arXiv:1511.00672·v1·Cosmology and Nongalactic Astrophysics
Bounds on very low reheating scenarios after Planck
P.F. de Salas🇪🇸 · M. Lattanzi🇮🇹 · G. Mangano🇮🇹 · G. Miele🇮🇹 · S. Pastor🇪🇸 · O. Pisanti🇮🇹
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.
Comments: 9 pages, 9 figures