Abstract:
A collisionless transport equation is derived from Maxwell's
equations for photons in a nonrandom moving medium. An effective
metric tensor, which depends on the 4-velocity of the medium and
the refractive index, is used in the material equations. The
equations for the density matrix of the photons, written down in
the relativistic Wigner representation, give the required
transport equation on the transition to the approximation of
geometrical optics. This equation makes it possible to determine
not only the intensity of the electromagnetic radiation in the
medium but also its polarization. The mean Minkowski and Abraham
energy-momentum tensors are calculated and their physical meaning
is discussed.