Density of dark matter in Solar system and perihelion precession of planets

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dc.creatorKhriplovich, I. B.
dc.date2007-02-09
dc.date2007-03-15
dc.date.accessioned2026-07-07T11:21:08Z
dc.date.available2026-07-07T11:21:08Z
dc.descriptionDirect 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.description4 pages; some explanations on derivation of master formula added
dc.identifierhttps://arxiv.org/abs/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.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194176
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
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