The s-process branching at Kr-85

Details The s-process branching at Kr-85 The s-process branching at Kr-85

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...155..247w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 155, no. 2, Feb. 1986, p. 247-255.

Astronomy and Astrophysics

Astrophysics

17

Absorption Cross Sections, Krypton 85, Meteoritic Composition, Neutron Cross Sections, Nuclear Reactions, Abundance, Fluence, Murchison Meteorite, Orgueil Meteorite, Rubidium Isotopes, Strontium Isotopes

Scientific paper

The Maxwellian average neutron capture cross sections of 86Kr, 85Rb and 87Rb have been measured at kT = 25 keV by activation. These data together with recently published neutron capture cross sections of Kr and Sr isotopes allow for a determination of the neutron density of the weak s-process component in the framework of the classical s-process model with two independent fluence distributions. The s-process abundances from this study are compared with the pure s-process krypton discovered in primitive meteorites.

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