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A note on cohomogeneity one Einstein metrics on closed 4-manifolds

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Abstract

K. Broder recently classified the closed Einstein 4-manifolds whose isometry groups have dimension at least three. The proof reduces the problem to the study of cohomogeneity-one Einstein metrics invariant under SU(2)SU(2), however a few cases are not treated. We reconcile the missing cases using Broder's techniques with minimal modifications.

Introduction

Broder [2 Theorem 1.1] states that if (M4,g)(M^4,g) is a connected closed Einstein 4-manifold with dim⁡Isom⁡(M,g)≥3\dim\operatorname{Isom}(M,g) \ge3, then gg is flat or its universal cover is homothetic to one of

(S4,ground),(CP2,gFS),(S2×S2,ground⊕ground),(CP2#CP‾2,gPage).(1)(S^4,g_{\mathrm{round}}), \qquad(\mathbb{CP}^2,g_{\mathrm{FS}}), \qquad(S^2 \times S^2,g_{\mathrm{round}} \oplus g_{\mathrm{round}}), \qquad(\mathbb{CP}^2\#\overline{\mathbb{CP}}^2,g_{\mathrm{Page}}). \tag*{(1)}

First, [3 Theorem 3] (see also [Bér82]) implies that only cohomogeneity one actions with 3-dimensional isometry group need to be considered. These actions are by SU(2)\mathrm{SU}(2) and are known, see [8, 6]. In this setting, every invariant Einstein metric is diagonal (c.f. [4 Theorem 3.1]); along a normal geodesic it can be uniquely given in the form

dt2+∑ifi2σi2.dt^2+\sum_i f_i^2\sigma_i^2.

The topologies and smoothness conditions depend on which fif_i vanishes at each singular orbit, and the possibilities are listed in [4 Table 4] (Table 1 below).

Let MnM_n be the space whose group diagram (see §2) is Zn⊂{U(1),U(1)}⊂SU(2)\mathbb{Z}_n \subset\{\mathrm{U}(1),\mathrm{U}(1)\} \subset\mathrm{SU}(2), (Modd≅CP2#CP‾2M_{\mathrm{odd}} \cong\mathbb{CP}^2\#\overline{\mathbb{CP}}^2 and Meven≅S2×S2M_{\mathrm{even}} \cong S^2 \times S^2). For n∈{1,2}n \in\{1,2\}, MnM_n appears twice in Table 1 as there are two configurations: either the same warping function vanishes at both ends (row (R5)), or different functions do (row (R6)). In [2 proof of Theorem 5.1] row (R6) on CP2#CP‾2\mathbb{CP}^2\#\overline{\mathbb{CP}}^2 is reduced to row (R5) by changing the group diagram by conjugating one singular orbit by an element of N(H)0N(H)_0, where HH is a principal isotropy. In [2 §6], on S2×S2S^2 \times S^2, only row (R6) is treated. This does not suffice since rows (R5) and (R6) genuinely must be treated separately; see §3. In this note, we close the remaining cases.

Theorem A. There is no SU(2)\mathrm{SU}(2)-invariant Einstein metric on S2×S2\mathrm{S}^{2} \times\mathrm{S}^{2} in row (R5), and there is no SU(2)\mathrm{SU}(2)-invariant Einstein metric on CP2#CP‾2\mathbb{CP}^{2}\#\overline{\mathbb{CP}}^{2} in row (R6). In particular, up to rescaling, the Page metric and the sum of round metrics are the only Einstein metrics on MnM_n invariant under the defined SU(2)\mathrm{SU}(2)-action.

We only need to consider n∈{1,2,4}n \in\{1,2,4\}, as otherwise the metric is U(2)\mathrm{U}(2)-invariant and thus classified in [Bér82]. One should note that only techniques from [2] are required to prove Theorem 3.5.

We introduce the required notation and preliminary results in § 3. In § 4, we show that the group diagram read off along a normal geodesic is determined by the metric up to interchanging K±K_{\pm} and simultaneous conjugation; see Proposition 3.2. Finally, we prove Theorem 3.5 in § 5 and § 6, the former dealing with S2×S2\mathrm{S}^{2} \times\mathrm{S}^{2} and the latter with CP2#CP‾2\mathbb{CP}^{2}\#\overline{\mathbb{CP}}^{2}.

