution of the diffusion trapping model of defect profiling with variable energy positrons

2013

We report an exact analytical solution of so-called positron diffusion trapping model. This model have been widely used for the treatment of the experimental data for defect profiling of the adjoin surface layer using the variable energy positron (VEP) beam technique. Hovewer, up to now this model could be treated only numerically with so-called VEPFIT program. The explicit form of the solutions is obtained for the realistic cases when defect profile is described by a discreet step-like function and continuous exponential-like function. Our solutions allow to derive the analytical expressions for typical positron annihilation characteristics including the positron lifetime spectrum. Latter …

PhysicsCondensed Matter - Materials ScienceGeneral Physics and AstronomyExperimental dataMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesTrappingFunction (mathematics)CoincidenceExact solutions in general relativityPositronPhysics::Accelerator PhysicsAtomic physicsDiffusion (business)Beam (structure)
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Nonlocal density correlations as a signature of Hawking radiation from acoustic black holes

2008

We have used the analogy between gravitational systems and nonhomogeneous fluid flows to calculate the density-density correlation function of an atomic Bose-Einstein condensate in the presence of an acoustic black hole. The emission of correlated pairs of phonons by Hawking-like process results into a peculiar long-range density correlation. Quantitative estimations of the effect are provided for realistic experimental configurations.

PhysicsCondensed Matter::Quantum GasesBOSONSSonic black holeQuantum field theory in curved spacetimePhononAtomic and Molecular Physics and OpticsBlack holeGravitationCorrelation function (statistical mechanics)General Relativity and Quantum CosmologyHIERARCHYQuantum mechanicsQuantum electrodynamicsANALOGOUTPUT COUPLERSignature (topology)ATOM LASERHawking radiation
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Scattering coefficients and gray-body factor for 1D BEC acoustic black holes: exact results

2015

A complete set of exact analytic solutions to the mode equation is found in the region exterior to the acoustic horizon for a class of 1D Bose-Einstein condensate (BEC) acoustic black holes. From these, analytic expressions for the scattering coefficients and gray-body factor are obtained. The results are used to verify previous predictions regarding the behaviors of the scattering coefficients and gray-body factor in the low frequency limit.

PhysicsCondensed Matter::Quantum GasesHigh Energy Physics - TheoryNuclear and High Energy Physicscond-mat.quant-ga010308 nuclear & particles physicsScatteringFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology3. Good healthGeneral Relativity and Quantum CosmologyExact resultsHigh Energy Physics - Theory (hep-th)Quantum Gases (cond-mat.quant-gas)Quantum electrodynamics0103 physical sciencesAcoustic wave equation010306 general physicsCondensed Matter - Quantum Gases
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Top-seesaw assisted technicolor model with 126 GeV Higgs boson

2013

We discuss a model which involves the top quark condensation and the walking technicolor. We focus on the scalar boson in such a model from the viewpoint of the observed scalar boson at the LHC.

PhysicsCondensed Matter::Quantum GasesTop quarkParticle physicsLarge Hadron ColliderHigh Energy Physics::PhenomenologyFOS: Physical sciencesTechnicolorScalar bosonHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryHiggs bosonHigh Energy Physics::ExperimentFocus (optics)
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The imprints of the Great Attractor and the Virgo cluster on the microwave background

1993

A fully non-linear model based on the Tolman-Bondi solution of the Einstein equations is used to describe the Great Attractor and the Virgo cluster. The background is a Friedmann-Robertson-Walker universe, and the inhomogeneity develops from physically motivated initial profiles of the energy density and the peculiar velocity. Accurate numerical integrations of the field equations of the null geodesics are carried out, and thus the angular temperature distribution of the microwave background produced by the chosen overdensities is found. The observer is located in the Local Group. The quadrupole Q produced by each overdensity is computed and divided into two parts: the relativistic Doppler …

PhysicsCosmic microwave backgroundLocal GroupAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsVirgo ClusterCosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeGreat AttractorSpace and Planetary ScienceFriedmann–Lemaître–Robertson–Walker metricQuadrupolesymbolsPeculiar velocityMonthly Notices of the Royal Astronomical Society
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