  We want to unify usual equation of motion laws of nature with "laws" about
initial conditions, second law of thermodynamics, cosmology. By introducing an
imaginary part -- of a similar form but different parameters as the usual real
part -- for the action to be used in the Feynmann path way integral we obtain a
model determining (not only equations of motion but) also the initial
conditions, for say a quantum field theory. We set up the formalism for e.g.
expectation values, classical approximation in such a model and show that
provided the imaginary part gets unimportant except in the Big Bang era the
model can match the usual theory. Speculatively requiring that there be place
for Dirac strings and thus in principle monopoles in the model we can push away
the effects of the imaginary part to be involved only with particles not yet
found. Most promising for seeing the initial condition determining effects from
the imaginary part is thus the Higgs particle. We predict that the width of the
Higgs particle shall likely turn out to be (appreciably perhaps) broader than
calculated by summing usual decay rates. Higgs machines will be hit by bad
luck.

High Energy Physics - Phenomenology;High Energy Physics - Theory