Axially symmetric dissipative fluids in the quasi-static approximation

DOI10.1142/S021827181650036XzbMath1339.83021arXiv1509.07970MaRDI QIDQ2806278

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Publication date: 17 May 2016

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

Full work available at URL: https://arxiv.org/abs/1509.07970

zbMATH Keywords

relativistic fluidsinterior solutionsnonspherical sources

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) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (3)

Axially symmetric null dust space-time, naked singularity, and cosmic time machine ⋮ Quasi static evolution of compact objects in modified gravity ⋮ Role of Strong Matter‐Field Coupling on Axial Complex Systems

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