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Constraints on the neutrino mass and mass hierarchy from cosmological observations
Constraints on the neutrino mass and mass hierarchy from cosmological observations
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Constraints on the neutrino mass and mass hierarchy from cosmological observations
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Constraints on the neutrino mass and mass hierarchy from cosmological observations
Constraints on the neutrino mass and mass hierarchy from cosmological observations
Journal Article

Constraints on the neutrino mass and mass hierarchy from cosmological observations

2016
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Overview
Considering the mass splitting between three active neutrinos, we represent the new constraints on the sum of neutrino mass ∑ m ν by updating the anisotropic analysis of the Baryon Acoustic Oscillation (BAO) scale in the CMASS and LOWZ galaxy samples from Data Release 12 of the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS DR12). Combining the BAO data of 6dFGS, MGS, LOWZ and CMASS with Planck  2015 data of temperature anisotropy and polarizations of the Cosmic Microwave Background (CMB), we find that the 95 % C.L. upper bounds on ∑ m ν refer to ∑ m ν , N H < 0.18 eV for the normal hierarchy (NH), ∑ m ν , I H < 0.20 eV for the inverted hierarchy (IH) and ∑ m ν , D H < 0.15 eV for the degenerate hierarchy (DH), respectively, and the normal hierarchy is slightly preferred over the inverted one ( Δ χ 2 ≡ χ NH 2 - χ IH 2 ≃ - 3.4 ). In addition, the additional relativistic degrees of freedom and massive sterile neutrinos are neither favored at present.

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