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Interaction- and charge-changing cross sections for neutron-rich 63−80Cu isotopes toward the derivation of neutron skin thickness

  • G. Takayama*
  • , M. Fukuda
  • , M. Tanaka
  • , M. Fukutome
  • , M. Takechi
  • , T. Suzuki
  • , A. Homma
  • , D. Nishimura
  • , T. Moriguchi
  • , D. S. Ahn
  • , A. Aimaganbetov
  • , M. Amano
  • , M. Amitani
  • , H. Arakawa
  • , H. Baba
  • , S. Bagchi
  • , K. H. Behr
  • , N. Burtebayev
  • , K. Chikaato
  • , H. Du
  • T. Fujii, N. Fukuda, C. Fukushima, H. Geissel, T. Hori, S. Hoshino, R. Igosawa, A. Ikeda, N. Inabe, K. Inomata, S. Ishitani, K. Itahashi, T. Izumikawa, D. Kamioka, N. Kanda, I. Kato, I. Kenzhina, Z. Korkulu, Y. Kuk, K. Kusaka, K. Matsuta, M. Mihara, E. Miyata, D. Nagae, S. Nakamura, M. Nassurlla, K. Nishimuro, K. Nishizuka, N. Noguchi, M. Ohtake, T. Ohtsubo, S. Omika, H. J. Ong, K. Onishi, A. Ozawa, A. Prochazka, S. K. Sakhiyev, H. Sakurai, C. Scheidenberger, Y. Shimizu, T. Sumikama, S. Suzuki, H. Suzuki, R. Taguchi, H. Takeda, Y. Tanaka, Y. Tanaka, I. Tanihata, Y. Togano, T. Wada, K. Wakayama, S. Yagi, T. Yamaguchi, R. Yanagihara, Y. Yanagisawa, A. Yano, K. Yasuda, K. Yoshida, T. K. Zholdybayev
*此作品的通讯作者
  • The University of Osaka
  • Kyushu University
  • Niigata University
  • Saitama University
  • Tokyo City University
  • University of Tsukuba
  • RIKEN
  • L.N. Gumilyov Eurasian National University
  • Indian Institute of Technology, Dhanbad
  • GSI Helmholtz Centre for Heavy Ion Research
  • Institute for Basic Science
  • CAS - Institute of Modern Physics

科研成果: 期刊稿件文章同行评审

摘要

We have measured the interaction cross sections (σI) and charge-changing cross sections (σcc) for neutron-rich copper isotopes with mass numbers A=63−80 using the transmission method at the RIBF facility, RIKEN. From these values, we aim to derive the proton distribution radius (Rp) and the neutron distribution radius (Rn) for each isotope through subsequent analysis. Then, we plan to determine the neutron skin thickness (ΔRnp=Rn−Rp) for each isotope. These results will provide a new constraint on the symmetry energy parameter L of the equation of state (EoS) of nuclear matter and contribute to a deeper understanding of the nuclear structure of exotic nuclei.

源语言英语
文章编号123261
期刊Nuclear Physics A
1065
DOI
出版状态已出版 - 1月 2026
已对外发布

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