Plasma effects on weak gravitational lensing and shadows of Sen black holes*

Abstract We investigate the optical properties of the spacetime surrounding a Sen black hole, focusing on the black hole shadow, weak gravitational lensing, and time delay effects. Our analysis reveals that the effective charge of the Sen black hole significantly influences these phenomena. Specifically, an increase in the effective charge leads to a decrease in the radius of the photon sphere and a corresponding decrease in the size of the black hole shadow. Additionally, the bending angle of light rays diminishes as the effective charge increases. Our study provides observational bounds on the effective charge based on these optical characteristics. We also examine the magnification of source brightness using the lens equation and analyze the time delay of light in the presence of a surrounding plasma medium. Our findings offer new insights into the impact of effective charge and plasma on the observational signatures of Sen black holes.

Authors

Institutions

Publication Details

Journal
Chinese Physics C
Published
2025-02-07
DOI
https://doi.org/10.1088/1674-1137/adb384
Citations
12
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
13.86
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Plasma effects on weak gravitational lensing and shadows of Sen black holes*

Sushant G. Ghosh, Farruh Atamurotov, Ahmadjon Abdujabbarov, Odil Yunusov et al.
12 citations
Chinese Physics C
Pulsars and Gravitational Waves Research
13.86
article

Plasma effects on weak gravitational lensing and shadows of Sen black holes*

Sushant G. Ghosh, Farruh Atamurotov, Ahmadjon Abdujabbarov, Odil Yunusov, Dilmurod Umarov
article en
12 citations

Abstract

Abstract We investigate the optical properties of the spacetime surrounding a Sen black hole, focusing on the black hole shadow, weak gravitational lensing, and time delay effects. Our analysis reveals that the effective charge of the Sen black hole significantly influences these phenomena. Specifically, an increase in the effective charge leads to a decrease in the radius of the photon sphere and a corresponding decrease in the size of the black hole shadow. Additionally, the bending angle of light rays diminishes as the effective charge increases. Our study provides observational bounds on the effective charge based on these optical characteristics. We also examine the magnification of source brightness using the lens equation and analyze the time delay of light in the presence of a surrounding plasma medium. Our findings offer new insights into the impact of effective charge and plasma on the observational signatures of Sen black holes.

Chinese Physics CVol. 49(5)
Khazar University (AZ), Urgench State University (UZ), Inha University in Tashkent (UZ), Tashkent Institute of Irrigation and Agricultural Mechanization Engineers (UZ), New Uzbekistan University (UZ), National University of Uzbekistan (UZ), Jamia Millia Islamia (IN), University of KwaZulu-Natal (ZA)
Openalex Percentile: Top 1%
Pulsars and Gravitational Waves Research
13.86
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Plasma effects on weak gravitational lensing and shadows of Sen black holes* — Sushant G. Ghosh, Farruh Atamurotov, et al. · Chinese Physics C (2025) | TGRS Research Map | TGRS