Particle Physics Proton Acceleration Gamma Rays Radiation Effects Neutrino Astronomy Particle Acceleration Neutrinos Cosmic Neutrinos Supernovae High-Energy Particles Energy Losses Research Studies Data Analysis Solar System Acceleration Mechanisms Interstellar Medium Solar Activity Muon Detection Gamma Ray Bursts Galaxies Neutrino Production High-Energy Neutrinos Black Holes Voyager 1 Space Science Cosmic Ray Subsystem Ionization Abundance Origins Ultra-High-Energy Cosmic Rays Dark Matter Space Weather Ultra-High-Energy Neutrinos Gamma-ray Observations Radiowaves Energetic Particles Gamma-ray Emission Quark-Gluon Plasma Particle Interactions Stellar Evolution Terrestrial Gamma-Ray Flashes Radiation Protection Pulsar Halos Radiolysis Neutrino Oscillation Galactic Cosmic Rays Subatomic Particles High-Energy Astrophysics Pulsars Diffusion Models Baryon Injection Impact on Comets Galactic Phenomena Magnetism Space Environment Gamma-Ray Observations Neutron Detection Cosmic Ray Detection Antimatter Particle Detection Charged Particles
The result gives modelers a firmer basis for interpreting cosmic-ray antinuclei, including potential dark-matter signals.
