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dc.date.accessioned 2021-12-13T18:58:31Z
dc.date.available 2021-12-13T18:58:31Z
dc.date.issued 2003-01
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/129533
dc.description.abstract We discuss the Penrose limit of the Chamseddine-Volkov BPS selfgravitating monopole in four dimensional N=4 supergravity theory with non-abelian gauge multiplets. We analyze the properties of the resulting supersymmetric pp-wave solutions when various Penrose limits are considered. Apart from the usual rescaling of coordinates and fields we find that a rescaling of the gauge coupling constant to zero is required, rendering the theory abelian. We also study the Killing spinor equations showing an enhancement of the supersymmetries preserved by the solutions and discuss the embedding of the pp-wave solution in d=10 dimensions. en
dc.format.extent 280-286 es
dc.language en es
dc.subject Penrose limit es
dc.subject Chamseddine–Volkov BPS selfgravitating monopole es
dc.subject Killing spinor equations es
dc.title PP-waves from BPS supergravity monopoles en
dc.type Articulo es
sedici.identifier.other arXiv:hep-th/0211093 es
sedici.identifier.other doi:10.1016/s0370-2693(02)03159-3 es
sedici.identifier.issn 0370-2693 es
sedici.creator.person Correa, Diego Hernán es
sedici.creator.person Moreno, Enrique Francisco es
sedici.creator.person Reuillon, S. es
sedici.creator.person Schaposnik, Fidel Arturo es
sedici.subject.materias Ciencias Exactas es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Exactas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physics Letters B es
sedici.relation.journalVolumeAndIssue vol. 552, no. 3-4 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)