Self-gravitating charged fluid spheres with anisotropic pressures

The coupled system of the spherically symmetric Einstein--Maxwell differential equations is solved under two different source conditions: non-zero electric charge and pressure anisotropy. Expressions for the metric functions, and pressures which extend the Tolman VII exact solution are deduced from...

Full description

Saved in:
Bibliographic Details
Main Authors Raghoonundun, Ambrish M, Hobill, David W
Format Journal Article
LanguageEnglish
Published 10.03.2016
Subjects
Physics - General Relativity and Quantum Cosmology
Online AccessGet full text

Cover

More Information
Summary:The coupled system of the spherically symmetric Einstein--Maxwell differential equations is solved under two different source conditions: non-zero electric charge and pressure anisotropy. Expressions for the metric functions, and pressures which extend the Tolman VII exact solution are deduced from the new solutions. By applying boundary conditions to these solutions, all integration constants are computed in terms of parameters that are physically meaningful.
DOI:10.48550/arxiv.1603.03373