Slowly rotating general relativistic superfluid neutron stars

DOI10.1088/0264-9381/18/6/302zbMath0976.83028arXivgr-qc/0009089OpenAlexW2950563498WikidataQ60713178 ScholiaQ60713178MaRDI QIDQ2723198

G. L. Comer, Nils Andersson

Publication date: 4 July 2001

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0009089

zbMATH Keywords

rotational frame-draggingsuperfluid neutron stars

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Observational and experimental questions in relativity and gravitational theory (83B05) Equations of motion in general relativity and gravitational theory (83C10)

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Stability and causality of Carter’s multifluid theory ⋮ COVARIANT ANALYSIS OF NEWTONIAN MULTI-FLUID MODELS FOR NEUTRON STARS I: MILNE–CARTAN STRUCTURE AND VARIATIONAL FORMULATION ⋮ Cylindrically symmetric stationary solution to the Einstein equations for a superfluid ⋮ A SCILAB PROGRAM FOR COMPUTING GENERAL-RELATIVISTIC MODELS OF ROTATING NEUTRON STARS BY IMPLEMENTING HARTLE'S PERTURBATION METHOD ⋮ Thermodynamics of uncharged relativistic multifluids ⋮ Rotating stars in relativity ⋮ Neutron stars structure in the context of massive gravity

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