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New quasi-Einstein metrics on a two-sphere

Alex Colling, Maciej Dunajski, Hari Kunduri, James Lucietti

Abstract

We construct all axi-symmetric non-gradient $m$-quasi-Einstein structures on a two-sphere. This includes the spatial cross-section of the extreme Kerr black hole horizon corresponding to $m=2$, as well as a family of new regular metrics with $m\neq 2$ given in terms of hypergeometric functions. We also show that in the case $m=-1$ with vanishing cosmological constant the only orientable compact solution in dimension two is the flat torus, which proves that there are no compact surfaces with a metrisable affine connection with skew Ricci tensor.

New quasi-Einstein metrics on a two-sphere

Abstract

We construct all axi-symmetric non-gradient -quasi-Einstein structures on a two-sphere. This includes the spatial cross-section of the extreme Kerr black hole horizon corresponding to , as well as a family of new regular metrics with given in terms of hypergeometric functions. We also show that in the case with vanishing cosmological constant the only orientable compact solution in dimension two is the flat torus, which proves that there are no compact surfaces with a metrisable affine connection with skew Ricci tensor.
Paper Structure (13 sections, 14 theorems, 65 equations)

This paper contains 13 sections, 14 theorems, 65 equations.

Key Result

Theorem 1.1

Let $(g, X)$ be a solution to the $m$-quasi-Einstein equation (QEE) on a two-dimensional connected surface $M$, with $\mathrm{d} X^\flat$ not identically zero, and a $U(1)$ isometric action.

Theorems & Definitions (30)

  • Theorem 1.1
  • Theorem 1.2
  • Proposition 2.1
  • proof
  • Remark 2.2
  • Lemma 2.3
  • proof
  • Proposition 2.4
  • proof
  • Proposition 3.1
  • ...and 20 more