A theory of the dark matter
  In an earlier paper I proposed a highly symmetric semi-classical initial
condition to describe the universe in the period leading up to the electroweak
transition and completely determine all cosmology after that. Nothing beyond
the Standard Model is assumed. Inflation is not needed. The initial symmetry
allows no adjustable parameters. It is a complete theory of the Standard Model
cosmological epoch, predictive and falsifiable. Here, the time evolution of the
initial condition is calculated in the classical approximation. The fields with
nontrivial classical values are the SU(2)-weak gauge field (the cosmological
gauge field or CGF) and the Higgs field. The CGF produces the electroweak
transition then evolves as a non-relativistic perfect fluid
($w_{\mathrm{CGF}}\approx 0$). At the present time, i.e. when $H=H_{0}$, the
CGF energy density satisfies $\Omega_{\Lambda}+\Omega_{\mathrm{CGF}}=1$. The
CGF is the dark matter. The dark matter is a classical phenomenon of the
Standard Model. The classsical universe contains only the dark matter, no
ordinary matter. At next to leading order the fluctuations of the Standard
Model fields will provide a calculable, relatively small amount of ordinary
matter such that
$\Omega_{\Lambda}+\Omega_{\mathrm{CGF}}+\Omega_{\mathrm{ordinary}}=1$.
