A Kerr black hole in the external gravitational field

The full metric describing a Kerr black hole in an arbitrary static and axisymmetric gravitational field is presented in a concise analytical form which allows a straightforward verification of the mass formula for black holes. A sufficient condition of the regularity of the metric in the region exterior to the black hole horizon is formulated. © 1997 Published by Elsevier Science B.V.

Authors
Bretón N.1 , Denisova T.E. 2 , Manko V.S.1
Number of issue
1-2
Language
English
Pages
7-11
Status
Published
Volume
230
Year
1997
Organizations
  • 1 Departamento de Física, CINVESTAV del IPN, A.P. 14-740, 07000 México D.F., Mexico
  • 2 Department of Mathematical Analysis, Peoples' Friendship Univ. of Russia, 6 Miklukho-Maklay Street, Moscow 117198, Russian Federation
Date of creation
19.10.2018
Date of change
19.10.2018
Short link
https://repository.rudn.ru/en/records/article/record/731/