Eur. Phys. J. Special Topics 156, 123-149 (2008)
DOI: 10.1140/epjst/e2008-00611-5
Gesellschaft für Schwerionenforschung Darmstadt, Planckstr. 1, 64259 Darmstadt, Germany
(Published online: 17 April 2008)
© EDP Sciences, Springer-Verlag 2008
DOI: 10.1140/epjst/e2008-00611-5
Selected topics in nuclear astrophysics
G. Martínez-PinedoGesellschaft für Schwerionenforschung Darmstadt, Planckstr. 1, 64259 Darmstadt, Germany
(Published online: 17 April 2008)
Abstract
In this lectures after a brief introduction to stellar
reaction rates and its implementation in nuclear networks I discuss
the nuclear aspects of the collapse of the inner core of massive
stars once it has run out of its nuclear energy source and of the
star's explosion as a type II supernova and the explosive
nucleosynthesis occurring during this explosion which leads to the
production of heavy elements by the rapid neutron capture process
and potentially also by the recently discovered
process.
© EDP Sciences, Springer-Verlag 2008


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