Neutrinos and Supermassive Stars: Prospects for Neutrino Emission and Detection
Authors: Xiangdong Shi and George
M. Fuller
Shi &
Fuller
1998 The Astrophysical Journal503307.
Provider: AAS Journals
Caption: Fig. 2.
Time evolution of the neutrino luminosity according to eq. (17), for ﹩M^{\mathrm{HC}\,}_{5}=1﹩. The neutrino emission stops when the radius of the core R enters the horizon.