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Nuclear astrophysics projects at the low-energy RI beam separator CRIB.

Authors :
Yamaguchi, H.
Hayakawa, S.
Shimizu, H.
Sakaguchi, Y.
Abe, K.
Imai, N.
Kitamura, N.
Kahl, D.
Yang, L.
Nakao, T.
Lee, P.
Lee, C. S.
Lee, K. B.
Akers, C.
Hashimoto, T.
Kwon, Y. K.
Moon, J. Y.
Jung, H. S.
Khiem, L. H.
Duy, N. N.
Source :
EPJ Web of Conferences; 2017, Vol. 165, p1-4, 4p, 1 Graph
Publication Year :
2017

Abstract

Studies on nuclear reactions relevant for astrophysics have been performed using the radioactive-isotope (RI) beams at the low-energy RI beam separator CRIB, operated by Center for Nuclear Study (CNS), the University of Tokyo. A type of measurement to study astrophysical reactions at CRIB is by the elastic resonant scattering with the thick-target method in inverse kinematics. We introduce the α resonant scattering with <superscript>7</superscript>Be beam, related to the astrophysical <superscript>7</superscript>Be(α, γ) reactions, which is relevant in the hot p-p chain and νp-process in supernovae. Other α resonant scattering measurements with <superscript>30</superscript>S, <superscript>10</superscript>Be, <superscript>15</superscript>O, and <superscript>18</superscript>Ne beams have been performed at CRIB, using the thick-target method. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
21016275
Volume :
165
Database :
Complementary Index
Journal :
EPJ Web of Conferences
Publication Type :
Conference
Accession number :
127183276
Full Text :
https://doi.org/10.1051/epjconf/201716501056