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

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

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_ea959ba8d6944cefaa903a98cb0c5113

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

About this item

Full title

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

Publisher

Les Ulis: EDP Sciences

Journal title

EPJ Web of conferences, 2024, Vol.311, p.00010

Language

English

Publication information

Publisher

Les Ulis: EDP Sciences

More information

Scope and Contents

Contents

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 astrophysical domain. This work reports on an almo...

Alternative Titles

Full title

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

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_doaj_primary_oai_doaj_org_article_ea959ba8d6944cefaa903a98cb0c5113

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_ea959ba8d6944cefaa903a98cb0c5113

Other Identifiers

ISSN

2101-6275

E-ISSN

2100-014X

DOI

10.1051/epjconf/202431100010

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