Pair conversion spectroscopy of the Hoyle state
Date
2013
Authors
Kibedi, Tibor
Stuchbery, Andrew
Copp, P
De Vries, Mitchell
Pitt, Robert
Alshahrani, Badriah
Margerin, Vincent
Dracoulis, George
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Abstract
The triple-alpha reaction leading to the formation of stable carbon in the Universe is one of the most important nuclear astrophysical processes. The radiative width of the so-called Hoyle state, involving the 7.654 MeV E0 and the 3.2148 MeV E2 transition
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Proceedings of Science
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Conference paper
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Open Access
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Creative Commons Attribution-NonCommercial-ShareAlike Licence.
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