Hitchin–Thorpe inequality explained

In differential geometry the Hitchin - Thorpe inequality is a relation which restricts the topology of 4-manifolds that carry an Einstein metric.

Statement of the Hitchin - Thorpe inequality

Let M be a closed, oriented, four-dimensional smooth manifold. If there exists a Riemannian metric on M which is an Einstein metric, then

\chi(M)\geq

3
2

|\tau(M)|,

where is the Euler characteristic of and is the signature of .

This inequality was first stated by John Thorpe in a footnote to a 1969 paper focusing on manifolds of higher dimension.[1] Nigel Hitchin then rediscovered the inequality, and gave a complete characterization of the equality case in 1974;[2] he found that if is an Einstein manifold for which equality in the Hitchin-Thorpe inequality is obtained, then the Ricci curvature of is zero; if the sectional curvature is not identically equal to zero, then is a Calabi–Yau manifold whose universal cover is a K3 surface.

Already in 1961, Marcel Berger showed that the Euler characteristic is always non-negative.[3] [4]

Proof

Let be a four-dimensional smooth Riemannian manifold which is Einstein. Given any point of, there exists a -orthonormal basis of the tangent space such that the curvature operator, which is a symmetric linear map of into itself, has matrix

\begin{pmatrix}λ1&0&0&\mu1&0&0\ 0&λ2&0&0&\mu2&0\ 0&0&λ3&0&0&\mu3\\mu1&0&0&λ1&0&0\ 0&\mu2&0&0&λ2&0\ 0&0&\mu3&0&0&λ3\end{pmatrix}

relative to the basis . One has that is zero and that is one-fourth of the scalar curvature of at . Furthermore, under the conditions and, each of these six functions is uniquely determined and defines a continuous real-valued function on .

According to Chern-Weil theory, if is oriented then the Euler characteristic and signature of can be computed by

\begin{align} \chi(M)&=1
4\pi2

\intM(λ

2)d\mu
g\\ \tau(M)&=1
3\pi2

\intM(λ1\mu1+λ2\mu2+λ3\mu3)d\mug. \end{align}

Equipped with these tools, the Hitchin-Thorpe inequality amounts to the elementary observation
2=\underbrace{(λ
λ
1-\mu
2+(λ
2-\mu
2+(λ
3-\mu
2}
\geq0

+2(λ1\mu1+λ2\mu2+λ3\mu3).

Failure of the converse

A natural question to ask is whether the Hitchin - Thorpe inequality provides a sufficient condition for the existence of Einstein metrics. In 1995, Claude LeBrun and Andrea Sambusetti independently showed that the answer is no: there exist infinitely many non-homeomorphic compact, smooth, oriented 4-manifolds that carry no Einstein metrics but nevertheless satisfy

\chi(M)>

3
2

|\tau(M)|.

LeBrun's examples are actually simply connected, and the relevant obstruction depends on the smooth structure of the manifold.[5] By contrast, Sambusetti's obstruction only applies to 4-manifolds with infinite fundamental group, but the volume-entropy estimate he uses to prove non-existence only depends on the homotopy type of the manifold.[6]

Footnotes

  1. J. . Thorpe . Some remarks on the Gauss-Bonnet formula . J. Math. Mech. . 18 . 8 . 1969 . 779–786 . 24893137 .
  2. N. . Hitchin . Compact four-dimensional Einstein manifolds . J. Diff. Geom. . 9 . 3 . 1974 . 435–442 . 10.4310/jdg/1214432419 . free .
  3. Berger . Marcel . 1961 . Sur quelques variétés d'Einstein compactes . Annali di Matematica Pura ed Applicata . fr . 53 . 1 . 89–95 . 10.1007/BF02417787 . 117985766 . 0373-3114. free .
  4. Book: Besse, Arthur L. . Einstein Manifolds . Springer . 1987 . 3-540-74120-8 . Classics in Mathematics . Berlin . registration.
  5. C. . LeBrun . Four-Manifolds without Einstein Metrics . Math. Res. Lett. . 3 . 2 . 1996 . 133–147 . 10.4310/MRL.1996.v3.n2.a1 . free .
  6. A. . Sambusetti . An obstruction to the existence of Einstein metrics on 4-manifolds . C. R. Acad. Sci. Paris . 322 . 12 . 1996 . 1213–1218 . 0764-4442 .

References