Angular-Momentum–Mass Inequality for Axisymmetric Black Holes

Sergio Dain
Phys. Rev. Lett. 96, 101101 – Published 16 March 2006

Abstract

The inequality Jm is proved for vacuum, asymptotically flat, maximal, and axisymmetric data close to extreme Kerr data. The physical significance of this inequality and its relation to the standard picture of the gravitational collapse are discussed.

  • Received 21 November 2005

DOI:https://doi.org/10.1103/PhysRevLett.96.101101

©2006 American Physical Society

Authors & Affiliations

Sergio Dain*

  • Albert-Einstein-Institut, am Mühlenberg 1, D-14476, Golm, Germany

  • *Electronic address: dain@aei.mpg.de

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Issue

Vol. 96, Iss. 10 — 17 March 2006

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