Abstract
We review different models used for reactions involved in nuclear astrophysics. The reaction rate is defined for resonant as well as for non-resonant processes. For low-density nuclei, we describe the DWBA method, the potential model, the R-matrix method, and microscopic cluster models. The statistical model is developed for high-level densities. Details of calculations in the low- and high-density regimes are illustrated with new results concerning transfer reactions and level densities. (c) 2004 Elsevier B.V. All rights reserved.
| Original language | English |
|---|---|
| Pages (from-to) | 137-156 |
| Number of pages | 20 |
| Journal | Nuclear Physics A |
| Volume | 777 |
| DOIs | |
| Publication status | Published - 17 Oct 2006 |
Keywords
- GAMMA-PROCESS
- THERMONUCLEAR REACTION-RATES
- STATISTICAL-MODEL CALCULATIONS
- RADIATIVE-CAPTURE REACTIONS
- DIRECT NEUTRON-CAPTURE
- ELASTIC-SCATTERING
- NUCLEAR-LEVEL DENSITY
- NON-SPHERICAL NUCLEI
- ASTROPHYSICAL REACTION-RATES
- SHELL NUCLEI
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