Neutron-induced cross section measurements

Massimi, C; Aberle, O; Alcayne, V; Altieri, S; Amaducci, S; Andrzejewski, J; Babiano-Suarez, V; Bacak, M; Balibrea, J; Beltrami, C; Bennett, S; Bernardes, AP; Berthoumieux, E; Boromiza, M; Bosnar, D; Caamano, M; Calvino, F; Calviani, M; Cano-Ott, D; Casanovas, A; Castelluccio, DM; Cerutti, F; Cescutti, G; Chasapoglou, S; Chiaveri, E; Colombetti, P; Colonna, N; Camprini, PC; Cortes, G; Cortes-Giraldo, MA; Cosentino, L; Cristallo, S; Dellmann, S; Di Castro, M; Di Maria, S; Diakaki, M; Dietz, M; Domingo-Pardo, C; Dressler, R; Dupont, E; Duran, I; Eleme, Z; Fargier, S; Fernandez, B; Fernandez-Dominguez, B; Finocchiaro, P; Fiore, S; Furman, V; Garcia-Infantes, F; Gawlik-Ramiega, A; Gervino, G; Gilardoni, S; Gonzalez-Romero, E; Guerrero, C; Gunsing, F; Gustavino, C; Heyse, J; Hillman, W; Jenkins, DG; Jericha, E; Junghans, A; Kadi, Y; Kaperoni, K; Kaur, G; Kimura, A; Knapova, I; Kokkoris, M; Kopatch, Y; Krticka, M; Kyritsis, N; Ladarescu, I; Lederer-Woods, C; Lerendegui-Marco, J; Lerner, G; Manna, A; Martinez, T; Masi, A; Mastinu, P; Mastromarco, M; Maugeri, EA; Mazzone, A; Mendoza, E; Mengoni, A; Michalopoulou, V; Milazzo, PM; Mucciola, R; Murtas, F; Musacchio-Gonzalez, E; Musumarra, A; Negret, A; De Rada, AP; Perez-Maroto, P; Patronis, N; Pavon-Rodriguez, JA; Pellegriti, MG; Perkowski, J; Petrone, C; Pirovano, E; Plaza, J; Pomp, S; Porras, I; Praena, J; Quesada, JM; Reifarth, R; Rochman, D; Romanets, Y; Rubbia, C; Sanchez, A; Sabate-Gilarte, M; Schillebeeckx, P; Schumann, D; Sekhar, A; Smith, AG; Sosnin, NV; Stamati, ME; Sturniolo, A; Tagliente, G; Tarrio, D; Torres-Sanchez, P; Urlass, S; Vagena, E; Valenta, S; Variale, V; Vaz, P; Vecchio, G; Vescovi, D; Vlachoudis, V; Vlastou, R; Wallner, A; Woods, PJ; Wright, T; Zarrella, R; Zugec, P

Massimi, C (通讯作者),Ist Nazl Fis Nucl, Sez Bologna, Bologna, Italy.;Massimi, C (通讯作者),Univ Bologna, Dipartimento Fis & Astron, Bologna, Italy.

NUCLEAR PHYSICS IN ASTROPHYSICS - X, NPA-X 2022, 2023; 279 ():

Abstract

Neutron-induced cross sections represent the main nuclear input to models of stellar and Big-Bang nucleosynthesis. While (n, gamma) reactions are rele......

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