Prof.
Sandrine Courtin
(IPHC STrasbourg)
20/06/2017, 14:30
Invited talk
Fusion reactions play an essential role in understanding the energy production, the nucleosyn- thesis of chemical elements and the evolution of massive stars. Thus, the direct measurement of key fusion reactions at thermonuclear energies is of very high interest. The carbon burning in stars is essentially driven by the 12C+12C fusion reaction. This reaction is known to show prominent...
Dr
Richard deBoer
(University of Notre Dame)
20/06/2017, 15:00
Underground nuclear astrophysics
Invited talk
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Dr
Michael Febbraro
(Oak Ridge National Laboratory)
20/06/2017, 15:30
Stellar evolution and nucleosynthesis
Oral
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Dr
Daniel Bemmerer
(Helmholtz-Zentrum Dresden-Rossendorf)
20/06/2017, 15:50
Oral
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Mr
Nicolas Hubbard
(University of York and Aarhus University)
20/06/2017, 16:10
Stellar evolution and nucleosynthesis
Oral
The
23 Na(α,p) 26 Mg reaction has been identified as having a significant impact on the nucleo-
synthesis of elements, such as
23 Na [1] and 26 Al [2], in massive stars, and of light isotopes in
type-Ia supernovae [3]. We will present new experimental results, as well as a combined reaction
rate based on all available data, and an assessment of its astrophysical impact on massive...
Dr
Hidetoshi Yamaguchi
(Center for Nuclear Study, the University of Tokyo)
20/06/2017, 16:30
Oral
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