Transmission and reflection coefficients for a scalar field inside a charged black hole

Details Transmission and reflection coefficients for a scalar field inside a charged black hole Transmission and reflection coefficients for a scalar field inside a charged black hole

1997-11-10

arxiv.org/abs/gr-qc/9711034v1

Phys.Rev. D57 (1998) 2621-2623

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, RevTeX, no figures. Accepted to Phys. Rev. D (Brief Report)

Scientific paper

10.1103/PhysRevD.57.2621

Using the late-time expansion we calculate the leading-order coefficients describing the evolution of a massless scalar field inside a Reissner-Nordstrom black hole. These coefficients may be interpreted as the reflection and transmission coefficients for scalar-field modes propagating from the event horizon to the Cauchy horizon. Our results agree with those obtained previously by Gursel et al by a different method.

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