Science ❯ Physics ❯ Astrophysics
Detection Methods WIMPs Axions Primordial Black Holes Dark Energy Gamma Rays Gravitational Effects LUX-ZEPLIN Experiment Research Self-Interacting Dark Matter Weakly Interacting Massive Particles (WIMPs) Dwarf Galaxies Dark Sector Research Formation of Small Galaxies Fermi Gamma-ray Space Telescope Clustering Properties Cosmological Models Galactic Evolution Dark Photons Research Initiatives New Physics Cosmic Void Research Pulsar Timing Arrays Hypothetical Particles Dark Fluid Models Theories Alternative Explanations SuperCDMS Experiment Massless Topological Defects Neutrino Interactions Nature of Dark Matter WIMP Particles SuperCDMS Galaxy Formation Cosmic Phenomena Galactic Dynamics Research Methods Cosmology Scalar Fields Weakly Interacting Massive Particles Halo Models Cosmic Structures Subhalo Abundance Cosmic Matter Distribution Massive Stars Detection Gamma-Ray Emissions Dark Charge Cosmic Glitch Gravitational Lensing Asymmetric Dark Matter Magnetic Fields Topological Defects Halo Structure Halo Mass Function Evidence Self-Interaction Cosmological Structures Galactic Nuclei Gravitational Waves Observational Evidence Gamma Radiation Theoretical Models Properties and Effects Sterile Neutrinos Cosmic Web Brown Dwarfs Anomalous Signals Mass and Gravity Dark Matter Halo Theoretical Implications Dark Matter Clouds
The peer-reviewed study argues that gamma-ray signals depend on a local mix of two dark matter particle types that only annihilate when they meet.
