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

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It 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.
6 pages. To appear in Classical and Quantum Gravity

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/194330

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0701061
 http://arxiv.org/abs/gr-qc/0701061
 Class.Quant.Grav.24:1049-1054,2007
 doi:10.1088/0264-9381/24/5/002

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arXiv