Mirror dark matter admixture via mutual mean-field shifts softens the nuclear EOS, raises central densities, lowers maximum masses, and moves the direct Urca onset to higher or lower masses depending on symmetry-energy stiffness.
Totani, JCAP11, 080 (2025), arXiv:2507.07209 [astro-ph.HE]
5 Pith papers cite this work. Polarity classification is still indexing.
5
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 5roles
background 1polarities
background 1representative citing papers
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.
Pixel-level Fermi-LAT analysis confirms a high-latitude 20 GeV Galactic halo excess consistent with ~0.55–0.72 TeV WIMP annihilation at ⟨σv⟩~10⁻²⁴ cm³ s⁻¹, with dwarf tension reduced to R≃1.6–9.3 by systematics.
Electroweak doublet dark matter with Higgs-portal interactions accounts for the Galactic halo gamma-ray excess via gauge boson annihilation and allows inelastic scattering with ~100 keV splitting.
citing papers explorer
-
A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter
Mirror dark matter admixture via mutual mean-field shifts softens the nuclear EOS, raises central densities, lowers maximum masses, and moves the direct Urca onset to higher or lower masses depending on symmetry-energy stiffness.
-
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.
-
The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation
Pixel-level Fermi-LAT analysis confirms a high-latitude 20 GeV Galactic halo excess consistent with ~0.55–0.72 TeV WIMP annihilation at ⟨σv⟩~10⁻²⁴ cm³ s⁻¹, with dwarf tension reduced to R≃1.6–9.3 by systematics.
-
Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess
Electroweak doublet dark matter with Higgs-portal interactions accounts for the Galactic halo gamma-ray excess via gauge boson annihilation and allows inelastic scattering with ~100 keV splitting.
- Lyman-$\alpha$ forest constraints on pure and mixed fuzzy dark matter