Proton Distribution Radii of C 12-19 Illuminate Features of Neutron Halos

R. Kanungo, W. Horiuchi, G. Hagen, G. R. Jansen, P. Navratil, F. Ameil, J. Atkinson, Y. Ayyad, D. Cortina-Gil, I. Dillmann, A. Estradé, A. Evdokimov, F. Farinon, H. Geissel, G. Guastalla, R. Janik, M. Kimura, R. Knöbel, J. Kurcewicz, Yu A. LitvinovM. Marta, M. Mostazo, I. Mukha, C. Nociforo, H. J. Ong, S. Pietri, A. Prochazka, C. Scheidenberger, B. Sitar, P. Strmen, Y. Suzuki, M. Takechi, J. Tanaka, I. Tanihata, S. Terashima, J. Vargas, H. Weick, J. S. Winfield

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Abstract

Proton radii of C12-19 densities derived from first accurate charge changing cross section measurements at 900A MeV with a carbon target are reported. A thick neutron surface evolves from ∼0.5 fm in C15 to ∼1 fm in C19. The halo radius in C19 is found to be 6.4±0.7 fm as large as Li11. Ab initio calculations based on chiral nucleon-nucleon and three-nucleon forces reproduce the radii well.

Original languageEnglish
Article number102501
JournalPhysical Review Letters
Volume117
Issue number10
DOIs
StatePublished - Sep 2 2016

Funding

The authors are thankful for the support of the GSI accelerator staff and the FRS technical staff for an efficient running of the experiment. The support from NSERC, Canada for this work is gratefully acknowledged. R. Kanungo thankfully acknowledges the HIC-for-FAIR program and JLU-Giessen for supporting part of the research stay. The support of the People's Republic of China government and Beihang University under the Thousand Talents Program is gratefully acknowledged. The experiment is partly supported by the grant-in-aid program of the Japanese government under the Grant No. 23224008. This work was supported by the Office of Nuclear Physics, U.S. Department of Energy (Oak Ridge National Laboratory), Grant No. DE-SC0008499 (NUCLEI SciDAC Collaboration), NERRSC Grant No. 491045-2011, and the Field Work Proposal ERKBP57 at Oak Ridge National Laboratory. Computer time was provided by the Innovative and Novel Computational Impact on Theory and Experiment program. TRIUMF receives funding via a contribution through the National Research Council Canada. This research used resources of the Oak Ridge Leadership Computing Facility located in the Oak Ridge National Laboratory, which is supported by the Office of Science of the Department of Energy under Contract No. DE-AC05-00OR22725 and used computational resources of the National Center for Computational Sciences and the National Institute for Computational Sciences.

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