On the Bartnik conjecture for the static vacuum Einstein equations

preprint2015arXivOpen access

Abstract

We prove that given any smooth metric γγ and smooth positive function HH on S2S^{2}, there is a constant λ>0λ> 0, depending on (γ,H)(γ, H), and an asymptotically flat solution (M,g,u)(M, g, u) of the static vacuum Einstein equations on M=R3∖B3M = {\mathbb R}^{3} \setminus B^{3}, such that the induced metric and mean curvature of (M,g,u)(M, g, u) at ∂M\partial M are given by (γ,λH)(γ, λH). This gives a partial resolution of a conjecture of Bartnik.

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On the Bartnik conjecture for the static vacuum Einstein equations | BZPEER