Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 9, Pages -Publisher
IOP Publishing Ltd
DOI: 10.1088/1475-7516/2020/09/051
Keywords
big bang nucleosynthesis; cosmological neutrinos
Funding
- JSPS KAKENHI [17H01131, 17K05434]
- MEXT KAKENHI [15H05889]
- World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan
- Program of Excellence in Photon Science
- JSPS [20J20248]
- U.S. Department of Energy (DOE) [DE-SC0009937]
- Grants-in-Aid for Scientific Research [20J20248] Funding Source: KAKEN
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We consider the cosmological effects of sterile neutrinos with the masses of 150-450 MeV. The decay of sterile neutrinos changes the thermal history of the Universe and affects the energy density of radiation at recombination and the big bang nucleosynthesis (BBN) results. We derive severe constraints on the parameters of sterile neutrinos from the primordial abundances of helium-4 and deuterium. We also find that in a particular model the constraints can be considerably relaxed by assuming a large lepton asymmetry in the active neutrinos. In this case, the consistent parameters result in N-eff similar or equal to 3.2-3.4 and can alleviate the Hubble tension.
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