Origin of the odd-even staggering in the A ≅ 80 solar r-abundance peak.

Details Origin of the odd-even staggering in the A ≅ 80 solar r-abundance peak. Origin of the odd-even staggering in the A ≅ 80 solar r-abundance peak.

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990zphya.336..357k&link_type=abstract

Z. Phys., A, Vol. 336, No. 3, p. 357 - 358

Physics

5

Nucleosynthesis: Solar Abundances

Scientific paper

In contrast to the conventional picture, the r-process yields in the A
≅ 80 abundance peak exhibit a pronounced odd-even staggering. It is
proposed that this behaviour may be due to strong β-delayed neutron
branching from a few odd-mass isotopes located in or close to the
r-process path.

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