Radiative Decay Branching Ratio of the Hoyle State in 12C via Charged Particle Coincidence Techniques

The properties of the Hoyle state in 12C (7.654 MeV, 0+) affect the rate at which carbon, one of the most abundant elements in the Universe, is forged in stars. Recent experiments reported values of its radiative decay branching ratio that are in tension, posing major implications especially in the...

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Bibliographic Details
Main Authors:	Dell’Aquila D., Lombardo I., Redigolo L., Vigilante M., Angelini F., Baldesi L., Barlini S., Best A., Camaiani A., Casini G., Ciampi C., Cicerchia M., D’Andrea M., Diklić J., Fabris D., Gongora Servin B., Gottardo A., Gramegna F., Imbriani G., Marchi T., Massara A., Mengoni D., Ordine A., Palada L., Pasquali G., Piantelli S., Pilotto E., Rapagnani D., Sigmund M., Stefanini A., Stramaccioni D., Tagnani D., Tišma I., Valdré S., Verde G., Vukman N.
Format:	Article
Language:	English
Published:	EDP Sciences 2024-01-01
Series:	EPJ Web of Conferences
Online Access:	https://www.epj-conferences.org/articles/epjconf/pdf/2024/21/epjconf_sotancp2024_00010.pdf
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Radiative Decay Branching Ratio of the Hoyle State in 12C via Charged Particle Coincidence Techniques

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