# Global solvability of the vacuum Einstein equation and the strong cosmic   censorship in four dimensions

**Authors:** Gabor Etesi

arXiv: 1903.02855 · 2021-03-03

## TL;DR

This paper proves that certain exotic smooth structures on four-manifolds admit complete Ricci-flat, self-dual, hyper-Kähler metrics, leading to new vacuum solutions in general relativity and insights into cosmic censorship and topology change.

## Contribution

It establishes the existence of complete Ricci-flat metrics on exotic smooth structures of four-manifolds, linking differential topology with solutions to Einstein's equations.

## Key findings

- Existence of Ricci-flat metrics on exotic four-manifolds.
- Construction of new vacuum solutions in Lorentzian geometry.
- Connection to cosmic censorship and topology change in physics.

## Abstract

Let $M$ be a connected, simply connected, oriented, closed, smooth four-manifold which is spin (or equivalently having even intersection form) and put $M^\times:=M\setminus\{{\rm point}\}$.In this paper we prove that if $X^\times$ is a smooth four-manifold homeomorphic but not necessarily diffeomorphic to $M^\times$ (more precisely, it carries a smooth structure \`a la Gompf) then $X^\times$ can be equipped with a complete Ricci-flat Riemannian metric. As a byproduct of the construction it follows that this metric is self-dual as well consequently $X^\times$ with this metric is in fact a hyper-K\"ahler manifold. In particular we find that the largest member of the Gompf--Taubes radial family of large exotic ${\mathbb R}^4$'s admits a complete Ricci-flat metric (and in fact it is a hyper-K\"ahler manifold). These Riemannian solutions are then converted into Ricci-flat Lorentzian ones thereby exhibiting lot of new vacuum solutions which are not accessable by the initial vaule formulation. A natural physical interpretation of them in the context of the strong cosmic censor conjecture and topology change is discussed.

## Full text

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## References

58 references — full list in the complete paper: https://tomesphere.com/paper/1903.02855/full.md

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Source: https://tomesphere.com/paper/1903.02855