A simple model for accretion disks in the post-Newtonian approximation
p { margin-bottom: 0.1in; direction: ltr; line-height: 120%; text-align: left; }a:link { } In this paper, the evolution of accretion disks in the post-Newtonian limit has been investigated. These disks are formed around gravitational compact objects such as black holes, neutron stars, or white dwa...
Main Authors: | R Ranjbar, M Roshan, SH Abbassi |
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Format: | Article |
Language: | English |
Published: |
Isfahan University of Technology
2019-09-01
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Series: | Iranian Journal of Physics Research |
Subjects: | |
Online Access: | http://ijpr.iut.ac.ir/article-1-2486-en.html |
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