During the helium burning phase of stellar nucleosynthesis, the production of 12C proceeds via a two-step process called the triple alpha reaction. In this reaction, two alpha particles react to form 8Be which is followed by the capture of a third alpha particle onto 8Be forming 12C. The second step of this reaction is enhanced by a narrow resonance with a 7.65 MeV 0+ state in 12C, the Hoyle state. The production rate of 12C is sensitive to the properties of the Hoyle state [1-4]. The work of Ref. [1] suggested the decay of Hoyle state proceeds almost exclusively through a sequential 8Beg.s. + α channel and placed an upper limit of 4% on the contribution of the direct decay to three alpha particles [1]. Recent controversial results of the decay properties of the Hoyle state identify two new exotic direct three alpha decay modes with a combined decay branch of 17%, which implies a decrease of 17% in the production rate of 12C at temperatures of 108 to 109 K [2]. Subsequent studies attempting to resolve the apparent discrepancy between the previous investigations support the findings of Ref. [1] and find little evidence of the two newly proposed direct three alpha decay modes [3,4]. The experimental details and results will be presented along with conclusions regarding the Hoyle state decay controversy.
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