Origin of cosmological temperature
  A classical solution of the Standard Model + General Relativity is given by
an elliptic function whose periodicity in imaginary time is the origin of
cosmological temperature. Nothing beyond the Standard Model is assumed. The
solution is a $\mathrm{Spin}(4)$-symmetric universe expanding prior to the
electroweak transition. A rapidly oscillating $\mathrm{SU}(2)$ gauge field
holds the Higgs field to $0$ with strength inversely proportional to the scale
factor $a$. When $a$ reaches $a_{\scriptscriptstyle\mathrm{EW}}$ the solution
becomes unstable and the electoweak transition begins.
$a_{\scriptscriptstyle\mathrm{EW}}$ is the only free parameter in the solution.
The temperature at $a_{\scriptscriptstyle\mathrm{EW}}$ is $m_{H}/{(6\pi)^{1/2}}
= 28.8\,\text{GeV} = 3.34 \times 10^{14}\, \text{K}$ whatever the value of
$a_{\scriptscriptstyle\mathrm{EW}}$.
