Search for Slow Magnetic Monopoles with the NOvA Detector on the Surface
NOvA Collaboration: M. A. Acero, P. Adamson, L. Aliaga, T. Alion, V., Allakhverdian, N. Anfimov, A. Antoshkin, E. Arrieta-Diaz, L. Asquith, A., Aurisano, A. Back, C. Backhouse, M. Baird, N. Balashov, P. Baldi, B. A., Bambah, S. Bashar, K. Bays, S. Bending, R. Bernstein

TL;DR
This study used the NOvA detector to search for slow magnetic monopoles in cosmic rays, setting new upper limits on their flux in a previously unexplored low-mass range.
Contribution
First search for slow magnetic monopoles with the NOvA detector, establishing new flux limits in the low-mass, low-velocity region of parameter space.
Findings
No monopole events detected.
Set upper flux limit of 2×10⁻¹⁴ cm⁻² s⁻¹ sr⁻¹.
Covered a previously unexplored low-mass monopole region.
Abstract
We report a search for a magnetic monopole component of the cosmic-ray flux in a 95-day exposure of the NOvA experiment's Far Detector, a 14 kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed, setting an upper limit on the flux of at 90% C.L. for monopole speed and mass greater than GeV. Because of NOvA's small overburden of 3 meters-water equivalent, this constraint covers a previously unexplored low-mass region.
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