Share Your Research, Maximize Your Social Impacts
Existence and Stability of the Equilibrium Points in the Photogravitational Magnetic Binaries Problem When the Both Primaries Are Oblate Spheriods
Journal: International Journal of Computational Engineering Research(IJCER) (Vol.6, No. 1)Publication Date: 2016-01-31
Authors : Mohd Arif;
Page : 01-09
Keywords : magnetic binaries problem; source of radiation; stability; equilibrium points; restricted three body problem; oblate body;
Source : Download
Find it from : Google Scholar
Abstract
In this article we have discussed the equilibrium points in the photogravitational magnetic binaries problem when the bigger primary is a oblate spheroid and source of radiation and the small primary is a oblate body and have investigated the stability of motion around these points.
Other Latest Articles
- Description of condensation and evaporation processes in cylindrical-type porous materials employing dual site-bond model
- Effect on heat transfer for laminar flow over Backward Facing Step with square cylinder placed inside using Higher Order Compact Scheme
- Description of condensation and evaporation processes in cylindrical-type porous materials employing dual site-bond model
- Effect on heat transfer for laminar flow over Backward Facing Step with square cylinder placed inside using Higher Order Compact Scheme
- EOQ Inventory Models for Deteriorating Item with Weibull Deterioration and Time-Varying Quadratic Holding Cost
Last modified: 2016-09-17 14:20:32