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Triangular Equilibria in R3BP under the Consideration of Yukawa Correction to Newtonian Potential

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  • M. Javed Idrisi
  • Teklehaimanot Eshetie
  • Tenaw Tilahun
  • Mitiku Kerebh
  • A. R. Ashrafi

Abstract

We study the triangular equilibrium points in the framework of Yukawa correction to Newtonian potential in the circular restricted three-body problem. The effects of α and λ on the mean-motion of the primaries and on the existence and stability of triangular equilibrium points are analyzed, where α∈−1,1 is the coupling constant of Yukawa force to gravitational force, and λ∈0,∞ is the range of Yukawa force. It is observed that as λ⟶∞, the mean-motion of the primaries n⟶1+α1/2 and as λ⟶0, n⟶1. Further, it is observed that the mean-motion is unity, i.e., n=1 for α=0, n>1 if α>0 and n

Suggested Citation

  • M. Javed Idrisi & Teklehaimanot Eshetie & Tenaw Tilahun & Mitiku Kerebh & A. R. Ashrafi, 2022. "Triangular Equilibria in R3BP under the Consideration of Yukawa Correction to Newtonian Potential," Journal of Applied Mathematics, Hindawi, vol. 2022, pages 1-6, June.
  • Handle: RePEc:hin:jnljam:4072418
    DOI: 10.1155/2022/4072418
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    Cited by:

    1. Saravanamoorthi, P. & Idrisi, M. Javed & Ullah, M. Shahbaz, 2023. "Effect of radiations on in-plane equilibrium points due to central primary in the photo-gravitational restricted eight-body problem," Chaos, Solitons & Fractals, Elsevier, vol. 175(P1).

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