Coulomb dissociation reactions on Mo isotopes for astrophysics applications

Autor: Adolf Bruenle, Rudrayoti Palit, Haik Simon, Thomas Berg, H. Emling, Martin Winkler, Wladyslaw Walus, Arnd R. Junghans, Tudi Le Bleis, Lionel Deveaux, Roy Crawford Lemmon, Yuri A. Litvinov, R. Kulessa, Beatriz Fernandez-Dominguez, Przemyslaw Adrich, H. Alvarez-Pol, Suemmerer Klaus, Stefanos Paschalis, G. Ickert, D. M. Rossi, Alina Movsesyan, Farouk Aksouh, Rene Reifarth, Michael Boehmer, Roland Beyer, Hans Geissel, O.A. Kiselev, Michael Elvers, Karl-Heinz Behr, Marielle Chartier, Magda Gorska, Peter Maierbeck, Ushasi Datta Pramanik, J. Benlliure, Grzegorz Surowka, Mario Babilon, Michael Heil, Helmut Weick, Thomas Nilsson, Håkan T Johansson, N. Kurz, O. Ershova, Marc Labiche, Enrique Casarejos, Margarete Hellstroem, Thomas Elze, C. Nociforo, Dario Vretenar, Thomas Aumann, Andreas Zilges, D. Cortina-Gil, Linda Schnorrenberger, M. Erhard, J. V. Kratz, F. Käppeler, A. Chatillon, Andreas Wagner, Nils Paar, Stephan Walter, W. Prokopowicz, Nicolas Winckler, Konstanze Boretzky, A. Klimkiewicz, K. Lindenberg, Sebastian mueller

Publikováno v: Proceedings of 11th Symposium on Nuclei in the Cosmos — PoS(NIC XI).

Photo-dissociation reactions play an important role in p-process nucleosynthesis, which takes place in supernova explosions. Theoretical calculations of isotopic abundances of the p-nuclei require a vast reaction network linking thousands of isotopes

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::d805490d0bdbfd1b5e71a7004f66d186
https://doi.org/10.22323/1.100.0232