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...

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Bibliographic Details
Main Authors: R Ranjbar, M Roshan, SH Abbassi
Format: Article
Language:English
Published: Isfahan University of Technology 2019-09-01
Series:Iranian Journal of Physics Research
Subjects:
Online Access:http://ijpr.iut.ac.ir/article-1-2486-en.html