On bare masses in time-symmetric initial-value solutions for two black holes

Details On bare masses in time-symmetric initial-value solutions for two black holes On bare masses in time-symmetric initial-value solutions for two black holes

1999-07-06

arxiv.org/abs/gr-qc/9907025v1

Phys.Rev.D61:064008,2000

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

LaTeX, 4 pages

Scientific paper

10.1103/PhysRevD.61.064008

The Brill-Lindquist time-symmetric initial-value solution for two uncharged black holes is rederived using the Hamiltonian constraint equation with Dirac delta distributions as a source for the binary black-hole field. The bare masses of the Brill-Lindquist black holes are introduced in a way which is applied, after straightforward modification, to the Misner-Linquist binary black-hole solution.

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