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Gravitational waves in hybrid quintessential inflationary models

2011Conference object Open Access
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dc.contributor.authorSá, Paulo
dc.contributor.authorHenriques, Alfredo B.
dc.contributor.editorAldaya, V
dc.contributor.editorBarcelo, C
dc.contributor.editorJaramillo, JL
dc.date.accessioned2018-12-07T14:58:31Z
dc.date.available2018-12-07T14:58:31Z
dc.date.issued2011
dc.description.abstractThe generation of primordial gravitational waves is investigated within the hybrid quintessential inflationary model. Using the method of continuous Bogoliubov coefficients, we calculate the full gravitational-wave energy spectrum. The post-inflationary kination period, characteristic of quintessential inflationary models, leaves a clear signature on the spectrum, namely, a sharp rise of the gravitational-wave spectral energy density Omega(GW) at high frequencies. For appropriate values of the parameters of the model, Omega(GW) can be as high as 10(-12) in the MHz-GHz range of frequencies.
dc.description.sponsorshipFundacao para a Ciencia e a Tecnologia, Portugal
dc.identifier.doi10.1088/1742-6596/314/1/012062
dc.identifier.issn1742-6588
dc.identifier.urihttp://hdl.handle.net/10400.1/12071
dc.language.isoeng
dc.peerreviewedyes
dc.publisherIop Publishing Ltd
dc.relation.ispartofseriesJournal of Physics Conference Series
dc.subjectGraviton creation
dc.subjectEnergy density
dc.subjectUniverse
dc.subjectRadiation
dc.subjectDetector
dc.titleGravitational waves in hybrid quintessential inflationary models
dc.typeconference object
dspace.entity.typePublication
oaire.citation.conferencePlaceInst Astrofisica Andalucia (IAA-CSIC), Granada, SPAIN
oaire.citation.startPageUNSP 012062
oaire.citation.titleSpanish Relativity Meeting (Ere 2010) on Gravity As A Crossroad In Physics
oaire.citation.volume314
person.familyNameSá
person.givenNamePaulo
person.identifier.ciencia-id4116-AE55-DC83
person.identifier.orcid0000-0003-4321-0801
person.identifier.ridAAD-7568-2019
person.identifier.scopus-author-id7003787777
rcaap.rightsopenAccess
rcaap.typeconferenceObject
relation.isAuthorOfPublicationd9afc9c7-e997-4cab-b844-c42f7e54e3ab
relation.isAuthorOfPublication.latestForDiscoveryd9afc9c7-e997-4cab-b844-c42f7e54e3ab

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