  Correlations between 1-10 Hz quasi-periodic oscillations (QPOs) and spectral
power law index have been reported for black hole (BH) candidate sources and
one neutron star source, 4U 1728-34. An examination of QPO frequency and index
relationships in Sco X-1 is reported herein. We discovered that Sco X-1,
representing Z-source groups, can be adequately modeled by a simple
two-component model of Compton up-scattering with a soft photon electron
temperature of about 0.4 keV, plus an Iron K-line. The results show a strong
correlation between spectral power law index and kHz QPOs. Because Sco X-1
radiates near the Eddington limit, one can infer that the geometrical
configuration of the Compton cloud (CC) is quasi-spherical because of high
radiation pressure in the CC. Thus, we conclude that the high Thomson optical
depth of the Compton cloud, in the range of ~5-6 from the best-fit model
parameters, is consistent with the neutron star's surface being obscured by
material. Moreover, a spin frequency of Sco X-1 is likely suppressed due to
photon scattering off CC electrons. Additionally, we demonstrate how the power
spectrum evolves when Sco X-1 transitions from the horizontal branch to the
normal branch.
