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Authordc.contributor.authorMooij, Sander 
Authordc.contributor.authorPalma Quilodrán, Gonzalo 
Admission datedc.date.accessioned2016-01-05T15:07:24Z
Available datedc.date.available2016-01-05T15:07:24Z
Publication datedc.date.issued2015
Cita de ítemdc.identifier.citationJournal of Cosmology and Astroparticle Physics Número: 11 Número de artículo: 025 (2015)en_US
Identifierdc.identifier.otherdoi: 10.1088/1475-7516/2015/11/025
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/136175
General notedc.descriptionArtículo de publicación ISIen_US
Abstractdc.description.abstractNon-attractor models of inflation are characterized by the super-horizon evolution of curvature perturbations, introducing a violation of the non-Gaussian consistency relation between the bispectrum's squeezed limit and the power spectrum's spectral index. In this work we show that the bispectrum's squeezed limit of non-attractor models continues to respect a relation dictated by the evolution of the background. We show how to derive this relation using only symmetry arguments, without ever needing to solve the equations of motion for the perturbations.en_US
Patrocinadordc.description.sponsorshipFondecyt, "Anillo" project - "Programa de Investigacion Asociativa", Greek national funds under the "ARISTEIA" Action, Dedicacion exclusica program at UDEA, Dedicacion Sostenibilidad program at UDEA, UDEA CODI project.en_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherIOP Pressen_US
Type of licensedc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectCosmological perturbation theoryen_US
Keywordsdc.subjectInflationen_US
Títulodc.titleConsistently violating the non-Gaussian consistency relationen_US
Document typedc.typeArtículo de revista


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Atribución-NoComercial-SinDerivadas 3.0 Chile
Except where otherwise noted, this item's license is described as Atribución-NoComercial-SinDerivadas 3.0 Chile