Acknowledgements

I discussed these issues with Kyle Broder after [2] appeared on arXiv. While working on a related project, I realised that the remaining cases could be resolved quite simply using the techniques of [2], which led to this short note. I would also like to thank Qiu Shi Wang for interesting conversations related to this topic.

Preliminaries

One familiar with [2], or cohomogeneity one actions more generally, should skip this section.

Suppose (M4,g)(M^4,g) is a closed simply-connected 4-manifold on which G=SU(2)G = \mathrm{SU}(2) acts isometrically and by cohomogeneity one. The orbit space is homeomorphic to a closed interval. Let c:[0,T]→Mc : [0,T] \to M be a unit speed geodesic between the singular orbits S−=G⋅c(0)S_{-} = G \cdot c(0) and S+=G⋅c(T)S_{+} = G \cdot c(T) that intersects each orbit orthogonally and exactly once; we call such geodesics normal. The principal isotropy is H=Gc(t)H = G_{c(t)} for t∈(0,T)t \in(0,T), and the singular isotropies are K−=Gc(0)K_{-} = G_{c(0)}, K+=Gc(T)K_{+} = G_{c(T)}. The diagram H⊂{K−,K+}⊂GH \subset\{K_{-},K_{+}\} \subset G determines MM. The diagrams obtained by interchanging K±K_{\pm}, simultaneous conjugation of H,K±H,K_{\pm} by an element of GG, and replacing K+K_{+} by aK+a−1aK_{+}a^{-1} with a∈N(H)0a \in N(H)_0 (c.f. [5]) also determine MM, up to equivariant diffeomorphism.

We will use notation introduced in [2 §2]. Fix an Ad⁡\operatorname{Ad}-invariant inner product QQ on su(2)\mathfrak{su}(2) and a QQ-orthonormal basis {Xi}i=13\{X_i\}_{i=1}^{3} with [Xi,Xi+1]=2Xi+2[X_i,X_{i+1}] = 2X_{i+2}, with {σi}\{\sigma_i\} a dual coframe of the action fields {Xi∗}\{X_i^*\}. A diagonal metric is given by g=dt2+∑ifi(t)2σi2g = \mathrm{d}t^2 + \sum_i f_i(t)^2 \sigma_i^2 on the principal part. It is known that any Einstein metric on gg can be written in a diagonal form, and that the functions fif_i are uniquely determined up to permutation (c.f. [4 Theorem 3.1]).

For {i,j,k}={1,2,3}\{i,j,k\} = \{1,2,3\} define

Li=fi′fi,Ri=fifjfk,S=∑iLi,Ai=Li+Rj+Rk−Ri,L_i = \frac{f_i'}{f_i}, \quad R_i = \frac{f_i}{f_jf_k}, \quad S = \sum_i L_i, \quad A_i = L_i + R_j + R_k - R_i,
ai=2RiAi−AjAk,uij=log⁡(fi/fj).a_i = 2R_iA_i - A_jA_k,\qquad u_{ij} = \log(f_i/f_j).

The Einstein equations, Ric⁡(g)=λg\operatorname{Ric}(g) = \lambda g, imply the following equations [2]:

Li′=−SLi+2Ri2−2(Rj−Rk)2−λ,Ri′=Ri(Li−Lj−Lk),Ai′=(Rj+Rk−3Ri−Ai)Ai+AjAk,ai′=Aj(ak−ai)+Ak(aj−ai),(2)\begin{aligned} L_i' &= -SL_i + 2R_i^2 - 2(R_j-R_k)^2-\lambda, & R_i' &= R_i(L_i-L_j-L_k),\\ A_i' &= (R_j+R_k-3R_i-A_i)A_i+A_jA_k, & a_i' &= A_j(a_k-a_i)+A_k(a_j-a_i), \tag*{(2)} \end{aligned}
uij′′+Suij′=4(Ri−Rj)(Ri+Rj−Rk)=4(fi2−fj2)(fi2+fj2−fk2)fi2fj2fk2.(3)u_{ij}''+Su_{ij}'=4(R_i-R_j)(R_i+R_j-R_k)=4\frac{(f_i^2-f_j^2)(f_i^2+f_j^2-f_k^2)}{f_i^2f_j^2f_k^2}. \tag*{(3)}

