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Nuclear reactions in ultra-magnetized supernovae
The statistical model is employed to investigate nuclear reactions in ultrastrong magnetic fields relevant for supernovae and neutron stars. For radiative capture processes the predominant mechanisms are argued to correspond to modifications of nuclear level densities, and gamma-transition energies...
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Lenguaje: | eng |
Publicado: |
2002
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Acceso en línea: | http://cds.cern.ch/record/747949 |