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...
The first part of the paper discusses nuclear properties relevant to predict compound reactions. The...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
Although important effort has been devoted in the last decades to measure reaction cross sections, m...
Theoretical reaction rates in the temperature range 0.01 x 10(9) less than or equal to T(K) less tha...
Modern computer technology has revolutionized theoretical calculations on stellar structure and stel...
Nuclear reaction rates for astrophysics applications are traditionally determined on the basis of Ha...
Context. Nuclear reaction rates of astrophysical applications are traditionally determined on the ba...
Abstract. Nuclear reaction rates for astrophysics applications are traditionally determined on the b...
Nuclear reaction rates determine the abundances of isotopes in stellar burning pro-cesses. A multitu...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
Neutron-induced reaction rates, including fission and neutron capture, are calculated in the tempera...
The relevant astrophysical reaction rates which are derived from the reaction cross sections are nec...
Astrophysical reaction rates, which are mostly derived from theoretical cross sections, are necessar...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
During the last 10 years, in the general context of nuclear energy applications and future reactors ...
The first part of the paper discusses nuclear properties relevant to predict compound reactions. The...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
Although important effort has been devoted in the last decades to measure reaction cross sections, m...
Theoretical reaction rates in the temperature range 0.01 x 10(9) less than or equal to T(K) less tha...
Modern computer technology has revolutionized theoretical calculations on stellar structure and stel...
Nuclear reaction rates for astrophysics applications are traditionally determined on the basis of Ha...
Context. Nuclear reaction rates of astrophysical applications are traditionally determined on the ba...
Abstract. Nuclear reaction rates for astrophysics applications are traditionally determined on the b...
Nuclear reaction rates determine the abundances of isotopes in stellar burning pro-cesses. A multitu...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
Neutron-induced reaction rates, including fission and neutron capture, are calculated in the tempera...
The relevant astrophysical reaction rates which are derived from the reaction cross sections are nec...
Astrophysical reaction rates, which are mostly derived from theoretical cross sections, are necessar...
Nuclear reaction rates are quantities of fundamental importance in astrophysics. Substantial efforts...
During the last 10 years, in the general context of nuclear energy applications and future reactors ...
The first part of the paper discusses nuclear properties relevant to predict compound reactions. The...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
Although important effort has been devoted in the last decades to measure reaction cross sections, m...