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dc.date.accessioned 2021-10-12T14:41:48Z
dc.date.available 2021-10-12T14:41:48Z
dc.date.issued 2016-11-03
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/126460
dc.description.abstract In this paper, we study gauged solutions associated with a massive vector field representing a spin-1 condensate, namely, the Proca field. We focus on regular spherically symmetric solutions which we construct either using a self-interaction potential or general relativity in order to glue the solutions together. We start generating nongravitating solutions—so-called Proca Q-balls and charged Proca Q-balls. Then we turn on backreaction on the metric, allowing gravity to hold together the Proca condensate, to study the so-called Proca stars, charged Proca stars, Proca Q-stars, and charged Proca Q-stars. en
dc.language en es
dc.subject Physics es
dc.subject Gravitation es
dc.subject General relativity es
dc.subject Stars es
dc.subject Field (physics) es
dc.subject Q-ball es
dc.subject Order (ring theory) es
dc.subject Mathematical physics es
dc.subject Classical mechanics es
dc.subject Vector field es
dc.title Charged Proca stars en
dc.type Articulo es
sedici.identifier.other arXiv:1608.00011 es
sedici.identifier.other doi:10.1103/physrevd.94.104006 es
sedici.identifier.issn 2470-0010 es
sedici.identifier.issn 2470-0029 es
sedici.creator.person Salazar Landea, Ignacio es
sedici.creator.person García, Federico es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physical Review D es
sedici.relation.journalVolumeAndIssue vol. 94, no. 10 es


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