The s-process between A = 120 and 124 - Signature of neutron density and temperature in red giants

Details The s-process between A = 120 and 124 - Signature of neutron density and temperature in red giants The s-process between A = 120 and 124 - Signature of neutron density and temperature in red giants

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...410..370k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 410, no. 1, p. 370-386.

Astronomy and Astrophysics

Astrophysics

15

Neutron Cross Sections, Nuclear Astrophysics, Red Giant Stars, Stellar Temperature, Abundance, Helium, Neutron Irradiation, Stellar Evolution, Stellar Models, Stellar Spectra

Scientific paper

To improve the s-process analysis in the mass range 120-130, additional cross section measurements were carried out on Sn-120, Sb-121, Sb-123, and Te-128. Improved calculations are also included for the cross sections of the branch point nuclei Sn-121 and Sb-122. Based on the new results, the astrophysical aspects are discussed with emphasis on detailed s-process analyses using the classical approach and a schematic stellar model, including also a first decomposition of the p-process abundance at A = 122.

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