An approximation scheme for scalar waves in a Reissner-Nordström geometry.

Details An approximation scheme for scalar waves in a Reissner-Nordström geometry. An approximation scheme for scalar waves in a Reissner-Nordström geometry.

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979gregr..11...71c&link_type=abstract

General Relativity and Gravitation, Volume 11, Issue 1, pp.71-77

Physics

2

Black Holes:Radiative Transfer

Scientific paper

The Reissner-Nordström geometry is approximated by a certain sequence of conformally flat shells. As an example of the use of this approximation, spectral curves of transmission coefficientT(w) vs. frequencyw are calculated for spherical waves of monochromatic scalar radiation imploding on the charged black hole by solving the scalar wave equation within each conformally flat space and matching across the interfaces. Spectral curves are found for several values of the charge that are less than or equal to the mass. For small charge, the results agree with those previously found in the Schwarzschild case.

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