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arXiv · 1112.3006

The Impact of Assuming Flatness in the Determination of Neutrino Properties from Cosmological Data

Aaron Smith·Maria Archidiacono·Asantha Cooray·Francesco De Bernardis·Alessandro Melchiorri·Joseph Smidt
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Abstract

Cosmological data have provided new constraints on the number of neutrino species and the neutrino mass. However these constraints depend on assumptions related to the underlying cosmology. Since a correlation is expected between the number of effective neutrinos N_{eff}, the neutrino mass \sum m_ν, and the curvature of the universe Ω_k, it is useful to investigate the current constraints in the framework of a non-flat universe. In this paper we update the constraints on neutrino parameters by making use of the latest cosmic microwave background (CMB) data from the ACT and SPT experiments and consider the possibility of a universe with non-zero curvature. We first place new constraints on N_{eff} and Ω_k, with N_{eff} = 4.03 +/- 0.45 and 10^3 Ω_k = -4.46 +/- 5.24. Thus, even when Ω_k is allowed to vary, N_{eff} = 3 is still disfavored with 95% confidence. We then investigate the correlation between neutrino mass and curvature that shifts the 95% upper limit of \sum m_ν< 0.45 eV to \sum m_ν< 0.95 eV. Thus, the impact of assuming flatness in neutrino cosmology is significant and an essential consideration with future experiments.

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Aaron Smith, Maria Archidiacono, Asantha Cooray, Francesco De Bernardis, Alessandro Melchiorri, Joseph Smidt. 2012-06-01. The Impact of Assuming Flatness in the Determination of Neutrino Properties from Cosmological Data. https://doi.org/10.1103/physrevd.85.123521

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