TY - JOUR
T1 - [Formula Presented] decay of [Formula Presented] and [Formula Presented] and implication for solar-neutrino detection
AU - Liu, W.
AU - Hellström, M.
AU - Collatz, R.
AU - Benlliure, J.
AU - Chulkov, L.
AU - Gil, D. Cortina
AU - Farget, F.
AU - Grawe, H.
AU - Hu, Z.
AU - Iwasa, N.
AU - Pfützner, M.
AU - Piechaczek, A.
AU - Raabe, R.
AU - Reusen, I.
AU - Roeckl, E.
AU - Vancraeynest, G.
AU - Wöhr, A.
N1 - Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.
PY - 1998
Y1 - 1998
N2 - The [Formula Presented] decay of [Formula Presented] and [Formula Presented] was studied by measuring the [Formula Presented]-delayed proton and [Formula Presented] emission. The half-lives for [Formula Presented] and [Formula Presented] were determined to be 54(2) and 82(3) ms, respectively. The experimental [Formula Presented]-decay strengths are compared with shell-model calculations and results from other measurements. The integrated Gamow-Teller strengths for [Formula Presented] and [Formula Presented] were found to be quenched, compared to the calculations, by factors of 0.79(3) and 0.93(3), respectively. Based on the experimental [Formula Presented]-decay strength, the neutrino absorption cross section and induced neutrino event rates for [Formula Presented] were determined to be [Formula Presented] and [Formula Presented] SNU, respectively.
AB - The [Formula Presented] decay of [Formula Presented] and [Formula Presented] was studied by measuring the [Formula Presented]-delayed proton and [Formula Presented] emission. The half-lives for [Formula Presented] and [Formula Presented] were determined to be 54(2) and 82(3) ms, respectively. The experimental [Formula Presented]-decay strengths are compared with shell-model calculations and results from other measurements. The integrated Gamow-Teller strengths for [Formula Presented] and [Formula Presented] were found to be quenched, compared to the calculations, by factors of 0.79(3) and 0.93(3), respectively. Based on the experimental [Formula Presented]-decay strength, the neutrino absorption cross section and induced neutrino event rates for [Formula Presented] were determined to be [Formula Presented] and [Formula Presented] SNU, respectively.
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U2 - 10.1103/PhysRevC.58.2677
DO - 10.1103/PhysRevC.58.2677
M3 - Article
AN - SCOPUS:0000131813
SN - 0556-2813
VL - 58
SP - 2677
EP - 2688
JO - Physical Review C - Nuclear Physics
JF - Physical Review C - Nuclear Physics
IS - 5
ER -