The standard model effective potential is calculated at finite temperature to
order g^4,\la^2 and a complete zero temperature renormalization is performed.
In comparison with lower order calculations the strength of the first order
phase transition has increased dramatically. This effect can be traced back to
infrared contributions from typical non-Abelian diagrams and to the infrared
behaviour of the scalar sector close to the critical temperature. Several
quantities, e.g. surface tension, latent heat and field expectation value are
analyzed for an SU(2)-Higgs model and for the full standard model in detail. An
explicit formula enabling further analytic or numerical study is presented.
(DESY-94-025)Comment: DESY-94-025, 18 pages, Latex, without figures. An easy way to obtain
a copy with figures: anonymous ftp to x4u2.desy.de and take the file
desy94-025.ps (postscrip file) or desy94-025.shar (uuencoded compressed file,
recover with the command 'sh') from directory /pub/preprints/desy/199