  We consider the PT symmetric flat Friedmann model of two scalar fields with
positive kinetic terms. While the potential of one ("normal") field is taken
real, that of the other field is complex. We study a complex classical solution
of the system of the two Klein-Gordon equations together with the Friedmann
equation. The solution for the normal field is real while the solution for the
second field is purely imaginary, realizing classically the "phantom" behavior.
The energy density and pressure are real and the corresponding geometry is
well-defined. The Lagrangian for the linear perturbations has the correct
potential signs for both the fields, so that the problem of stability does not
arise. The background dynamics is determined by an effective action including
two real fields one normal and one "phantom". Remarkably, the phantom phase in
the cosmological evolution is transient and the Big Rip never occurs. Our model
is contrasted to well-known quintom models, which also include one normal and
one phantom fields.
