5D radiating black holes in einstein-yang-mills-gauss-bonnet gravity

dc.contributor.authorGhosh, S. G.
dc.date.accessioned2012-03-04T13:41:33Z
dc.date.available2012-03-04T13:41:33Z
dc.date.issued2011-08-25
dc.description.abstractWe derive nonstatic spherically symmetric solutions of a null uid, in ve dimension (5D), to Einstein-Yang-Mills (EYM) equations with the coupling of Gauss-Bonnet (GB) combination of quadratic curvature terms, namely, 5D-EYMGB radiating black hole solution. It is shown that, in the limit, we can recover known radiating black hole solutions. The spherically symmetric known 5D static black hole solutions are also retrieved. The e ect of the GB term and Yang-Mills (YM) gauge charge on the structure and location of horizons, of the 5D radiating black hole, is also discussed.en_US
dc.identifier.urihttp://hdl.handle.net/11007/319
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprints;18/2011
dc.subjectBonnet gravityen_US
dc.subjectEinsteinen_US
dc.subjectBlack holesen_US
dc.subject5Den_US
dc.title5D radiating black holes in einstein-yang-mills-gauss-bonnet gravityen_US
dc.typeArticleen_US

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