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- Destruction of the cosmic γ-ray emitter 26Al in massive stars: study of the key 26Al(n,p) reaction (2021)
- Claudia Lederer-Woods Philip John Woods Thomas Davinson David Kahl Sarah Jane Lonsdale Oliver Aberle Simone Amaducci Józef Andrzejewski Laurent Audouin Michael Bacak Javier Balibrea-Correa Massimo Barbagallo František Bečvář Eric Berthoumieux Jon Billowes Damir Bosnar Adam Brown Manuel Caamaño Francisco Calviño Marco Calviani Daniel Cano-Ott Roberto Cardella Adria Casanovas Francesco Cerutti Y. H. Chen Enrico Chiaveri Nicola Colonna Guillem Cortés Miguel Antonio Cortés-Giraldo Luigi Cosentino Sergio Cristallo Lucia Anna Damone Maria Diakaki Cesar Domingo-Pardo Rugard Dressler Emmeric Dupont Ignacio Durán Beatriz Fernández-Domínguez Alfredo Ferrari Paulo Ferreira Francesc J. Ferrer Paolo Finocchiaro Valter Furman Kathrin Göbel Aczel Regino García Aleksandra Gawlik Simone Gilardoni Tudor Glodariu Isabel F. Gonçalves Enrique González-Romero Erich Griesmayer Carlos Guerrero Frank Gunsing Hideo Harada Stephan Heinitz Jan Heyse David G. Jenkins Erwin Jericha Franz Käppeler Yacine Kadi Antigoni Kalamara Pavel Kavrigin Atsushi Kimura Nikolai Kivel Michael Kokkoris Milan Krtička Deniz Kurtulgil E. Leal-Cidoncha Helmut Leeb Jorge Lerendegui-Marco Sergio Lo Meo Daniela Macina Alice Manna Justyna Marganiec Trinitario Martínez Alessandro Masi Cristian Massimi Pierfrancesco Mastinu Mario Mastromarco Emilio-Andrea Maugeri Annamaria Mazzone Emilio Mendoza Alberto Mengoni Paolo M. Milazzo Federica Mingrone Agatino Musumarra Alexandru Negret Ralf Nolte Andreea Oprea Nikolas Patronis Andreas Pavlik Jarosław Perkowski Ignacio Porras Javier Praena José-Manuel Quesada Desiree Radeck Thomas Rauscher René Reifarth Carlo Rubbia James A. Ryan Marta Sabaté-Gilarte Alok Saxena Peter Schillebeeckx Dorothea Schumann Pavel V. Sedyshev Alastair G. Smith Nikolay V. Sosnin Athanasios Stamatopoulos Giuseppe Tagliente José L. Tain Ariel Tarifeño-Saldivia Laurent Tassan-Got Stanislav Valenta Gianni Vannini Vincenzo Variale Pedro Vaz Alberto Ventura Vasilis Vlachoudis Rosa Vlastou Anton Wallner Stuart Warren Christina Weß Tobias Wright Petar Žugec
- The 26Al(n,p)26Mg reaction is the key reaction impacting on the abundances of the cosmic γ-ray emitter 26Al produced in massive stars and impacts on the potential pollution of the early solar system with 26Al by asymptotic giant branch stars. We performed a measurement of the 26Al(n,p)26Mg cross section at the high-flux beam line EAR-2 at the n_TOF facility (CERN). We report resonance strengths for eleven resonances, nine being measured for the first time, while there is only one previous measurement for the other two. Our resonance strengths are significantly lower than the only previous values available. 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.
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