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Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes

The nuclear shell structure, which originates in the nearly independent motion of nucleons in an average potential, provides an important guide for our understanding of nuclear structure and the underlying nuclear forces. Its most remarkable fingerprint is the existence of the so-called magic number...

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Autores principales: Tran, D. T., Ong, H. J., Hagen, G., Morris, T. D., Aoi, N., Suzuki, T., Kanada-En’yo, Y., Geng, L. S., Terashima, S., Tanihata, I., Nguyen, T. T., Ayyad, Y., Chan, P. Y., Fukuda, M., Geissel, H., Harakeh, M. N., Hashimoto, T., Hoang, T. H., Ideguchi, E., Inoue, A., Jansen, G. R., Kanungo, R., Kawabata, T., Khiem, L. H., Lin, W. P., Matsuta, K., Mihara, M., Momota, S., Nagae, D., Nguyen, N. D., Nishimura, D., Otsuka, T., Ozawa, A., Ren, P. P., Sakaguchi, H., Scheidenberger, C., Tanaka, J., Takechi, M., Wada, R., Yamamoto, T.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5913314/
https://www.ncbi.nlm.nih.gov/pubmed/29686394
http://dx.doi.org/10.1038/s41467-018-04024-y
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author Tran, D. T.
Ong, H. J.
Hagen, G.
Morris, T. D.
Aoi, N.
Suzuki, T.
Kanada-En’yo, Y.
Geng, L. S.
Terashima, S.
Tanihata, I.
Nguyen, T. T.
Ayyad, Y.
Chan, P. Y.
Fukuda, M.
Geissel, H.
Harakeh, M. N.
Hashimoto, T.
Hoang, T. H.
Ideguchi, E.
Inoue, A.
Jansen, G. R.
Kanungo, R.
Kawabata, T.
Khiem, L. H.
Lin, W. P.
Matsuta, K.
Mihara, M.
Momota, S.
Nagae, D.
Nguyen, N. D.
Nishimura, D.
Otsuka, T.
Ozawa, A.
Ren, P. P.
Sakaguchi, H.
Scheidenberger, C.
Tanaka, J.
Takechi, M.
Wada, R.
Yamamoto, T.
author_facet Tran, D. T.
Ong, H. J.
Hagen, G.
Morris, T. D.
Aoi, N.
Suzuki, T.
Kanada-En’yo, Y.
Geng, L. S.
Terashima, S.
Tanihata, I.
Nguyen, T. T.
Ayyad, Y.
Chan, P. Y.
Fukuda, M.
Geissel, H.
Harakeh, M. N.
Hashimoto, T.
Hoang, T. H.
Ideguchi, E.
Inoue, A.
Jansen, G. R.
Kanungo, R.
Kawabata, T.
Khiem, L. H.
Lin, W. P.
Matsuta, K.
Mihara, M.
Momota, S.
Nagae, D.
Nguyen, N. D.
Nishimura, D.
Otsuka, T.
Ozawa, A.
Ren, P. P.
Sakaguchi, H.
Scheidenberger, C.
Tanaka, J.
Takechi, M.
Wada, R.
Yamamoto, T.
author_sort Tran, D. T.
collection PubMed
description The nuclear shell structure, which originates in the nearly independent motion of nucleons in an average potential, provides an important guide for our understanding of nuclear structure and the underlying nuclear forces. Its most remarkable fingerprint is the existence of the so-called magic numbers of protons and neutrons associated with extra stability. Although the introduction of a phenomenological spin–orbit (SO) coupling force in 1949 helped in explaining the magic numbers, its origins are still open questions. Here, we present experimental evidence for the smallest SO-originated magic number (subshell closure) at the proton number six in (13–20)C obtained from systematic analysis of point-proton distribution radii, electromagnetic transition rates and atomic masses of light nuclei. Performing ab initio calculations on (14,15)C, we show that the observed proton distribution radii and subshell closure can be explained by the state-of-the-art nuclear theory with chiral nucleon–nucleon and three-nucleon forces, which are rooted in the quantum chromodynamics.
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spelling pubmed-59133142018-04-25 Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes Tran, D. T. Ong, H. J. Hagen, G. Morris, T. D. Aoi, N. Suzuki, T. Kanada-En’yo, Y. Geng, L. S. Terashima, S. Tanihata, I. Nguyen, T. T. Ayyad, Y. Chan, P. Y. Fukuda, M. Geissel, H. Harakeh, M. N. Hashimoto, T. Hoang, T. H. Ideguchi, E. Inoue, A. Jansen, G. R. Kanungo, R. Kawabata, T. Khiem, L. H. Lin, W. P. Matsuta, K. Mihara, M. Momota, S. Nagae, D. Nguyen, N. D. Nishimura, D. Otsuka, T. Ozawa, A. Ren, P. P. Sakaguchi, H. Scheidenberger, C. Tanaka, J. Takechi, M. Wada, R. Yamamoto, T. Nat Commun Article The nuclear shell structure, which originates in the nearly independent motion of nucleons in an average potential, provides an important guide for our understanding of nuclear structure and the underlying nuclear forces. Its most remarkable fingerprint is the existence of the so-called magic numbers of protons and neutrons associated with extra stability. Although the introduction of a phenomenological spin–orbit (SO) coupling force in 1949 helped in explaining the magic numbers, its origins are still open questions. Here, we present experimental evidence for the smallest SO-originated magic number (subshell closure) at the proton number six in (13–20)C obtained from systematic analysis of point-proton distribution radii, electromagnetic transition rates and atomic masses of light nuclei. Performing ab initio calculations on (14,15)C, we show that the observed proton distribution radii and subshell closure can be explained by the state-of-the-art nuclear theory with chiral nucleon–nucleon and three-nucleon forces, which are rooted in the quantum chromodynamics. Nature Publishing Group UK 2018-04-23 /pmc/articles/PMC5913314/ /pubmed/29686394 http://dx.doi.org/10.1038/s41467-018-04024-y Text en © The Author(s) 2018 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.
spellingShingle Article
Tran, D. T.
Ong, H. J.
Hagen, G.
Morris, T. D.
Aoi, N.
Suzuki, T.
Kanada-En’yo, Y.
Geng, L. S.
Terashima, S.
Tanihata, I.
Nguyen, T. T.
Ayyad, Y.
Chan, P. Y.
Fukuda, M.
Geissel, H.
Harakeh, M. N.
Hashimoto, T.
Hoang, T. H.
Ideguchi, E.
Inoue, A.
Jansen, G. R.
Kanungo, R.
Kawabata, T.
Khiem, L. H.
Lin, W. P.
Matsuta, K.
Mihara, M.
Momota, S.
Nagae, D.
Nguyen, N. D.
Nishimura, D.
Otsuka, T.
Ozawa, A.
Ren, P. P.
Sakaguchi, H.
Scheidenberger, C.
Tanaka, J.
Takechi, M.
Wada, R.
Yamamoto, T.
Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes
title Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes
title_full Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes
title_fullStr Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes
title_full_unstemmed Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes
title_short Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes
title_sort evidence for prevalent z = 6 magic number in neutron-rich carbon isotopes
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5913314/
https://www.ncbi.nlm.nih.gov/pubmed/29686394
http://dx.doi.org/10.1038/s41467-018-04024-y
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