Only one smoothness condition is needed in this work: a diagonal metric gg on MnM_n is smooth about S−S_- if and only if there are smooth functions ϕi:(−ε,ε)→R\phi_i:(-\varepsilon,\varepsilon)\to\mathbb{R}, such that [9]

f12=n2t2+t4ϕ1(t2),f2,32=ϕ2(t2)±t4/nϕ3(t2),(4)f_1^2=n^2t^2+t^4\phi_1(t^2),\qquad f_{2,3}^2=\phi_2(t^2)\pm t^{4/n}\phi_3(t^2), \tag*{(4)}

where ϕ2\phi_2 is positive and ϕ3\phi_3 necessarily vanishes unless n∈{1,2,4}n\in\{1,2,4\}. The smoothness condition at S+S_+ is given similarly; substitute t↦T−tt\mapsto T-t and permute indices if required. Table 1 lists all possible smoothness conditions:

Actiont→0t\to0t→Tt\to TEinstein metrics
(R1) SO⁡(3)\operatorname{SO}(3) on S4S^4(2.4), n=4n=4(2.4), n=4n=4, f1↔f3f_1\leftrightarrow f_3round [2 Thm. 3.2]
(R2) SO⁡(3)\operatorname{SO}(3) on CP2\mathbb{CP}^2(2.4), n=4n=4(2.4), n=2n=2, f1↔f3f_1\leftrightarrow f_3Fubini–Study [2 Thm. 4.2]
(R3) SU⁡(2)\operatorname{SU}(2) on S4S^4fixed pointfixed pointround [2 Thm. 3.1]
(R4) SU⁡(2)\operatorname{SU}(2) on CP2\mathbb{CP}^2fixed point(2.4), n=1n=1Fubini–Study [2 Thm. 4.1]
(R5) MnM_n, nn odd(2.4)(2.4)Page [2 Thm. 5.1]
(R5) MnM_n, nn even(2.4)(2.4)none, Theorem 4.1
(R6) M2M_2(2.4)(2.4), f1↔f3f_1\leftrightarrow f_3product [2 Thm. 6.1]
(R6) M1M_1(2.4)(2.4), f1↔f3f_1\leftrightarrow f_3none, Theorem 5.4

Table 1. The configurations of [4 Table 4] and where they are treated.

Equivariant diffeomorphisms and the smoothness conditions

This section is a clarification of [4 Remark 2.9].

Definition 3.1. A GG-invariant metric gg is compatible with the group diagram H⊂{K−,K+}⊂GH\subset\{K_-,K_+\}\subset G if some normal geodesic cc of gg realises it, that is,

Gc(0)=K−,Gc(T)=K+,Gc(t)=Hfor all t∈(0,T).G_{c(0)}=K_-,\qquad G_{c(T)}=K_+,\qquad G_{c(t)}=H\quad\text{for all }t\in(0,T).

There may exist metrics compatible with some group diagram that are not compatible with others representing the same action. In particular, a metric gg being compatible with a given group diagram is only preserved by interchanging K±K_{\pm} and simultaneous conjugation. That is, the diagram obtained by replacing K±K_{\pm} by aK±a−1aK_{\pm}a^{-1} with a∈N(H)0a \in N(H)_0 (c.f. [5]) has the same space of invariant metrics, but need not have the same space of compatible metrics.

Proposition 3.2. Let gg be compatible with H⊂{K−,K+}⊂GH \subset\{K_{-},K_{+}\} \subset G.

