On the parameters of the Kerr-NUT-(anti-)de Sitter space-time

Article

On the parameters of the Kerr-NUT-(anti-)de Sitter space-time

Griffiths, J. B; Podolský, J.

Class. Quantum Grav. 24(0), 1687-1689 (2007)

doi ↗ arXiv:gr-qc/0702042 ↗ link ↗

Abstract

Different forms of the metric for the Kerr-NUT-(anti-)de Sitter space-time are being widely used in its extension to higher dimensions. The purpose of this note is to relate the parameters that are being used to the physical parameters (mass, rotation, NUT and cosmological constant) in the basic four dimensional situation.

Keywords

General Relativity and Quantum Cosmology, High Energy Physics - Theory

Institute authors

Podolský, Jiří

Supported by

GACR 202/06/0041 — Contemporary problems of general relativity and gravitation
LC06014 — Centrum teoretické astrofyziky

BibTeX

@article{UTF189,
  author        = {Griffiths, J. B and Podolský, J.},
  title         = {{On the parameters of the Kerr-NUT-(anti-)de Sitter space-time}},
  journal       = {Class. Quantum Grav.},
  volume        = {24},
  number        = {0},
  pages         = {1687-1689},
  year          = {2007},
  doi           = {10.1088/0264-9381/24/6/N02},
  eprint        = {gr-qc/0702042},
  archivePrefix = {arXiv},
  url           = {http://www.iop.org/EJ/article/-search=53367931.2/0264-9381/24/6/N02/cqg7\_6\_n02.pdf},
}