© CAMBRIDGE UNIVERSITY PRESS 2000 |
13.3. Rotating frame
It should be stressed that an orbit can appear open in one frame of reference and closed in another. In fact, suppose we move to a rotating frame for which the polar coordinates are (r, ), with = - _{p}; here _{p} is the angular velocity of the rotating frame. Then orbits are described by the new Hamiltonian ("Jacobi integral")
(30) |
with p_{} = J, so that H = E - J _{p}. In the rotating frame, the important ratio 2 / becomes 2( - _{p}) / , which then may be rational or not depending on our choice of _{p}. In the dynamics of galaxies there are sometimes physical reasons that identify a specific value of the angular velocity of the rotating frame. The three important possible conditions of 2( - _{p}) / = -1, 0, +1 are often called condition of Inner Lindblad Resonance, Corotation, and Outer Lindblad Resonance, respectively (see Fig. 13.4). Thus, in the rotating frame, at the Lindblad resonances orbits appear closed into ellipses centered at r = 0. This feature, and the fact that - / 2 can be approximately constant on a wide radial range, led B. Lindblad to conjecture that two-armed spiral structure could persist as a kinematical wave in a differentially rotating disk (see Fig. 13.5).
The shear flow pattern associated with the differential rotation in an axisymmetric disk, with the flow "reversal" at the corotation circle is somewhat reminiscent of certain magnetic surface configurations noted in magnetically confined toroidal plasmas, where a suitable projection of the magnetic field changes sign on a "neutral" surface.