Speaker
Description
The production of the light p-nuclei 113In and 115Sn has been a long-standing problem for
This work is supported by U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0017799 and Contract Nos. DE-FG02-97ER41033 and DE-FG02-97ER41042.
References
[1] Zs. Németh et al., Astrophys. J 426, 357 (1994).
[2] Ch. Theis et al., Astrophys. J 500, 1039 (1998).
[3] A. Psaltis et al., Phys. Rev. C 99, 065807 (2019).
Length of presentation requested | Oral presentation: 17 min + 3 min questions |
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Please select a keyword related to your abstract | Stellar Models and Galactic Chemical Evolution |