Dynamical dark energy in minimally modified gravity

2022
journal article
article
8
dc.abstract.enMinimally modified gravity is a class of models with only the two tensor degrees of freedom as in general relativity. Using the framework with auxiliary constraints these models can maintain a dynamical cosmological background. The form of the constraints is thereby restricted by the requirement of dynamical dark energy and the avoidance of a breakdown of perturbation theory. Studying the linear perturbations around the FLRW background the results are, however, quite insensitive to the details of the constraints leading to a modified effective gravitational constant or a non-vanishing sound speed for dust.pl
dc.affiliationWydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut Fizyki Teoretycznejpl
dc.contributor.authorGanz, Alexander - 444046 pl
dc.date.accessioned2023-02-07T09:55:50Z
dc.date.available2023-02-07T09:55:50Z
dc.date.issued2022pl
dc.description.number8pl
dc.description.volume2022pl
dc.identifier.articleid074pl
dc.identifier.doi10.1088/1475-7516/2022/08/074pl
dc.identifier.eissn1475-7516pl
dc.identifier.urihttps://ruj.uj.edu.pl/xmlui/handle/item/307385
dc.languageengpl
dc.language.containerengpl
dc.rightsUdzielam licencji. Uznanie autorstwa 4.0 Międzynarodowa*
dc.rights.licenceBez licencji otwartego dostępu
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/legalcode.pl*
dc.source.integratorfalse
dc.subject.enmodified gravitypl
dc.subject.endark energy theorypl
dc.subject.encosmological perturbation theory in GR and beyondpl
dc.subject.engravitational waves in GR and beyond : theorypl
dc.subtypeArticlepl
dc.titleDynamical dark energy in minimally modified gravitypl
dc.title.journalJournal of Cosmology and Astroparticle Physicspl
dc.typeJournalArticlepl
dspace.entity.typePublication
dc.abstract.enpl
Minimally modified gravity is a class of models with only the two tensor degrees of freedom as in general relativity. Using the framework with auxiliary constraints these models can maintain a dynamical cosmological background. The form of the constraints is thereby restricted by the requirement of dynamical dark energy and the avoidance of a breakdown of perturbation theory. Studying the linear perturbations around the FLRW background the results are, however, quite insensitive to the details of the constraints leading to a modified effective gravitational constant or a non-vanishing sound speed for dust.
dc.affiliationpl
Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut Fizyki Teoretycznej
dc.contributor.authorpl
Ganz, Alexander - 444046
dc.date.accessioned
2023-02-07T09:55:50Z
dc.date.available
2023-02-07T09:55:50Z
dc.date.issuedpl
2022
dc.description.numberpl
8
dc.description.volumepl
2022
dc.identifier.articleidpl
074
dc.identifier.doipl
10.1088/1475-7516/2022/08/074
dc.identifier.eissnpl
1475-7516
dc.identifier.uri
https://ruj.uj.edu.pl/xmlui/handle/item/307385
dc.languagepl
eng
dc.language.containerpl
eng
dc.rights*
Udzielam licencji. Uznanie autorstwa 4.0 Międzynarodowa
dc.rights.licence
Bez licencji otwartego dostępu
dc.rights.uri*
http://creativecommons.org/licenses/by/4.0/legalcode.pl
dc.source.integrator
false
dc.subject.enpl
modified gravity
dc.subject.enpl
dark energy theory
dc.subject.enpl
cosmological perturbation theory in GR and beyond
dc.subject.enpl
gravitational waves in GR and beyond : theory
dc.subtypepl
Article
dc.titlepl
Dynamical dark energy in minimally modified gravity
dc.title.journalpl
Journal of Cosmology and Astroparticle Physics
dc.typepl
JournalArticle
dspace.entity.type
Publication
Affiliations

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