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3-Form Cosmology: Phantom Behaviour, Singularities and Interactions

dc.contributor.authorMorais, João
dc.contributor.authorBouhmadi Lopez, Mariam
dc.contributor.authorMarto, João
dc.date.accessioned2018-03-06T09:34:03Z
dc.date.available2018-03-06T09:34:03Z
dc.date.issued2017
dc.description.abstractThe latest cosmological observations by the Planck collaboration (and combined with others) are compatible with a phantom-like behaviour (w < − 1) for the dark energy equation of state that drives the current acceleration of the Universe. With this mindset, we look into models where dark energy is described by a 3-form field minimally coupled to gravity. When compared to a scalar field, these models have the advantage of more naturally accommodating a cosmological-constant and phantom-like behaviours. We show how the latter happens for a fairly general class of positive-valued potentials, and through a dynamical system approach, we find that in such cases the 3-form field leads the Universe into a Little Sibling of the Big Rip singular event into the future. In this work, we explore the possibility of avoiding such singularity via an interaction in the dark sector between cold dark matter and the 3-form field. For the kind of interactions considered, we deduce a condition for replacing the LSBR by a late time de Sitter phase. For specific examples of interactions that meet this condition, we look for distinctive imprints in the statefinder hierarchy { S 3 ( 1 ) ; S 4 ( 1 ) } , { S 3 ( 1 ) ; S 5 ( 1 ) } , and in the growth rate of matter, e ( z ) , through the composite null diagnostic (CND).pt_PT
dc.description.sponsorshipThe work of MBL is supported by the Portuguese Agency “Fundação para a Ciência e Tecnologia” through an Investigador FCT Research contract, with reference IF/01442/2013/ CP1196/CT0001. She and JMorais wish to acknowledge the partial support from the Basque government Grant No. IT592-13 (Spain) and FONDOS FEDER under grant FIS2014-57956-P (Spanish government). J. Morais is also thankful to UPV/EHU for a PhD fellowship and UBI for hospitality during the completion of part of this work. The authors acknowledge the COST Action CA15117 (CANTATA).
dc.description.versioninfo:eu-repo/semantics/publishedVersionpt_PT
dc.identifier.doi10.3390/universe3010021pt_PT
dc.identifier.urihttp://hdl.handle.net/10400.6/4610
dc.language.isoengpt_PT
dc.peerreviewedyespt_PT
dc.publisherMDPIpt_PT
dc.relationWhat is the hand that rocks the "cradle” of the accelerating universe?
dc.relation.publisherversionhttp://www.mdpi.com/2218-1997/3/1/21pt_PT
dc.subjectDark energy 3-formspt_PT
dc.subjectDM-DE interactionpt_PT
dc.subjectDark energy 3-formspt_PT
dc.subjectFuture singularitiespt_PT
dc.subjectCosmographypt_PT
dc.subjectStatefinders approachpt_PT
dc.subjectGrowth ratept_PT
dc.subjectDynamical systemspt_PT
dc.title3-Form Cosmology: Phantom Behaviour, Singularities and Interactionspt_PT
dc.typejournal article
dspace.entity.typePublication
oaire.awardTitleWhat is the hand that rocks the "cradle” of the accelerating universe?
oaire.awardURIinfo:eu-repo/grantAgreement/FCT/Investigador FCT/IF%2F01442%2F2013%2FCP1196%2FCT0001/PT
oaire.citation.issue1pt_PT
oaire.citation.startPage21pt_PT
oaire.citation.volume3pt_PT
oaire.fundingStreamInvestigador FCT
person.familyNameMorais
person.familyNameBouhmadi Lopez
person.familyNamePedro de Jesus Marto
person.givenNameJoão
person.givenNameMariam
person.givenNameJoão
person.identifier.ciencia-idCF1F-8611-C989
person.identifier.ciencia-id2F16-67B1-A930
person.identifier.orcid0000-0001-5090-8015
person.identifier.orcid0000-0002-1529-1889
person.identifier.orcid0000-0003-3974-9177
person.identifier.scopus-author-id55756497200
person.identifier.scopus-author-id6508339470
project.funder.identifierhttp://doi.org/10.13039/501100001871
project.funder.nameFundação para a Ciência e a Tecnologia
rcaap.rightsopenAccesspt_PT
rcaap.typearticlept_PT
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relation.isAuthorOfPublication9ec4e1a6-1809-4e39-b616-dca11241026d
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