Testing the Lense-Thirring Precession Origin of the QPO in Swift J1727.8$-$1613
Ruican Ma, Chris Done, Aya Kubota

TL;DR
This study analyzes the QPOs in Swift J1727.8$-$1613 to test if their origin is due to Lense-Thirring precession, finding strong agreement with the model despite some parameter uncertainties.
Contribution
It provides the first detailed spectral and timing analysis of Swift J1727.8$-$1613 during outburst, testing the Lense-Thirring precession model for QPOs with broadband data.
Findings
The corona radius decreases from 45 to 9 Rg during state transitions.
The observed r_cor vs. QPO frequency trend agrees with LT precession predictions.
The hot flow radius remains roughly constant, suggesting jet power is independent of accretion changes.
Abstract
We present a comprehensive spectral and timing analysis of the newly discovered black hole transient Swift J1727.81613, based on broadband (2150 keV) observations from -HXMT during its 2023 outburst. We use the flexible, energy-conserving SSsed model to model both the outer disc and inner, complex Comptonisation, using the expected disc emissivity to constrain the corona radius, . This decreases from 45 to 9 during the transition from the hard to hard intermediate and then soft intermediate state. We plot versus the centroid frequency of the strong quasi-periodic oscillations (QPOs; ) seen in these data to test the inner hot flow Lense-Thirring (LT) precession model. The overall slope of the observed trend is in strong agreement with the predictions of LT precession, despite the complexities of accretion behavior,…
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