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dc.date.accessioned2022-11-23T17:42:45Z
dc.date.available2022-11-23T17:42:45Z
dc.date.created2022-11-21T10:46:24Z
dc.date.issued2022
dc.identifier.citationde la Cruz Dombriz, Álvaro Maldonado Torralba, Francisco José Mota, David . Dark matter candidate from torsion. Physics Letters B. 2022, 834
dc.identifier.urihttp://hdl.handle.net/10852/97784
dc.description.abstractThe stable pseudo-scalar degree of freedom of the quadratic Poincaré Gauge theory of gravity is shown to be a suitable dark matter candidate. We find the parameter space of the theory which can account for all the predicted cold dark matter, and constrain such parameters with astrophysical observations.
dc.languageEN
dc.publisherNorth-Holland
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleDark matter candidate from torsion
dc.title.alternativeENEngelskEnglishDark matter candidate from torsion
dc.typeJournal article
dc.creator.authorde la Cruz Dombriz, Álvaro
dc.creator.authorMaldonado Torralba, Francisco José
dc.creator.authorMota, David
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin2077104
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physics Letters B&rft.volume=834&rft.spage=&rft.date=2022
dc.identifier.jtitlePhysics Letters B
dc.identifier.volume834
dc.identifier.pagecount6
dc.identifier.doihttps://doi.org/10.1016/j.physletb.2022.137488
dc.subject.nviVDP::Astrofysikk, astronomi: 438
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0370-2693
dc.type.versionPublishedVersion
cristin.articleid137488


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