A cylindrically symmetric stationary solution of Einstein's equations describing a perfect fluid of finite radius

Details A cylindrically symmetric stationary solution of Einstein's equations describing a perfect fluid of finite radius A cylindrically symmetric stationary solution of Einstein's equations describing a perfect fluid of finite radius

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cqgra..17.2499d&link_type=abstract

Classical and Quantum Gravity, Volume 17, Issue 13, pp. 2499-2507 (2000).

Physics

4

Scientific paper

A two-parameter cylindrically symmetric solution of Einstein's equations is derived for a perfect fluid of finite radius in steady rigid-body rotation. The solution is physically well behaved, with the equation of state, µ + 3p = constant, without singularity and of regular axis. The spacetime is of Petrov type D. The metric is matched at the boundary by a vacuum solution, leaving one free parameter in the complete metric.

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