Monopole-induced IGMF oscillations collimate blazar cascade particles and tighten monopole flux bounds to 6e-23 cm^-2 s^-1 sr^-1 from halo observations of 1ES 0229+200.
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A self-consistent Parker bound, anchored in the dynamo seed eigenmode and including turbulent pre-acceleration of monopoles, relaxes the standard extended Parker bound by roughly two orders of magnitude at low and intermediate monopole masses.
Global monopoles plus dilaton/axion/Born-Infeld yield regular self-gravitating magnetic monopoles and dyons with positive ADM mass, finite energy and linear exterior EM stability.
LHC diphoton data exclude magnetic monopoles and multiply charged particles with masses up to tens of TeV across various spins and charges.
Magnetic monopoles are theoretically well-motivated but remain unobserved after extensive searches in cosmic rays and at particle colliders such as the LHC.
citing papers explorer
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Magnetic monopole plasma oscillations and implications for TeV blazars
Monopole-induced IGMF oscillations collimate blazar cascade particles and tighten monopole flux bounds to 6e-23 cm^-2 s^-1 sr^-1 from halo observations of 1ES 0229+200.
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Self-Consistent Parker Bound on Magnetic Monopoles
A self-consistent Parker bound, anchored in the dynamo seed eigenmode and including turbulent pre-acceleration of monopoles, relaxes the standard extended Parker bound by roughly two orders of magnitude at low and intermediate monopole masses.
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Self-Gravitating Magnetic Monopoles and Dyons in String-Inspired Models: Structure and Stability
Global monopoles plus dilaton/axion/Born-Infeld yield regular self-gravitating magnetic monopoles and dyons with positive ADM mass, finite energy and linear exterior EM stability.
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Constraining magnetic monopoles and multiply charged particles with diphoton events at the LHC
LHC diphoton data exclude magnetic monopoles and multiply charged particles with masses up to tens of TeV across various spins and charges.
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Magnetic Monopoles -- From Dirac to the Large Hadron Collider
Magnetic monopoles are theoretically well-motivated but remain unobserved after extensive searches in cosmic rays and at particle colliders such as the LHC.