We consider cosmological models with a non-scale-invariant spectrum of primordial perturbations and assess whether they represent a viable alternative to the concordance Lambda CDM model. We find that in the framework of a model selection analysis, the WMAP and 2dF data do not provide any conclusive evidence in favor of one or the other kind of model. However, when a marginalization over the entire space of nuisance parameters is performed, models with a modified primordial spectrum and Omega(A) = 0 are strongly disfavored.

Inflation with primordial broken power law spectrum as an alternative to the concordance cosmological model / Pandolfi, Stefania; Elena, Giusarma; Massimiliano, Lattanzi; Melchiorri, Alessandro. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 81:10(2010), pp. 103007-103014. [10.1103/physrevd.81.103007]

Inflation with primordial broken power law spectrum as an alternative to the concordance cosmological model

PANDOLFI, STEFANIA;MELCHIORRI, Alessandro
2010

Abstract

We consider cosmological models with a non-scale-invariant spectrum of primordial perturbations and assess whether they represent a viable alternative to the concordance Lambda CDM model. We find that in the framework of a model selection analysis, the WMAP and 2dF data do not provide any conclusive evidence in favor of one or the other kind of model. However, when a marginalization over the entire space of nuisance parameters is performed, models with a modified primordial spectrum and Omega(A) = 0 are strongly disfavored.
2010
01 Pubblicazione su rivista::01a Articolo in rivista
Inflation with primordial broken power law spectrum as an alternative to the concordance cosmological model / Pandolfi, Stefania; Elena, Giusarma; Massimiliano, Lattanzi; Melchiorri, Alessandro. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 81:10(2010), pp. 103007-103014. [10.1103/physrevd.81.103007]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/376042
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