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

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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.
LaTeX, 4 pages

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/202241

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/9907025
 http://arxiv.org/abs/gr-qc/9907025
 Phys.Rev.D61:064008,2000
 doi:10.1103/PhysRevD.61.064008

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arXiv