Abstract
We consider the case of very low reheating scenarios () with a better calculation of the production of the relic neutrino background (with three-flavor oscillations). At 95% confidence level, a lower bound on the reheating temperature MeV is obtained from Big Bang Nucleosynthesis, while MeV from Planck data for very light ( eV) neutrinos. If neutrino masses are allowed to vary, Planck data yield MeV, the most stringent bound on the reheating temperature to date. Neutrino masses as large as 1 eV are possible for very low reheating temperatures.
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