  The measurements of the Higgs mass and top Yukawa coupling indicate that we
live in a very special Universe, at the edge of the absolute stability of the
electroweak vacuum. If fully stable, the Standard Model (SM) can be extended
all the way up to the inflationary scale and the Higgs field, non-minimally
coupled to gravity with strength $\xi$, can be responsible for inflation. We
show that the successful Higgs inflation scenario can also take place if the SM
vacuum is not absolutely stable. This conclusion is based on two effects that
were overlooked previously. The first one is associated with the effective
renormalization of the SM couplings at the energy scale $M_P/\xi$, where $M_P$
is the Planck scale. The second one is a symmetry restoration after inflation
due to high temperature effects that leads to the (temporary) disappearance of
the vacuum at Planck values of the Higgs field.
