Gravity modes in rapidly rotating polytropic stars
Solar and Stellar Astrophysics
2009-12-10 v1
Abstract
Using the Two-dimensional Oscillation Program (TOP), we have explored the effects of rapid rotation on gravity modes in polytropic stars. Coriolis force, centrifugal distortion as well as compressible effects have been taken into account. Thanks to our complete calculation, we have first studied the validity domain of perturbative methods and started to explore properties of these modes. We focus on l=1 in this analysis.
Cite
@article{arxiv.0912.1679,
title = {Gravity modes in rapidly rotating polytropic stars},
author = {J. Ballot and F. Lignières and D. R. Reese and M. Rieutord},
journal= {arXiv preprint arXiv:0912.1679},
year = {2009}
}
Comments
Proc. HELAS Workshop on `New insights into the Sun', Ponte de Lima, Portugal, 2009, M. S. Cunha & M. J. Thompson (eds)