Search for Ferromagnetically Trapped Magnetic Monopoles of Cosmic-Ray Origin

Eiichi Goto, Henry H. Kolm, and Kenneth W. Ford
Phys. Rev. 132, 387 – Published 1 October 1963
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Abstract

Magnetic monopoles, if they exist, should be trapped and accumulated in ferromagnetic materials. Using the high field of a pulsed magnet, we have sought to extract monopoles from a magnetite outcrop on the earth's surface and from fragments of a stony-iron meteorite. In the nuclear emulsions used for detection, no tracks were found satisfying our geometric criteria and having an energy-loss rate compatible with the theoretical expectation for monopoles. The area-time product of the magnetite cosmic-ray exposure is estimated to be about 1013 cm2 sec. From the negative results, upper-limit monopole production cross sections in the atmosphere are estimated as a function of assumed monopole mass.

  • Received 21 May 1963

DOI:https://doi.org/10.1103/PhysRev.132.387

©1963 American Physical Society

Authors & Affiliations

Eiichi Goto*

  • Department of Physics, University of Tokyo, Tokyo, Japan

Henry H. Kolm

  • National Magnet Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts

Kenneth W. Ford*,†

  • Department of Physics, Brandeis University, Waltham, Massachusetts

  • *Work performed while two of the authors (E. G. and K. F.) were at the Massachusetts Institute of Technology on leave from their home universities.
  • Work supported in part by the National Science Foundation.

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Vol. 132, Iss. 1 — October 1963

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