Beam production of 18 Ne with in-flight method for alpha scattering at CRIB

N. N. Duy, K. Y. Chae, S. M. Cha, H. Yamaguchi, K. Abe, S. H. Bae, D. N. Binh, S. H. Choi, K. I. Hahn, S. Hayakawa, Byungsik Hong, N. Iwasa, D. Kahl, L. H. Khiem, A. Kim, D. H. Kim, E. J. Kim, G. W. Kim, M. J. Kim, K. KwakM. S. Kwag, E. J. Lee, S. I. Lim, B. Moon, J. Y. Moon, S. Y. Park, V. H. Phong, H. Shimizu, L. Yang, Z. Ge, T. V.Nhan Hao

Research output: Contribution to journalArticlepeer-review

2 Citations (Scopus)


We conducted a measurement of 18 Ne + α scattering in inverse kinematics, in order to search for experimental evidence of α-cluster structure in 22 Mg above the alpha threshold (E thr =8.14MeV) and determine the astrophysical rates of the 18 Ne(α p) 21 Na reaction under the conditions of break-out from the Hot-CNO cycle. A high intensity 18 Ne beam at 2.54 AMeV was successfully produced at CRIB (CNS Radioactive Ion Beam separator) of the Center for Nuclear Study, the University of Tokyo. This paper presents the in-flight production of the radioactive 18 Ne beam by using the production reaction 3 He( 16 O, 18 Ne)n with a windowed cryogenic gas target, which was employed in the mentioned resonant α-scattering experiment.

Original languageEnglish
Pages (from-to)8-13
Number of pages6
JournalNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Publication statusPublished - 2018 Jul 21


  • Alpha cluster
  • Alpha scattering
  • Inverse kinematics
  • RI beam production

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Instrumentation

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