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1Wallner, A, Bichler, M, Buczak, K, Dillmann, I, Käppeler, F, Karakas, A, Lederer, C, Lugaro, M, Mair, K, Mengoni, A, Schätzel, G, Steier, P, Trautvetter, H P“…The effect of the new stellar cross sections on the s process in low-mass asymptotic giant branch stars was studied for stellar models of 2M⊙ initial mass, and solar and 1/10th solar metallicity.…”
Հրապարակվել է 2016
Ստացեք ամբողջական տեքստը
Ստացեք ամբողջական տեքստը
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2Lederer-Woods, C, Woods, P J, Davinson, T, Kahl, D, Lonsdale, S J, Aberle, O, Amaducci, S, Andrzejewski, J, Audouin, L, Bacak, M, Balibrea, J, Barbagallo, M, Bečvář, F, Berthoumieux, E, Billowes, J, Bosnar, D, Brown, A, Caamaño, M, Calviño, F, Calviani, M, Cano-Ott, D, Cardella, R, Casanovas, A, Cerutti, F, Chen, Y H, Chiaveri, E, Colonna, N, Cortés, G, Cortés-Giraldo, M A, Cosentino, L, Cristallo, S, Damone, L A, Diakaki, M, Domingo-Pardo, C, Dressler, R, Dupont, E, Durán, I, Fernández-Domínguez, B, Ferrari, A, Ferreira, P, Ferrer, F J, Finocchiaro, P, Furman, V, Göbel, K, García, A R, Gawlik, A, Gilardoni, S, Glodariu, T, Gonçalves, I F, González-Romero, E, Griesmayer, E, Guerrero, C, Gunsing, F, Harada, H, Heinitz, S, Heyse, J, Jenkins, D G, Jericha, E, Käppeler, F, Kadi, Y, Kalamara, A, Kavrigin, P, Kimura, A, Kivel, N, Kokkoris, M, Krtička, M, Kurtulgil, D, Leal-Cidoncha, E, Leeb, H, Lerendegui-Marco, J, Lo Meo, S, Macina, D, Manna, A, Marganiec, J, Martínez, T, Masi, A, Massimi, C, Mastinu, P, Mastromarco, M, Maugeri, E A, Mazzone, A, Mendoza, E, Mengoni, A, Milazzo, P M, Mingrone, F, Musumarra, A, Negret, A, Nolte, R, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Porras, I, Praena, J, Quesada, J M, Radeck, D, Rauscher, T, Reifarth, R, Rubbia, C, Ryan, J A, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schumann, D, Sedyshev, P, Smith, A G, Sosnin, N V, Stamatopoulos, A, Tagliente, G, Tain, J L, Tarifeño-Saldivia, A, Tassan-Got, L, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vlachoudis, V, Vlastou, R, Wallner, A, Warren, S, Weiss, C, Wright, T, Žugec, P“…Our cross-section data range to 150 keV neutron energy, which is sufficient for a reliable determination of astrophysical reactivities up to 0.5 GK stellar temperature.…”
Հրապարակվել է 2021
Ստացեք ամբողջական տեքստը
Ստացեք ամբողջական տեքստը