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2Cm ALF Spaces and Collapsing Ricci-Flat Metrics 0.2Cm 0.1Cm on the K3 Surface

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2Cm ALF Spaces and Collapsing Ricci-Flat Metrics 0.2Cm 0.1Cm on the K3 Surface ALF spaces and collapsing Ricci-flat metrics on the K3 surface Lorenzo Foscolo Stony Brook University Simons Collaboration on Special Holonomy Workshop, SCGP, Stony Brook, September 8 2016 September 7, 2016 The Kummer construction as the prototypical example of the formation of orbifold singularities in sequences of Einstein 4{manifolds: A sequence (Mi ; gi ) of Einstein 4{manifolds with uniform bounds on Euler characteristic, total volume and diameter converges to an Einstein orbifold M1 with finitely many singularities. The geometry around points where the curvature concentrates is modelled by ALE spaces (complete Ricci-flat 4{manifolds with maximal volume growth). The Kummer construction Gibbons{Pope (1979): construction of approximately Ricci-flat metrics on 4 the K3 surface. Desingularise T =Z2 by gluing in 16 rescaled copies of the Eguchi{Hanson metric. Rigorous constructions by Topiwala, LeBrun{Singer and Donaldson The Kummer construction Gibbons{Pope (1979): construction of approximately Ricci-flat metrics on 4 the K3 surface. Desingularise T =Z2 by gluing in 16 rescaled copies of the Eguchi{Hanson metric. Rigorous constructions by Topiwala, LeBrun{Singer and Donaldson The Kummer construction as the prototypical example of the formation of orbifold singularities in sequences of Einstein 4{manifolds: A sequence (Mi ; gi ) of Einstein 4{manifolds with uniform bounds on Euler characteristic, total volume and diameter converges to an Einstein orbifold M1 with finitely many singularities. The geometry around points where the curvature concentrates is modelled by ALE spaces (complete Ricci-flat 4{manifolds with maximal volume growth). Page (1981): consider the Kummer construction along a 1{parameter family 4 3 1 of \split" 4-tori T = T × S` with a circle of length ` ! 0. A \periodic but nonstationary" gravitational instanton asymptotic to 3 1 (R × S )=Z2 appears as a rescaled limit. In this talk Page's suggestion is regarded as a simple case of a more general construction, in which the trivial product T3 × S 1 is replaced by a non-trivial circle bundle over a punctured 3{torus and more general gravitational instantons of cubic volume growth appear as rescaled limits. 4 3 1 The Kummer construction on T = T × S` In the Ricci-flat case if we drop the diameter bound collapsing can occur: inj gi ! 0 everywhere (Anderson, 1992) and the collapse occurs with bounded curvature outside a definite number of points (Cheeger{Tian, 2006). Question: What is the structure of the points where the curvature concentrates? In this talk Page's suggestion is regarded as a simple case of a more general construction, in which the trivial product T3 × S 1 is replaced by a non-trivial circle bundle over a punctured 3{torus and more general gravitational instantons of cubic volume growth appear as rescaled limits. 4 3 1 The Kummer construction on T = T × S` In the Ricci-flat case if we drop the diameter bound collapsing can occur: inj gi ! 0 everywhere (Anderson, 1992) and the collapse occurs with bounded curvature outside a definite number of points (Cheeger{Tian, 2006). Question: What is the structure of the points where the curvature concentrates? Page (1981): consider the Kummer construction along a 1{parameter family 4 3 1 of \split" 4-tori T = T × S` with a circle of length ` ! 0. A \periodic but nonstationary" gravitational instanton asymptotic to 3 1 (R × S )=Z2 appears as a rescaled limit. 4 3 1 The Kummer construction on T = T × S` In the Ricci-flat case if we drop the diameter bound collapsing can occur: inj gi ! 0 everywhere (Anderson, 1992) and the collapse occurs with bounded curvature outside a definite number of points (Cheeger{Tian, 2006). Question: What is the structure of the points where the curvature concentrates? Page (1981): consider the Kummer construction along a 1{parameter family 4 3 1 of \split" 4-tori T = T × S` with a circle of length ` ! 0. A \periodic but nonstationary" gravitational instanton asymptotic to 3 1 (R × S )=Z2 appears as a rescaled limit. In this talk Page's suggestion is regarded as a simple case of a more general construction, in which the trivial product T3 × S 1 is replaced by a non-trivial circle bundle over a punctured 3{torus and more general gravitational instantons of cubic volume growth appear as rescaled limits. 