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EMERGENT UNIVERSE SCENARIO AND THE LOW CMB MULTIPOLES

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dc.creatorPEDRO ALBERTO LABRAÑA MORAGA
dc.date2015
dc.date.accessioned2025-01-10T14:38:05Z
dc.date.available2025-01-10T14:38:05Z
dc.date.issued2015
dc.description.abstractIN THIS PAPER, BASED ON PHYS. REV. D 91, NO. 8, 083534 (2015), WE STUDY SUPER INFLATION IN THE CONTEXT OF THE EMERGENT UNIVERSE (EU) SCENARIO. THE EXISTENCE OF A SUPER INFLATING PHASE BEFORE THE ONSET OF SLOW ROLL INFLATION ARISES IN ANY EMERGENT UNIVERSE MODEL. WE FOUND THAT THE SUPER INFLATIONARY PERIOD IN THE EU SCENARIO PRODUCES A SUPPRESSION OF THE CMB ANISOTROPIES AT LARGE SCALE WHICH COULD BE RESPONSIBLE OF THE OBSERVED LACK OF POWER AT LARGE ANGULAR SCALES OF THE CMB.
dc.formatapplication/pdf
dc.identifier.doi10.1088/1742-6596/720/1/012016
dc.identifier.issn2470-0029
dc.identifier.issn2470-0010
dc.identifier.issn1550-2368
dc.identifier.issn1550-7998
dc.identifier.urihttps://repositorio.ubiobio.cl/handle/123456789/8288
dc.languagespa
dc.publisherPHYSICAL REVIEW D
dc.relation.uri10.1088/1742-6596/720/1/012016
dc.rightsPUBLICADA
dc.titleEMERGENT UNIVERSE SCENARIO AND THE LOW CMB MULTIPOLES
dc.typeARTÍCULO
dspace.entity.typePublication
ubb.EstadoPUBLICADA
ubb.Otra ReparticionDEPARTAMENTO DE FISICA
ubb.SedeCONCEPCIÓN
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