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Junction conditions of Palatini f (R,T) gravity

dc.contributor.authorRosa, Joao Luis
dc.contributor.authorRubiera García, Diego
dc.date.accessioned2023-06-22T12:27:53Z
dc.date.available2023-06-22T12:27:53Z
dc.date.issued2022-11-06
dc.description© 2022 American Physical Society J. L. R. is supported by the European Regional Development Fund and the program Mobilitas Pluss (MOBJD647), and thanks the Department of Theoretical Physics at the Complutense University of Madrid for their hospitality during the elaboration of this work. D. R.-G. is funded by the Atraccion de Talento Investigador program of the Comunidad de Madrid (Spain) No. 2018T1/TIC-10431 and acknowledges further support from the Ministerio de Ciencia, Innovacion y Universidades (Spain) Project No. PID2019-108485 GB-I00/AEI/10.13039/501100011033 ("PGC Generacion de Conocimiento") and the FCT Projects No. PTDC/FIS-PAR/31938/2017 and No. PTDC/FIS-OUT/29048/2017. This work is also supported by the project PROMETEO/2020/079 (Generalitat Valenciana) and the Edital 006/2018 PRONEX (FAPESQ-PB/CNPQ, Brazil, Grant No. 0015/2019). This article is based upon work from COST Action CA18108, supported by COST (European Cooperation in Science and Technology).
dc.description.abstractWe work out the junction conditions for the Palatini f(R, T) extension of general relativity, where f is an arbitrary function of the curvature scalar R of an independent connection, and of the trace T of the stress -energy tensor of the matter fields. We find such conditions on the allowed discontinuities of several geometrical and matter quantities, some of which depart from their metric counterparts, and in turn extend their Palatini f(R) versions via some new T-dependent terms. Moreover, we also identify some "exceptional cases " of f(R,T) Lagrangians such that some of these conditions can be discarded, thus allowing for further discontinuities in R and T and, in contrast with other theories of gravity, they are shown to not give rise to extra components in the matter sector, e.g., momentum fluxes and double gravitational layers. We discuss how these junction conditions, together with the nonconservation of the stress-energy tensor ascribed to these theories, may induce nontrivial changes in the shape of specific applications such as traversable thin-shell wormholes.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. Horizonte 2020
dc.description.sponsorshipFondo Europeo de Desarrollo Regional (FEDER)
dc.description.sponsorshipMinisterio de Ciencia, Innovacion y Universidades (MICIU)
dc.description.sponsorshipComunidad de Madrid
dc.description.sponsorshipGeneralitat Valenciana
dc.description.sponsorshipFundação para a Ciência e a Tecnologia (FCT)
dc.description.sponsorshipFAPESQPB/CNPQ
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/75360
dc.identifier.doi10.1103/PhysRevD.106.064007
dc.identifier.issn2470-0010
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevD.106.064007
dc.identifier.relatedurlhttps://journals.aps.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/72571
dc.issue.number6
dc.journal.titlePhysical review D
dc.language.isoeng
dc.publisherAmer Physical Soc
dc.relation.projectIDCA18108
dc.relation.projectIDMobilitas Pluss (MOBJD647)
dc.relation.projectIDPID2019-108485-GB-I00/AEI/10.13039/501100011033
dc.relation.projectID2018T1/TIC-10431
dc.relation.projectIDPROMETEO/2020/079
dc.relation.projectID(PTDC/FIS-PAR/31938/2017, PTDC/FIS-OUT/29048/2017)
dc.relation.projectID006/2018 PRONEX; 0015/2019
dc.rights.accessRightsopen access
dc.subject.cdu51-73
dc.subject.keywordInflation
dc.subject.keywordWormholes
dc.subject.keywordStars
dc.subject.ucmFísica-Modelos matemáticos
dc.subject.ucmFísica matemática
dc.titleJunction conditions of Palatini f (R,T) gravity
dc.typejournal article
dc.volume.number106
dspace.entity.typePublication
relation.isAuthorOfPublication3729ced5-9cbe-4f32-9550-6f320f10832a
relation.isAuthorOfPublication.latestForDiscovery3729ced5-9cbe-4f32-9550-6f320f10832a

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