Study the Non-Linear Stability of Non-Collinear Libration Point in the Restricted Three-Body Configuration When the Shapes of the Primaries are Taken as …

B Singh, K Shalini, SN Prasad, AA Ansari - Solar System Research, 2023 - Springer
The main focus of the present research work is to analyze the non-linear stability of the
triangular equilibrium points and in the restricted three-body problem (R3BP). The condition …

Non-Linear Stability in the CR3B Problem under the Effects of Beyond-Newtonian Dynamics and Kerr Like Primaries

SN Prasad, Abdullah, B Singh, K Shalini - Astronomy Reports, 2024 - Springer
In the present research work, we have carried out an analysis of the non-linear stability of
the circular restricted three-body problem (CR3BP) with Kerr-like primaries. The model …

Effect of perturbed potential of heterogeneous triaxial rigid bodies of N layers on the stability of libration points in the R3BP

K Shalini, P Sharma, K Ranjana - New Astronomy, 2024 - Elsevier
In this paper, we investigate the motion of an infinitesimal mass m 3 in the restricted three-
body problem by taking both the primaries as heterogeneous triaxial rigid bodies with N …

(R2086) Circular Restricted Three-Body Interaction Problem With Various Perturbations

SK Sahdev - Applications and Applied Mathematics …, 2024 - digitalcommons.pvamu.edu
The motion properties of the infinitesimal body is studied under the forces due to kerr-like
oblate heterogeneous primary, continuation fractional potential for secondary, solar sail …

Circular Restricted Three-Body Interaction Problem With Various Perturbations.

SK Sahdev - Applications & Applied Mathematics, 2024 - search.ebscohost.com
The motion properties of the infinitesimal body is studied under the forces due to kerr-like
oblate heterogeneous primary, continuation fractional potential for secondary, solar sail …