A consistent first-order model for relativistic heat flow

DOI10.1088/0264-9381/28/19/195023zbMath1226.83025arXiv1107.0165OpenAlexW3098250673MaRDI QIDQ3096499

Cesar S. Lopez-Monsalvo, Nils Andersson

Publication date: 11 November 2011

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

Full work available at URL: https://arxiv.org/abs/1107.0165

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (12)

Stability and causality of Carter’s multifluid theory ⋮ Global high-order numerical schemes for the time evolution of the general relativistic radiation magneto-hydrodynamics equations ⋮ Vorticity and helicity in relativistic heat-conducting fluid ⋮ A general class of Euclidean stars ⋮ Linearizing a non-linear formulation for general relativistic dissipative fluids ⋮ Bulk viscosity in relativistic fluids: from thermodynamics to hydrodynamics ⋮ Applying the Gibbs stability criterion to relativistic hydrodynamics ⋮ Cylindrically symmetric relativistic fluids: a study based on structure scalars ⋮ Relativistic fluid dynamics: physics for many different scales ⋮ Thermal vorticity and thermal chirality in relativistic thermally conducting fluid ⋮ Multi-fluid theory and cosmology: A convective variational approach to interacting dark-sector ⋮ Heat conduction in general relativity

This page was built for publication: A consistent first-order model for relativistic heat flow