COVARIANT ANALYSIS OF NEWTONIAN MULTI-FLUID MODELS FOR NEUTRON STARS III: TRANSVECTIVE, VISCOUS, AND SUPERFLUID DRAG DISSIPATION

DOI10.1142/S0218271805006845zbMath1085.83503arXivastro-ph/0410660OpenAlexW3105969615WikidataQ60556079 ScholiaQ60556079MaRDI QIDQ5312418

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Publication date: 31 August 2005

Published in: (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0410660

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