Oppenheimer-Volkoff Equation in Relativistic MOND Theory

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dc.creatorJin, Xing-hua
dc.creatorLi, Xin-zhou
dc.date2006-05-09
dc.date2006-06-23
dc.date.accessioned2026-07-07T07:09:42Z
dc.date.available2026-07-07T07:09:42Z
dc.descriptionIn this paper, we discuss the internal and external metric of the semi-realistic stars in relativistic MOND theory. We show the Oppenheimer-Volkoff equation in relativistic MOND theory and get the metric and pressure inside the stars to order of post-Newtonian corrections. We study the features of motion around the static, spherically symmetric stars by Hamilton-Jacobi mothod, and find there are only some small corrections in relativistic MOND theory.
dc.description10 pages, no figure
dc.identifierhttps://arxiv.org/abs/gr-qc/0605046
dc.identifierhttp://arxiv.org/abs/gr-qc/0605046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111170
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOppenheimer-Volkoff Equation in Relativistic MOND Theory
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