Radial Photon Trajectories Near an Evaporating Black Hole

Details Radial Photon Trajectories Near an Evaporating Black Hole Radial Photon Trajectories Near an Evaporating Black Hole

2008-02-12

arxiv.org/abs/0802.1660v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 figures

Scientific paper

The 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.

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