論文

査読有り
2016年7月

High energy-resolution measurement of the Se-82(He-3,t)Br-82 reaction for double-beta decay and for solar neutrinos

PHYSICAL REVIEW C
  • D. Frekers
  • M. Alanssari
  • T. Adachi
  • B. T. Cleveland
  • M. Dozono
  • H. Ejiri
  • S. R. Elliott
  • H. Fujita
  • Y. Fujita
  • M. Fujiwara
  • K. Hatanaka
  • M. Holl
  • D. Ishikawa
  • H. Matsubara
  • H. Okamura
  • P. Puppe
  • K. Suda
  • A. Tamii
  • J. Thies
  • H. P. Yoshida
  • 全て表示

94
1
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1103/PhysRevC.94.014614
出版者・発行元
AMER PHYSICAL SOC

A high-resolution (He-3,t) charge-exchange experiment at an incident energy of 420 MeV has been performed on the double beta (beta beta) decay nucleus Se-82. A detailed Gamow-Teller (GT(-)) strength distribution in Br-82 has been extracted, which provides information to the beta beta-decay nuclear matrix elements. Three strong and isolated transitions, which are to the 75, 1484 and the 2087 keV states in Br-82, are found to dominate the low-excitation region below approximate to 2.1 MeV. Above 2.1 MeV a sudden onset of a strong GT fragmentation is observed. The degree of fragmentation resembles a situation found in the neighboring A = 76 system (Ge-76), whereas the observed concentration of strength in the three low-lying states is reminiscent of the heavier neighbors Zr-96 and Mo-100. The strong GT transition to the 75 keV (1(+)) state makes Se-82 interesting for solar neutrino detection. The Se-82(nu(e),e(-))Br-82 solar neutrino capture rate in a nonoscillation scenario is therefore evaluated to 668 +/- 12(stat) +/- 60(sys) SNU, and some of the advantages of using selenium for solar neutrino studies are discussed.

リンク情報
DOI
https://doi.org/10.1103/PhysRevC.94.014614
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000380110000006&DestApp=WOS_CPL
ID情報
  • DOI : 10.1103/PhysRevC.94.014614
  • ISSN : 2469-9985
  • eISSN : 2469-9993
  • Web of Science ID : WOS:000380110000006

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