(a) gg is compatible with another group diagram H′⊂{K−′,K+′}⊂GH' \subset\{K'_{-},K'_{+}\} \subset G if and only if there exists b∈Gb \in G such that H′=bHb−1H'=bHb^{-1} and

(K−′,K+′)=(bK−b−1,bK+b−1)or(K−′,K+′)=(bK+b−1,bK−b−1).(K'_{-},K'_{+})=(bK_{-}b^{-1},bK_{+}b^{-1}) \qquad\text{or} \qquad(K'_{-},K'_{+})=(bK_{+}b^{-1},bK_{-}b^{-1}).

That is, the new diagram is obtained by conjugating all three isotropy subgroups by the same element, possibly after interchanging K−K_{-} and K+K_{+}.

(b) If φ:M′→M\varphi:M'\to M is a GG-equivariant diffeomorphism, then φ∗g\varphi^{*}g is compatible with the same group diagrams as gg.

Proof. Let cc be a normal geodesic of gg realising H⊂{K−,K+}⊂GH \subset\{K_{-},K_{+}\} \subset G.

(a): If the new diagram is of this form, then b⋅cb\cdot c (or t↦b⋅c(T−t)t\mapsto b\cdot c(T-t) if K±K_{\pm} are interchanged) is a normal geodesic of gg realising the new diagram. Conversely, suppose gg is compatible with a group diagram that is realised by c~\widetilde c a normal geodesic of gg. Reversing c~\widetilde c if necessary, we may assume that c~(0)∈S−\widetilde c(0)\in S_{-}, say c~(0)=h⋅c(0)\widetilde c(0)=h\cdot c(0) with h∈Gh\in G. Then h−1c~h^{-1}\widetilde c is a normal geodesic starting at c(0)c(0). By the slice theorem, K−=Gc(0)K_{-}=G_{c(0)} acts transitively on ∂B(Tc(0)S−⊥)\partial B(T_{c(0)}S_{-}^{\perp}), i.e., the space of unit vectors perpendicular to S−S_{-} (c.f. [4 proof of Lemma 2.6]). Thus, there is a k∈K−k\in K_{-} that maps the initial velocity of cc to that of h−1c~h^{-1}\widetilde c, i.e.,

c′(0)=(k−1h−1c~)′(0).c'(0)=(k^{-1}h^{-1}\widetilde c)'(0).

By uniqueness of geodesics, c~=b⋅c\widetilde c=b\cdot c with b=hkb=hk, and

Gc~(t)=bGc(t)b−1G_{\widetilde c(t)}=bG_{c(t)}b^{-1}

for all t∈[0,T]t\in[0,T].

(b): The map φ\varphi is an isometry from (M′,φ∗g)(M',\varphi^{*}g) to (M,g)(M,g) mapping orbits to orbits, so φ−1∘c\varphi^{-1}\circ c is a normal geodesic of φ∗g\varphi^{*}g. By equivariance, Gφ(p)=GpG_{\varphi(p)}=G_p, so φ−1∘c\varphi^{-1}\circ c realises the same group diagram as cc.

Suppose GG acts via cohomogeneity one on (M,g)(M,g) and let cc be a normal geodesic. Let g\mathfrak{g} be the Lie algebra of GG and let h\mathfrak{h} be the Lie algebra of HH, a principal isotropy. Let n\mathfrak{n} be an Ad⁡H\operatorname{Ad}_{H}-invariant subspace of g\mathfrak{g} such that n⊕h=g\mathfrak{n}\oplus\mathfrak{h}=\mathfrak{g}. Identifying on the principal part of MM with (G/H)×(0,T)(G/H)\times(0,T) via (h,t)↦h⋅c(t)(h,t)\mapsto h\cdot c(t), the metric takes the form g=dt2+gtg=dt^{2}+g_{t}, where gt(X,Y)=g(X∗,Y∗)∣c(t)g_{t}(X,Y)=g(X^{*},Y^{*})|_{c(t)} is an inner product on n\mathfrak{n} for each t∈(0,T)t\in(0,T). The following well known and simple result specifies to which group diagram a specific metric belongs along cc.

