Stationary Circularly Symmetric 2+1 Gravity Coupled to a Differentially Rotating Perfect Fluid

Details Stationary Circularly Symmetric 2+1 Gravity Coupled to a Differentially Rotating Perfect Fluid Stationary Circularly Symmetric 2+1 Gravity Coupled to a Differentially Rotating Perfect Fluid

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1136g&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

The general solution for a stationary circularly symmetric metric ds2 = -N(r)2dt2 + dr2/F(r)2 + r2 (dϕ + W(r)dt)2, coupled to a differentially rotating perfect fluid and a cosmological constant, is determined through arbitrarily given functions N(r), and W(r), which allow the evaluation of the structural function F(r), the energy density, and the isotropic pressure.

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