The impact of the locally measured Hubble parameter on the mass of Sterile neutrino
arXiv:1910.08046 · doi:10.1093/mnras/stz2122
Abstract
We present a precise analysis to test hypothetical models involving sterile neutrinos beyond the standard flat-CDM cosmology with the CMB observations from the mission and BAO measurements. This analysis shows that adding the locally measured Hubble parameter = km Mp to the data removes the need for the informative physical prior in CMB constraints of . Under the constraints from the data containing the locally measured we obtain an upper limit eV scale mass for the massive sterile neutrino, and an upper limit eV scale mass for the three degenerate massive neutrino (95 per cent confidence level). We also obtain the value = (95 per cent confidence level), which is in compatibility with the constraints from 2015 CMB data at the 1 level. We find that introducing parameter to the model of cosmology reduces the 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 values.
arXiv comment8 pages, 4 figures
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