Neutron-induced astrophysical reaction rates (Panov+, 2010)

Physics – Atomic Physics

Scientific paper

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Atomic Physics

Scientific paper

The organization of Tables 3-6 with calculated rates for 24 different values of T9 is extremely simple - all data are in 8 columns. The columns give, in this order, the target element, the atomic mass number A of the target, the temperature in T9, partition function of the target, neutron-induced fission rate for the ground state, neutron-induced fission rate with thermally populated target states, neutron capture rate for the ground state, neutron capture rate with thermally populated target states.
The rates in Tables 3-6 were calculated on the basis of different mass and fission barrier predictions: ETFSI, TF and FRDM(masses)+TF(barriers), respectively (see main text of the paper for details).
The fitting coefficients for the (n,g), (g,n), and neutron-induced fission rates (n,f) with different mass and fission-barrier predictions are placed in the Tables 7-18 (see example on how to use them in Appendix A of the main paper). The columns in Tables 7-18 are organized as follows: target element, atomic mass number A of the target, target charge number Z, the number of fitting curves i_{fit}, seven coefficients of the forward reaction a_i, and the mean square error for direct reactions.
A value i{fit}=0 means that there is only one seven-parameter set to fit the rate. Values i_{fit}>1 give the number of parameter sets which have to be added up to yield the final rate, i.e. the rate r is calculated as r={sum.on.i}ri, with each ri computed from the i-th parameter set and using Eq. ri=exp(a0+a1/T9+a2/T91/3+a3*T91/3+a4*T9+a5*T95/3^+a6*ln(T9)) (4).
(16 data files).

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