Neutron production by cosmic-ray muons at shallow depth

F. Boehm, J. Busenitz, B. Cook, G. Gratta, H. Henrikson, J. Kornis, D. Lawrence, K. B. Lee, K. McKinny, L. Miller, V. Novikov, A. Piepke, B. Ritchie, D. Tracy, P. Vogel, Y-F. Wang, and J. Wolf (Palo Verde Collaboration)
Phys. Rev. D 62, 092005 – Published 12 October 2000
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Abstract

The yield of neutrons produced by cosmic ray muons at a shallow depth of 32 meters of water equivalent has been measured. The Palo Verde neutrino detector, containing 11.3 tons of Gd loaded liquid scintillator and 3.5 tons of acrylic, served as a target. The rate of one and two neutron captures was determined. Modeling the neutron capture efficiency allowed us to deduce the total yield of neutrons, Ytot=(3.60±0.09±0.31)×105 neutrons per muon and g/cm2. This yield is consistent with previous measurements at similar depths.

  • Received 23 June 2000

DOI:https://doi.org/10.1103/PhysRevD.62.092005

©2000 American Physical Society

Authors & Affiliations

F. Boehm3, J. Busenitz1, B. Cook3, G. Gratta4, H. Henrikson3, J. Kornis1, D. Lawrence2, K. B. Lee3, K. McKinny1, L. Miller4, V. Novikov3, A. Piepke1,3, B. Ritchie2, D. Tracy4, P. Vogel3, Y-F. Wang4, and J. Wolf1 (Palo Verde Collaboration)

  • 1Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama 35487
  • 2Department of Physics and Astronomy, Arizona State University, Tempe, Arizona 85287
  • 3Department of Physics, California Institute of Technology, Pasadena, California 91125
  • 4Physics Department, Stanford University, Stanford, California 94305

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Vol. 62, Iss. 9 — 1 November 2000

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