In CP arguments, we argue against a Standard Model explanation of the
baryon asymmetry of the universe in the presence of a first order phas
e transition. A CP-asymmetry is found in the reflection coefficients o
f quarks hitting the phase boundary created during the electroweak tra
nsition. The problem is analyzed both in an academic zero temperature-
case and in the realistic finite temperature one. The building blocks
are similar in both cases: Kobayashi-Maskawa CP-violation, CP-even pha
ses in the reflection coefficients of quarks, and physical transitions
due to fermion self-energies. In both cases an effect is present at o
rder alpha(W)2 in rate. A regular GIM behavior is found as intuitively
expected. In the finite temperature case, a crucial role is played by
the damping rate of quasiparticles in a hot plasma, which is a releva
nt scale together with M(W) and the temperature. The effect is many or
ders of magnitude below what observation requires, and indicates that
non-standard physics is indeed needed in the cosmological scenario.