Speaker
Andre Sieverding
(Oak Ridge National Laboratory)
Description
The radioactive isotope 10Be is among those that have been present when the solar system formed.
We review the production of this isotope in core-collapse supernovae via the ν-process considering
results from modern multi-dimensional simulations, as well as the sensitivity to nuclear reactions.
Recent nuclear experiments suggest that the cross-section of the most important destructive reaction,
10Be(p,α)7Li, is higher than previously assumed, significantly reducing the expected production of
10Be by supernovae.
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| Please select a main topic related to your abstract | Explosive Stellar Objects and Nuclear Physics |
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Primary authors
Andre Sieverding
(Oak Ridge National Laboratory)
Dr
Jaspreet Randhawa
(University of Notre Dame)
Mr
Daniel Zetterberg
(University of Tennessee)
Dr
Riccardo Mancino
(GSI Helmholtz Centre for Heavy Ion Research)
Dr
Tan Ahn
(University of Notre Dame)
Prof.
Richard, J. DeBoer
(University of Notre Dame)
Prof.
Gabriel Martinez-Pinedo
(GSI Helmholtz Centre for Heavy Ion Research)
Prof.
William R. Hix
(Oak Ridge National Laboratory)
