Radial Photon Trajectories Near an Evaporating Black Hole

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dc.creatorBrown, Beth A.
dc.creatorLindesay, James
dc.date2008-02-12
dc.date.accessioned2026-07-07T09:20:16Z
dc.date.available2026-07-07T09:20:16Z
dc.descriptionThe radial motion of photons emitted near the horizon of a black hole that evaporates at a steady rate is examined. The space-time of the black hole is generated using non-orthogonal coordinates. It is shown that some photons that are initially drawn towards the singularity can escape falling into the horizon. The behaviors of various outgoing and ingoing photons are clearly demonstrated through the use of a Penrose diagram.
dc.description4 figures
dc.identifierhttps://arxiv.org/abs/0802.1660
dc.identifierhttp://arxiv.org/abs/0802.1660
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/154668
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRadial Photon Trajectories Near an Evaporating Black Hole
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