Neutrino-induced nucleosynthesis and the site of the r process

W. C. Haxton, K. Langanke, Y. Z. Qian

Research output: Contribution to journalArticlepeer-review

60 Scopus citations

Abstract

If the r process occurs deep within a type II supernova, probably the most popular of the proposed sites, abundances of r -process elements may be altered by the intense neutrino flux. We point out that the effects would be especially pronounced for eight isotopes that can be efficiently synthesized by the neutrino reactions following r -process freeze-out. We show that the observed abundances of these isotopes are entirely consistent with neutrino-induced nucleosynthesis, strongly arguing for a supernova r -process site. The deduced neutrino fluences place stringent constraints on the freeze-out radius and dynamic time scale of the r process.

Original languageEnglish (US)
Pages (from-to)2694-2697
Number of pages4
JournalPhysical review letters
Volume78
Issue number14
DOIs
StatePublished - Apr 7 1997
Externally publishedYes

Fingerprint Dive into the research topics of 'Neutrino-induced nucleosynthesis and the site of the r process'. Together they form a unique fingerprint.

Cite this