β decay of 40Ti and 41Ti and implication for solar-neutrino detection

W. Liu, M. Hellström, R. Collatz, J. Benlliure, L. Chulkov, D. Cortina Gil, F. Farget, H. Grawe, Z. Hu, N. Iwasa, M. Pfützner, A. Piechaczek, R. Raabe, I. Reusen, E. Roeckl, G. Vancraeynest, and A. Wöhr
Phys. Rev. C 58, 2677 – Published 1 November 1998
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Abstract

The β decay of 40Ti and 41Ti was studied by measuring the β-delayed proton and γ emission. The half-lives for 40Ti and 41Ti were determined to be 54(2) and 82(3) ms, respectively. The experimental β-decay strengths are compared with shell-model calculations and results from other measurements. The integrated Gamow-Teller strengths for 40Ti and 41Ti were found to be quenched, compared to the calculations, by factors of 0.79(3) and 0.93(3), respectively. Based on the experimental 40Tiβ-decay strength, the neutrino absorption cross section and induced neutrino event rates for 40Ar were determined to be 14.3(3)×1043cm2 and 9.4±0.2(stat)1.6+1.3(syst) SNU, respectively.

  • Received 26 March 1998

DOI:https://doi.org/10.1103/PhysRevC.58.2677

©1998 American Physical Society

Authors & Affiliations

W. Liu1,*, M. Hellström1, R. Collatz1, J. Benlliure1, L. Chulkov2, D. Cortina Gil1, F. Farget1, H. Grawe1, Z. Hu1, N. Iwasa1, M. Pfützner1,3, A. Piechaczek4, R. Raabe4, I. Reusen4, E. Roeckl1, G. Vancraeynest4, and A. Wöhr4

  • 1Gesellschaft für Schwerionenforschung, D-64291 Darmstadt, Germany
  • 2Kurchatov Institute, 123182 Moscow, Russian Federation
  • 3Institute of Experimental Physics, University of Warsaw, PL-00681 Warsaw, Poland
  • 4Institut voor Kern-en Stralingsfysika, Katholieke Universiteit, B-3030 Leuven, Belgium

  • *Permanent address: China Institute of Atomic Energy, P.O. Box 275(60), Beijing 102413, People’s Republic of China

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Vol. 58, Iss. 5 — November 1998

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