Difference between revisions of "User:Tohline/Apps/RotatingPolytropes/BarmodeLinearTimeDependent"

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* [https://ui.adsabs.harvard.edu/abs/2006ApJ...651.1068O/abstract S. Ou & J. E. Tohline (2006)], ApJ, 651, 1068:  ''Unexpected Dynamical Instabilities in Differentially Rotating Neutron Stars''
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* [https://ui.adsabs.harvard.edu/abs/2007CoPhC.177..288C/abstract P. Cerda-Duran, V. Quilos & J. A. Font (2007)], Comp. Phys. Comm., 177, 288: ''AMR simulations of the low T/|W| bar-mode instability of neutron stars''
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Revision as of 20:50, 1 July 2019

Simulating the Onset of a Barmode Instability

Whitworth's (1981) Isothermal Free-Energy Surface
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Index of Relevant Publications

Here is a list of relevant research papers as enumerated by Y. Kojima & M. Saijo (2008), Phys. Rev. D, vol. 78, Issue 12, id. 124001: Amplification of azimuthal modes with odd wave numbers during dynamical bar-mode growth in rotating stars

See Also


Whitworth's (1981) Isothermal Free-Energy Surface

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Recommended citation:   Tohline, Joel E. (2021), The Structure, Stability, & Dynamics of Self-Gravitating Fluids, a (MediaWiki-based) Vistrails.org publication, https://www.vistrails.org/index.php/User:Tohline/citation