Semi-annihilating dark matter in cosmological structures yields a boosted flux that can rival or exceed the galactic signal, and structure formation requires ⟨σ₂→₁v⟩ ≤ 4.2×10⁻¹⁹ (mχ/1 GeV) cm³/s.
On the Possibility of Separating Coherent and Incoherent (Anti)neutrino Scattering on Nuclei
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Cosmological signals of dark matter semi-annihilation
Semi-annihilating dark matter in cosmological structures yields a boosted flux that can rival or exceed the galactic signal, and structure formation requires ⟨σ₂→₁v⟩ ≤ 4.2×10⁻¹⁹ (mχ/1 GeV) cm³/s.