1996
DOI: 10.4310/mrl.1996.v3.n2.a1
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Four-Manifolds without Einstein Metrics

Abstract: It is shown that there are infinitely many compact orientable smooth 4-manifolds which do not admit Einstein metrics, but nevertheless satisfy the strict Hitchin-Thorpe inequality 2χ > 3|τ |. The examples in question arise as non-minimal complex algebraic surfaces of general type, and the method of proof stems from Seiberg-Witten theory. * Supported in part by NSF grant DMS-9505744.

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Cited by 129 publications
(173 citation statements)
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“…Details are left to the interested reader. ♦ Remark Corollary 3.4 is the direct descendant of an analogous result in [28], where, using only scalar curvature estimates, a similar conclusion was proved for k ≥ 2 3 c 2 1 (X). It was later pointed out by Kotschick [22] that such a result alone suffices to imply the existence of homeomorphic pairs consisting of an Einstein manifold and a 4-manifold which does not admit Einstein metrics; however, the examples that arise by this method are quite complicated, and have huge c 2 1 .…”
Section: Einstein Metricsmentioning
confidence: 79%
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“…Details are left to the interested reader. ♦ Remark Corollary 3.4 is the direct descendant of an analogous result in [28], where, using only scalar curvature estimates, a similar conclusion was proved for k ≥ 2 3 c 2 1 (X). It was later pointed out by Kotschick [22] that such a result alone suffices to imply the existence of homeomorphic pairs consisting of an Einstein manifold and a 4-manifold which does not admit Einstein metrics; however, the examples that arise by this method are quite complicated, and have huge c 2 1 .…”
Section: Einstein Metricsmentioning
confidence: 79%
“…It was later pointed out by Kotschick [22] that such a result alone suffices to imply the existence of homeomorphic pairs consisting of an Einstein manifold and a 4-manifold which does not admit Einstein metrics; however, the examples that arise by this method are quite complicated, and have huge c 2 1 . The intermediate step between [28] and Corollary 3.4 may be found in [30], where Seiberg-Witten estimates of Weyl curvature were first introduced. While crude by present standards, the method used there did lead to an obstruction when k ≥ 25 57 c 2 1 (X), or about two-thirds of the way to the present result.…”
Section: Einstein Metricsmentioning
confidence: 99%
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