Physics – Fluid Dynamics
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983gregr..15..567l&link_type=abstract
General Relativity and Gravitation, Volume 15, Issue 6, pp.567-579
Physics
Fluid Dynamics
12
Fluid Dynamics:Relativity Theory, Relativity Theory:Fluid Dynamics
Scientific paper
Stationary solutions of the Einstein equation are investigated when the source is a rigidly rotating fluid. Using the three-dimensional spin coefficient method the angular dependence of the metric tensor can be analytically calculated if the eigenray congruence is geodesic and shear free. The nonstatic solutions of this class do not describe physically realistic bodies, but, instead, bodies with NUT-type geometry.
Lukacs Béla
Newman Ezra Ted
Sparling George
Winicour Jeffrey
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