Observational Constraints on f(R,T) gravity coupled with NED from Black Hole Quasi Periodic Oscillations

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Main Authors: Hazarika, Bidyut, Baruah, Abhishek, Phukon, Prabwal
Format: Preprint
Published: 2025
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author Hazarika, Bidyut
Baruah, Abhishek
Phukon, Prabwal
author_facet Hazarika, Bidyut
Baruah, Abhishek
Phukon, Prabwal
contents In this work, we examine the influence of nonlinear electrodynamics (NED) and $f(R,T)$ gravity on quasi-periodic oscillations (QPOs) around a magnetically charged black hole. By analyzing the effective potential, specific energy, and angular momentum of circular orbits, we study how the NED parameter $α$ and the gravitational coupling parameter $β$ affect orbital dynamics. Increasing $α$ leads to systematic deviations from the Reissner Nordstrom behavior, reflected in shifts in the ISCO radius and orbital frequencies. We further explore QPO-generating radii using the Relativistic Precession (RP), Warped Disk (WD), and Epicyclic Resonance (ER2-ER4) models. We further extend our analysis by performing an MCMC-based parameter estimation using QPO data from black holes spanning a wide range of mass scales. This approach yields consistent observational constraints on the model parameters.
format Preprint
id arxiv_https___arxiv_org_abs_2508_02213
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Observational Constraints on f(R,T) gravity coupled with NED from Black Hole Quasi Periodic Oscillations
Hazarika, Bidyut
Baruah, Abhishek
Phukon, Prabwal
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this work, we examine the influence of nonlinear electrodynamics (NED) and $f(R,T)$ gravity on quasi-periodic oscillations (QPOs) around a magnetically charged black hole. By analyzing the effective potential, specific energy, and angular momentum of circular orbits, we study how the NED parameter $α$ and the gravitational coupling parameter $β$ affect orbital dynamics. Increasing $α$ leads to systematic deviations from the Reissner Nordstrom behavior, reflected in shifts in the ISCO radius and orbital frequencies. We further explore QPO-generating radii using the Relativistic Precession (RP), Warped Disk (WD), and Epicyclic Resonance (ER2-ER4) models. We further extend our analysis by performing an MCMC-based parameter estimation using QPO data from black holes spanning a wide range of mass scales. This approach yields consistent observational constraints on the model parameters.
title Observational Constraints on f(R,T) gravity coupled with NED from Black Hole Quasi Periodic Oscillations
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2508.02213