TY  - JOUR
A1  - Lederer-Woods, Claudia
A1  - Woods, Philip John
A1  - Davinson, Thomas
A1  - Kahl, David
A1  - Lonsdale, Sarah Jane
A1  - Aberle, Oliver
A1  - Amaducci, Simone
A1  - Andrzejewski, Józef
A1  - Audouin, Laurent
A1  - Bacak, Michael
A1  - Balibrea Correa, Javier
A1  - Barbagallo, Massimo
A1  - Bečvář, František
A1  - Berthoumieux, Eric
A1  - Billowes, Jonathan
A1  - Bosnar, Damir
A1  - Brown, Adam
A1  - Caamaño, Manuel
A1  - Calviño Tavares, Francisco
A1  - Calviani, Marco
A1  - Cano-Ott, Daniel
A1  - Cardella, Roberto
A1  - Casanovas Hoste, Adrià
A1  - Cerutti, Francesco
A1  - Chen, Yonghao
A1  - Chiaveri, Enrico
A1  - Colonna, Nicola
A1  - Cortés Rossell, Guillem Pere
A1  - Cortés-Giraldo, Miguel Antonio
A1  - Cosentino, Luigi
A1  - Cristallo, Sergio
A1  - Damone, Lucia Anna
A1  - Diakaki, Maria
A1  - Domingo-Pardo, César
A1  - Dressler, Rugard
A1  - Dupont, Emmeric
A1  - Durán, Ignacio
A1  - Fernández Domínguez, Beatriz
A1  - Ferrari, Alfredo
A1  - Ferreira, Paulo
A1  - Ferrer, Francisco Javier
A1  - Finocchiaro, Paolo
A1  - Furman, Valter
A1  - Göbel, Kathrin
A1  - García Ríos, Aczel Regino
A1  - Gawlik, Aleksandra
A1  - Gilardoni, Simone
A1  - Glodariu, Tudor
A1  - Gonçalves, Isabel Maria Ferro
A1  - González Romero, Enrique Miguel
A1  - Griesmayer, Erich
A1  - Guerrero Sánchez, Carlos
A1  - Gunsing, Frank
A1  - Harada, Hideo
A1  - Heinitz, Stephan
A1  - Heyse, Jan
A1  - Jenkins, David
A1  - Jericha, Erwin
A1  - Käppeler, Franz
A1  - Kadi, Yacine
A1  - Kalamara, Antigoni
A1  - Kavrigin, Pavel
A1  - Kimura, Atsushi
A1  - Kivel, Nikolay
A1  - Kokkoris, Michael
A1  - Krtička, Milan
A1  - Kurtulgil, Cem Deniz
A1  - Leal Cidoncha, Esther
A1  - Leeb, Helmut
A1  - Lerendegui-Marco, Jorge
A1  - Lo Meo, Sergio
A1  - Macina, Daniela
A1  - Manna, Alice
A1  - Marganiec, Justyna
A1  - Martínez, Trinitario
A1  - Masi, Alessandro
A1  - Massimi, Cristian
A1  - Mastinu, Pierfrancesco
A1  - Mastromarco, Mario
A1  - Maugeri, Emilio Andrea
A1  - Mazzone, Annamaria
A1  - Mendoza Cembranos, Emilio
A1  - Mengoni, Alberto
A1  - Milazzo, Paolo Maria
A1  - Mingrone, Federica
A1  - Musumarra, Agatino
A1  - Negret, Alexandru
A1  - Nolte, Ralf
A1  - Oprea, Andreea
A1  - Patronis, Nikolas
A1  - Pavlik, Andreas
A1  - Perkowski, Jarosław
A1  - Porras Sánchez, José Ignacio
A1  - Praena, Javier
A1  - Quesada Molina, José Manuel
A1  - Radeck, Désirée
A1  - Rauscher, Thomas
A1  - Reifarth, René
A1  - Rubbia, Carlo
A1  - Ryan, James A.
A1  - Sabaté-Gilarte, Marta
A1  - Saxena, Alok
A1  - Schillebeeckx, Peter
A1  - Schumann, Dorothea
A1  - Sedyshev, Pavel  V.
A1  - Smith, Alastair G.
A1  - Sosnin, Nikolay V.
A1  - Stamatopoulos, Athanasios
A1  - Tagliente, Giuseppe
A1  - Taı́n Enríquez, José Luis
A1  - Tarifeño-Saldivia, Ariel
A1  - Tassan-Got, Laurent
A1  - Valenta, Stanislav
A1  - Vannini, Gianni
A1  - Variale, Vincenzo
A1  - Vaz, Pedro
A1  - Ventura, Alberto
A1  - Vlachoudis, Vasilis
A1  - Vlastou, Rosa
A1  - Wallner, Anton
A1  - Warren, Stuart
A1  - Weß, Christina
A1  - Wright, Tobias
A1  - Žugec, Petar
T1  - Destruction of the cosmic γ-ray emitter 26Al in massive stars: study of the key 26Al(n,p) reaction
T2  - Physical Review C
N2  - 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.
Y1  - 2021
UR  - http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/62268
UR  - https://nbn-resolving.org/urn:nbn:de:hebis:30:3-622682
SN  - 2469-9993
N1  - This work was supported be the Austrian Science Fund (FWF), project J3503, by the UK Science and Technologies Facilities Council (STFC), projects ST/L005824/1 and ST/M006085/1, and the European Research Council ERC-2015-STG Nr. 677497.
VL  - 104
IS  - 2, art. L022803
SP  - 1
EP  - 7
PB  - Inst.
CY  - Woodbury, NY
ER  -