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.

UR - http://www.scopus.com/inward/record.url?scp=0000131813&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0000131813&partnerID=8YFLogxK

U2 - 10.1103/PhysRevC.58.2677

DO - 10.1103/PhysRevC.58.2677

M3 - Article

AN - SCOPUS:0000131813

VL - 58

SP - 2677

EP - 2688

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

SN - 0556-2813

IS - 5

ER -