How well do integral-of-motion distribution functions describe Milky Way-analogue halos?
astro-ph.GA, astro-ph.CO, hep-ph
Submitted: 2026-09-28
Updated: 2026-09-28
Terminology
Sources
- Overview and public data release of the augmented Auriga Project: cosmological simulations of dwarf and Milky Way-mass galaxies
- Dark Matter Velocity Distributions: Comparing Numerical Simulations to Analytic Results
- Clumps and streams in the local dark matter distribution
- Dark Matter Annihilation Rates with Velocity-Dependent Annihilation Cross Sections
- Gamma-ray evidences of the dark matter clumps
- The impact of the phase-space density on the indirect detection of dark matter
- Sommerfeld-Enhanced $J$-Factors For Dwarf Spheroidal Galaxies
- Interpreting Dark Matter Direct Detection Independently of the Local Velocity and Density Distribution
- Phase-space structure in the local dark matter distribution and its signature in direct detection experiments
- Annual Modulation of Dark Matter: A Review
- The Structure of Cold Dark Matter Halos: Recent Insights from High Resolution Simulations
- The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
- Velocity-dependent J-factors for annihilation radiation from cosmological simulations
- Inferred Evidence For Dark Matter Kinematic Substructure with SDSS-Gaia
- CYGNUS: Feasibility of a nuclear recoil observatory with directional sensitivity to dark matter and neutrinos
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