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Black holes in models with dilaton field and electric or electric and magnetic charges

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dc.contributor.author Kyriakopoulos, E en
dc.date.accessioned 2014-03-01T01:23:40Z
dc.date.available 2014-03-01T01:23:40Z
dc.date.issued 2006 en
dc.identifier.issn 0264-9381 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/17079
dc.subject Electromagnetic Field en
dc.subject Satisfiability en
dc.subject Black Hole en
dc.subject Strong Energy Condition en
dc.subject.classification Astronomy & Astrophysics en
dc.subject.classification Physics, Multidisciplinary en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other BARYON NUMBER en
dc.subject.other HAIR en
dc.subject.other NONEXISTENCE en
dc.subject.other SOLITONS en
dc.title Black holes in models with dilaton field and electric or electric and magnetic charges en
heal.type journalArticle en
heal.identifier.primary 10.1088/0264-9381/23/24/027 en
heal.identifier.secondary http://dx.doi.org/10.1088/0264-9381/23/24/027 en
heal.identifier.secondary 027 en
heal.language English en
heal.publicationDate 2006 en
heal.abstract Exact static spherically symmetric charged black holes in four dimensions are presented. One of them has only electric charge and another electric and magnetic charges. In these solutions the metric is asymptotically flat, has two horizons, irremovable singularity only at r = 0, and the dilaton field is singular only at r = 0. The solution with electric charge only is characterized by three free parameters, the ADM mass, the electric charge and an additional free parameter. It can be considered as a modification of the GHS-GM solution obtained by changing the coupling between dilaton and electromagnetic field. The general dyonic solution is again characterized by three free parameters, the ADM mass, the magnetic charge and an additional free parameter, which is not the electric charge. According to a definition of the no-hair conjecture the solutions are 'hairy'. A very interesting special case of the dyonic solution is characterized by three free parameters, the ADM mass and the electric and magnetic charges. The solutions satisfy the dominant as well as the strong energy condition outside and on the external horizon. © 2006 IOP Publishing Ltd. en
heal.publisher IOP PUBLISHING LTD en
heal.journalName Classical and Quantum Gravity en
dc.identifier.doi 10.1088/0264-9381/23/24/027 en
dc.identifier.isi ISI:000242327900030 en
dc.identifier.volume 23 en
dc.identifier.issue 24 en
dc.identifier.spage 7591 en
dc.identifier.epage 7602 en


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