Lemma 3.3. (gt)t∈(0,T)(g_{t})_{t\in(0,T)} extend continuously to positive semi-definite forms g0g_{0} and gTg_{T} satisfying

k−=ker⁡g0⊕handk+=ker⁡gT⊕h,\mathfrak{k}_{-}=\ker g_{0}\oplus\mathfrak{h} \qquad\text{and}\qquad \mathfrak{k}_{+}=\ker g_{T}\oplus\mathfrak{h},

where k±\mathfrak{k}_{\pm} are the Lie algebras of K−=Gc(0)K_{-}=G_{c(0)} and K+=Gc(T)K_{+}=G_{c(T)}.

Proof. We consider t=0t=0; the argument at t=Tt=T is the same. gtg_t extends continuously to a positive semi-definite form g0g_0 since for any X∈nX\in\mathfrak n, gt(X,X)=∣X∗(c(t))∣2⟶t→0∣X∗(c(0))∣2g_t(X,X)=\lvert X^*(c(t))\rvert^2 \mathop{\longrightarrow}_{t\to0}\lvert X^*(c(0))\rvert^2. An element X∈nX\in\mathfrak n also lies in k−\mathfrak k_- precisely when X∗(c(0))=0X^*(c(0))=0, i.e., X∈ker⁡g0X\in\ker g_0. That is, n∩k−=ker⁡g0\mathfrak n\cap\mathfrak k_-=\ker g_0 and the result now follows since h⊂k−\mathfrak h\subset\mathfrak k_-.

We now specialise to the case of cohomogeneity one actions on 4 manifolds. In particular, due to the Einstein condition, we may assume that the metric is diagonal. Recall that we only consider the case where G=SU(2)G=\mathrm{SU}(2), K±K_\pm are U(1)\mathrm{U}(1) subgroups of SU(2)\mathrm{SU}(2), and H=ZnH=\mathbb{Z}_n.

Corollary 3.4. Let g=dt2+∑ifi(t)2σi2g=dt^2+\sum_i f_i(t)^2\sigma_i^2 be diagonal with respect to a normal geodesic cc and a basis X1,X2,X3X_1,X_2,X_3 of su(2)\mathfrak{su}(2) as in §2. If fif_i vanishes at t=0t=0 and fjf_j vanishes at t=Tt=T, then k−=span⁡(Xi)\mathfrak k_-=\operatorname{span}(X_i) and k+=span⁡(Xj)\mathfrak k_+=\operatorname{span}(X_j).

Proof. By Lemma 3.3, k−=ker⁡g0\mathfrak k_-=\ker g_0 is spanned by the XkX_k for which fk(0)=0f_k(0)=0.

We say a GG-invariant metric g=dt2+gtg=dt^2+g_t on MM is diagonalisable if there exists a single choice of basis of n\mathfrak n as in §2 such that gtg_t is diagonal for all t∈(0,T)t\in(0,T).

Corollary 3.5. We say g∈Mn,sGg\in M_{n,s}^G if gg is a diagonalisable GG-invariant metric on MnM_n such that for some choice of geodesic and some choice of basis of su(2)\mathfrak{su}(2), the same can function vanishes at both ends. Similarly, we say g∈Mn,dGg\in M_{n,d}^G if different functions can vanish. Mn,sGM_{n,s}^G and Mn,dGM_{n,d}^G are disjoint and invariant under pull-back by GG-equivariant diffeomorphisms Mn→MnM_n\to M_n.

The Page metric belongs to M1,sGM_{1,s}^G (R5) and the Riemannian sum of round metrics belongs to M2,dGM_{2,d}^G (R6).

Proof. Note that the row to which each metric belongs follows from Corollary 3.4. The latter also implies that k−=k+\mathfrak k_-=\mathfrak k_+ for some group diagram if and only if g∈Mn,sGg\in M_{n,s}^G. Since the condition k−=k+\mathfrak k_-=\mathfrak k_+ is preserved under conjugation, the result follows immediately from Proposition 3.2.

