Class of solutions for the strong-gravity equations

We solve the Einstein equations for strong gravity in the limit that weak gravity is neglected. The class of solutions we find reduces to the Schwarzschild solution (with the weak-gravity Newtonian constant replaced by a strong-coupling parameter) in the limit M²→0, where M is the mass of the strong-gravity spin-2 meson. These solutions may be of relevance for the problem of defining temperature and confinement in hadronic physics.