Kibedi, TiborStuchbery, AndrewCopp, PDe Vries, MitchellPitt, RobertAlshahrani, BadriahMargerin, VincentDracoulis, George2015-12-13August 5-1http://hdl.handle.net/1885/82955The 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 transitionCopyright owned by the author(s)https://creativecommons.org/licenses/by-nc-sa/4.0/20132015-12-11Creative Commons Attribution-NonCommercial-ShareAlike Licence.