Interacting Geodesics: Binary Systems around a Black Hole

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dc.creatorGueron, Eduardo
dc.creatorLetelier, Patricio S.
dc.date2003-02-27
dc.date.accessioned2026-07-07T02:07:44Z
dc.date.available2026-07-07T02:07:44Z
dc.descriptionWe present a novel method to study interacting orbits in a fixed mean gravitational field associated with a solution of the Einstein field equations. The idea is to consider the Newton gravity among the orbiting particles in a geometry given by the main source. We apply the technique in the of study two and three self-gravitating particles moving around a black hole, i.e., in a Schwarzschild geometry. We also compare with the equivalent Newtonian problem and noted differences in the structural stability, e.g., binary systems were found only in the general relativistic approach.
dc.descriptionrevtex, 15 eps figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0302578
dc.identifierhttp://arxiv.org/abs/astro-ph/0302578
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5792
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleInteracting Geodesics: Binary Systems around a Black Hole
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