The well-tempered cosmological constant

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dc.contributor.authorLinder, Eric V.
dc.contributor.authorAppleby, Stephen
dc.contributor.authorAppleby, Stephen
dc.date.accessioned2025-08-18T15:50:08Z
dc.date.available2025-08-18T15:50:08Z
dc.date.issued2018-07-01
dc.description.abstractWithin cubic Horndeski gravity we construct ‘well-tempered’ models where scalar self-tuning cancels any cosmological constant while preserving radiation/matter eras and enabling de Sitter expansion with H independent of Λ, avoiding the usual suppression of all sources.en
dc.identifier.citationAppleby, S.; Linder, E. V. (2018). The well-tempered cosmological constant. JCAP, 2018(07), 034. DOI: 10.1088/1475-7516/2018/07/034en
dc.identifier.doi10.1088/1475-7516/2018/07/034
dc.identifier.issn1475-7516
dc.identifier.otherFilename:10.1088_1475-7516_2018_07_034.pdf
dc.identifier.urihttps://doi.org/10.1088/1475-7516/2018/07/034
dc.identifier.urihttps://nur.nu.edu.kz/handle/123456789/9313
dc.language.isoen
dc.publisherIOP Publishing / SISSA
dc.relation.ispartofJournal of Cosmology and Astroparticle Physicsen
dc.sourceJournal of Cosmology and Astroparticle Physics, 2018(07), 034, (2018)en
dc.subjectscalar-tensor gravityen
dc.subjectself tuningen
dc.subjectcosmological constant problemen
dc.subjectHorndeski theoryen
dc.subjectmodified gravityen
dc.subjectmodified gravityen
dc.titleThe well-tempered cosmological constanten
dc.typeJournal Articleen

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