Abstract
Maxwellian-averaged cross sections and astrophysical reaction rates were calculated for neutron capture, fission, (n,p), (n, α), and some threshold reactions based on a microscopic neutron cross section data library, the Japanese Evaluated Nuclear Data Library Version 3.3 (JENDL-3.3). The calculation was made for temperatures (kT) from 1 keV to 1 MeV including the most important range in astrophysical nucleosynthesis. Results are presented in the tables and graphs. The Maxwellian-averaged neutron capture cross sections are compared with recommendations of other authors. Implications of the differences between the present data and previous ones to s-process nucleosynthesis are discussed.
| Original language | English |
|---|---|
| Pages (from-to) | 77-186 |
| Number of pages | 110 |
| Journal | Atomic Data and Nuclear Data Tables |
| Volume | 91 |
| Issue number | 2 |
| DOIs | |
| State | Published - Nov 2005 |
| Externally published | Yes |
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