Rotating and twisting locally rotationally symmetric imperfect fluids
General Relativity and Quantum Cosmology
2017-12-06 v2
Abstract
Rotating and twisting locally rotationally symmetric imperfect fluids in general relativity admit a much larger set of solutions than the self-similar ones recently suggested in the literature. Explicit forms of the metrics are given and the self-similar sub-cases are discussed.
Keywords
Cite
@article{arxiv.1710.06179,
title = {Rotating and twisting locally rotationally symmetric imperfect fluids},
author = {Norbert Van den Bergh},
journal= {arXiv preprint arXiv:1710.06179},
year = {2017}
}
Comments
6 pages, corrected several typos, added comments