http://arxiv.org/abs/1708.04899
We show that the reheating temperature of a matter-domination era in the early universe can be pushed down close to $1 \mathinner{\mathrm{MeV}}$ if the reheating takes place through non-hadronic decays of the dominant matter and neutrino-antineutrino asymmetries are still large enough, $|L| \gtrsim \mathcal{O}(10^{-2}-1)$ (depending on the neutrino flavor) at the end of reheating.
G. Barenboim and W. Park
Thu, 17 Aug 17
35/50
Comments: 6 pages, 2 figures