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

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dc.creatorJaranowski, Piotr
dc.creatorSchäfer, Gerhard
dc.date1999-07-06
dc.date.accessioned2026-07-07T11:46:29Z
dc.date.available2026-07-07T11:46:29Z
dc.descriptionThe 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.
dc.descriptionLaTeX, 4 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/9907025
dc.identifierhttp://arxiv.org/abs/gr-qc/9907025
dc.identifierPhys.Rev.D61:064008,2000
dc.identifierdoi:10.1103/PhysRevD.61.064008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202241
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn bare masses in time-symmetric initial-value solutions for two black holes
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