nuclear evolution

Nuclear evolution in the Sun and in first generation stars

Science

195

3. The NS acts as a giant nucleus, decaying with the emission of neutrons (Q = 10-22 Mev/neutron; t_1/2 approximatly equals to 10¹⁰ years) [Abstract 1041, Lunar Planetary Science Conference XXXII, LPI Contribution No. 1080, ISSN No. 0161-5297, (2001)].

Meteoritics

⁴³

The above scenario is consistent with isotopic ratios in the solar wind (SW) and with the observed fluxes of solar neutrinos and SW-protons