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20202026
most citedNoncommutative Schwarzschild black hole surrounded by quintessence: Thermodynamics, Shadows and Quasinormal modes

39 citations · 115 across the 10 of their papers we have counts for

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gr-qc2026

Born-Infeld AdS Black Holes Surrounded by Perfect Fluid Dark Matter

Behzad Eslam Panah, Bilel Hamil, Manuel E. Rodrigues

We obtain exact charged AdS black hole solutions in Einstein Lambda gravity including the effects of Born Infeld nonlinear electrodynamics and Perfect Fluid Dark Matter. The influe…

gr-qc2025★ 18 cited

Nonlinear Magnetically Charged Black Holes with Phantom Global Monopoles: Thermodynamics, Geodesics, Quasinormal Modes, and Grey-Body Factors

B. Hamil, B. C. Lütfüoğlu

We study the properties of a nonlinear magnetic-charged black hole in the presence of a phantom global monopole. By incorporating nonlinear electrodynamics (NLE) and exotic scalar…

gr-qc2024★ 39 cited

Noncommutative Schwarzschild black hole surrounded by quintessence: Thermodynamics, Shadows and Quasinormal modes

B. Hamil, B. C. Lütfüoğlu

{In (Sci. Rep. \textbf{12}, 8516 (2022)), Campos et al studied} the quasinormal modes and shadows of noncommutative Schwarzschild black holes. Since we know that the quintessence m…

gr-qc2022★ 22 cited

Effect of Snyder-de Sitter model on the Black hole thermodynamics in the context of rainbow gravity

B. Hamil, B. C. Lütfüoğlu

One of the foremost goals of theoretical modern physics is to obtain a reliable theory of quantum gravity. In so doing, new fundamental scales are being proposed. For example, in t…

gr-qc2021★ 26 cited

Black hole thermodynamics in the presence of a maximal length and minimum measurable in momentum

Bilel Hamil, Bekir Can Lütfüoğlu

In this work, incorporating the effect of the minimum measurable in momentum and maximal length, we studied thermodynamics property of Schwarzschild black hole and the Unruh effect…

gr-qc2020★ 3 cited

Three dimensional DKP oscillator in a curved Snyder space

B. Hamil, M. Merad, T. Birkandan

The Snyder-de Sitter model is an extension of the Snyder model to a de Sitter background. It is called triply special relativity (TSR) because it is based on three fundamental para…