An analysis of the linear, adiabatic oscillations of a star in terms of potential fields

DOI10.1007/BF00643044zbMath0406.76048MaRDI QIDQ1257800

Morris L. Aizenman, Paul Smeyers

Publication date: 1977

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

Gaseous SphereHelmholtz's TheoremOscillations of StarsSpherical Equilibrium Configuration

Mathematics Subject Classification ID

Series solutions to PDEs (35C10) Galactic and stellar structure (85A15) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (2)

SELF-GRAVITATING ASTROPHYSICAL MASS WITH SINGULAR CENTRAL DENSITY VIBRATING IN FUNDAMENTAL MODE ⋮ Variational principles for the linear and adiabatic oscillations of a spherical star, and related definitions of canonical energy density and of canonical energy flux

Cites Work

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• A General Variational Principle Governing the Radial and the Non-Radial Oscillations of Gaseous Masses.
• Schwarzschild's Criterion for Instability
• Nonradial Oscillations of Stars.

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