Rescuing Overabundant Dark Matter with a Strongly First Order Phase Transition in the Dark Sector
hep-ph, astro-ph.CO, hep-th
Submitted: 2026-02-18
Updated: 2026-09-08
Comments: 13 pages, 2 figures. Final published version
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Particle Dark Matter: Evidence, Candidates and Constraints
- Direct Detection of WIMP Dark Matter: Concepts and Status
- A review of indirect searches for particle dark matter
- Dark Matter Searches at Colliders
- Secluded WIMP Dark Matter
- Dark Matter and Dark Radiation
- The Four Basic Ways of Creating Dark Matter Through a Portal
- Dark Sectors and New, Light, Weakly-Coupled Particles
- The Dark Photon
- Illuminating Dark Photons with High-Energy Colliders
- Discovery Prospects for a Minimal Dark Matter Model at Cosmic and Intensity Frontier Experiments
- Indirect Dark Matter Signatures in the Cosmic Dark Ages I. Generalizing the Bound on s-wave Dark Matter Annihilation from Planck
- Enhanced Dark Matter Abundance in First-Order Phase Transitions
- Forbidden dark matter assisted by first-order phase transition and associated gravitational waves
- Physical Parameters and Renormalization of U(1)_a x U(1)_b Models
- Implications of Generalized Z-Z' Mixing
- The Physics of Heavy Z' Gauge Bosons
- Planck 2018 results. VI. Cosmological parameters
- First Dark Matter Search Results from the XENON1T Experiment
- Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment
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