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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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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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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1768544314877542400 |