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]

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Abstract or Description

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
Identification Number (DOI):	https://doi.org/10.1007/BF01645624
Departments, Centres and Research Units:	Computing
Dates:	Date Event June 1973 Published
Item ID:	31607
Date Deposited:	14 Mar 2022 15:28
Last Modified:	14 Mar 2022 15:28
Peer Reviewed:	Yes, this version has been peer-reviewed.
URI:	https://research.gold.ac.uk/id/eprint/31607

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