Effect of perturbations on the linear stability of triangular libration points of the generalized photogravitational robes restricted three-body problem

摘要

The critical mass obtained depends on the small changes in the Coriolis and centrifugal forces, oblateness of the rigid shell and radiation of the second the second primary as well as the density parameter k. The stability of the triangular points depends largely on the values of k. The destabilizing tendencies of the centrifugal force, oblateness and radiation factors were enhanced when k>0and weakened for k<0.