Exact solutions of Einstein and Einstein-scalar equations in 2 + 1 dimensions

Abstract

A nonstatic and circularly symmetric exact solution of the Einstein equations (with a cosmological constant $\Lambda$ and null fluid) in $2+1$ dimensions is given. This is a nonstatic generalization of the uncharged spinless BTZ metric. For $\Lambda =0$, the spacetime is though not flat, the Kretschmann invariant vanishes. The energy, momentum, and power output for this metric are obtained. Further a static and circularly symmetric exact solution of the Einstein-massless scalar equations is given, which has a curvature singularity at $r=0$ and the scalar field diverges at $r=0$ as well as at infinity .

8 pages, Latex, no number

References in corpus (3)

• The Black Hole in Three Dimensional Space Time
• Vacuum polarization around a three-dimensional black hole
• Solution to 2+1 Gravity in DreiBein formalism

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