Bounded L2L^2-curvature conjecture for the Einstein scalar field equations

Let (Σ,g,k,u0,u1)(\Sigma,g,k,u_{0},u_{1}) be a smooth initial data set for the Einstein scalar field equations on a three-dimensional manifold Σ\Sigma, satisfying the constraint equations. Here gg is a Riemannian metric, kk is a symmetric 22-tensor, and u0,u1u_{0},u_{1} are functions on Σ\Sigma representing the initial scalar field and its normal derivative.

Bounded L2L^2-curvature conjecture. The Einstein scalar field equations admit local Cauchy developments for initial data sets (Σ,g,k,u0,u1)(\Sigma,g,k,u_{0},u_{1}) with locally finite L2L^{2}-curvature, locally finite L2L^{2}-norm of the first covariant derivatives of kk, locally finite L2L^{2}-norm of the covariant derivatives up to second order of u0u_{0}, and locally finite L2L^{2}-norm of the covariant derivatives up to first order of u1u_{1}.

This conjecture extends the bounded L2L^{2}-curvature local-development result for the Einstein vacuum equations to the Einstein scalar field system. The corresponding vacuum conjecture was solved by Klainerman, Rodnianski and Szeftel, while the scalar-field assertion remains proposed in the source.

Sources & referencesView supporting material

Primary source

Yi Li, “Local curvature estimates for the Ricci-harmonic flow”, arXiv:1810.09760 (2018).

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