Ideal magnetohydrodynamics with radiative terms: energy conditions

DOI10.1088/1361-6382/aa61d3zbMath1368.83017arXiv1612.03299OpenAlexW2562943817MaRDI QIDQ5348173

Guillermo A. González, F. D. Lora-Clavijo, Oscar M. Pimentel

Publication date: 14 August 2017

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

Full work available at URL: https://arxiv.org/abs/1612.03299

zbMATH Keywords

magnetohydrodynamicsself-gravitating systemsclassical general relativityenergy conditionscontinous media and classical

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (3)

Shear and expansion evolution for dissipative fluids ⋮ Variations in the expansion and shear scalars for dissipative fluids ⋮ General relativistic razor-thin disks with magnetically polarized matter

Uses Software

• WhiskyMHD

This page was built for publication: Ideal magnetohydrodynamics with radiative terms: energy conditions