Secondary cascades in the TAXN absorber produce a substantial millicharged particle flux that complements primary production and boosts FORMOSA signals by ~50% for m_χ below 0.1 GeV.
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QGSM-based prompt muon calculations match IceCube spectra above 500 TeV, while lower charm-production models require extra flux from rare decays of eta, eta', rho, omega, and phi mesons.
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A New Source of Millicharged Particles: Secondary Showers in the LHC Forward Absorber
Secondary cascades in the TAXN absorber produce a substantial millicharged particle flux that complements primary production and boosts FORMOSA signals by ~50% for m_χ below 0.1 GeV.
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High-energy atmospheric muon flux calculations in comparison with recent measurements
QGSM-based prompt muon calculations match IceCube spectra above 500 TeV, while lower charm-production models require extra flux from rare decays of eta, eta', rho, omega, and phi mesons.