Dynamical Tsallis q during WIMP freeze-out leaves residual nonextensivity that alters neutrino energy density and N_eff through a phenomenological memory channel while staying within observational limits.
Cosmic abundances of stable particles: Improved analysis,
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Dynamical Tsallis WIMP Freeze-Out and Residual Memory Channels in the Radiation Sector
Dynamical Tsallis q during WIMP freeze-out leaves residual nonextensivity that alters neutrino energy density and N_eff through a phenomenological memory channel while staying within observational limits.