Remark 3.6. In general, to study the space of all cohomogeneity one metrics on MM of the form dt2+gtdt^2+g_t, Proposition 3.2 shows that one must consider many different group diagrams. In particular, given an action with some group diagram H⊂{K−,K+}⊂GH\subset\{K_-,K_+\}\subset G, one must check the space of metrics compatible with the diagram H⊂{K−,aK+a−1}⊂GH\subset\{K_-,aK_+a^{-1}\}\subset G for a∈N(H)0a\in N(H)_0. It suffices to let aa range over a set of representatives of the double cosets of

L−\(L−⋅N(H)0⋅L+)/L+,where L±:=N(H)∩N(K±).L_-\backslash(L_-\cdot N(H)_0\cdot L_+)/L_+,\qquad\text{where }L_\pm:=N(H)\cap N(K_\pm).

This formulation is essentially given in [7]. If K−K_- and K+K_+ are not conjugate to each other by an element of N(H)N(H), then each double coset represents a different class of compatible invariant metrics. If K−K_- and K+K_+ are conjugate to each other by an element c∈N(H)c\in N(H), then one could also account for reversing the normal geodesic. That is, the diagrams $H\subset {K,cKc−1}⊂G\{K,cKc^{-1}\}\subset G and H⊂{K,bKb−1}⊂GH\subset\{K,bKb^{-1}\}\subset G for b∈N(H)0cb\in N(H)_0c or b∈N(H)0c−1b\in N(H)_0c^{-1} have the same space of compatible metrics if and only if

b∈N(K)∩N(H)⋅c⋅N(K)∩N(H)b\in N(K)\cap N(H)\cdot c\cdot N(K)\cap N(H)

or

b∈N(K)∩N(H)⋅c−1⋅N(K)∩N(H)b\in N(K)\cap N(H)\cdot c^{-1}\cdot N(K)\cap N(H)

respectively.

S2×S2S^2\times S^2 in row (R5)

Theorem 4.1. For nn even, MnM_n carries no SU(2)-invariant Einstein metric in row (R5).

This follows using the exact same treatment as in Theorem 5.1 (see also Theorem 3.1 and Theorem 4.1) of [2] (which we repeat below for the convenience of the reader).

Proof. Suppose f1f_1 vanishes at both ends. By (2.4), as t→0t\to0 and t→Tt\to T, f2/f3→1f_2/f_3\to1 and f1/f3→0f_1/f_3\to0. Suppose some ratio fi/f3f_i/f_3 with i∈{1,2}i\in\{1,2\} exceeds 1 somewhere, and hence is attained at an interior point t0t_0. Let j∈{1,2}j\in\{1,2\}, j≠ij\ne i be the remaining index. At t0t_0, we have that fj(t0)≤fi(t0)f_j(t_0)\le f_i(t_0), 0<f3(t0)<fi(t0)0<f_3(t_0)<f_i(t_0) and ui3=log⁡(fi/f3)u_{i3}=\log(f_i/f_3) reaches an interior maximum, but (2.3) gives

ui3′′(t0)=4(fi2−f32)(fi2+f32−fj2)fi2fj2f32∣t0>0,u_{i3}''(t_0)=4\left.\frac{(f_i^2-f_3^2)(f_i^2+f_3^2-f_j^2)}{f_i^2f_j^2f_3^2}\right|_{t_0}>0,

a contradiction. Thus the ratio f2/f3f_2/f_3 does not exceed 1, i.e., f2≤f3f_2\le f_3. Similarly, f3≤f2f_3\le f_2, so f2≡f3f_2\equiv f_3. This implies that the metric is U(2)-invariant and we can appeal to the classification of U(2)-invariant compact Einstein manifolds [Bér82].

CP2#CP2\mathbb{CP}^2\#\mathbb{CP}^2 in row (R6)

We now rule out Einstein metrics in row (R6). This is achieved by using the conditions at the endpoints to contradict the forward invariant cone {a1−a2,a2−a3>0}\{a_1-a_2,a_2-a_3>0\}. To show that this cone is forward invariant, we use the maximum principal from the previous section and the positivity of AiA_i. This follows along the lines of the proof of Theorem 3.2 of [2].

