All solutions of Einstein's equations in 2+1 dimensions: $\Lambda$-vacuum, pure radiation, or gyratons
Jiri Podolsky, Robert Svarc, Hideki Maeda

TL;DR
This paper derives the complete set of solutions to Einstein's equations in 2+1 dimensions with various matter fields and cosmological constants, including new vacuum solutions and special classes like Robinson-Trautman and Kundt.
Contribution
It provides the first comprehensive classification of all Einstein solutions in 2+1 dimensions with null matter, gyratons, and cosmological constant, including new vacuum solutions.
Findings
Derived general solutions for Einstein's equations with null matter in 2+1 dimensions.
Identified specific subclasses such as Robinson-Trautman, Kundt, VSI, and CSI spacetimes.
Connected solutions to physical models like the photon rocket and pp-waves.
Abstract
Under a weak assumption of the existence of a geodesic null congruence, we present the general solution of the Einstein field equations in three dimensions with any value of the cosmological constant, admitting an aligned null matter field, and also gyratons (a matter field in the form of a null dust with an additional internal spin). The general local solution consists of the expanding Robinson-Trautman class and the non-expanding Kundt class. The gyratonic solutions reduce to spacetimes with a pure radiation matter field when the spin is set to zero. Without matter fields, we obtain new forms of the maximally symmetric vacuum solutions. We discuss these complete classes of solutions and their various subclasses. In particular, we identify the gravitational field of an arbitrarily accelerating source (the Kinnersley photon rocket, which reduces to a Vaidya-type non-moving object) in…
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