Radiation drag in the field of a non-spherical source
The motion of a test particle in the gravitational field of a non-spherical source endowed
with both mass and mass quadrupole moment is investigated when a test
radiation field is also present. The background is described by the Erez-Rosen solution,
which is a static spacetime belonging to the Weyl class of solutions to the
vacuum Einstein's field equations, and reduces to the familiar Schwarzschild solution
when the quadrupole parameter vanishes. The radiation flux has a fixed but arbitrary
(non-zero) angular momentum.






