Document Type : Regular article
Authors
1 Department of Physics, Institute of Applied Sciences and Humanities, GLA University, Mathura 281406, Uttar Pradesh, India;
2 Department of Physics, Institute of Applied Sciences and Humanities, GLA University, Mathura 281406, Uttar Pradesh, India; Visiting Associate: Inter-University Center of Astronomy and Astrophysics (IUCAA), Pune
3 Department of Physics, K.L.S. College, Nawada, Magadh University, Bodh Gaya, Bihar 805110, India; Canadian Quantum Research Center 204-3002 32 Ave Vernon, BC V1T 2L7 Canada; Department of General & Theoretical Physics, L. N. Gumilyov Eurasian National University, Astana, 010008, Kazakhstan; Visiting Associate: Inter-University Center of Astronomy and Astrophysics (IUCAA), Pune
Abstract
In this paper, we derive the black hole solution in the context of nonlinear electrodynamics (NLED) coupled to a perfect fluid dark matter (PFDM) field. The resulting black hole solution interpolates between the AdS Ayón-Beato-GarcÍa (ABG) black hole in the absence of the PFDM field and the Schwarzschild black hole devoid of magnetic monopole charges and PFDM influence. A numerical investigation of the horizon structure and thermodynamic properties, including both local and global stability, is conducted for the obtained black hole solution. The presence of the NLED and PFDM fields shows that the thermodynamic quantities are modified. We observe that the behaviour of thermodynamical quantities of black holes depends on these parameters significantly. We also discuss the stability and phase transition dependency on these parameters.
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