Speaker
Andrés Franco Grisales, KTH Royal Institut of Technology
Abstract
In a recent work, Ringström proposed a geometric notion of initial data on big bang singularities. Moreover, he conjectured that initial data on the singularity could be used to parameterize quiescent solutions to Einstein’s equations; that is, roughly speaking, solutions whose leading order asymptotics are convergent. In this talk, I will present results showing that given initial data on the singularity for the Einstein-nonlinear scalar field equations in 4 spacetime dimensions, as defined by Ringström, there is a corresponding unique development of the data. We do not assume any symmetry or analyticity, and allow for arbitrary closed spatial topology. Our results thus present an important step towards resolving Ringström’s conjecture. Furthermore, our results show that the Einstein-nonlinear scalar field equations have a geometric singular initial value problem formulation, which is analogous to the classical result by Choquet-Bruhat and Geroch for initial data on a Cauchy hypersurface.