Stability of power-law discs - I. The Fredholm integral equation

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

29

Instabilities, Methods: Analytical, Methods: Numerical, Celestial Mechanics, Stellar Dynamics, Galaxies: Kinematics And Dynamics, Galaxies: Spiral

Scientific paper

The power-law discs are a family of infinitesimally thin, axisymmetric stellar discs of infinite extent. The rotation curve can be rising, falling or flat. The self-consistent power-law discs are scale-free, so that all physical quantities vary as a power of radius. They possess simple equilibrium distribution functions depending on the two classical integrals, energy and angular momentum. While maintaining the scale-free equilibrium force law, the power-law discs can be transformed into cut-out discs by preventing stars close to the origin (and sometimes also at large radii) from participating in any disturbance. This paper derives the homogeneous Fredholm integral equation for the in-plane normal modes in the self-consistent and the cut-out power-law discs. This is done by linearizing the collisionless Boltzmann equation to find the response density corresponding to any imposed density and potential. The normal modes - that is, the self-consistent modes of oscillation - are found by requiring the imposed density to equal the response density. In practice, this scheme is implemented in Fourier space, by decomposing both imposed and response densities in logarithmic spirals. The Fredholm integral equation then relates the transform of the imposed density to the transform of the response density. Numerical strategies to solve the integral equation and to isolate the growth rates and the pattern speeds of the normal modes are discussed.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Stability of power-law discs - I. The Fredholm integral equation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Stability of power-law discs - I. The Fredholm integral equation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of power-law discs - I. The Fredholm integral equation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1098806

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.