Light spinless particle coupled to photons

dc.contributor.authorMassó i Soler, Eduard, 1954-cat
dc.contributor.authorToldrà Sabaté, Ramoncat
dc.date.accessioned2010-05-06T09:07:41Z
dc.date.available2010-05-06T09:07:41Z
dc.date.issued1995cat
dc.description.abstractA pseudoscalar or scalar particle $\phi$ that couples to two photons but not to leptons, quarks and nucleons would have effects in most of the experiments searching for axions, since these are based on the $a \gamma \gamma $ coupling. We examine the laboratory, astrophysical and cosmological constraints on $\phi$ and study whether it may constitute a substantial part of the dark matter. We also generalize the $\phi$ interactions to possess $SU(2) \times U(1)$ gauge invariance, and analyze the phenomenological implications.
dc.format.extent9 p.cat
dc.format.mimetypeapplication/pdfeng
dc.identifier.idgrec508063cat
dc.identifier.issn0556-2821cat
dc.identifier.urihttps://hdl.handle.net/2445/12355
dc.language.isoengeng
dc.publisherThe American Physical Societyeng
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.52.1755cat
dc.relation.ispartofPhysical Review D, 1995, vol. 52, núm, 4, p. 1755-1763cat
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.52.1755
dc.rights(c) The American Physical Society, 1995eng
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física de la Matèria Condensada)
dc.subject.classificationAstronomiacat
dc.subject.classificationAstrofísicacat
dc.subject.classificationPartícules (Física nuclear)cat
dc.subject.otherAstronomyeng
dc.subject.otherAstrophysicseng
dc.subject.otherParticles (Nuclear physics)eng
dc.subject.otherDark matter (Astronomy)cat
dc.subject.otherMatèria fosca (Astronomia)eng
dc.titleLight spinless particle coupled to photonseng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion

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