The Symmetries of Kerr Black Holes
Hughston, L P; and Sommers, P.
1973.
The Symmetries of Kerr Black Holes.
Communications in Mathematical Physics, 33(2),
pp. 129-133.
ISSN 0010-3616
[Article]
The Kerr solution describes, in Einstein's theory, the gravitational field of a rotating black hole. The axial symmetry and stationarity of the solution are shown here to arise in a simple way from properties of the curvature tensor.
Item Type | Article |
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Departments, Centres and Research Units | Computing |
Date Deposited | 14 Mar 2022 15:28 |
Last Modified | 14 Mar 2022 15:28 |