Future stability of the Einstein-non-linear scalar field system

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Lectures on black holes and linear waves (2008, background): “There are a number of important results applicable in cosmological settings, due to Friedrich [83], Andersson-Moncrief [3], and most recently Ringstrom [134].”
The global non-linear stability of the Kerr-de Sitter family of black holes (2016, methodology): “Earlier global non-linear stability results for the Einstein equation include Friedrich’s work [Fri86] on the stability of (3 + 1)-dimensional de Sitter space, the monumental proof by Christodoulou and Klainerman [CK93] of the stability of (3 + 1)-dimensional Minkowski space, and partial simplificat”
The evolution problem in general relativity (2008, background): “There are a number of important results applicable in cosmological settings, due to Friedrich [75], Andersson-Moncrief [3], and most recently Ringstrom [126].”
The Cauchy Problem in General Relativity (2009, methodology): “Since the methods used by Friedrich and Anderson seem to be dependent on conformal invariance properties of the equations, we developed a different approach to proving stability in [17].”