4 Hyperk¨ahler ) Ricci-flat: cr ≤ Vol(Br ) ≤ Cr . a Minerbe (2010): if Vol Br (p) ≤ Cr with a < 4 for all p 2 M then a ≤ 3. Moreover, if a = 3 then (M; g) is ALF: There exists a compact set K ⊂ M, R > 0 and a finite group Γ < O(3) acting freely on S 2 such that M n K is the total space of a circle fibration 3 over (R n BR )=Γ. The metric g is asymptotic to a Riemannian submersion 2 −τ 3 g = gR =Γ + θ + O(r ); τ > 0: If Γ = id then we say that M is an ALF space of cyclic type. If Γ = Z2 we say that M is an ALF space of dihedral type. ALF gravitational instantons Gravitational instantons: complete hyperk¨ahler4{manifolds with decaying curvature at infinity( kRmkL2 < 1. Stronger assumption: faster than quadratic curvature decay, jRmj = O(r −2−), > 0) Moreover, if a = 3 then (M; g) is ALF: There exists a compact set K ⊂ M, R > 0 and a finite group Γ < O(3) acting freely on S 2 such that M n K is the total space of a circle fibration 3 over (R n BR )=Γ. The metric g is asymptotic to a Riemannian submersion 2 −τ 3 g = gR =Γ + θ + O(r ); τ > 0: If Γ = id then we say that M is an ALF space of cyclic type. If Γ = Z2 we say that M is an ALF space of dihedral type. ALF gravitational instantons Gravitational instantons: complete hyperk¨ahler4{manifolds with decaying curvature at infinity( kRmkL2 < 1. Stronger assumption: faster than quadratic curvature decay, jRmj = O(r −2−), > 0) 4 Hyperk¨ahler ) Ricci-flat: cr ≤ Vol(Br ) ≤ Cr . a Minerbe (2010): if Vol Br (p) ≤ Cr with a < 4 for all p 2 M then a ≤ 3. ALF gravitational instantons Gravitational instantons: complete hyperk¨ahler4{manifolds with decaying curvature at infinity( kRmkL2 < 1. Stronger assumption: faster than quadratic curvature decay, jRmj = O(r −2−), > 0) 4 Hyperk¨ahler ) Ricci-flat: cr ≤ Vol(Br ) ≤ Cr . a Minerbe (2010): if Vol Br (p) ≤ Cr with a < 4 for all p 2 M then a ≤ 3. Moreover, if a = 3 then (M; g) is ALF: There exists a compact set K ⊂ M, R > 0 and a finite group Γ < O(3) acting freely on S 2 such that M n K is the total space of a circle fibration 3 over (R n BR )=Γ. The metric g is asymptotic to a Riemannian submersion 2 −τ 3 g = gR =Γ + θ + O(r ); τ > 0: If Γ = id then we say that M is an ALF space of cyclic type. If Γ = Z2 we say that M is an ALF space of dihedral type. 3 Example: x1;:::; xn 2 R , ki 2 Z>0, λ ≥ 0, n X ki h = λ + 2 jx − xi j i=1 2 Near xi : smooth (orbifold) metric on C =Zki . At infinity: ALE if λ = 0, ALF if λ > 0. The Gibbons{Hawking ansatz Gibbons{Hawking (1978): local form of hyperk¨ahlermetrics in dimension 4 with a triholomorphic circle action. 3 U open subset of R h positive harmonic function on U P ! U a principal U(1){bundle with a connection θ (h; θ) satisfies the monopole equation ∗dh = dθ () gh −1 2 3 g = h gR + h θ is a hyperk¨ahlermetric on P The Gibbons{Hawking ansatz Gibbons{Hawking (1978): local form of hyperk¨ahlermetrics in dimension 4 with a triholomorphic circle action. 3 U open subset of R h positive harmonic function on U P ! U a principal U(1){bundle with a connection θ (h; θ) satisfies the monopole equation ∗dh = dθ () gh −1 2 3 g = h gR + h θ is a hyperk¨ahlermetric on P 3 Example: x1;:::; xn 2 R , ki 2 Z>0, λ ≥ 0, n X ki h = λ + 2 jx − xi j i=1 2 Near xi : smooth (orbifold) metric on C =Zki . At infinity: ALE if λ = 0, ALF if λ > 0. Minerbe (2011): All ALF spaces of cyclic type are multi-Taub{NUT metrics. In particular, an An ALF metric is asymptotic to the Gibbons{Hawking metric obtained from the harmonic function n + 1 h = 1 + : 2 jxj ALF spaces of cyclic type In the previous example, the metrics with ki = 1 for all i and λ > 0 are called multi-Taub{NUT metrics. A multi-Taub{NUT metric with n + 1 \nuts" is also called an An ALF metric. The A0 ALF metric is the Taub{NUT metric. ALF spaces of cyclic type In the previous example, the metrics with ki = 1 for all i and λ > 0 are called multi-Taub{NUT metrics. A multi-Taub{NUT metric with n + 1 \nuts" is also called an An ALF metric. The A0 ALF metric is the Taub{NUT metric. Minerbe (2011): All ALF spaces of cyclic type are multi-Taub{NUT metrics. In particular, an An ALF metric is asymptotic to the Gibbons{Hawking metric obtained from the harmonic function n + 1 h = 1 + : 2 jxj G. Chen { X. Chen (2015) classified ALF spaces of dihedral type: The D0 ALF space is the Atiyah{Hitchin manifold (1988). The D1 ALF metrics are the double cover of the Atiyah{Hitchin metric and its Dancer deformations (1993).
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