COVARIANT ANALYSIS OF NEWTONIAN MULTI-FLUID MODELS FOR NEUTRON STARS II: STRESS–ENERGY TENSORS AND VIRIAL THEOREMS

DOI10.1142/S0218271805006821zbMath1084.83508arXivastro-ph/0312414WikidataQ60556076 ScholiaQ60556076MaRDI QIDQ5312416

Brandon Carter, Nicolas Chamel

Publication date: 31 August 2005

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0312414

zbMATH Keywords

stress tensorhydrodynamicsvirial theoremMilneBernoulli theoremJoukowski theoremNewton--Cartan

Mathematics Subject Classification ID

Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (10)

Covariant Newtonian and relativistic dynamics of (magneto)-elastic solid model for neutron star crust ⋮ Generalization of the Kutta–Joukowski theorem for the hydrodynamic forces acting on a quantized vortex ⋮ Wavefronts in a relativistic two-phase turbulent flow ⋮ Relativistic fluid dynamics: physics for many different scales ⋮ Relativistic fluid dynamics: physics for many different scales ⋮ Physics of neutron star crusts ⋮ ENTRAINMENT COEFFICIENT AND EFFECTIVE MASS FOR CONDUCTION NEUTRONS IN NEUTRON STAR CRUST: MACROSCOPIC TREATMENT ⋮ GALILEAN COVARIANCE AND THE GRAVITATIONAL FIELD ⋮ On the Lie subalgebra of Killing–Milne and Killing–Cartan vector fields in Newtonian spacetime ⋮ NEWTONIAN MECHANICS OF NEUTRON SUPERFLUID IN ELASTIC STAR CRUST

Cites Work

• Jeans' Formula for Gravitational Instability
• CANONICALLY COVARIANT FORMULATION OF LANDAU'S NEWTONIAN SUPERFLUID DYNAMICS
• COVARIANT ANALYSIS OF NEWTONIAN MULTI-FLUID MODELS FOR NEUTRON STARS I: MILNE–CARTAN STRUCTURE AND VARIATIONAL FORMULATION

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