Let g=dt2+∑i=13fi(t)2σi2g=dt^2+\sum_{i=1}^{3}f_i(t)^2\sigma_i^2 be an SU(2)-invariant Einstein metric on M1M_1 in row (R6), i.e., with f1f_1 vanishing at t=0t=0 and f3f_3 at t=Tt=T. Recall that a compact Einstein manifold with a non-abelian identity component of the isometry group implies the Einstein constant is positive. As in [4], define the constants β−=1/f2(0)2=1/f3(0)2\beta_- = 1/f_2(0)^2 = 1/f_3(0)^2 and β+=1/f2(T)2=1/f1(T)2\beta_+ = 1/f_2(T)^2 = 1/f_1(T)^2, and also parametrise the reverse direction by ss; s=T−ts=T-t. Solving (2.1) order by order about t=0t=0 using (2.4) gives,

L1=1t+O(t),L2,L3=4β−−λ2t+O(t3),R1=β−t+O(t3),R2,R3=1t+2β−3+O(t3),L_1=\frac{1}{t}+O(t),\quad L_2,L_3=\frac{4\beta_- -\lambda}{2}t+O(t^3),\quad R_1=\beta_-t+O(t^3),\quad R_2,R_3=\frac{1}{t}+\frac{2\beta_-}{3}+O(t^3),

and hence around s=0s=0,

L1,L2=λ−4β+2s+O(s3), L3=−1s+O(s), R1,R2=1s+2β+3+O(s3), R3=β+s+O(s3).L_1,L_2=\frac{\lambda-4\beta_+}{2}s+O(s^3),\ L_3=-\frac{1}{s}+O(s),\ R_1,R_2=\frac{1}{s}+\frac{2\beta_+}{3}+O(s^3),\ R_3=\beta_+s+O(s^3).

In particular, about t=0t=0,

A1=3t+O(t), A2,A3=6β−−λ2t+O(t3), a1=6β−+O(t2), a2,a3=λ−6β−2+O(t2),A_1=\frac{3}{t}+O(t),\ A_2,A_3=\frac{6\beta_- -\lambda}{2}t+O(t^3),\ a_1=6\beta_-+O(t^2),\ a_2,a_3=\frac{\lambda-6\beta_-}{2}+O(t^2),

and about s=0s=0,

A1,A2=λ−2β+2s+O(s3), A3=1s+O(s), a1,a2=λ−2β+2+O(s2), a3=2β++O(s2).A_1,A_2=\frac{\lambda-2\beta_+}{2}s+O(s^3),\ A_3=\frac{1}{s}+O(s),\ a_1,a_2=\frac{\lambda-2\beta_+}{2}+O(s^2),\ a_3=2\beta_++O(s^2).

Lemma 5.1. On (0,T)(0,T), f2>f1,f3f_2>f_1,f_3. In particular R2>R1,R3R_2>R_1,R_3 on (0,T)(0,T).

Proof. By applying a similar argument to the one in Theorem 4.1, f3/f2,f1/f2≤1f_3/f_2,f_1/f_2\leq1. If, at some t0∈(0,T)t_0\in(0,T), fi(t0)=f2(t0)f_i(t_0)=f_2(t_0) for i≠2i\ne2, then f2≥fif_2\geq f_i implies that fi′(t0)=f2′(t0)f_i'(t_0)=f_2'(t_0), but then uniqueness implies that fi≡f2f_i\equiv f_2, which contradicts the initial conditions in (R6).

Lemma 5.2. 0<λ<6β−,6β+0<\lambda<6\beta_-,6\beta_+, and on (0,T)(0,T), Ai>0A_i>0.

Proof. Equation (2.2) implies that for εi∈{±1}\varepsilon_i\in\{\pm1\} such that ε1ε2ε3=1\varepsilon_1\varepsilon_2\varepsilon_3=1 the cone {εiAi>0}\{\varepsilon_iA_i>0\} is forward invariant. By the initial and final conditions, we have that A1(t)>0A_1(t)>0 for small tt and A3(s)>0A_3(s)>0 for small ss. In particular, if A2′(0)≠0A_2'(0)\ne0, then, since A2A_2 and A3A_3 share the same sign for sufficiently small t>0t>0, they must both be positive. If A2′(0)=A3′(0)=0A_2'(0)=A_3'(0)=0, then they both contain at the lowest third order terms. However, using the initial conditions and (2.2),

