NEUTRINO PROCESS NUCLEOSYNTHESIS AND THE B-11 B-10 RATIO

We consider the evolution of the light elements (Li, Be, and B) incorp orating the effects of their production by both neutrino process and c osmic-ray nucleosynthesis. We test the viability of the neutrino proce ss to resolve the long standing problem of the B-11/B-10 isotopic rati o which amounts to 4 at the time of the formation of the solar system. This hypothesis may be ultimately constrained by the B/Be ratio obser ved in halo stars. Though we are able to obtain a solar isotopic ratio B-11/B-10 approximately 4, the current paucity of data at low metalli city prevents us from making a definitive conclusion regarding the res olution of this problem. We show, however, that neutrino process nucle osynthesis leads to a relatively model independent prediction that the B/Be elemental ratio is large (>50) at low metallicities ([Fe/H] < -3 .0), if Be is produced as a secondary element (as is the case in the c onventional scenario of galactic cosmic-ray nucleosynthesis).