Non-linear development of the secular bar-mode instability in rapidly rotating neutron stars | Zendy

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Non-linear development of the secular bar-mode instability in rapidly rotating neutron stars

Author(s) -

Shangli Ou

Publication year - 2022

Language(s) - English

Resource type - Dissertations/theses

DOI - 10.31390/gradschool_dissertations.4005

Subject(s) - physics , instability , classical mechanics , gravitational wave , neutron star , angular momentum , mechanics , astrophysics

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