(A2A3)′=1tQ(A2A3)+B(t)(A2A3)\begin{pmatrix} A_2 \\ A_3 \end{pmatrix}'=\frac{1}{t}Q\begin{pmatrix} A_2 \\ A_3 \end{pmatrix}+B(t)\begin{pmatrix} A_2 \\ A_3 \end{pmatrix}

for some bounded matrix B(t)B(t) and Q=(−233−2)Q=\begin{pmatrix}-2&3\\3&-2\end{pmatrix}. The eigenvalues of QQ are −5-5 and 11, so by Lemma 2.5 of [2], A2≡0≡A3A_2\equiv0\equiv A_3, for small t>0t>0 and hence on (0,T)(0,T) by uniqueness, which again contradicts the behaviour of A3A_3 near TT. By symmetry of the Einstein equations, β+\beta_+ must also satisfy this bound.

Note that (2.2) implies that

(Ai−Aj)′=(Rj+Rk−3Ri−Ai−Aj−Ak)(Ai−Aj)+4(Rj−Ri)Aj.(5)(A_i-A_j)'=(R_j+R_k-3R_i-A_i-A_j-A_k)(A_i-A_j)+4(R_j-R_i)A_j. \tag*{(5)}

Lemma 5.3. On (0,T)(0,T), A2<A1,A3A_2<A_1,A_3.

Proof. Recall that on (0,T)(0,T), R2>R1,R3R_2>R_1,R_3 and Ai>0A_i>0 by Lemmas 5.1 and 5.2. By (5.1), Ai−Aj>0A_i-A_j>0 is preserved, so it suffices to show the lemma holds for sufficiently small t>0t>0. This is trivial for A1A_1 by the initial conditions. For A3A_3, we integrate (5.1) to see that for positive t0t_0,

(A3−A2)(t0)=e∫0t0c dt∫0t0e−∫0tc dt(R2−R3)A2 dt>0(A_3-A_2)(t_0)=e^{\int_0^{t_0}c\,dt}\int_0^{t_0}e^{-\int_0^t c\,dt}(R_2-R_3)A_2\,dt>0

where c=R1+R2−3R3−A1−A2−A3c=R_1+R_2-3R_3-A_1-A_2-A_3.

Theorem 5.4. There is no SU(2)\mathrm{SU}(2)-invariant Einstein metric on CP2#CP‾2\mathbb{CP}^{2}\#\overline{\mathbb{CP}}^{2} in row (R6).

Proof. By (2.2),

(a1−a2)′=−(2A3+A2)(a1−a2)+(A1−A2)(a2−a3)(a2−a3)′=−(2A1+A2)(a2−a3)+(A3−A2)(a1−a2).(6)\begin{aligned} (a_1-a_2)'&=-(2A_3+A_2)(a_1-a_2)+(A_1-A_2)(a_2-a_3)\\ (a_2-a_3)'&=-(2A_1+A_2)(a_2-a_3)+(A_3-A_2)(a_1-a_2). \tag*{(6)} \end{aligned}

Lemma 5.3 implies that the cone a1−a2,a2−a3>0a_1-a_2,a_2-a_3>0 is forward invariant on (0,T)(0,T). The initial conditions and Lemma 5.2 implies that (a1−a2)(0)=18β−−λ2>0(a_1-a_2)(0)=\frac{18\beta_{-}-\lambda}{2}>0 and (a2−a3)(T)=λ−6β+2<0(a_2-a_3)(T)=\frac{\lambda-6\beta_{+}}{2}<0. Thus, for a contradiction, it suffices to show that a2−a3a_2-a_3 is positive at some time. As before, we integrate (5.2) to see that for positive t0t_0:

(a2−a3)(t0)=e−∫0t02A1+A2∫0t0e∫0t2A1+A2(A3−A2)(a1−a2) dt>0.(a_2-a_3)(t_0)=e^{-\int_0^{t_0}2A_1+A_2}\int_0^{t_0}e^{\int_0^t2A_1+A_2}(A_3-A_2)(a_1-a_2)\,dt>0.

References

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