2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/213728The cosmological sector to the full non-linear topologically massive gravity (TMG) is obtained for localized sources of mass $m$ and spin $σ$ besides the asymptotically spinning conical flat sector previously obtained. In a small region near but outside the sources, the metric resembles the spinning conical flat metric, but we find that the mass $m$ creates a negative deficit angle of $3m$ as opposed to $m$. Furthermore, it is not possible to recover the results of pure Einstein gravity in the limit $μ\to \infty$ unlike the flat sector.8 pages, no figuresGeneral Relativity and Quantum Cosmologytext