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Please use this identifier to cite or link to this item: http://hdl.handle.net/11129/2040

Title: Effect of NUT parameter on the analytic extension of the Cauchy horizon that develop in colliding wave spacetimes
Authors: Gürtuğ, Özay
Halilsoy, Mustafa
Keywords: gravity
general relativity
colliding wave spacetimes
Issue Date: 2009
Publisher: International Journal of Modern Physics A, World Scientific Publishing
Citation: Ozay Gurtug and Mustafa Halilsoy, “Effect of NUT Parameter on the Analytic Extension of the Cauchy Horizon that Develop in Colliding Wave Space – Times”, Int. Jour. Mod. Phys. A, Vol:24, pp:3171-3190, (2009) .
Series/Report no.: ;IJMPA, 24 (2009) 3171.
Abstract: The Cauchy horizon forming colliding wave solution due to Chandrasekhar and Xanthopoulos (CX) has been generalized by inclusion of the NUT (Newman - Unti - Tamburino) parameter. This is done by transforming the part of the inner horizon region of a Kerr-Newman-NUT black hole into the space of colliding waves. By taking appropriate combination of Killing vectors and analytically extending beyond the Cauchy horizon the time-like hyperbolic sigularities are resolved as well. This provides another example of its kind among the type - D metrics with special emphasis on the role of the NUT parameter. Finally, it is shown that horizons of colliding higher dimensional plane waves obtained from the black p-branes undergoes a similar procedure of analytic extension.
Description: The file in this item is the post-print version of the article (author’s copy; author’s final manuscript, accepted for publication after peer-review process). Due to copyright restrictions, the access to the publisher version (published version) of this article is only available via subscription. You may click URI (with DOI: 10.1142/S0217751X09044243) and have access to the Publisher Version of this article through the publisher web site or online databases, if your Library or institution has subscription to the related journal or publication.
URI: http://dx.doi.org/10.1142/S0217751X09044243
http://hdl.handle.net/11129/2040
ISSN: 1793-656X (online)
0217-751X (print)
Appears in Collections:PHY – Journal Articles: Publisher & Author Versions (Post-Print Author Versions) – Physics

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