Linear Stability of Equilibrium Points in the Generalized Photogravitational Chermnykh's Problem

Simple item page
dc.creatorKushvah, Badam Singh
dc.date2008-06-06
dc.date.accessioned2026-07-07T12:38:29Z
dc.date.available2026-07-07T12:38:29Z
dc.descriptionThe 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 effect of radiation pressure has been discussed numerically. The collinear points are linearly unstable and triangular points are stable in the sense of Lyapunov stability provided $μ< μ_{Routh}=0.0385201$. The effect of gravitational potential from the belt is also examined. The mathematical properties of this system are different from the classical restricted three body problem.
dc.identifierhttps://arxiv.org/abs/0806.1132
dc.identifierhttp://arxiv.org/abs/0806.1132
dc.identifierAstrophysics and Space Science, Volume 318, Numbers 1-2 / November, 2008
dc.identifierdoi:10.1007/s10509-008-9898-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218779
dc.subjectDynamical Systems
dc.subject70F15
dc.titleLinear Stability of Equilibrium Points in the Generalized Photogravitational Chermnykh's Problem
dc.typetext

Files

Collections

arXiv