Looking for extra dimensions in the observed quasi-periodic oscillations of black holes
Indrani Banerjee, Sumanta Chakraborty, Soumitra SenGupta

TL;DR
This study investigates how extra spatial dimensions could influence black hole quasi-periodic oscillations, using observational data to estimate a tidal charge parameter that signals the presence of extra dimensions.
Contribution
It introduces a method to analyze QPOs in rotating braneworld black holes and constrains the tidal charge parameter using observational data, indicating potential evidence for extra dimensions.
Findings
Most models predict a negative tidal charge parameter.
Observations are consistent with negative tidal charge within 1-sigma confidence.
Eight out of eleven models favor negative tidal charge values.
Abstract
Quasi-periodic oscillations, often present in the power density spectrum of accretion disk around black holes, are useful probes for the understanding of gravitational interaction in the near-horizon regime of black holes. Since the presence of an extra spatial dimension modifies the near horizon geometry of black holes, it is expected that the study of these quasi-periodic oscillations may shed some light on the possible existence of these extra dimensions. Intriguingly, most of the extra dimensional models, which are of significant interest to the scientific community, predicts the existence of a tidal charge parameter in black hole spacetimes. This tidal charge parameter can have an overall negative sign and is a distinctive signature of the extra dimensions. Motivated by this, we have studied the quasi-periodic oscillations for a rotating braneworld black hole using the available…
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