10–11 Sept 2009
Max-Planck Institut fuer Extraterrestrische Physik (MPE)
Europe/Berlin timezone

Session

gamma-process II

10 Sept 2009, 15:45
Seminar room 1.18 (Max-Planck Institut fuer Extraterrestrische Physik (MPE))

Seminar room 1.18

Max-Planck Institut fuer Extraterrestrische Physik (MPE)

TU Munich Campus Garching D-85748 Garching

Presentation materials

There are no materials yet.

  1. Artemis Spyrou (National Superconducting Cyclotron Laboratory and Department of Physics & Astronomy, Michigan State University, East Lansing, Michigan 48824, USA)
    10/09/2009, 15:45
    Proton, neutron and alpha-particle capture reactions are the main contributors towards the understanding of the p-process nucleosynthesis. Although the reactions involved in this process are mainly photodisintegrations, measuring the inverse reactions can be even more helpful than the measurement of the gamma -induced reactions themselves. Recently there have been major experimental...
    Go to contribution page
  2. Michael Heil (GSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, Germany)
    10/09/2009, 16:15
    E062 Collaboration
    Go to contribution page
  3. Jens Hasper (Institut fuer Kernphysik, Universitaet zu Koeln, 50937 Koeln, Germany)
    10/09/2009, 16:45
    The p-process is the most promising astrophysical scenario for the nucleosynthesis of about 35 proton-rich nuclei referred to as p nuclei. This process involves an extensive reaction network of about 2000 nuclei and more than 20000 reactions, especially photodisintegration reactions, under explosive physical conditions. The huge number of reaction rates are mainly adopted from...
    Go to contribution page
Building timetable...