Effect of viscosity and thermal conductivity on the radial oscillation and relaxation of relativistic stars

DOI10.1088/1361-6382/AB472EzbMath1478.85007arXiv1904.00907OpenAlexW2975997080MaRDI QIDQ5159998

Dániel Barta

Publication date: 28 October 2021

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

Full work available at URL: https://arxiv.org/abs/1904.00907

zbMATH Keywords

oscillationrelativitydissipativeneutron stars

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Cites Work

• An Eulerian-Lagrangian approach for incompressible fluids: Local theory
• The stability of relativistic gas spheres⋆
• Relativistic Hydrodynamics
• The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
• Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
• The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid

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