English

On the Bartnik conjecture for the static vacuum Einstein equations

Differential Geometry 2015-12-16 v2 General Relativity and Quantum Cosmology

Abstract

We prove that given any smooth metric γ\gamma and smooth positive function HH on S2S^{2}, there is a constant λ>0\lambda > 0, depending on (γ,H)(\gamma, H), and an asymptotically flat solution (M,g,u)(M, g, u) of the static vacuum Einstein equations on M=R3B3M = {\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)(\gamma, \lambda H). This gives a partial resolution of a conjecture of Bartnik.

Keywords

Cite

@article{arxiv.1507.05887,
  title  = {On the Bartnik conjecture for the static vacuum Einstein equations},
  author = {Michael T. Anderson},
  journal= {arXiv preprint arXiv:1507.05887},
  year   = {2015}
}

Comments

Substantial simplification of proof of main theorem. To appear in Class. Quantum Gravity

R2 v1 2026-06-22T10:15:46.186Z