Black holes in general relativity coupled with NEDs surrounded by PFDM: thermodynamics, epicyclic oscillations, QPOs, and shadow
Faizuddin Ahmed, Sardor Murodov, Bekzod Rahmatov

TL;DR
This paper explores the thermodynamics, particle dynamics, QPOs, and shadow of a regular black hole in a PFDM environment, linking theoretical models with observational data to identify potential signatures.
Contribution
It introduces a comprehensive analysis combining thermodynamics, particle motion, QPO modeling, and shadow imaging for black holes in PFDM, constrained by observational data.
Findings
Black hole thermodynamics indicate stability regions.
QPO frequencies match observational data for specific parameters.
Black hole shadow characteristics depend on geometric parameters.
Abstract
In this work, we investigate the thermodynamics and motion of neutral test particles around a regular black hole immersed in a perfect fluid dark matter environment. We begin by examining the horizon structure and key thermodynamic properties, with particular emphasis on quantities such as the Hawking temperature and the specific heat capacity. These aspects provide important insight into the stability and physical behavior of the black hole system. We then proceed to analyze the dynamics of neutral test particles using the Hamiltonian formalism, through which we derive the effective potential governing particle motion. Using the effective potential, we further study quasiperiodic oscillations by determining the associated epicyclic frequencies and comparing them with available observational data. Using the observed QPO data of XTE J1550-564, GRO J1655-40, GRS 1915+105, and M82 X-1, we…
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