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2019MNRAS.488.5763E - Mon. Not. R. Astron. Soc., 488, 5763-5770 (2019/October-1)

The impact of the locally measured Hubble parameter on the mass of sterile neutrino.

EBADINEJAD M.

Abstract (from CDS):

We present a precise analysis to test hypothetical models involving sterile neutrinos beyond the standard flat-ΛCDM cosmology with the CMB observations from the Planck mission and BAO measurements. This analysis shows that adding the locally measured Hubble parameter H0 = 73.00 ± 1.75 km s–1 Mpc–1 to the data removes the need for the informative physical m_ sterile_^ thermal^ prior in CMB constraints of m_ν, sterile_^ eff^. Under the constraints from the data containing the locally measured H0 we obtain an upper limit m_ν, sterile_^ eff^ < 0.306 eV scale mass for the massive sterile neutrino, and an upper limit Σmν < 0.214 eV scale mass for the three degenerate massive neutrino (95 per cent confidence level). We also obtain the value σ8 = 0.81+0.05–0.06 (95 per cent confidence level), which is in compatibility with the constraints from Planck 2015 CMB data at the 1σ level. We find that introducing parameter m_ν, sterile_^ eff^ to the model of cosmology reduces the σ8 value and moves it closer to the obtained value for this parameter from the KiDS-450 analysis. Our results show that the locally measured Hubble parameter can increase constraints on σ8 values.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): astroparticle physics - neutrinos - cosmic background radiation - early Universe - cosmology: observations

Simbad objects: 1

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