Neutrino Nucleosynthesis

Preprint

31 July 2003

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0307546

Abstract

We study neutrino process nucleosynthesis in massive stars using newly calculated cross sections, an expanded reaction network, and complete and self-consistent models of the progenitor star. We reevaluate the production of light isotopes from abundant progenitors as well as that of rare, heavy, proton-rich isotopes. In particular, new results are given for B11, F19, La138, and Ta180. The production of these isotopes places limits on neutrino spectrum and oscialltions.

Keywords

NEUTRINO NUCLEOSYNTHESIS
PROCESS NUCLEOSYNTHESIS
NEUTRINO PROCESS
STUDY NEUTRINO
MASSIVE STARS
USING NEWLY
ISOTOPES
STARS

All Related Versions

Version 1, 2003-07-31, ArXiv
Published version: Physics Letters B, 606 (3-4), 258.

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