Classical Einstein-Langevin equation and proposed applications

DOI10.1007/s10714-018-2418-9zbMath1400.85004arXiv1509.08196OpenAlexW3104243178WikidataQ129542418 ScholiaQ129542418MaRDI QIDQ1622146

Seema E. Satin

Publication date: 12 November 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1509.08196

zbMATH Keywords

metric perturbationsstochastic gravityrelativistic stars

Mathematics Subject Classification ID

Applications of statistics to physics (62P35) Galactic and stellar structure (85A15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (4)

Correspondences of matter field fluctuations in semiclassical and classical gravity in the decoherence limit ⋮ Stochastic metric perturbations (radial) in gravitationally collapsing spherically symmetric relativistic star ⋮ Formalism for stochastic perturbations and analysis in relativistic stars ⋮ A linear response relation for perturbed Einstein’s equations with a Langevin source: applications to perturbations in compact stars

Cites Work

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• Gravitational collapse of an isentropic perfect fluid with a linear equation of state
• The Quantum Theory of Motion
• Semiclassicality and decoherence of cosmological perturbations
• The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
• Stochastic Problems in Physics and Astronomy
• Stochastic gravity: theory and applications

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