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dc.contributor.authorKhriplovich, I. B.
dc.date.accessioned2019-10-24T18:55:33Z
dc.date.available2019-10-24T18:55:33Z
dc.date.created2017-02-28 01:18
dc.date.issued2007-02-09
dc.identifieroai:arXiv.org:astro-ph/0702260
dc.identifierhttp://arxiv.org/abs/astro-ph/0702260
dc.identifierInt.J.Mod.Phys.D16:1475-1478,2007
dc.identifierdoi:10.1142/S0218271807010869
dc.identifier.doi10.1142/S0218271807010869
dc.identifier.urihttp://hdl.handle.net/20.500.12424/1018733
dc.description.abstractDirect relation is pointed out between the secular perihelion precession of a planet and the density of dark matter at its orbit. It is valid under the only assumption that the density is spherically-symmetric, with the center coinciding with the Sun. This relation, combined with the observational data on perihelion precession of planets, results in upper limits on local values of the dark matter density in the Solar system.
dc.description.abstractComment: 4 pages; some explanations on derivation of master formula added
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDensity of dark matter in Solar system and perihelion precession of planets
dc.typetext
ge.collectioncodeOAIDATA
ge.dataimportlabelOAI metadata object
ge.identifier.legacyglobethics:10655986
ge.identifier.permalinkhttps://www.globethics.net/gtl/10655986
ge.lastmodificationdate2017-02-28 01:18
ge.lastmodificationuseradmin@pointsoftware.ch (import)
ge.submissions0
ge.oai.exportid149001
ge.oai.repositoryid58
ge.oai.setnameAstrophysics
ge.oai.setnameGeneral Relativity and Quantum Cosmology
ge.oai.setnameHigh Energy Physics - Phenomenology
ge.oai.setspecphysics:astro-ph
ge.oai.setspecphysics:gr-qc
ge.oai.setspecphysics:hep-ph
ge.oai.streamid5
ge.setnameGlobeTheoLib
ge.setspecglobetheolib
ge.linkhttp://arxiv.org/abs/astro-ph/0702260


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