Publication
DBI Galileon inflation in the light of Planck 2015
dc.contributor.author | Kumar, K. Sravan | |
dc.contributor.author | Sánchez, Juan C. Bueno | |
dc.contributor.author | Escamilla-Rivera, Celia | |
dc.contributor.author | Marto, João | |
dc.contributor.author | Moniz, Paulo | |
dc.date.accessioned | 2018-11-26T15:59:09Z | |
dc.date.available | 2018-11-26T15:59:09Z | |
dc.date.issued | 2016 | |
dc.description.abstract | In this work we consider a DBI Galileon (DBIG) inflationary model and constrain its parameter space with the Planck 2015 and BICEP2/Keck array and Planck (BKP) joint analysis data by means of a potential independent analysis. We focus our attention on inflationary solutions characterized by a constant or varying sound speed as well as warp factor. We impose bounds on stringy aspects of the model, such as the warp factor (f) and the induced gravity parameter (tilde m). We study the parameter space of the model and find that the tensor-to-scalar ratio can be as low as r sime 6 × 10−4 and inflation happens to be at GUT scale. In addition, we obtain the tilt of the tensor power spectrum and test the standard inflationary consistency relation (r = −8nt) against the latest bounds from the combined results of BKP+Laser Interferometer Gravitational-Waves Observatory (LIGO), and find that DBIG inflation predicts a red spectral index for the tensor power spectrum. | pt_PT |
dc.description.version | info:eu-repo/semantics/publishedVersion | pt_PT |
dc.identifier.citation | K. Sravan Kumar et al JCAP02(2016)063 | pt_PT |
dc.identifier.doi | 10.1088/1475-7516/2016/02/063 | pt_PT |
dc.identifier.uri | http://hdl.handle.net/10400.6/6500 | |
dc.language.iso | eng | pt_PT |
dc.peerreviewed | yes | pt_PT |
dc.publisher | IOP Publishing | pt_PT |
dc.relation.publisherversion | https://doi.org/10.1088/1475-7516/2016/02/063 | pt_PT |
dc.subject | Inflation | pt_PT |
dc.title | DBI Galileon inflation in the light of Planck 2015 | pt_PT |
dc.type | journal article | |
dspace.entity.type | Publication | |
oaire.awardURI | info:eu-repo/grantAgreement/FCT/5876/UID%2FMAT%2F00212%2F2013/PT | |
oaire.citation.endPage | 063 | pt_PT |
oaire.citation.issue | 02 | pt_PT |
oaire.citation.startPage | 063 | pt_PT |
oaire.citation.title | Journal of Cosmology and Astroparticle Physics | pt_PT |
oaire.citation.volume | 2016 | pt_PT |
oaire.fundingStream | 5876 | |
person.familyName | KUMAR | |
person.familyName | Pedro de Jesus Marto | |
person.familyName | Moniz | |
person.givenName | K. SRAVAN | |
person.givenName | João | |
person.givenName | Paulo | |
person.identifier | 277693 | |
person.identifier.ciencia-id | 5014-F2B1-1CEC | |
person.identifier.ciencia-id | 2F16-67B1-A930 | |
person.identifier.ciencia-id | B410-D0B7-55C1 | |
person.identifier.orcid | 0000-0002-3126-8195 | |
person.identifier.orcid | 0000-0003-3974-9177 | |
person.identifier.orcid | 0000-0001-7170-8952 | |
person.identifier.rid | M-9845-2013 | |
person.identifier.scopus-author-id | 56896293800 | |
person.identifier.scopus-author-id | 6701832578 | |
project.funder.identifier | http://doi.org/10.13039/501100001871 | |
project.funder.name | Fundação para a Ciência e a Tecnologia | |
rcaap.embargofct | Copyright cedido à editora no momento da publicação | pt_PT |
rcaap.rights | closedAccess | pt_PT |
rcaap.type | article | pt_PT |
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