The angular momentum and mass formulas for rotating stationary quasi-black holes

Details The angular momentum and mass formulas for rotating stationary quasi-black holes The angular momentum and mass formulas for rotating stationary quasi-black holes

2009-01-24

arxiv.org/abs/0901.3860v1

Phys.Rev.D79:044020,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

14 pages

Scientific paper

10.1103/PhysRevD.79.044020

We consider the quasi-black hole limit of a stationary body when its boundary approaches its own gravitational radius, i.e., its quasi-horizon. It is shown that there exists a perfect correspondence between the different mass contributions and the mass formula for quasi-black and black holes in spite of difference in derivation and meaning of the formulas in both cases. For extremal quasi-black holes the finite surface stresses give zero contribution to the total mass. Conclusions similar to those for the properties of mass are derived for the angular momentum.

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