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Precision evaluation of the Ga71(νe,e−) solar neutrino capture rate from the (He3,t) charge-exchange reaction

D. Frekers1, T. Adachi2, H. Akimune3, M. Alanssari1, B. A. Brown4, B. T. Cleveland5,*, H. Ejiri2, H. Fujita2, Y. Fujita2,6 et al.

M. Fujiwara2, V. N. Gavrin7, M. N. Harakeh8,9, K. Hatanaka2, M. Holl1, C. Iwamoto2, A. Lennarz1, A. Okamoto2, H. Okamura2,†, T. Suzuki2, and A. Tamii2

  • 1Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, D-48149 Münster, Germany
  • 2Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 567-0047, Japan
  • 3Department of Physics, Konan University, Kobe 658-8501, Japan
  • 4National Superconducting Cyclotron Laboratory, The Joint Institute for Nuclear Astrophysics and the Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
  • 5Department of Physics, University of Washington, Seattle WA98195, USA
  • 6Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
  • 7Institute for Nuclear Research, Russian Academy of Sciences, Moscow, 117312, Russia
  • 8Kernfysisch Versneller Instituut, University of Groningen, NL-9747 AA Groningen, The Netherlands
  • 9GSI Helmholtzzentrum für Schwerinonenforschung GmbH, D-64291 Darmstadt, Germany

  • *Also at SNOLAB, Lively, Ontario, Canada.
  • †Deceased.
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Phys. Rev. C 91, 034608 – Published 13 March, 2015Erratum Phys. Rev. C 100, 049901 (2019)

DOI: https://doi.org/10.1103/PhysRevC.91.034608

Abstract

A precision measurement of the Ga71(He3,t)Ge71 charge-exchange reaction was performed. By using a rather complete set of theoretical form factors to describe the cross-section angular distributions over a large angular range, the Gamow-Teller strength distribution up to the effective neutron-separation energy in Ge71 was extracted. The data and the analysis constrain the Ga71(νe,e−) solar neutrino rate in a neutrino nonoscillation scenario. For nonoscillating neutrinos we report a solar neutrino capture rate of 122.4±3.4(stat)±1.1(sys) SNU, which is lower than the presently accepted value of 132±18 SNU, though not in disagreement given the quoted errors.

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Erratum

Erratum: Precision evaluation of the Ga71(νe,e−) solar neutrino capture rate from the (He3,t) charge-exchange reaction [Phys. Rev. C 91, 034608 (2015)]

D. Frekers, T. Adachi, H. Akimune, M. Alanssari, B. A. Brown, B. T. Cleveland, H. Ejiri, H. Fujita, Y. Fujita, M. Fujiwara, V. N. Gavrin, M. N. Harakeh, K. Hatanaka, M. Holl, C. Iwamoto, A. Lennarz, A. Okamoto, H. Okamura, T. Suzuki, and A. Tamii
Phys. Rev. C 100, 049901 (2019)

Article Text

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Phys. Rev. C 91, 034608– Published 13 March, 2015
  • Received 19 January 2015

©2015 American Physical Society

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