Towards the pair spectroscopy of the Hoyle state in 12C
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Kibedi, Tibor
Stuchbery, Andrew
Dracoulis, George
Robertson, Kalman
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EPJ Web of Conferences
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The triple-alpha process 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 transitions
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