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Related papers: Nonlinear Stability in the Generalised Photogravit…

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In this paper we have examined the linear stability of triangular equilibrium points in the generalised photogravitational restricted three body problem with Poynting-Robertson drag. We have found the position of triangular equilibrium…

Dynamical Systems · Mathematics 2013-11-07 B. Ishwar , B. S. Kushvah

In this paper,we have found the equations of motion of Generalized Photogravitational restricted three body problem with Poynting-Robertson drag. The problem is generalized in the sense that smaller primary is supposed to be an oblate…

Dynamical Systems · Mathematics 2007-05-23 B. S. Kushvah , B. Ishwar

In this paper we have studied non-linear stability of triangular equilibrium points. We have performed first order normalization in the generalized photogravitational restricted three body problem with Poynting-Robertson drag. In this…

Dynamical Systems · Mathematics 2007-05-23 B. S. Kushvah , J. P. Sharma , B. Ishwar

The equilibrium points and their linear stability has been discussed in the generalized photogravitational Chermnykh's problem. The bigger primary is being considered as a source of radiation and small primary as an oblate spheroid. The…

Dynamical Systems · Mathematics 2009-02-08 Badam Singh Kushvah

We have examined the stability of triangular equilibrium points in Robes's generalised restricted three body problem. The problem is generalised in the sense that more massive primary has been taken as an oblate spheroid. We have found the…

Dynamical Systems · Mathematics 2007-05-23 K. T. Singh , B. S. Kushvah , B. Ishwar

Normal forms of Hamiltonian are very important to analyze the nonlinear stability of a dynamical system in the vicinity of invariant objects. This paper presents the normalization of Hamiltonian and the analysis of nonlinear stability of…

Chaotic Dynamics · Physics 2019-06-12 Ram Kishor , M. Xavier James Raj , Bhola Ishwar

We have examined the stability of collinear in Robes's generalised restricted three body problem. The problem is generalised in the sense that more massive primary has been taken as an oblate spheroid. We have found the position of…

Dynamical Systems · Mathematics 2007-05-23 K. T. Singh , B. S. Kushvah , B. Ishwar

We have discussed non-linear stability in photogravitational non-planar restricted three body problem with oblate smaller primary. By photogravitational we mean that both primaries are radiating. We normalised the Hamiltonian using Lie…

Dynamical Systems · Mathematics 2015-05-30 B. Ishwar , J. P. Sharma

The existence of equilibrium points and the effect of radiation pressure have been discussed numerically. The problem is generalized by considering bigger primary as a source of radiation and small primary as an oblate spheroid. We have…

Dynamical Systems · Mathematics 2009-02-08 Badam Singh Kushvah

The multi-dissipative photogravitational triaxial elliptic restricted three body problem is treated. The perturbed locations of triangular points are computed. The stability of the triangular points under changing one or more perturbing…

Earth and Planetary Astrophysics · Physics 2015-06-10 F. A. Abd El-Salam

The main goal of the present paper is to evaluate the perturbed locations and investigate the linear stability of the triangular points. We studied the problem in the elliptic restricted three body problem frame of work. The problem is…

Dynamical Systems · Mathematics 2021-09-29 M. Radwan , Nihad S. Abdel-Motelp

Linearization of the Hamiltonian is being performed around the triangular equilibrium points in the generalized photogravitational Chermnykh's problem. The bigger primary is being considered as a source of radiation and small primary as an…

Dynamical Systems · Mathematics 2010-03-23 Badam Singh Kushvah

We have performed normalization of Hamiltonian in the generalized photogravitational restricted three body problem with Poynting-Robertson drag. In this problem we have taken bigger primary as source of radiation and smaller primary as an…

Dynamical Systems · Mathematics 2007-09-27 B. S. Kushvah , J. P. Sharma , B. Ishwar

The Poynting-Robertson(P-R) effect on Lyapunov stability of equilibrium points is being discussed in the the generalized photogravitational Chermnykh's problem when bigger primary is a sours of radiation and smaller primary is an oblate…

Dynamical Systems · Mathematics 2010-03-23 Badam Singh Kushvah

Continuing work initiated in an earlier publication [Yamada, Tsuchiya, and Asada, Phys. Rev. D 91, 124016 (2015)], we reexamine the linear stability of the triangular solution in the relativistic three-body problem for general masses by the…

General Relativity and Quantum Cosmology · Physics 2017-11-08 Kei Yamada , Takuya Tsuchiya

The dynamics of the four-body problem have attracted increasing attention in recent years. In this paper, we extend the basic equilateral four-body problem by introducing the effect of radiation pressure, Poynting-Robertson drag, and solar…

Chaotic Dynamics · Physics 2020-03-12 J. E. Osorio-Vargas , Guillermo A. González , F. L. Dubeibe

We consider the modified restricted three body problem with power-law density profile of disk, which rotates around the center of mass of the system with perturbed mean motion. Using analytical and numerical methods we have found…

Dynamical Systems · Mathematics 2015-05-28 Badam Singh Kushvah , Ram Kishor , Uday Dolas

Since the strong degeneracies present in the N-body problem, even in the basic case of the planar three-body problem, nobody inspects the problem of nonlinear stability of Lagrange relative equilibrium. We introduce a new coordinate system…

Dynamical Systems · Mathematics 2022-07-01 Xiang Yu

This study examines the dynamics of the third body in an elliptic restricted three-body problem (ERTBP) framework, taking into account perturbations from radiation pressure, oblateness, and elongation of the primary bodies, as well as…

Earth and Planetary Astrophysics · Physics 2026-01-21 M. B. Saputra , H. S. Ramadhan , Ibnu N. Huda , Leonardus B. Putra

We investigate the stability of motion close to the Lagrangian equilibrium points L4 and L5 in the framework of the spatial, elliptic, restricted three- body problem, subject to the radial component of Poynting-Robertson drag. For this…

Earth and Planetary Astrophysics · Physics 2015-06-23 Christoph Lhotka , Alessandra Celletti
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