Next Article in Journal
Near-Field THz Nanoscopy with Novel Accelerator-Based Photon Sources
Previous Article in Journal
Single-Use Paper Cups Circularity Improvement and Environmental Impact Mitigation Measures for Lappeenranta University of Technology Campus
 
 
Search for Articles:
Title / Keyword
Author / Affiliation / Email
Journal
Article Type
 
 
Advanced Search
 
Section
Special Issue
Volume
Issue
Number
Page
 
Journals
Proceedings
Volume 17
Issue 1
10.3390/proceedings2019017006
proceedings-logo
Submit to this Journal
► Article Menu

Article Menu

share Share announcement Help format_quote Cite question_answer Discuss in SciProfiles thumb_up
...
Endorse textsms
...
Comment
first_page
settings
Order Article Reprints
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
Proceeding Paper

Boosted Kerr Black Hole in the Presence of Plasma †

by
Carlos A. Benavides-Gallego
1,* and
Ahmadjon-Abdujabbarov Abdujabbarov
1,2
1
Center for Field Theory and Particle Physics and Department of Physics, Fudan University, Shanghai 200438, China
2
Ulugh Beg Astronomical Institute, Astronomicheskaya 33, Tashkent 100052, Uzbekistan
*
Author to whom correspondence should be addressed.
†
Presented at the Recent Progress in Relativistic Astrophysics, Shanghai, China, 6–8 May 2019.
Proceedings 2019, 17(1), 6; https://doi.org/10.3390/proceedings2019017006
Published: 4 September 2019
(This article belongs to the Proceedings of Recent Progress in Relativistic Astrophysics)
Review Reports Versions Notes

Abstract

In this work, we obtain the deflection angle for a boosted Kerr black hole in the weak field approximation using the optics in a curved spacetime developed by J. L. Synge in 1960. We study the behavior of light in the presence of plasma by considering different distributions: uniform plasma, singular isothermal sphere, non-singular isothermal gas sphere, and plasma in a galaxy cluster. We found that the dragging of the inertial system along with the boosted parameter Λ affect the value of the deflection angle. As an application, we studied the magnification for both uniform and singular isothermal distributions.
Keywords: optics in curved spacetimes; gravitational lensing; weak field limit; boosted Kerr metric; plasma distribuions; magnification optics in curved spacetimes; gravitational lensing; weak field limit; boosted Kerr metric; plasma distribuions; magnification

Share and Cite

MDPI and ACS Style

Benavides-Gallego, C.A.; Abdujabbarov, A.-A. Boosted Kerr Black Hole in the Presence of Plasma. Proceedings 2019, 17, 6. https://doi.org/10.3390/proceedings2019017006

AMA Style

Benavides-Gallego CA, Abdujabbarov A-A. Boosted Kerr Black Hole in the Presence of Plasma. Proceedings. 2019; 17(1):6. https://doi.org/10.3390/proceedings2019017006

Chicago/Turabian Style

Benavides-Gallego, Carlos A., and Ahmadjon-Abdujabbarov Abdujabbarov. 2019. "Boosted Kerr Black Hole in the Presence of Plasma" Proceedings 17, no. 1: 6. https://doi.org/10.3390/proceedings2019017006

APA Style

Benavides-Gallego, C. A., & Abdujabbarov, A. -A. (2019). Boosted Kerr Black Hole in the Presence of Plasma. Proceedings, 17(1), 6. https://doi.org/10.3390/proceedings2019017006

Article Metrics

Back to TopTop