Correlations between kilohertz quasi-periodic oscillations and low-frequency features attributed to radial oscillations and diffusive propagation in the viscous boundary layer around a neutron star

We present a dimensional analysis of two characteristic timescales in the b oundary layer where the disk adjusts to the rotating neutron star (NS). The boundary layer is treated as a transition region between the NS surface an d the first Keplerian orbit. The radial transport of the angular momentum i n this layer is controlled by a viscous force defined by the Reynolds numbe r, which in turn is related to the mass accretion rate. We show that the ob served low-Lorentzian frequency is associated with radial oscillations in t he boundary layer, where the observed break frequency is determined by the characteristic diffusion time of the inward motion of the matter in the acc retion flow. Predictions of our model regarding relations between those two frequencies and the frequencies of kilohertz quasi-periodic oscillations ( kHz QPOs) compare favorably with recent observations of the source 4U 1728- 34. This Letter contains a theoretical classification of kHz QPOs in NS bin aries and the related low-frequency features. Thus, results concerning the relationship between the low-lorentzian frequency of viscous oscillations a nd the break frequency are presented in the framework of our model of kHz Q POs viewed as Keplerian oscillations in a rotating frame of reference.