Spherically symmetric Poincaré solution of gauge gravity theory in the presence of dark energy

Based on the generalization of the general theory of relativity (GTR) on the Poincaré gauge theory of gravity (GT) and the modification of the cosmological constant of GTR carried out by E.V. Gliner, a spherically symmetric solution of GT in the presence of dark energy with an extremely minimal self-action was found. The solution found is conformal to the well-known Yilmaz-Rosen metric, which is close to the Schwarzild metric, but has no singularity at the gravitational radius, which leads to the absence of black holes and their replacement with quasi-black holes.