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A varying dark energy effective speed of sound parameter in the phantom Universe

dc.contributor.authorAlbarran, Imanol
dc.contributor.authorBouhmadi Lopez, Mariam
dc.contributor.authorMarto, João
dc.date.accessioned2021-09-16T10:41:42Z
dc.date.available2021-09-16T10:41:42Z
dc.date.issued2021-09-09
dc.description.abstractWe analyse the phenomenological effects of a varying Dark Energy (DE) effective speed of sound parameter, c2sd, on the cosmological perturbations of three phantom DE models. Each of these models induce a particular abrupt future event known as Big Rip (BR), Little Rip (LR), and Little Sibling of the Big Rip (LSBR). In this class of abrupt events, all the bound structures in the Universe would be ripped apart at a finite cosmic time. We compute the evolution of the perturbations, fσ8 growth rate and forecast the current matter power spectrum. We vary the c2sd parameter in the interval [0, 1] and compute the relative deviation with respect c2sd=1. In addition, we analyse the effect of gravitational potential sign flip that occurs at very large scale factors as compared with the current one.pt_PT
dc.description.sponsorshipThe research of M. B.-L. is supported by the Basque Foundation of Science Ikerbasque. She also would like to acknowledge the partial support from the Basque government Grant No. IT956-16 (Spain) and the project FIS2017-85076-P (MINECO/AEI/FEDER, UE). IA and JM are supported by the grant UIDB/MAT/00212/2020pt_PT
dc.description.sponsorshipThe research of M. B.-L. is supported by the Basque Foundation of Science Ikerbasque. She also would like to acknowledge the partial support from the Basque government Grant No. IT956-16 (Spain) and the project FIS2017- 85076-P (MINECO/AEI/FEDER, UE). IA and JM are supported by the grant UIDB/MAT/00212/2020.
dc.description.versioninfo:eu-repo/semantics/publishedVersionpt_PT
dc.identifier.citationAlbarran, I., Bouhmadi-López, M. & Marto, J. A varying dark energy effective speed of sound parameter in the phantom Universe. Eur. Phys. J. C 81, 803 (2021). https://doi.org/10.1140/epjc/s10052-021-09546-2pt_PT
dc.identifier.doi10.1140/epjc/s10052-021-09546-2pt_PT
dc.identifier.urihttp://hdl.handle.net/10400.6/11210
dc.language.isoengpt_PT
dc.peerreviewedyespt_PT
dc.publisherSpringerpt_PT
dc.relationCenter of Mathematics and Applications of University of Beira Interior
dc.relation.publisherversionhttps://link.springer.com/article/10.1140/epjc/s10052-021-09546-2pt_PT
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/pt_PT
dc.subjectDark energypt_PT
dc.subjectPhantom modelspt_PT
dc.subjectCosmological perturbationspt_PT
dc.titleA varying dark energy effective speed of sound parameter in the phantom Universept_PT
dc.typejournal article
dspace.entity.typePublication
oaire.awardTitleCenter of Mathematics and Applications of University of Beira Interior
oaire.awardURIinfo:eu-repo/grantAgreement/FCT/6817 - DCRRNI ID/UIDB%2F00212%2F2020/PT
oaire.citation.issue9pt_PT
oaire.citation.titleThe European Physical Journal Cpt_PT
oaire.citation.volume81pt_PT
oaire.fundingStream6817 - DCRRNI ID
person.familyNameAlbarran
person.familyNameBouhmadi Lopez
person.familyNamePedro de Jesus Marto
person.givenNameImanol
person.givenNameMariam
person.givenNameJoão
person.identifier.ciencia-idCF1F-8611-C989
person.identifier.ciencia-id2F16-67B1-A930
person.identifier.orcid0000-0003-4278-9372
person.identifier.orcid0000-0002-1529-1889
person.identifier.orcid0000-0003-3974-9177
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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