Trojan Horse Investigation for AGB Stellar Nucleosynthesis

0555175 - ÚJF 2023 RIV CH eng J - Journal Article
Sergi, M. L. - D'Agata, Giuseppe - Guardo, G. L. - Rapisarda, G. G. - Burjan, Václav - Cherubini, S. - Gulino, M. - Indelicato, I. - La Cognata, M. - Lamia, L. - Lattuada, D. - Mrázek, Jaromír - Oliva, A. A. - Pizzone, R. G. - Romano, S. - Sparta, R. - Trippella, O. - Tumino, A.
Trojan Horse Investigation for AGB Stellar Nucleosynthesis.
Universe. Roč. 8, č. 2 (2022), č. článku 128. E-ISSN 2218-1997
R&D Projects: GA MŠMT(CZ) EF16_013/0001679; GA MŠMT LM2018115
Institutional support: RVO:61389005
Keywords : nuclear astrophysics * AGB nucleosynthesis * indirect methods
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 2.9, year: 2022
Method of publishing: Open access
https://doi.org/10.3390/universe8020128

Asymptotic Giant Branch (AGB) stars are among the most important astrophysical sites influencing the nucleosynthesis and the chemical abundances in the Universe. From a pure nuclear point of view, several processes take part during this peculiar stage of stellar evolution thus requiring detailed experimental cross section measurements. Here, we report on the most recent results achieved via the application of the Trojan Horse Method (THM) and Asymptotic Normalization Coefficient (ANC) indirect techniques, discussing the details of the experimental procedure and the deduced reaction rates. In addition, we report also on the on going studies of interest for AGB nucleosynthesis.
Permanent Link: http://hdl.handle.net/11104/0329703