From the Kerr metric (26.70) derive Eqs. (26.84) for the surface area of a spinning black holes
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From the Kerr metric (26.70) derive Eqs. (26.84) for the surface area of a spinning black hole’s horizon—that is, the surface area of the 2-dimensional surface {r = rH, t = constant}.
Equations.
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Related Book For
Modern Classical Physics Optics Fluids Plasmas Elasticity Relativity And Statistical Physics
ISBN: 9780691159027
1st Edition
Authors: Kip S. Thorne, Roger D. Blandford
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