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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
*Corresponding author for this work
  • 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

Research output: Contribution to journalArticlepeer-review

Abstract

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.

Original languageEnglish
Article number123261
JournalNuclear Physics A
Volume1065
DOIs
StatePublished - Jan 2026
Externally publishedYes

Keywords

  • Charge-changing cross section
  • EoS
  • Interaction cross section
  • Neutron skin thickness
  • Neutron-rich copper isotopes
  • Nuclear equation of state

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