Cosmic ray protons scattering off dark matter produce the Galactic Center gamma-ray excess through inelastic up-scattering followed by decay or direct elastic 2-to-3 photon production.
Abiet al.(DUNE), (2020), 10.2172/1599307, arXiv:2002.03005 [hep-ex]
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World data on isoscalar DIS cross-section ratios exhibit near-perfect cancellation of nuclear effects in the valence region 0.25 ≤ x ≤ 0.35 across nuclei.
In a 3+1 model with eV-scale sterile neutrino, cosmological bounds on sum of neutrino masses restrict sterile mixing angle θ14 and lightest active neutrino mass for vanishing |M_ee|, while JUNO precision on θ12 adds little constraint due to extra CP phase cancellations.
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Producing the GeV Galactic Center Excess via Cosmic Ray-Dark Matter Scattering
Cosmic ray protons scattering off dark matter produce the Galactic Center gamma-ray excess through inelastic up-scattering followed by decay or direct elastic 2-to-3 photon production.
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On the Cancellation of Nuclear Effects in the Valence Region
World data on isoscalar DIS cross-section ratios exhibit near-perfect cancellation of nuclear effects in the valence region 0.25 ≤ x ≤ 0.35 across nuclei.
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Phenomenology of Vanishing Effective Majorana Mass with a Sterile Neutrino under Cosmological and JUNO Constraints
In a 3+1 model with eV-scale sterile neutrino, cosmological bounds on sum of neutrino masses restrict sterile mixing angle θ14 and lightest active neutrino mass for vanishing |M_ee|, while JUNO precision on θ12 adds little constraint due to extra CP phase cancellations.