  Presuming that CMB photons are described by the deconfining phase of an SU(2)
Yang-Mills theory with the critical temperature for the
deconfining-preconfining phase transition matching the present CMB temperature
$T_0\sim 2.725\,$K (SU(2)$_{\tiny{CMB}}$), we investigate how CMB temperature
$T$ connects with the cosmological scale factor $a$ in a
Friedmann-Lema\^itre-Robertson-Walker Universe. Owing to a violation of
conformal scaling at late times, the tension between the (instantaneous)
redshift of reionisation from CMB observation ($z_{\tiny{re}}\sim 11$) and
quasar spectra ($z_{\tiny{re}}\sim 6$) is repealed. Also, we find that the
redshift of CMB decoupling moves from $z_{\tiny{dec}}\sim 1100$ to
$z_{\tiny{dec}}\sim 1775$ which questions $\Lambda$CDM cosmology at high
redshifts. Adapting this model to the conventional physics of three flavours of
massless cosmic neutrinos, we demonstrate inconsistency with the value
N$_{\tiny{eff}}\sim 3.36$ extracted from Planck data. Interactions between
cosmic neutrinos and the CMB implies a {\sl common} temperature $T$ of (no
longer separately conserved) CMB and neutrino fluids. N$_{\tiny{eff}}\sim 3.36$
then entails a universal, temperature induced cosmic neutrino mass $m_\nu=\xi
T$ with $\xi=3.973$. Our above results on $z_{\tiny{re}}$ and $z_{\tiny{dec}}$,
derived from SU(2)$_{\tiny{CMB}}$ alone, are essentially unaffected when
including such a neutrino sector.
