A flux-conservative formalism for convective and dissipative multi-fluid systems, with application to Newtonian superfluid neutron stars
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Publication:5492745
DOI10.1088/0264-9381/23/18/003zbMath1101.85003arXivphysics/0509241OpenAlexW3105425060WikidataQ60713147 ScholiaQ60713147MaRDI QIDQ5492745
Publication date: 16 October 2006
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/physics/0509241
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)
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