Quark-Gluon Plasma as the Possible Source of Cosmological Dark Radiation
  The effective number of neutrinos, $N_{\text{eff}}$, obtained from CMB
fluctuations accounts for all effectively massless degrees of freedom present
in the Universe, including but not limited to the three known neutrinos. Using
a lattice-QCD derived QGP equation of state, we constrain the observed range of
$N_{\text{eff}}$ in terms of the the freeze-out of unknown degrees of freedom
near to quark-gluon hadronization. We explore limits on the coupling of these
particles, applying methods of kinetic theory. We present bounds on the
coupling of such particles and discuss the implications of a connection between
$N_{\text{eff}}$ and the QGP transformation for laboratory studies of QGP.
