Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/1939
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dc.contributor.authorSatin, S.-
dc.date.accessioned2020-11-20T05:14:50Z-
dc.date.available2020-11-20T05:14:50Z-
dc.date.issued2018-
dc.identifier.citationGeneral Relativity and Gravitation, 50(8).en_US
dc.identifier.other10.1007/s10714-018-2418-9-
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85049793054&doi=10.1007%2fs10714-018-2418-9&origin=inward&txGid=26199fecc967b87721e806211c102044-
dc.identifier.urihttp://hdl.handle.net/123456789/1939-
dc.description.abstractWe propose a Classical Einstein–Langevin equation, for certain applications in Astrophysics and Cosmology. The domain of applications and the formulation are quite different than its semiclassical counterpart, which is an active area of research and inspires one to carry out this new formalism. The field of study can be seen to emerge out of well established ideas and results in Stochastic Processes in Newtonian Physics and the Physics in curved spacetime. This is an effort to combine ideas from the two areas to get meaningful and new physical results in astrophysics and cosmology. A brief calculation, to demonstrate the contribution of stochasticity and induced fluctuations to the spacetime metric, for static spherically symmetric relativistic stars by heuristic solution of the Classical Einstein–Langevin equation is given. The applicability of the proposed formalism can have a wider expanse than is mentioned in this article.en_US
dc.language.isoenen_US
dc.publisherSpringer New York LLCen_US
dc.subjectMetric perturbationsen_US
dc.subjectRelativistic starsen_US
dc.subjectStochastic gravityen_US
dc.titleClassical Einstein–Langevin equation and proposed applicationsen_US
dc.typeArticleen_US
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