NEWTONIAN MECHANICS OF NEUTRON SUPERFLUID IN ELASTIC STAR CRUST

DOI10.1142/S0218271806009145zbMath1111.85002arXivastro-ph/0601658OpenAlexW2145061449MaRDI QIDQ3426972

Brandon Carter, Elie Chachoua

Publication date: 14 March 2007

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0601658

zbMATH Keywords

elasticityneutron star crustneutron superfluid

Mathematics Subject Classification ID

Statistical mechanics of superfluids (82D50) Galactic and stellar structure (85A15)

Related Items (4)

Symmetry evolution for the imperfect fluid under perturbations ⋮ Relativistic fluid dynamics: physics for many different scales ⋮ Physics of neutron star crusts ⋮ On the Lie subalgebra of Killing–Milne and Killing–Cartan vector fields in Newtonian spacetime

Cites Work

• Covariant Newtonian and relativistic dynamics of (magneto)-elastic solid model for neutron star crust
• PULSAR ASTROPHYSICS: THE GLITCH PHENOMENON
• Rheometric structure theory, convective differentiation and continuum electrodynamics
• 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
• ENTRAINMENT COEFFICIENT AND EFFECTIVE MASS FOR CONDUCTION NEUTRONS IN NEUTRON STAR CRUST: MACROSCOPIC TREATMENT
• Foundations of general relativistic high-pressure elasticity theory
• COVARIANT ANALYSIS OF NEWTONIAN MULTI-FLUID MODELS FOR NEUTRON STARS I: MILNE–CARTAN STRUCTURE AND VARIATIONAL FORMULATION

This page was built for publication: NEWTONIAN MECHANICS OF NEUTRON SUPERFLUID IN ELASTIC STAR CRUST