Trojan Horse Investigation for AGB Stellar Nucleosynthesis

Author:

Sergi Maria LetiziaORCID,D’Agata GiuseppeORCID,Guardo Giovanni Luca,Rapisarda Giuseppe GabrieleORCID,Burjan Vaclav,Cherubini Silvio,Gulino MarisaORCID,Indelicato Iolanda,La Cognata MarcoORCID,Lamia LivioORCID,Lattuada DarioORCID,Mrázek Jaromir,Oliva Alessandro Alberto,Pizzone Rosario GianlucaORCID,Romano Stefano,Spartá RobertaORCID,Trippella Oscar,Tumino Aurora

Abstract

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.

Publisher

MDPI AG

Subject

General Physics and Astronomy

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