Are There Exact Black Hole Solutions in Non-Asymptotically Flat Spacetimes?

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Are there any EXACT solutions similar to Schwarzschild or Kerr in a spacetime which is not asymptotically flat; e.g. FLRW or other cosmological metrics? I am already familiar with the "Swiss cheese" approximations.
 
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We also have exact solutions for the 4 basic black holes in asymptotically de Sitter or anti de Sitter spacetimes. De Sitter spacetime corresponds to eternal inflation.
 
Isn't "Swiss Cheese" exactly what you want? A single hole version of this is the classic paper "Conformal Structure of a Schwarzschild Black Hole Immersed in a Friedman Universe" by Sussman ("General Relativity and Gravitation, Vol. 17, No. 3, 1985) Abstract:

The evolution of a Schwarzschild black hole in an expanding Friedman universe is described using the same coordinate patch for both geometries. Comoving and extended Kruskal coordinates are considered and compared for the cases k = 0 and k = 1. The conformal structure and some global topological aspects of the Schwarzschild-Friedman system are examined with the help of diagrams in comoving and extended Kruskal coordinates.
 
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In Philippe G. Ciarlet's book 'An introduction to differential geometry', He gives the integrability conditions of the differential equations like this: $$ \partial_{i} F_{lj}=L^p_{ij} F_{lp},\,\,\,F_{ij}(x_0)=F^0_{ij}. $$ The integrability conditions for the existence of a global solution ##F_{lj}## is: $$ R^i_{jkl}\equiv\partial_k L^i_{jl}-\partial_l L^i_{jk}+L^h_{jl} L^i_{hk}-L^h_{jk} L^i_{hl}=0 $$ Then from the equation: $$\nabla_b e_a= \Gamma^c_{ab} e_c$$ Using cartesian basis ## e_I...
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