Mixing electromagnetic radiation with dark radiation between BBN and recombination dilutes the baryon-to-entropy ratio, tightening the allowed total extra radiation to at most ~25% more than dark-radiation-only scenarios.
Precision early universe ther- modynamics made simple:N eff and neutrino decou- pling in the Standard Model and beyond
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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.
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Constraints on the Injection of Radiation in the Early Universe
Mixing electromagnetic radiation with dark radiation between BBN and recombination dilutes the baryon-to-entropy ratio, tightening the allowed total extra radiation to at most ~25% more than dark-radiation-only scenarios.
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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.