Temporal variability from the two-component advective flow solution and its observational evidence
Broja G. Dutta, Sandip K. Chakrabarti

TL;DR
This paper investigates the temporal variability and QPO behavior in black hole systems using the two-component advective flow model, providing observational evidence and explaining time lag evolution during outbursts.
Contribution
It offers a unified explanation for QPO time lags in high and low-inclination black hole sources within the TCAF framework, supported by RXTE data analysis.
Findings
Systematic evolution of QPO frequency and hard lags during outbursts.
Lag changes from positive to negative at a specific crossing frequency.
Smooth decrease and increase of time lag during rising and declining phases.
Abstract
In the propagating oscillatory shock model, the oscillation of the post-shock region, i.e., the Compton cloud, causes the observed low-frequency quasi-periodic oscillations (QPOs). The evolution of QPO frequency is explained by the systematic variation of the Compton cloud size, i.e., the steady radial movement of the shock front, which is triggered by the cooling of the post-shock region. Thus, analysis of energy-dependent temporal properties in different variability time scales can diagnose the dynamics and geometry of accretion flows around black holes. We study these properties for the high inclination black hole source XTE J1550-564 during its 1998 outburst and the low-inclination black hole source GX 339-4 during its 2006-07 outburst using RXTE/PCA data, and we find that they can satisfactorily explain the time lags associated with the QPOs from these systems. We find a smooth…
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