"Non-1/r" Newtonian gravitation and stellar structure

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dc.creatorSeidov, Zakir F.
dc.date1999-07-12
dc.date.accessioned2026-07-07T02:32:28Z
dc.date.available2026-07-07T02:32:28Z
dc.descriptionSome analytical spherical-symmetric equilibrium solutions are cosidered in the Newtonian theory of gravitation with deviations from 1/r law. Stability of star against a first-order phase-transition is shown to be particularly influenced by the deviations of degree in the power-law potential.
dc.description5 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9907136
dc.identifierhttp://arxiv.org/abs/astro-ph/9907136
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14473
dc.subjectAstrophysics
dc.title"Non-1/r" Newtonian gravitation and stellar structure
dc.typetext

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