Probing deflection angle inspired by weak field of specific black holes in non plasma and plasma field

The light bending (global and topological) phenomenon in the presence of black holes (BHs) will be examined by using the Gauss–Bonnet theorem (GBT) to understand the intricate physics . BHs inspired by non-minimal curvature-matter coupling with global monopole and dark matter halo, respectively, will be considered for analysing the above mentioned phenomenon. The deflection angle of light in the presence of weak field limits will be calculated by using well-known methodology called Gibbons–Werner. The effect of plasma medium will be assumed for analysing the bending of light phenomenon. We will also graphically examine the impact of different BH parameters on the computed bending angle. In the last, we also investigate the thermodynamic quantities such as sparsity and emission energy rate for both BHs.

Authors

Publication Details

Journal
Physics of the Dark Universe
Published
2025-03-07
DOI
https://doi.org/10.1016/j.dark.2025.101872
Citations
11
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
12.70

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article

Probing deflection angle inspired by weak field of specific black holes in non plasma and plasma field

Mohammad Mahtab Alam, Farzan Mushtaq, Abdul Jawad, Tiecheng Xia et al.
11 citations
Physics of the Dark Universe
Astrophysical Phenomena and Observations
12.70
article

Probing deflection angle inspired by weak field of specific black holes in non plasma and plasma field

Mohammad Mahtab Alam, Farzan Mushtaq, Abdul Jawad, Tiecheng Xia, Sanjar Shaymatov
article en
11 citations

Abstract

The light bending (global and topological) phenomenon in the presence of black holes (BHs) will be examined by using the Gauss–Bonnet theorem (GBT) to understand the intricate physics . BHs inspired by non-minimal curvature-matter coupling with global monopole and dark matter halo, respectively, will be considered for analysing the above mentioned phenomenon. The deflection angle of light in the presence of weak field limits will be calculated by using well-known methodology called Gibbons–Werner. The effect of plasma medium will be assumed for analysing the bending of light phenomenon. We will also graphically examine the impact of different BH parameters on the computed bending angle. In the last, we also investigate the thermodynamic quantities such as sparsity and emission energy rate for both BHs.

Physics of the Dark UniverseVol. 48
King Khalid University
Climate action
Openalex Percentile: Top 1%
Astrophysical Phenomena and Observations
12.70
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Probing deflection angle inspired by weak field of specific black holes in non plasma and plasma field — Mohammad Mahtab Alam, Farzan Mushtaq, et al. · Physics of the Dark Universe (2025) | TGRS Research Map | TGRS