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Positive Einstein metrics with $\mathbb {S}^{4m+3}$ as the principal orbit

Published online by Cambridge University Press:  08 April 2024

Hanci Chi*
Affiliation:
Department of Foundational Mathematics, Xi'an Jiaotong–Liverpool University, Suzhou 215123, PR China hanci.chi@xjtlu.edu.cn
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Abstract

We prove that there exists at least one positive Einstein metric on $\mathbb {HP}^{m+1}\sharp \overline {\mathbb {HP}}^{m+1}$ for $m\geq ~2$. Based on the existence of the first Einstein metric, we give a criterion to check the existence of a second Einstein metric on $\mathbb {HP}^{m+1}\sharp \overline {\mathbb {HP}}^{m+1}$. We also investigate the existence of cohomogeneity-one positive Einstein metrics on $\mathbb {S}^{4m+4}$ and prove the existence of a non-standard Einstein metric on $\mathbb {S}^8$.

Information

Type
Research Article
Copyright
© 2024 The Author(s). The publishing rights in this article are licensed to Foundation Compositio Mathematica under an exclusive licence
Figure 0

Figure 1. Each graph shows the horizontal line $\theta =\pi$ and the level curve $2\sqrt {(2m+2)(2m+3)}z_0- (({n-1})/{n})H\sin (\theta )\cos (\theta )=0$. The cross at $\{H=1\}$ is $A_0^+$. The plots show that for $m=1$, the graph of $\Pi$ must be above $\Psi +(0,\pi )$ and hence $\theta _*>\pi$. On the other hand, for $m=5$, the graph of $\Pi$ is below $\Psi +(0,\pi )$ and hence $\theta _*<\pi$. (a) $m=1,\ \Psi (\eta ), \eta \geq 0$. (b) $m=1,\ \Psi (\eta ), \eta \in \mathbb {R}$. (c) $m=1,\ \Psi (\eta )+(0,\pi ), \eta \in \mathbb {R}$. (d) $m=5,\ \Psi (\eta ), \eta \geq 0$. (e) $m=5,\ \Psi (\eta ), \eta \in \mathbb {R}$. (f) $m=5,\ \Psi (\eta )+(0,\pi ), \eta \in \mathbb {R}$.

Figure 1

Figure 2. (a) $m=1$. (b) $m=2$. (c) $m=5$. (d) $m=10$. (e) $m=29$. (f) $m=100$.

Figure 2

Figure A.1. The set $\mathcal {S}$ is degenerate as shown in Proposition 4.2. Hence, only one integral curve $\gamma _{s_\star}\!$ is known to join $p_0^\pm$ and it represents the Bohm's metric. The graphs indicate that $\gamma _{s_1}$ converges to $q_1^-$ for $s_1\in (0,s_\star )$ and converges to $q_3^-$ for $s_1\in (s_{\star },\infty )$. (a) $\gamma _{s_1}$ for $m=1$. (b) $s_1\in (0,s_\star )$. (c) $s_2\in (s_\star,\infty )$.

Figure 3

Figure A.2. Theorems 1.1 and 1.2 claim that for $m\geq 2$ there are at least two integral curves $\gamma _{s_\star }$ and $\gamma _{s_{\star \star }}$ that join $p_0^\pm$. The graphs indicate that $\gamma _{s_1}$ converges to $q_1^-$ for $s_1\in (0,s_\star )\cup (s_{\star \star },\infty )$ and converges to $q_2^-$ for $s_1\in (s_{\star },s_{\star \star })$. (a) $\gamma _{s_1}$ for $m=2$. (b) $s_1\in (0,s_\star )$. (c) $s_2\in (s_\star,s_{\star \star })$. (d) $s_2\in (s_{\star \star },\infty )$.

Figure 4

Figure A.3. These plots are a realization of Theorem 1.3. For $m=1$, the graph of $\zeta _0$ is the straight line that joins $p_1^\pm$. As $s_2$ increases from $0$, the integral curve $\zeta _{s_2}$ converges to $q_1^-$, until $\zeta _{ {1}/({2m+6})}$ converges to $p_0^-$. For $s_2> {1}/({2m+6})$, the integral curve $\zeta _{s_2}$ converges to $q_3^-$, until $s_2=s_\bullet$ once again joins $p_1^\pm$. For the $s_2>s_\bullet$, the integral curve $\zeta _{s_2}$ converges again to $q_1^-$. (a) $\zeta _{s_2}$ for $m=1$. (b) $s_2\in (0, {1}/({2m+6}))$. (c) $s_2\in ( {1}/({2m+6}),s_\bullet )$. (d) $s_2\in (s_\bullet,\infty )$.

Figure 5

Figure A.4. For $m\geq 2$, the behavior of $\zeta _{s_2}$ is relatively simpler. For $s_2\in (0, {1}/({2m+6}))$, the integral curve $\zeta _{s_2}$ converges to $q_1^-$. For $s_2> {1}/({2m+6})$, the integral curve $\zeta _{s_2}$ converges to $q_2^-$. (a) $\zeta _{s_2}$ for $m=1$. (b) $s_2\in (0, {1}/({2m+6}))$. (c) $s_2\in ( {1}/({2m+6}),\infty )$.