Scaling relations for the supernova γ-process and the 176Lu nuclear cosmochronometer

Details Scaling relations for the supernova γ-process and the 176Lu nuclear cosmochronometer Scaling relations for the supernova γ-process and the 176Lu nuclear cosmochronometer

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nupha.758..525h&link_type=abstract

Nuclear Physics A, Volume 758, p. 525-528.

Physics

Nuclear Physics

5

Scientific paper

Analyzing the solar system abundances, we find two universal scaling relations concerning the p- and s-nuclei. These scalings indicate that the γ-process nucleosynthesis in supernova (SN) explosions is the most probable origin of the p-nuclei. In addition the scalings lead to new concepts: a universality of the γ-process and a new nuclear cosmochronometer. Calculations of the γ-process are carried out for typical core-collapse SN explosion models. These confirm the observed scalings.

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