On bare masses in time-symmetric initial-value solutions for two black holes
广义相对论与量子宇宙学
2008-11-26 v1
摘要
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.
引用
@article{arxiv.gr-qc/9907025,
title = {On bare masses in time-symmetric initial-value solutions for two black holes},
author = {Piotr Jaranowski and Gerhard Schäfer},
journal= {arXiv preprint arXiv:gr-qc/9907025},
year = {2008}
}
备注
LaTeX, 4 pages