Do superfluid instabilities prevent neutron star precession?
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/394/4/1908/4034385/mnras0394-1908.pdf
Reference42 articles.
1. Observational Constraints on the Internal Structure and Dynamics of the Vela Pulsar
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3. On the dynamical coupling between the superfluid interior and the crust of a neutron star
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5. A flux-conservative formalism for convective and dissipative multi-fluid systems, with application to Newtonian superfluid neutron stars
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2. A Superfluid Perspective on Neutron Star Dynamics;Universe;2021-01-15
3. Turbulent, pinned superfluids in neutron stars and pulsar glitch recoveries;Monthly Notices of the Royal Astronomical Society;2020-09-04
4. Hydrodynamical instabilities in the superfluid interior of neutron stars with background flows between the components;Physical Review D;2019-12-02
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