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dc.contributor.authorBarrow, John D
dc.date.accessioned2020-02-20T13:32:00Z
dc.date.available2020-02-20T13:32:00Z
dc.date.issued2020-02-20
dc.date.submitted2019-09-19
dc.identifier.issn0264-9381
dc.identifier.othercqgab7074
dc.identifier.otherab7074
dc.identifier.othercqg-106431.r1
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/302431
dc.descriptionFunder: STFC
dc.description.abstractAbstract: We show that cosmological sudden singularities that respect the energy conditions can occur at finite times in Brans–Dicke and more general scalar-tensor theories of gravity. We construct these explicitly in the Friedmann universes. Higher-order versions of these singularities are also possible, including those that arise with when scalar fields have a self-interaction potential of power-law form.
dc.languageen
dc.publisherIOP Publishing
dc.rightsAttribution 4.0 International (CC BY 4.0)en
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en
dc.subjectPaper
dc.subjectcosmology
dc.subjectscalar–tensor gravity
dc.subjectsingularities
dc.titleSudden Brans–Dicke singularities
dc.typeArticle
dc.date.updated2020-02-20T13:31:59Z
prism.issueIdentifier6
prism.publicationNameClassical and Quantum Gravity
prism.volume37
dc.identifier.doi10.17863/CAM.49502
dcterms.dateAccepted2020-01-27
rioxxterms.versionofrecord10.1088/1361-6382/ab7074
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
dc.contributor.orcidBarrow, John D [0000-0002-6083-9751]
dc.identifier.eissn1361-6382


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Attribution 4.0 International (CC BY 4.0)
Except where otherwise noted, this item's licence is described as Attribution 4.0 International (CC BY 4.0)