For axisymmetric disturbances, , the wavevector is fixed, so there is no winding/swing mechanism. Take and set . Eliminating pressure with incompressibility gives
The axisymmetric incompressible epicyclic wave has inviscid frequency
where is the radial epicyclic frequency.
In a Keplerian flow and . The axisymmetric disturbances therefore execute stable inertial/epicyclic oscillations, with viscous amplitude decay . Rotation opposes sustained radial displacement through angular-momentum conservation. There can be bounded exchanges of kinetic energy between components, but no large Reynolds-number-dependent amplification of this axisymmetric family. Indeed, with , inviscid motion conserves
Since the physical velocity norm is , Keplerian energy amplification is at most ; viscosity can only reduce that bound. A pure initial azimuthal disturbance can attain the inviscid factor four after a quarter epicyclic period. By contrast, the two-dimensional nonaxisymmetric Orr mechanism remains available in a Keplerian flow and has the gain derived above.
In non-rotating shear, while remains nonzero. The axisymmetric solution is
Cross-stream motion transports the basic shear and generates an azimuthal streak: this is the lift-up effect. Inviscid azimuthal velocity grows linearly and its energy quadratically, rather than oscillating. With viscosity, the gain for a suitable initial cross-stream disturbance scales as at large Reynolds number, appreciably stronger than the two-dimensional scaling. For instance, and fixed give the leading optimized gain at . Neither mechanism is an exponentially growing hydrodynamic normal mode. Rotation bounds axisymmetric lift-up in Keplerian shear; without rotation, lift-up gives strong algebraic transient growth. If as well as , incompressibility forces and removes this coupling altogether.