Early universe sources for CMB non-gaussianity

In the framework of inflationary models with non-vacuum initial states for cosmological perturbations, we study non-Gaussian signatures on the cosmic microwave background (CMB) radiation produced by a broken-scale-invariant model which incorporates a feature at a privileged scale in the primordial p...

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Publicado: 2002
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Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0217751X_v17_n29_p4273_Gangui
http://hdl.handle.net/20.500.12110/paper_0217751X_v17_n29_p4273_Gangui
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spelling paper:paper_0217751X_v17_n29_p4273_Gangui2023-06-08T15:21:07Z Early universe sources for CMB non-gaussianity Cosmic microwave background Inflation calculation conference paper cosmos mathematical analysis microwave radiation physics vacuum In the framework of inflationary models with non-vacuum initial states for cosmological perturbations, we study non-Gaussian signatures on the cosmic microwave background (CMB) radiation produced by a broken-scale-invariant model which incorporates a feature at a privileged scale in the primordial power spectrum. 2002 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0217751X_v17_n29_p4273_Gangui http://hdl.handle.net/20.500.12110/paper_0217751X_v17_n29_p4273_Gangui
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Cosmic microwave background
Inflation
calculation
conference paper
cosmos
mathematical analysis
microwave radiation
physics
vacuum
spellingShingle Cosmic microwave background
Inflation
calculation
conference paper
cosmos
mathematical analysis
microwave radiation
physics
vacuum
Early universe sources for CMB non-gaussianity
topic_facet Cosmic microwave background
Inflation
calculation
conference paper
cosmos
mathematical analysis
microwave radiation
physics
vacuum
description In the framework of inflationary models with non-vacuum initial states for cosmological perturbations, we study non-Gaussian signatures on the cosmic microwave background (CMB) radiation produced by a broken-scale-invariant model which incorporates a feature at a privileged scale in the primordial power spectrum.
title Early universe sources for CMB non-gaussianity
title_short Early universe sources for CMB non-gaussianity
title_full Early universe sources for CMB non-gaussianity
title_fullStr Early universe sources for CMB non-gaussianity
title_full_unstemmed Early universe sources for CMB non-gaussianity
title_sort early universe sources for cmb non-gaussianity
publishDate 2002
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0217751X_v17_n29_p4273_Gangui
http://hdl.handle.net/20.500.12110/paper_0217751X_v17_n29_p4273_Gangui
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