ENTRAINMENT COEFFICIENT AND EFFECTIVE MASS FOR CONDUCTION NEUTRONS IN NEUTRON STAR CRUST: MACROSCOPIC TREATMENT

DOI10.1142/S0218271806008504zbMath1115.85301arXivastro-ph/0408083WikidataQ60556064 ScholiaQ60556064MaRDI QIDQ5485762

Nicolas Chamel, Pawel Haensel, Brandon Carter

Publication date: 4 September 2006

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0408083

zbMATH Keywords

effective massneutron star crustneutron superfluid

Mathematics Subject Classification ID

Galactic and stellar structure (85A15)

Related Items

Stability and causality of Carter’s multifluid theory ⋮ Supersymmetric backgrounds in \((1 + 1)\) dimensions and inhomogeneous field theory ⋮ Symmetry evolution for the imperfect fluid under perturbations ⋮ Thermodynamics of uncharged relativistic multifluids ⋮ Bulk viscosity in relativistic fluids: from thermodynamics to hydrodynamics ⋮ Relativistic fluid dynamics: physics for many different scales ⋮ Physics of neutron star crusts ⋮ NEWTONIAN MECHANICS OF NEUTRON SUPERFLUID IN ELASTIC STAR CRUST

Cites Work

• Covariant Newtonian and relativistic dynamics of (magneto)-elastic solid model for neutron star crust
• Gravitational waves from instabilities in relativistic stars
• COVARIANT ANALYSIS OF NEWTONIAN MULTI-FLUID MODELS FOR NEUTRON STARS II: STRESS–ENERGY TENSORS AND VIRIAL THEOREMS
• COVARIANT ANALYSIS OF NEWTONIAN MULTI-FLUID MODELS FOR NEUTRON STARS III: TRANSVECTIVE, VISCOUS, AND SUPERFLUID DRAG DISSIPATION
• COVARIANT ANALYSIS OF NEWTONIAN MULTI-FLUID MODELS FOR NEUTRON STARS I: MILNE–CARTAN STRUCTURE AND VARIATIONAL FORMULATION