Astronomy and astrophysics Definition
Stellar pulsation
Builds on Hydrostatic equilibriumNormal modeSpherical harmonics
Definition
Consider a spherically symmetric star in hydrostatic equilibrium, modelled as a self-gravitating fluid. Linearise the equations of fluid motion, of gravity and of energy about this equilibrium. A pulsation mode of the star is a normal mode of the linearised equations. For a non-rotating star the radial component of its displacement field has the form Its horizontal components are proportional to the angular derivatives of . Here are spherical coordinates and is a spherical harmonic. The integer is the radial order, which counts the radial nodes of . The number is the frequency. Stellar pulsation is the oscillation of a star as a superposition of such modes. The mode is radial if and non-radial if .
Remarks
For example, in a radial mode with the star expands and contracts while staying spherical; the classical Cepheid variables pulsate in this way. A non-example is a star whose light changes because of eclipses by a companion: there is no oscillation of the star about equilibrium. Modes with pressure as the main restoring force are called p modes, and modes with buoyancy as the restoring force are called g modes. In the adiabatic approximation the frequencies are real and the problem is a self-adjoint eigenvalue problem; non-adiabatic effects make complex and decide whether a mode grows or decays.
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Further reading
About this page
| Tag | FX6ER3Q77K |
|---|---|
| URI | m2://FX6ER3Q77K |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A15, 76E20 |
| Defines | Stellar pulsation |
| Uses | Hydrostatic equilibrium, Normal mode, Spherical harmonics |
| Changed | 3 November 2026 |
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