The aim of the present work is to work out the analytic expression of the gravitational potential for a cylindrical mass distribution where the origin is arbitrarily situated outside the distributed mass. The analytic findings are supported with some graphical plots obtained numerically. The line of interest in this direction of research lies on problems of Newtonian gravity, which is highly relevant to modern engineering where massive objects are involved. Especially the above work is relevant to technologies of satellite motions and general theory of relativity. Relevance of the work: In general the Gravitational Potential (GP) has implications in General Theory of Relativity (Ellis et al. in General Relativity and Gravitation 32:127–144, 2000). As the galaxies have different shapes like elliptical, disc, spiral, the calculation of GP due to masses of such shapes are important in Astrophysics. Knowledge of the GP due to such bodies will help to understand the dynamics of cluster of galaxies and gravitational bending of light due to galaxies of various shapes.

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Modeling Gravitational Potential of a Uniform Solid Cylinder at any Point Outside the Mass

  • R Chakravarty,
  • T Som

摘要

The aim of the present work is to work out the analytic expression of the gravitational potential for a cylindrical mass distribution where the origin is arbitrarily situated outside the distributed mass. The analytic findings are supported with some graphical plots obtained numerically. The line of interest in this direction of research lies on problems of Newtonian gravity, which is highly relevant to modern engineering where massive objects are involved. Especially the above work is relevant to technologies of satellite motions and general theory of relativity. Relevance of the work: In general the Gravitational Potential (GP) has implications in General Theory of Relativity (Ellis et al. in General Relativity and Gravitation 32:127–144, 2000). As the galaxies have different shapes like elliptical, disc, spiral, the calculation of GP due to masses of such shapes are important in Astrophysics. Knowledge of the GP due to such bodies will help to understand the dynamics of cluster of galaxies and gravitational bending of light due to galaxies of various shapes.