Numerical Relativity: Solving Geodesics equation for Massive Particle Around Black Holes Horizon

Authors

  • Shohel Ahmed Department of Mathematics, Bangladesh University of Engineering & Technology, Dhaka-1000
  • Md Showkat Ali Department of Mathematics, University of Dhaka, Dhaka-1000

DOI:

https://doi.org/10.3329/ganit.v35i0.28571

Keywords:

Static and rotating black holes, Geodesics equation, Schwarzschild solution, Kerr solution

Abstract

General relativity is the most beautiful physical theory ever invented. It describes one of the most pervasive features of the world we experience - gravitation. The gravitational field acts on nearby matter defines by the curvature of space-time. The black holes of nature are the most perfect macroscopic objects there are in the universe that constructed our concept of space-time. In this paper we use Einsteins general relativity to model the motions of massive particles around the two black holes: static and rotating. These equations of motion around black holes will be studied with special focus towards the variation of symmetry by the change of gravitational effect.

GANIT J. Bangladesh Math. Soc.Vol. 35 (2015) 79-85

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Author Biography

Shohel Ahmed, Department of Mathematics, Bangladesh University of Engineering & Technology, Dhaka-1000



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Published

2016-06-28

How to Cite

Ahmed, S., & Ali, M. S. (2016). Numerical Relativity: Solving Geodesics equation for Massive Particle Around Black Holes Horizon. GANIT: Journal of Bangladesh Mathematical Society, 35, 79–85. https://doi.org/10.3329/ganit.v35i0.28571

Issue

Vol. 35 (2015)

Section

Articles

License

The copyright of GANIT: Journal of Bangladesh Mathematical Society is reserved by Bangladesh Mathematical Society (web: https://bdmathsociety.org/)