Epicyclic frequency

From Wikipedia, the free encyclopedia
Jump to: navigation, search

In astrophysics, particularly the study of accretion disks, the epicyclic frequency is the frequency at which a radially displaced fluid parcel will oscillate. It can be referred to as a "Rayleigh discriminant". When considering an astrophysical disc with differential rotation , the epicyclic frequency is given by

, where R is the radial co-ordinate.[1]

This quantity can be used to examine the 'boundaries' of an accretion disc - when becomes negative then small perturbations to the (assumed circular) orbit of a fluid parcel will become unstable, and the disc will develop an 'edge' at that point. For example, around a Schwarzschild black hole, the Innermost Stable Circular Orbit (ISCO) occurs at 3x the event horizon - at .

For a Keplerian disk, .

References[edit]

  1. ^ p161, Astrophysical Flows, Pringle and King 2007