Reversal of the amplitude difference of kHz QPOs in six atoll sources
Gabriel Torok

TL;DR
This study examines the amplitude relationship of twin kHz QPOs in six neutron-star atoll sources, revealing a common ratio where their amplitudes equalize, suggesting a shared physical mechanism or orbital feature.
Contribution
It identifies a consistent amplitude ratio point across multiple sources, linking QPO amplitude behavior to potential orbital and energy exchange processes.
Findings
Amplitude equality occurs near R=1.5 in all sources.
Similar ratios around R=1.33 or R=1.25 are observed.
Amplitude differences suggest energy interchange between QPO modes.
Abstract
AIMS: For six neutron-star atoll sources (4U 1608-52, 4U 1636-53, 4U 0614+09, 4U 1728-34, 4U 1820-30 and 4U 1735-44) we investigate the relationship between the observed fractional rms amplitudes of the twin kHz QPOs. We discuss whether this displays features that could have a physical meaning in terms of the proposed QPO models. METHOD: We consider the difference in rms amplitude between the upper and lower kHz QPOs, as a function of the frequency ratio R. We compare two data sets. Set I is a collection taken from published data. Set II has rms amplitude values obtained by automatic fitting of continuous segments of RXTE-PCA observations. RESULTS: For each of the six sources, we find that there is a point in the R domain around which the amplitudes of the two twin kHz QPOs are the same. We find such a point located inside a narrow interval R=1.5 +-3%. Further investigation is needed in…
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