Kinematics of discretely self-similar spherically symmetric spacetimes
Kinematics of discretely self-similar spherically symmetric spacetimes
We summarize the consequences of the twin assumptions of (discrete) self-similarity and spherical symmetry for the global structure of a spacetime. All such spacetimes can be constructed from two building blocks: the "fan" and "splash." Each building block contains one radial null geodesic that is invariant under the self-similarity (self-similarity horizon).
064019-[11pp]
Gundlach, Carsten
586f1eb5-3185-4b2b-8656-c29c436040fc
Martín-García, José M.
4d46af63-2651-477e-b0f0-67245eba67f0
29 September 2003
Gundlach, Carsten
586f1eb5-3185-4b2b-8656-c29c436040fc
Martín-García, José M.
4d46af63-2651-477e-b0f0-67245eba67f0
Gundlach, Carsten and Martín-García, José M.
(2003)
Kinematics of discretely self-similar spherically symmetric spacetimes.
Physical Review D, 68 (6), .
(doi:10.1103/PhysRevD.68.064019).
Abstract
We summarize the consequences of the twin assumptions of (discrete) self-similarity and spherical symmetry for the global structure of a spacetime. All such spacetimes can be constructed from two building blocks: the "fan" and "splash." Each building block contains one radial null geodesic that is invariant under the self-similarity (self-similarity horizon).
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Published date: 29 September 2003
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Local EPrints ID: 29195
URI: http://eprints.soton.ac.uk/id/eprint/29195
ISSN: 1550-7998
PURE UUID: cf01c078-6d6b-4f57-a38b-f1ca9d720981
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Date deposited: 12 May 2006
Last modified: 16 Mar 2024 03:15
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Author:
José M. Martín-García
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