High-field magnets and solid-state track detectors have been used in an endeavor to extract and observe magnetic monopoles from ferromanganese pavement that was deposited at the bottom of the North Atlantic Ocean during the last 16 million years. The failure to observe poles sets new and restrictive limits on the abundance of monopoles and upon their production cross sections. For proton-nucleon collisions, the new cross sections are ≤ if the monopole mass is one proton mass and ≤2× at . Any magnetic charge up to 60 times Dirac's value of could have been detected. The flux of monopoles reaching the ocean floor is less than 4× at the 90% confidence level, so that no portion of the cosmic-ray energy spectrum up to ≅ eV is composed dominantly of magnetic monopoles.
- Received 28 April 1969
- Published in the issue dated August 1969
© 1969 The American Physical Society