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Higher order normalizations are performed in the generalized photogravitational restricted three body problem with Poynting-Robertson drag. In this problem we have taken bigger primary as a source of radiation and smaller primary as an…

Dynamical Systems · Mathematics 2007-10-31 B. S. Kushvah , J. P. Sharma , B. Ishwar

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

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

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

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

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

The Nonlinear stability of triangular equilibrium points has been discussed in the generalised photogravitational restricted three body problem with Poynting-Robertson drag. The problem is generalised in the sense that smaller primary is…

Dynamical Systems · Mathematics 2007-12-01 B. S. Kushvah , J. P. Sharma , B. Ishwar

We announce a new bi-Hamiltonian integrable two-component system admitting the scalar 3rd-order Burgers equation as a reduction.

Exactly Solvable and Integrable Systems · Physics 2012-10-24 D. Talati , R. Turhan

We consider {\em discretized} Hamiltonian PDEs associated with a Hamiltonian function that can be split into a linear unbounded operator and a regular nonlinear part. We consider splitting methods associated with this decomposition. Using a…

Numerical Analysis · Mathematics 2008-12-01 Erwan Faou , Benoit Grebert , Eric Paturel

We consider Hamiltonian PDEs that can be split into a linear unbounded operator and a regular non linear part. We consider abstract splitting methods associated with this decomposition where no discretization in space is made. We prove a…

Numerical Analysis · Mathematics 2008-11-26 Erwan Faou , Benoit Grebert , Eric Paturel

We revisit a classical perturbative approach to the Hamiltonian related to the motions of Trojan bodies, in the framework of the Planar Circular Restricted Three-Body Problem (PCRTBP), by introducing a number of key new ideas in the…

Earth and Planetary Astrophysics · Physics 2015-09-09 Rocio Isabel Paez , Ugo Locatelli

In this paper we describe optimal reduction for the system of two bodies in $\mathbb{R}^3$ whose Hamiltonian is invariant under rotations and translations. In doing this, we introduce parametrizations and charts which help giving explicit…

Mathematical Physics · Physics 2024-06-04 Hernán Cendra , María Eugenia García

In this work, a method for solving the constraints of general relativity is presented, where first all geometrical objects are written in terms of a set of orthonormal triads and a flat Weitzenbock connection, which depends on the triads…

General Relativity and Quantum Cosmology · Physics 2017-07-18 Daniel W. F. Alves

The paper presents the conservative dynamics of two-body point-mass systems up to the third post-Newtonian order ($1/c^6$). The two-body dynamics is given in terms of a higher order ADM Hamilton function which results from a third…

General Relativity and Quantum Cosmology · Physics 2014-11-17 Piotr Jaranowski , Gerhard Schaefer

Generalized pseudo-Hamiltonian normal forms (GPHNF) and an effective method of obtaining them are introduced for two-dimensional systems of autonomous ODEs with a Hamiltonian quasi-homogeneous unperturbed part of an arbitrary degree. The…

Dynamical Systems · Mathematics 2012-05-31 Arthur Vaganyan , Vladimir Basov

This paper details a calculation of the second order normal form of the Stark effect Hamiltonian after regularization, using the Kustaanheimo- Stiefel mapping. After reduction we obtain an integrable two degree of freedom system on $S^2_h…

Symplectic Geometry · Mathematics 2022-06-23 Richard Cushman

A previously found momentum-dependent regularization ambiguity in the third post-Newtonian two point-mass Arnowitt-Deser-Misner Hamiltonian is shown to be uniquely determined by requiring global Poincar\'e invariance. The phase-space…

General Relativity and Quantum Cosmology · Physics 2014-11-17 Thibault Damour , Piotr Jaranowski , Gerhard Schäfer

A gravitational close encounter of a small body with a planet may produce a substantial change of its orbital parameters which can be studied using the circular restricted three-body problem. In this paper we provide parametric…

Classical Physics · Physics 2023-11-30 Massimiliano Guzzo

The problem of stability of the triangular libration points in the planar circular restricted three-body problem is considered. A software package, intended for normalization of autonomous Hamiltonian systems by means of computer algebra,…

Earth and Planetary Astrophysics · Physics 2013-12-30 I. I. Shevchenko

The three-particle Hamiltonian obtained by replacing the two-body trigonometric potential of the Sutherland problem by a three-body one of a similar form is shown to be exactly solvable. When written in appropriate variables, its…

High Energy Physics - Theory · Physics 2008-02-03 C. Quesne
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