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dc.contributor.authorBrihaye, Yves
dc.contributor.authorHartmann, Betti
dc.contributor.authorUrrestilla Urizabal, Jon ORCID
dc.date.accessioned2018-11-22T13:38:26Z
dc.date.available2018-11-22T13:38:26Z
dc.date.issued2018-06-14
dc.identifier.citationJournal of High Energy Physics 2018(6) : (2018) // Article ID 074es_ES
dc.identifier.issn1029-8479
dc.identifier.urihttp://hdl.handle.net/10810/29746
dc.description.abstractWe demonstrate the existence of static, spherically symmetric globally regular, i.e. solitonic solutions of a shift-symmetric scalar-tensor gravity model with negative cosmological constant. The norm of the Noether current associated to the shift symmetry is finite in the full space-time. We also discuss the corresponding black hole solutions and demonstrate that the interplay between the scalar-tensor coupling and the cosmological constant leads to the existence of new branches of solutions. To linear order in the scalar-tensor coupling, the asymptotic space-time corresponds to an Anti-de Sitter space-time with a non-trivial scalar field on its conformal boundary. This allows the interpretation of our solutions in the context of the AdS/CFT correspondence. Finally, we demonstrate that-for physically relevant, small values of the scalar-tensor coupling-solutions with positive cosmological constant do not exist in our model.es_ES
dc.description.sponsorshipBH would like to thank FAPESP for financial support under grant number 2016/12605-2 and CNPq for financial support under Bolsa de Produtividade Grant 304100/2015-3.es_ES
dc.language.isoenges_ES
dc.publisherSpringeres_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectblack holeses_ES
dc.subjectclassical theories of gravityes_ES
dc.subjectfield-equationses_ES
dc.subjectGW170817es_ES
dc.titleSolitons and black hole in shift symmetric scalar-tensor gravity with cosmological constantes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.holderThis article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.es_ES
dc.rights.holderAtribución 3.0 España*
dc.relation.publisherversionhttps://link.springer.com/article/10.1007%2FJHEP06%282018%29074es_ES
dc.identifier.doi10.1007/JHEP06(2018)074
dc.departamentoesFísica teórica e historia de la cienciaes_ES
dc.departamentoeuFisika teorikoa eta zientziaren historiaes_ES


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This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.
Except where otherwise noted, this item's license is described as This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.