Spinning Down a Black Hole With Scalar Fields

Details Spinning Down a Black Hole With Scalar Fields Spinning Down a Black Hole With Scalar Fields

1997-03-06

arxiv.org/abs/gr-qc/9703018v1

Phys.Rev.Lett. 78 (1997) 3249-3251

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages (including 3 postscript figures), Revtex, uses epsf.tex, twocolumn.sty and header.sty (included). Submitted to Physica

Scientific paper

10.1103/PhysRevLett.78.3249

We study the evolution of a Kerr black hole emitting scalar radiation via the
Hawking process. We show that the rate at which mass and angular momentum are
lost by the black hole leads to a final evolutionary state with nonzero angular
momentum, namely $a/M \approx 0.555$.

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