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Using the Two-dimensional Oscillation Program (TOP), we have explored theeffects of rapid rotation on gravity modes in polytropic stars. Coriolis force,centrifugal distortion as well as compressible effects have been taken intoaccount. Thanks to our complete calculation, we have first studied the validitydomain of perturbative methods and started to explore properties of thesemodes. We focus on l=1 in this analysis.

Gravity modes in rapidly rotating polytropic stars