Harmonic oscillation and orbital morphology for spinning charged quantum corrected black hole
Abstract
This study investigates the dynamical behavior of particle's test around a spinning charged Einstein-Maxwell-dilaton (EMd) quantum corrected black hole (QCBH) by examining the effects of spinning parameter a, quantum correction parameter b, and charge parameter Q. Using EMd spacetime geometry, we analyze the effective potential and effective force to determine the stability and structure of the circular orbits in a strong gravitational field. Furthermore, we calculate the oscillation frequencies radial (Ωr), vertical (Ωθ), and angular (Ωϕ), as well as the corresponding Periapsis and Lense-Thirring precession frequencies. The spin parameter primarily determines the spinning properties of spacetime, while the quantum correction and charge particle introduce additional biases to Kerr-Newman geometry, particularly near the event horizon. These corrections alter the position and stability of the circular orbits, and the spectrum effectively associates with particle's motion. The results provide a comprehensive description of the orbital dynamics of spinning EMd QCBH through future high-precision astrophysical observations.
Versions
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BibTeX
@misc{khalid2026harmonic,
title = {{Harmonic oscillation and orbital morphology for spinning charged quantum corrected black hole}},
author = {Rameez Khalid and Muhammad Yasir and Shahid Qaisar and Faisal Javed},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2607.17658},
eprint = {2607.17658},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2607.17658},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Harmonic oscillation and orbital morphology for spinning charged quantum corrected black hole
AU - Rameez Khalid
AU - Muhammad Yasir
AU - Shahid Qaisar
AU - Faisal Javed
PY - 2026
DA - 2026/10/29
PB - arXiv
DO - 10.48550/arxiv.2607.17658
UR - https://arxiv.org/abs/2607.17658
AB - This study investigates the dynamical behavior of particle's test around a spinning charged Einstein-Maxwell-dilaton (EMd) quantum corrected black hole (QCBH) by examining the effects of spinning parameter a, quantum correction parameter b, and charge parameter Q. Using EMd spacetime geometry, we analyze the effective potential and effective force to determine the stability and structure of the circular orbits in a strong gravitational field. Furthermore, we calculate the oscillation frequencies radial (Ω_r), vertical (Ω_θ), and angular (Ω_ϕ), as well as the corresponding Periapsis and Lense-Thirring precession frequencies. The spin parameter primarily determines the spinning properties of spacetime, while the quantum correction and charge particle introduce additional biases to Kerr-Newman geometry, particularly near the event horizon. These corrections alter the position and stability of the circular orbits, and the spectrum effectively associates with particle's motion. The results provide a comprehensive description of the orbital dynamics of spinning EMd QCBH through future high-precision astrophysical observations.
ER -