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Relativistic Magnetic Monopole Flux Constraints from RICE
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We report an upper limit on the flux of relativistic monopoles based on the non-observation of in-ice showers by the Radio Ice Cherenkov Experiment (RICE) at the South Pole. We obtain a 95% C.L. limit of order 10^{-18}/(cm^2-s-sr) for intermediate mass monopoles of 10^7<gamma<10^{12} at the anticipated energy E=10^{16} GeV. This bound is over an order of magnitude stronger than all previously published experimental limits for this range of boost parameters gamma, and exceeds two orders of magnitude improvement over most of the range. We review the physics of radio detection, describe a Monte Carlo simulation including continuous and stochastic energy losses, and compare to previous experimental limits.
Forward citations
Cited by 2 Pith papers
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Timing-Based Search for Magnetic Monopoles with the NOvA Detector on the Surface
NOvA's 7.5-year search found zero magnetic monopole candidates and sets a 90% confidence upper limit of 8e-16 cm^-2 s^-1 sr^-1 for monopole speeds near 0.001c and masses above 1e9 GeV.
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Cosmology-Independent Constraints on Irreducible Magnetic Monopole Background
Cosmic-ray collisions with interstellar gas create monopoles that would drain galactic magnetic fields, yielding new cosmology-independent Parker-like bounds on light monopoles.
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