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SUPERNOVA NEUTRINO NUCLEOSYNTHESIS OF THE RADIOACTIVE Nb-92 OBSERVED IN PRIMITIVE METEORITES

Authors
Hayakawa, T.Nakamura, K.Kajino, T.Chiba, S.Iwamoto, N.Cheoun, M. K.Mathews, G. J.
Issue Date
10-Dec-2013
Publisher
IOP PUBLISHING LTD
Keywords
meteorites, meteors, meteoroids; neutrinos; supernovae: general
Citation
ASTROPHYSICAL JOURNAL LETTERS, v.779, no.1
Journal Title
ASTROPHYSICAL JOURNAL LETTERS
Volume
779
Number
1
URI
http://scholarworks.bwise.kr/ssu/handle/2018.sw.ssu/11093
DOI
10.1088/2041-8205/779/1/L9
ISSN
2041-8205
Abstract
The isotope Nb-92 decays to Zr-92 with a half-life of 3.47 x 10(7) yr. Although this isotope does not exist in the current solar system, initial abundance ratios for Nb-92/Nb-93 at the time of solar system formation have been measured in primitive meteorites. The astrophysical origin of this material, however, has remained unknown. In this Letter, we present new calculations which demonstrate a novel origin for Nb-92 via neutrino-induced reactions in core-collapse supernovae (nu-process). Our calculated result shows that the observed ratio of Nb-92/Nb-93 similar to 10(-5) can be explained by the nu-process.
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