Nuclear input for core-collapse models
Copyright policy )Nuclear input for core-collapse models
We review the nuclear physics input necessary for the study of the collapse of massive stars as precursor to supernova explosions. Recent theoretical advances for the calculation of the relevant weak-interaction processes and their influence in the collapse and postbounce dynamics are discussed. Future improvements are expected to come with the advent of radioactive ion-beam facilities.
37 pages, 11 figures, for special issue of Nucl. Phys. A
- University of Basel Switzerland
- University of Münster Germany
- University of Toronto Canada
- Canadian Institute for Theoretical Astrophysics Canada
- Autonomous University of Barcelona Spain
Nuclear Theory (nucl-th), Nuclear Theory, Astrophysics (astro-ph), FOS: Physical sciences, Nuclear Experiment (nucl-ex), Astrophysics, Nuclear Experiment
Nuclear Theory (nucl-th), Nuclear Theory, Astrophysics (astro-ph), FOS: Physical sciences, Nuclear Experiment (nucl-ex), Astrophysics, Nuclear Experiment
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