Gamma-Ray spectroscopy studies of explosive stellar phenomena
A handful of nuclear reactions have been identified as vital for our understanding of explosive stellar phenomena and the nucleosynthesis associated with these scenarios. The 22Ne(α, γ)26Mg reaction in massive stars is responsible for using the neon fuel required for the 22Ne(α, n) 25 Mg, which is a...
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University of Surrey
2018
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.736892 |