Publication:
Spontaneous scalarization

dc.contributor.coauthorDoneva, Daniela D.
dc.contributor.coauthorSilva, Hector O.
dc.contributor.coauthorSotiriou, Thomas P.
dc.contributor.coauthorYazadjiev, Stoytcho S.
dc.contributor.departmentDepartment of Physics
dc.contributor.kuauthorRamazanoğlu, Fethi Mübin
dc.contributor.otherDepartment of Physics
dc.contributor.schoolcollegeinstituteCollege of Sciences
dc.date.accessioned2024-12-29T09:39:37Z
dc.date.issued2024
dc.description.abstractScalarization is a mechanism that endows strongly self -gravitating bodies, such as neutron stars and black holes, with a scalar -field configuration. It resembles a phase transition in that the scalar configuration appears only when a certain quantity that characterizes the compact object, for example, its compactness or spin, is beyond a threshold. A critical and comprehensive review of scalarization, including the mechanism itself, theories that exhibit it, its manifestation in neutron stars, black holes and their binaries, potential extension to other fields, and a thorough discussion of future perspectives, is provided.
dc.description.indexedbyWoS
dc.description.indexedbyScopus
dc.description.issue1
dc.description.publisherscopeInternational
dc.description.sponsorsD. D. D. acknowledges financial support via the Emmy Noether Research Group, which was funded by the German Research Foundation (DFG) under Grant No. DO 1771/1-1. S. S. Y. thanks the University of Tubingen for the financial support and acknowledges partial support from Bulgarian NSF Grant No. KP-06-H28/7. T. P. S. acknowledges partial support from STFC Consolidated Grants No. ST/T000732/1 and No. ST/V005596/1. F. M. R. acknowledges support from 2020 Bilim Akademisi GEB & Idot;P award and TUB & Idot;TAK Project No. 122F097. H. O. S. acknowledges funding from Deutsche Forschungsgemeinschaft (DFG) Project No. 386119226. We also acknowledge the networking support of COST Actions No. CA16104 and No. CA15117.
dc.description.volume96
dc.identifier.doi10.1103/RevModPhys.96.015004
dc.identifier.eissn1539-0756
dc.identifier.issn0034-6861
dc.identifier.quartileQ1
dc.identifier.scopus2-s2.0-85187526381
dc.identifier.urihttps://doi.org/10.1103/RevModPhys.96.015004
dc.identifier.urihttps://hdl.handle.net/20.500.14288/23067
dc.identifier.wos1187950600001
dc.keywordsGravitation
dc.keywordsStars
dc.keywordsBlack holes
dc.keywordsCompact objects
dc.keywordsFuture perspectives
dc.keywordsGravitating body
dc.keywordsNeutron stars
dc.keywordsScalar fields
dc.keywordsScalarization
dc.languageen
dc.publisherAmerican Physical Society
dc.relation.grantnoEmmy Noether Research Group - German Research Foundation (DFG)
dc.relation.grantnoUniversity of Tubingen
dc.relation.grantnoBulgarian NSF [ST/T000732/1]
dc.relation.grantnoSTFC [ST/V005596/1, 386119226]
dc.relation.grantnoDeutsche Forschungsgemeinschaft (DFG) [CA15117]
dc.relation.grantnoCOST Actions [DO 1771/1-1. S. S]
dc.relation.grantno[KP-06-H28/7]
dc.relation.grantno[CA16104]
dc.sourceReviews of Modern Physics
dc.subjectBlack holes
dc.subjectNeutron stars
dc.subjectGeneral relativity
dc.titleSpontaneous scalarization
dc.typeReview
dspace.entity.typePublication
local.contributor.kuauthorRamazanoğlu, Fethi Mübin
relation.isOrgUnitOfPublicationc43d21f0-ae67-4f18-a338-bcaedd4b72a4
relation.isOrgUnitOfPublication.latestForDiscoveryc43d21f0-ae67-4f18-a338-bcaedd4b72a4

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