A simple mechanichal problem of the force-free motion of a relativistic bea
d inside a rotating pipe is examined. A relevant change of shape of the pip
e is considered. The force-free motion of the bead along the rotating pipe
is examined as the motion in a differentially rotating medium. The differen
tial rotation proves to be resembling a well known case of the Couette flow
without outer cylinder. The determination of vectoral fields (magnetic fie
ld) in the rotating charged mediums (plasma) is problematic for the laborat
ory observer. Therefore the same problem is examined in the framework of ge
neral relativity, that is the physical quantities are considered in the ine
rtial frame and non-inertial frame with no rotational inhomogeneity. The pr
oblematic character of the determination of the physical quantity in the di
fferentially rotating madium relative to the inertial observer is explained
. It is shown that at certain large distances from the rotation center the
pipe does not rotate. However, at rather small distances its shape takes on
the appearance of an expanded spiral-like configuration. A possible releva
nce of the obtained results to the motion of a relativistic plasma flows in
pulsar magnetosphere is pointed out. The areas of Crab pulsar's dipole rad
iation are estimated.