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Swelling of doubly magic $^{48}$Ca core in Ca isotopes beyond $N=28$

Authors :
Tanaka, M.
Takechi, M.
Homma, A.
Fukuda, M.
Nishimura, D.
Suzuki, T.
Tanaka, Y.
Moriguchi, T.
Ahn, D. S.
Aimaganbetov, A.
Amano, M.
Arakawa, H.
Bagchi, S.
Behr, K. -H.
Burtebayev, N.
Chikaato, K.
Du, H.
Ebata, S.
Fujii, T.
Fukuda, N.
Geissel, H.
Hori, T.
Horiuchi, W.
Hoshino, S.
Igosawa, R.
Ikeda, A.
Inabe, N.
Inomata, K.
Itahashi, K.
Izumikawa, T.
Kamioka, D.
Kanda, N.
Kato, I.
Kenzhina, I.
Korkulu, Z.
Kuk, Y.
Kusaka, K.
Matsuta, K.
Mihara, M.
Miyata, E.
Nagae, D.
Nakamura, S.
Nassurlla, M.
Nishimuro, K.
Nishizuka, K.
Ohnishi, K.
Ohtake, M.
Ohtsubo, T.
Omika, S.
Ong, H. J.
Ozawa, A.
Prochazka, A.
Sakurai, H.
Scheidenberger, C.
Shimizu, Y.
Sugihara, T.
Sumikama, T.
Suzuki, H.
Suzuki, S.
Takeda, H.
Tanaka, Y. K.
Tanihata, I.
Wada, T.
Wakayama, K.
Yagi, S.
Yamaguchi, T.
Yanagihara, R.
Yanagisawa, Y.
Yoshida, K.
Zholdybayev, T. K.
Source :
Phys. Rev. Lett. 124, 102501 (2020)
Publication Year :
2019

Abstract

Interaction cross sections for $^{42\textrm{-}51}$Ca on a carbon target at 280 MeV/nucleon have been measured for the first time. The neutron number dependence of derived root-mean-square matter radii shows a significant increase beyond the neutron magic number $N=28$. Furthermore, this enhancement of matter radii is much larger than that of the previously measured charge radii, indicating a novel growth in neutron skin thickness. A simple examination based on the Fermi-type distribution, and the Mean-Field calculations point out that this anomalous enhancement of the nuclear size beyond $N=28$ results from an enlargement of the core by a sudden increase in the surface diffuseness of the neutron density distribution, which implies the swelling of the bare $^{48}$Ca core in Ca isotopes beyond $N=28$.<br />Comment: 6 pages, 3 figures

Subjects

Subjects :
Nuclear Experiment

Details

Database :
arXiv
Journal :
Phys. Rev. Lett. 124, 102501 (2020)
Publication Type :
Report
Accession number :
edsarx.1911.05262
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevLett.124.102501