Analytical estimates indicate that a geometric warp in the inner accretion disk unifies the evolution of broad-band noise and low-frequency QPO types during state transitions in black hole X-ray binaries.
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Disk warping and black hole X-ray binaries I. Tentative unification of low-frequency quasi-periodic oscillations
Analytical estimates indicate that a geometric warp in the inner accretion disk unifies the evolution of broad-band noise and low-frequency QPO types during state transitions in black hole X-ray binaries.