27-31 May 2024
ADEIT - Valencia
Europe/Madrid timezone

Contribution List

85 / 85
Sandra Zavatarelli (INFN - Genova), Prof. Antonio Caciolli (Universita' di Padova and INFN), Dr. Francesca Cavanna (INFN - Sezione di Torino), Dr. Eliana Masha (Helmholtz-Zentrum Dresden-Rossendorf), Dr. Ragandeep Singh Sidhu (SUPA, School of Physics and Astronomy, University of Edinburgh)
28/05/2024, 17:10
oral contribution

Among the hydrogen burning processes in stars, proton reactions with Ne isotopes are very relevant to constrain the production and abundances of neon and sodium isotopes in massive stars, novae and supernovae. In particular the 20Ne(p,γ)21Na reaction is the first and slowest reaction of the NeNa cycle and it controls the speed at which the entire cycle proceeds: its rate affects the synthesis ...

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