1999/04/19 by Marco Cavaglia
Physics and Astronomy · #gr-qc
published as Grav.Cosmol. 5 (1999) 101-103 · 7 pages, no figures, LaTeX
arxiv created 1999/04/19 · arxiv updated 2009/11/30
We derive the general Σ2× S solution of topologically massive gravity in vacuum and in presence of a cosmological constant. The field equations reduce to three-dimensional Einstein equations and the solution has constant Ricci tensor. We briefly discuss the emergence of non-Ricci flat solutions when spin is introduced.