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Destruction of the cosmic $\gamma$-ray emitter $^{26}$Al in massive stars: Study of the key $^{26}$Al$(n,p)$ reaction
The $^{26}$Al$(n,p)$ $^{26}$Mg reaction is the key reaction impacting on the abundances of the cosmic γ -ray emitter $^{26}$Al produced in massive stars and impacts on the potential pollution of the early solar system with $^{26}$Al by asymptotic giant branch stars. We performed a measurement...
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Lenguaje: | eng |
Publicado: |
2021
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevC.104.L022803 http://cds.cern.ch/record/2780489 |