Tables of nuclear cross sections and reaction rates : An addendum to the paper "Astrophysical reaction rates from statistical model calculations"

By T. Rauscher, Friedrich-Karl Thielemann. 2001

195 citations recorded by the source corpus.

In a previous publication (ATOMIC DATA AND NUCLEAR DATA TABLES 75, 1 (2000)), we gave seven-parameter analytical fits to theoretical reaction rates derived from nuclear cross sections calculated in the statistical model (Hauser-Feshbach formalism) for targets with 10 less than or equal to Z less than or equal to 83 (Ne to Bi) and for a mass range reaching the neutron and proton driplines. Reactions considered were (n,gamma), (n,p), (n,alpha), (p,gamma), (p,alpha), (alpha,gamma), and their inverse reactions. Here, we present the theoretical nuclear cross sections and astrophysical reaction rates from which those rate fits were derived, and we provide these data as on-line electronic files. Corresponding to the fitted rates, two complete data sets are provided, one of which includes a phenomenological treatment of shell quenching for neutron-rich nuclei. (C) 2001 Academic Press.

Subfields: Nuclear and High Energy Physics, Radiation

View Paper: https://www.semanticscholar.org/paper/014f4736ca9f2d02951950e308ad5a358b486d3c

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Citations in the corpus

CHARGED-PARTICLE AND NEUTRON-CAPTURE PROCESSES IN THE HIGH-ENTROPY WIND OF CORE-COLLAPSE SUPERNOVAE (2010, methodology): “Details on the nuclear spectroscopy used in the calculation of these rates are given in Rauscher & Thielemann (2001).”
Improved predictions of nuclear reaction rates with the TALYS reaction code for astrophysical applications (2008, methodology): “This is the case of MOST (Aikawa et al. 2005, Arnould & Goriely 2006) and now TALYS, but this is not the case of neither the original work of Holmes et al. (1976), nor the code SMOKER (Thielemann et al. 1987) nor NON-SMOKER (Rauscher & Thielemann 2001).”
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics (2001, methodology): “Low-lying nuclear levels had to be used for a few cases and in such a case the same information as for the NON-SMOKER calculation was utilized (Rauscher & Thielemann 2001).”
Origin of the heaviest elements: The rapid neutron-capture process (2019, methodology): “This improved level density description is part of the statistical model packages NON-SMOKER and SMARAGD developed by Rauscher (Rauscher and Thielemann, 2001; Rauscher, 2011).”