Bounds for Mass and Rotation of Black Holes in the Observable Universe

Details Bounds for Mass and Rotation of Black Holes in the Observable Universe Bounds for Mass and Rotation of Black Holes in the Observable Universe

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.225..221d&link_type=abstract

Astrophysics and Space Science, Volume 225, Issue 2, pp.221-226

Mathematics

Mathematical Physics

2

Black Holes, General Relativity, Cosmology, Mathematical Physics

Scientific paper

The bounds for the energy change rate of a Maxwell field in the outer space of a rotating black hole, calculated by de Vries (1994) and de Vries (1995), enable us to deduce limits for the rotation and the mass of black holes. For this purpose we assume that a certain part of the anisotropies of the cosmic background radiation is due to absorption or superradiance of black holes (Teukolsky, 1973, Starobinskii and Churilov, 1973). The knowledge of these anisotropies yields bounds for rotation and mass of the black holes in the observable universe.

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