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Measurement of the β-asymmetry parameter of Cu67 in search for tensor-type currents in the weak interaction

G. Soti, F. Wauters, M. Breitenfeldt, P. Finlay, P. Herzog, A. Knecht, U. Köster, I. S. Kraev, T. Porobic, P. N. Prashanth, I. S. Towner, C. Tramm, D. Zákoucký, and N. Severijns
Phys. Rev. C 90, 035502 – Published 25 September 2014

Abstract

Background: Precision measurements at low energy search for physics beyond the standard model in a way complementary to searches for new particles at colliders. In the weak sector the most general β-decay Hamiltonian contains, besides vector and axial-vector terms, also scalar, tensor, and pseudoscalar terms. Current limits on the scalar and tensor coupling constants from neutron and nuclear β decay are on the level of several percent.

Purpose: Extracting new information on tensor coupling constants by measuring the β-asymmetry parameter in the pure Gamow-Teller decay of Cu67, thereby testing the V-A structure of the weak interaction.

Method: An iron sample foil into which the radioactive nuclei were implanted was cooled down to mK temperatures in a 3He4He dilution refrigerator. An external magnetic field of 0.1 T, in combination with the internal hyperfine magnetic field, oriented the nuclei. The anisotropic β radiation was observed with planar high-purity germanium detectors operating at a temperature of about 10 K. An on-line measurement of the β asymmetry of Cu68 was performed as well for normalization purposes. Systematic effects were investigated using geant4 simulations.

Results: The experimental value, Ã=0.587(14), is in agreement with the standard model value of 0.5991(2) and is interpreted in terms of physics beyond the standard model. The limits obtained on possible tensor-type charged currents in the weak interaction Hamiltonian are 0.045<(CT+CT)/CA<0.159 (90% C.L.).

Conclusions: The obtained limits are comparable to limits from other correlation measurements in nuclear β decay and contribute to further constraining tensor coupling constants.

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  • Received 24 April 2014

DOI:https://doi.org/10.1103/PhysRevC.90.035502

©2014 American Physical Society

Authors & Affiliations

G. Soti1,*, F. Wauters1,†, M. Breitenfeldt1, P. Finlay1, P. Herzog2, A. Knecht1,3, U. Köster4, I. S. Kraev1, T. Porobic1, P. N. Prashanth1, I. S. Towner5, C. Tramm2, D. Zákoucký6, and N. Severijns1

  • 1KU Leuven, Instituut voor Kern-en Stralingsfysica, Celestijnenlaan 200D, 3001 Leuven, Belgium
  • 2Helmholtz-Institut fuer Strahlen-und Kernphysik, Universitaet Bonn, D-53115 Bonn, Germany
  • 3PH Department, CERN, CH-1211 Geneva 23, Switzerland
  • 4Institut Laue Langevin, 71 avenue des Martyrs, F-38042 Grenoble Cedex, France
  • 5Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA
  • 6Nuclear Physics Institute, Academy of Sciences of the Czech Republic, 250 68 Řež, Czech Republic

  • *Corresponding author: gergelj.soti@fys.kuleuven.be
  • Current address: Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.

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Vol. 90, Iss. 3 — September 2014

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