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dc.contributor.authorGalli, Pietro-
dc.contributor.authorGoldstein, K.-
dc.contributor.authorKatmadas, Stefanos-
dc.contributor.authorPerz, Jan-
dc.date.accessioned2011-10-26T11:41:49Z-
dc.date.available2011-10-26T11:41:49Z-
dc.date.issued2011-06-01-
dc.identifier.citationJournal of High Energy Physics 06: 070 (2011)es_ES
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/10261/41755-
dc.description28 páginas.-- This article is distributed under the terms of the Creative Commons Attribution Noncommercial License.es_ES
dc.description.abstractWe derive a generalised form of flow equations for extremal static and rotating non-BPS black holes in four-dimensional ungauged N = 2 supergravity coupled to vector multiplets. For particular charge vectors, we give stabilisation equations for the scalars, analogous to the BPS case, describing full known solutions. Based on this, we propose a generic ansatz for the stabilisation equations, which surprisingly includes ratios of harmonic functions.es_ES
dc.description.sponsorshipThe work of P.G. has been supported in part by grants FIS2008-06078- C03-02 and FPA2008-03811-E/INFN of Ministerio de Ciencia e Innovación (Spain) and ACOMP/2010/213 from Generalitat Valenciana. This work is also part of the ERC Advanced Grant research program no. 246974, “Supersymmetry: a window to non-perturbative physics”. J.P.’s work has been supported in part by the FWO-Vlaanderen project G.0235.05 and the Federal Office for Scientific, Technical and Cultural Affairs through the ‘Interuniversity Attraction Poles Programme-Belgian Science Policy’ P6/11-P, and in part by the Spanish Ministry of Science and Education grant FPA2009-07692, the Comunidad de Madrid grant HEPHACOS S2009ESP-1473 and the Spanish Consolider-Ingenio 2010 program CPAN CSD2007-00042.es_ES
dc.language.isoenges_ES
dc.publisherSpringeres_ES
dc.publisherInstitute of Physics Publishinges_ES
dc.rightsopenAccesses_ES
dc.subjectBlack holes in string theoryes_ES
dc.subjectSupergravity modelses_ES
dc.titleFirst-order flows and stabilisation equations for non-BPS extremal black holeses_ES
dc.typeartículoes_ES
dc.identifier.doihttp://dx.doi.org/10.1007/JHEP06(2011)070-
dc.description.peerreviewedPeer reviewedes_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1007/JHEP06(2011)070es_ES
dc.identifier.e-issn1029-8479-
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