Skip to main content
16–18 Oct 2024
Europe/Budapest timezone

The origin of the rare 113In and 115Sn p-nuclei revisited

16 Oct 2024, 16:20
20m
Oral presentation Afternoon session

Speaker

Dr Thanassis Psaltis (Triangle Universities Nuclear Laboratory)

Description

The production of the light p-nuclei 113In and 115Sn has been a long-standing problem for γ-process nucleosynthesis [1,2]. The reaction flow in the Cd-In-Sn region is rather complicated due to the existance of several long-lived β-decaying isomers, which leads to a general underproduction of these isotopes compared to the other p-nuclei. In this talk, I will discuss the current status of the origin of 113In and 115Sn along with their different production mechanisms and a recent experimental measurement regarding the production of 113In [3].

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
Please select a keyword related to your abstract Stellar Models and Galactic Chemical Evolution

Author

Dr Thanassis Psaltis (Triangle Universities Nuclear Laboratory)

Presentation materials