Dynamical Tsallis WIMP Freeze-Out and Residual Memory Channels in the Radiation Sector
hep-ph, astro-ph.CO, cond-mat.stat-mech
Submitted: 2026-05-27
Updated: 2026-09-09
Comments: Is an error in how we define the thermodynamics since we do not take the derivatives of the dynamical parameter "q(T)" and we need to do a re-do
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- Particle Dark Matter: Evidence, Candidates and Constraints
- Relic neutrino decoupling including flavour oscillations
- Towards a precision calculation of $N_{\rm eff}$ in the Standard Model II: Neutrino decoupling in the presence of flavour oscillations and finite-temperature QED
- Dark Matter Freeze Out with Tsallis Statistics in the Early Universe
- Neutrino decoupling including flavour oscillations and primordial nucleosynthesis
- A precision calculation of relic neutrino decoupling
- Constraining Tsallis Corrections to Photon Reheating from Electron-Positron Annihilation: A Phenomenological Approach
- Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
- Constraints on Tsallis Cosmology from Big Bang Nucleosynthesis and the Relic Abundance of Cold Dark Matter Particles
- Relic neutrino decoupling with flavour oscillations revisited
- Precision Early Universe Thermodynamics made simple: $N_{\rm eff}$ and Neutrino Decoupling in the Standard Model and beyond
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