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• W2146353485 abstract "The detection of the 1809 keV emission line associated with the decay of 26 Al in the interstellar medium provides a direct evidence of recent nucleosynthesis events in our galaxy. 26 Al is thought to be mainly produced in massive stars, but in order to have a quantita- tive understanding of the 26 Al distribution, the cross section of all the nuclear reactions involved in its production should be accurately known. A recent sensitivity study demonstrated that the 25 Mg( ,n) 28 Si is the reaction with the strongest impact on the synthesis of 26 Al during explosive Neon and Carbon burning (4). In order to improve the experimental knowledge of the 25 Mg( ,n) 28 Si cross section, a new direct measurement has been performed at Legnaro National Laboratories. The experimental setup, the data analysis and preliminary results are discussed." @default.
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• W2146353485 date "2014-01-01" @default.
• W2146353485 modified "2023-10-17" @default.
• W2146353485 title "Measurement of the25Mg(α,n)28Si reaction cross section at LNL" @default.
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• W2146353485 doi "https://doi.org/10.1051/epjconf/20146607002" @default.
• W2146353485 hasPublicationYear "2014" @default.
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