Local stellar stability

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

6

Differential Equations, Dynamic Stability, Hydrodynamic Equations, Stellar Models, Stellar Structure, Eigenvalues, Eigenvectors, Function Space, Stellar Evolution, Thermodynamics

Scientific paper

A formalism is presented for investigating local stellar stability in terms of ordinary differential equations. Local stability is defined as being related to continuous branches of eigenvalues expressible as functions of position in the star, and a systematic approach is outlined for tracing these continuous branches. Attention is focused on stellar situations where the partial differential eigenvalue problem can be reduced to a system of ordinary differential equations. Distributions in a generalized function space and superregularizations are evaluated as solutions to the differential system, and it is shown that the introduction of superregularizations allows continuous branches of eigenvalues to be associated with all spectral equations defining linear stellar stability in radial as well as nonradial dynamical, vibrational, and secular stability problems. The present approach is illustrated by short analyses of the radial and nonradial dynamical stability problems.

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

Local stellar stability 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 Local stellar stability, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Local stellar stability will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1413079

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