The C-metric as a colliding plane wave space-time

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dc.creatorGriffiths, J. B.
dc.creatorHalburd, R. G.
dc.date2007-01-10
dc.date.accessioned2026-07-07T11:21:40Z
dc.date.available2026-07-07T11:21:40Z
dc.descriptionIt is explicitly shown that part of the C-metric space-time inside the black hole horizon may be interpreted as the interaction region of two colliding plane waves with aligned linear polarization, provided the rotational coordinate is replaced by a linear one. This is a one-parameter generalization of the degenerate Ferrari-Ibanez solution in which the focussing singularity is a Cauchy horizon rather than a curvature singularity.
dc.description6 pages. To appear in Classical and Quantum Gravity
dc.identifierhttps://arxiv.org/abs/gr-qc/0701061
dc.identifierhttp://arxiv.org/abs/gr-qc/0701061
dc.identifierClass.Quant.Grav.24:1049-1054,2007
dc.identifierdoi:10.1088/0264-9381/24/5/002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194330
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe C-metric as a colliding plane wave space-time
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