This https://t.co/n6y0GZ5iA9 has been replaced. Links: https://t.co/hwm6FKYxAL https://t.co/rnuSNckGLQ https://t.co/T5b3RFmquU https://t.co/7Vwee5Laej
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https://t.co/mFxeXx754F Z Lin, Y Wang Stability of rotating gaseous stars https://t.co/XFh8lwQedR
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linear instability of rotating stars. Moreover, we gave a complete description of the spectra and sharp growth estimates for the linearized Euler-Poisson equation. [5/5 of https://t.co/JwFBwgnxUK]
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points of the total mass. By contrast, we proved that the turning point principle is true for the family of slowly rotating stars with fixed angular momentum distribution. When the angular velocity is Rayleigh unstable, we proved [4/5 of https://t.co/JwFBw