The distribution law of stellar p-modes

Details The distribution law of stellar p-modes The distribution law of stellar p-modes

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..83..311p&link_type=abstract

Astrophysics and Space Science, vol. 83, no. 1-2, Apr. 1982, p. 311-333.

Astronomy and Astrophysics

Astrophysics

2

Acoustic Velocity, Asymptotic Methods, Stellar Models, Stellar Oscillations, Stellar Structure, Acoustic Frequencies, Density Distribution, Distribution Functions, Eigenvalues, Equations Of Motion, Heuristic Methods, Integral Equations, Pressure Oscillations, Spherical Harmonics, Vibration Mode

Scientific paper

It is shown that the overall density of asymptotic acoustic frequencies of a star obeys a Weyl law involving the dimensionality (D) of the oscillating stellar configuration. For realistic stars having a finite nonzero surface sound speed, D is equal to the actual dimensionality of the star, D equals 3. For formal models having a vanishing sound velocity at the surface, heuristic arguments lead to a dimensionality parameter D equals 4.5.

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