Turning points of massive particles in Schwarzschild geometry

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dc.creatorPolonyi, J.
dc.creatorRadosz, A.
dc.creatorSiwek, A.
dc.creatorOstasiewicz, K.
dc.date2009-02-22
dc.date.accessioned2026-07-07T12:45:32Z
dc.date.available2026-07-07T12:45:32Z
dc.descriptionThe stable geodesics in Schwarzschild geometry can not approach the center closer than the radius of the photon sphere, 3/2 times the Schwarzschild radius. In other words, massive particles moving along geodesics that cross the photon sphere do not escape, they fall into the black hole.
dc.description2 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/0902.3808
dc.identifierhttp://arxiv.org/abs/0902.3808
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/221114
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTurning points of massive particles in Schwarzschild geometry
dc.typetext

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