Semiclassical analysis of stellar p modes

Details Semiclassical analysis of stellar p modes Semiclassical analysis of stellar p modes

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.485..345r&link_type=abstract

In: Proceedings of the First Eddington Workshop on Stellar Structure and Habitable Planet Finding, 11 - 15 June 2001, Córdoba, S

Computer Science

1

Waves, Methods: Numerical, Stars: Oscillations

Scientific paper

We present a brief overview of our first studies in developing classical
and semiclassical approximations for low-degree stellar p modes, as an
alternative to the formal high-frequency asymptotic expansions used
earlier. The complete account of this work can be found in Roxburgh and
Vorontsov (2000, 2001).

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