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dc.date.accessioned2017-08-15T13:17:44Z
dc.date.available2017-08-15T13:17:44Z
dc.date.created2015-01-14T10:23:33Z
dc.date.issued2014
dc.identifier.citationLlinares, Claudio Pogosian, Levon . Domain walls coupled to matter: The symmetron example. Physical Review D. 2014, 90(12)
dc.identifier.urihttp://hdl.handle.net/10852/57055
dc.description.abstractWe study properties of domain walls in the symmetron model, in which the scalar gravitational degree of freedom decouples from matter in regions of high density and exhibits a spontaneously broken Z2 symmetry at low densities. The nonminimal coupling of the scalar to matter leads to a host of interesting properties of the domain walls that are not present in minimally coupled theories. We estimate the cosmological energy fraction in domain walls and find that this leads to an upper bound on the redshift of the symmetry breaking. We also show that a spherical symmetron wall can remain stable if it is “pinned” on matter halos and derive a criterion for the stability. In addition, we present results of numerical simulations of representative interactions between domain walls and matter overdensities. © 2014 American Physical Societyen_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleDomain walls coupled to matter: The symmetron exampleen_US
dc.typeJournal articleen_US
dc.creator.authorLlinares, Claudio
dc.creator.authorPogosian, Levon
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1197393
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review D&rft.volume=90&rft.spage=&rft.date=2014
dc.identifier.jtitlePhysical Review D
dc.identifier.volume90
dc.identifier.issue12
dc.identifier.pagecount12
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevD.90.124041
dc.identifier.urnURN:NBN:no-59805
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn1550-7998
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/57055/1/PhysRevD.90.124041.pdf
dc.type.versionPublishedVersion
cristin.articleid124041


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