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

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Additional references identified through the above set of references:
Additional references identified through the above set of references:
* [https://ui.adsabs.harvard.edu/abs/2018PhRvD..98b4003S/abstract M. Saijo (2018)], Phys. Rev. D, 98, 024003:  ''Determining the stiffness of the equation of state using low T/W dynamical instabilities in differentially rotating stars''
* [https://ui.adsabs.harvard.edu/abs/2018PhRvD..98b4003S/abstract M. Saijo (2018)], Phys. Rev. D, 98, 024003:  ''Determining the stiffness of the equation of state using low T/W dynamical instabilities in differentially rotating stars''
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We investigate the nature of low T/W dynamical instabilities in various ranges of the stiffness of the equation of state in differentially rotating stars &hellip; We analyze these instabilities in both a linear perturbation analysis and a three-dimensional hydrodynamical simulation.
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=See Also=
=See Also=

Revision as of 21:00, 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

Additional references identified through the above set of references:

  • M. Saijo (2018), Phys. Rev. D, 98, 024003: Determining the stiffness of the equation of state using low T/W dynamical instabilities in differentially rotating stars
 

We investigate the nature of low T/W dynamical instabilities in various ranges of the stiffness of the equation of state in differentially rotating stars … We analyze these instabilities in both a linear perturbation analysis and a three-dimensional hydrodynamical simulation.

See Also


Whitworth's (1981) Isothermal Free-Energy Surface

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