Relic cooling across muon annihilation 2026-10-14
A relativistic relic that decouples between pion and muon annihilation keeps constant. The coupled bath initially contains photons, electron-positron pairs, muon-antimuon pairs and three neutrino-antineutrino species, with entropy degrees of freedom . After muon annihilation this is , giving the displayed temperature ratio. After neutrino decoupling, electron-positron annihilation heats photons by , so the final relic-to-photon ratio becomes . This counting assumes the species are relativistic when counted and treats annihilations and decoupling as sharp equilibrium transitions.
A relativistic species decoupling before ordinary neutrino decoupling cools as . Cosmological entropy conservation in the remaining bath gives , where counts that bath just after the early species has left it. Subsequent electron-positron annihilation in cosmology gives . For the ideal high-temperature relativistic entropy content of the Standard Model, the resulting ratio is about .
Weak-decoupling temperature estimate 2026-10-14
In natural units with unreduced Planck mass , the radiation-era Hubble parameter scales as , while a low-energy weak interaction rate scales as . Their equality gives a decoupling scale of order one MeV. Distinct weak processes have distinct rate coefficients: neutrino decoupling and cosmological weak freeze-out of neutron-proton conversion are nearby events, not an identical precise temperature inferred from the power laws alone.