Self-interacting dark matter from radiative bound-state-formation feedback
hep-ph, astro-ph.CO, astro-ph.GA
Submitted: 2026-10-19
Updated: 2026-10-19
Related papers
- Classification of g-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
- Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event
- A Unified Bogoliubov Approach to Primordial Gravitational Waves: From Inflation to Reheating
- Probing Memory-Burdened Primordial Black Holes with High-Energy Neutrinos
- From Axion Detection to Dark Matter Astronomy
- Enhanced Dark Matter Quantum Sensing via Phase-Space Geometric Interferometry