Abstract
This paper examines the motion of a test particle in the vicinity of the triangular points L 4,5 by considering the more massive primary as a source of radiation in the framework of the relativistic restricted three-body problem (R3BP). It is found that the position and stability of the triangular point are affected by both the relativistic factor and radiation pressure.
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Singh, J., Bello, N. Effect of radiation pressure on the stability of L 4,5 in the relativistic R3BP. Astrophys Space Sci 351, 483–490 (2014). https://doi.org/10.1007/s10509-014-1858-2
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DOI: https://doi.org/10.1007/s10509-014-1858-2