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dc.contributor.author
Munch, M.  
dc.contributor.author
Alcorta, M.  
dc.contributor.author
Fynbo, H. O. U.  
dc.contributor.author
Albers, M.  
dc.contributor.author
Almaraz Calderon, S.  
dc.contributor.author
Avila, M. L.  
dc.contributor.author
Ayangeakaa, A. D.  
dc.contributor.author
Back, B. B.  
dc.contributor.author
Bertone, P. F.  
dc.contributor.author
Carnelli, Patricio Francisco Florencio  
dc.contributor.author
Carpenter, M. P.  
dc.contributor.author
Chiara, C. J.  
dc.contributor.author
Clark, J. A.  
dc.contributor.author
DiGiovine, B.  
dc.contributor.author
Greene, J. P.  
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Harker, J. L.  
dc.contributor.author
Hoffman, C. R.  
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Hubbard, N. J.  
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Jiang, C. L.  
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Kirsebom, O. S.  
dc.contributor.author
Lauritsen, T.  
dc.contributor.author
Laursen, K. L.  
dc.contributor.author
Marley, S. T.  
dc.contributor.author
Nair, C.  
dc.contributor.author
Nusair, O.  
dc.contributor.author
Santiago Gonzalez, D.  
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Sethi, J.  
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Seweryniak, D.  
dc.contributor.author
Talwar, R.  
dc.contributor.author
Ugalde, C.  
dc.contributor.author
Zhu, S.  
dc.date.available
2018-06-11T16:19:05Z  
dc.date.issued
2016-06  
dc.identifier.citation
Munch, M.; Alcorta, M.; Fynbo, H. O. U.; Albers, M.; Almaraz Calderon, S.; et al.; Independent measurement of the Hoyle state β feeding from B 12 using Gammasphere; American Physical Society; Physical Review C; 93; 6; 6-2016  
dc.identifier.issn
2469-9993  
dc.identifier.uri
http://hdl.handle.net/11336/48071  
dc.description.abstract
Using an array of high-purity Compton-suppressed germanium detectors, we performed an independent measurement of the β-decay branching ratio from 12B to the second-excited state, also known as the Hoyle state, in 12C. Our result is 0.64(11)%, which is a factor ∼2 smaller than the previously established literature value, but is in agreement with another recent measurement. This could indicate that the Hoyle state is more clustered than previously believed. The angular correlation of the Hoyle state γ cascade has also been measured for the first time. It is consistent with theoretical predictions.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
American Physical Society  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Hoyle State  
dc.subject
12b  
dc.subject
12c  
dc.subject
Gammasphere  
dc.subject.classification
Astronomía  
dc.subject.classification
Ciencias Físicas  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Independent measurement of the Hoyle state β feeding from B 12 using Gammasphere  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2018-05-28T14:39:06Z  
dc.journal.volume
93  
dc.journal.number
6  
dc.journal.pais
Estados Unidos  
dc.journal.ciudad
New York  
dc.description.fil
Fil: Munch, M.. University Aarhus; Dinamarca  
dc.description.fil
Fil: Alcorta, M.. Westbrook Mall; Canadá. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Fynbo, H. O. U.. University Aarhus; Dinamarca  
dc.description.fil
Fil: Albers, M.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Almaraz Calderon, S.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Avila, M. L.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Ayangeakaa, A. D.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Back, B. B.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Bertone, P. F.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Carnelli, Patricio Francisco Florencio. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica; Argentina  
dc.description.fil
Fil: Carpenter, M. P.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Chiara, C. J.. Argonne National Laboratory; Estados Unidos. University of Maryland; Estados Unidos  
dc.description.fil
Fil: Clark, J. A.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: DiGiovine, B.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Greene, J. P.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Harker, J. L.. Argonne National Laboratory; Estados Unidos. University of Maryland; Estados Unidos  
dc.description.fil
Fil: Hoffman, C. R.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Hubbard, N. J.. University of York; Reino Unido  
dc.description.fil
Fil: Jiang, C. L.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Kirsebom, O. S.. University Aarhus; Dinamarca  
dc.description.fil
Fil: Lauritsen, T.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Laursen, K. L.. University Aarhus; Dinamarca  
dc.description.fil
Fil: Marley, S. T.. Argonne National Laboratory; Estados Unidos. Western Michigan University; Estados Unidos  
dc.description.fil
Fil: Nair, C.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Nusair, O.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Santiago Gonzalez, D.. Argonne National Laboratory; Estados Unidos. State University of Louisiana; Estados Unidos  
dc.description.fil
Fil: Sethi, J.. Argonne National Laboratory; Estados Unidos. University of Maryland; Estados Unidos  
dc.description.fil
Fil: Seweryniak, D.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Talwar, R.. Argonne National Laboratory; Estados Unidos  
dc.description.fil
Fil: Ugalde, C.. Argonne National Laboratory; Estados Unidos. University of Chicago; Estados Unidos. Joint Institute for Nuclear Astrophysics; Estados Unidos  
dc.description.fil
Fil: Zhu, S.. Argonne National Laboratory; Estados Unidos  
dc.journal.title
Physical Review C  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/https://dx.doi.org/10.1103/PhysRevC.93.065803  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prc/abstract/10.1103/PhysRevC.93.065803