Second order Einstein deformations

We study the integrability to second order of infinitesimal Einstein deformations on compact Riemannian and in particular on Kähler manifolds. We find a new way of expressing the necessary and sufficient condition for integrability to second order, which also gives a very clear and compact way of writing the Koiso obstruction. As an application we consider the Kähler case, where the condition can be further simplified and in complex dimension 3 turns out to be purely algebraic. One of our main results is the complete and explicit description of integrable to second order infinitesimal Einstein deformations on the complex 2-plane Grassmannian, which also has a quaternion Kähler structure. As a striking consequence we find that the symmetric Einstein metric on the Grassmannian $\mathrm{Gr}_{2}(\mathbb{C}^{n+2})$ for $n$ odd is rigid.

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Publication Details

Journal
Journal of the Mathematical Society of Japan
Published
2025-02-20
DOI
https://doi.org/10.2969/jmsj/92169216
Primary Topic
Geometric Analysis and Curvature Flows
Type
article
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article

Second order Einstein deformations

Uwe Semmelmann, Paul-Andi Nagy
Journal of the Mathematical Society of Japan
Geometric Analysis and Curvature Flows
article

Second order Einstein deformations

Uwe Semmelmann, Paul-Andi Nagy
article en

Abstract

We study the integrability to second order of infinitesimal Einstein deformations on compact Riemannian and in particular on Kähler manifolds. We find a new way of expressing the necessary and sufficient condition for integrability to second order, which also gives a very clear and compact way of writing the Koiso obstruction. As an application we consider the Kähler case, where the condition can be further simplified and in complex dimension 3 turns out to be purely algebraic. One of our main results is the complete and explicit description of integrable to second order infinitesimal Einstein deformations on the complex 2-plane Grassmannian, which also has a quaternion Kähler structure. As a striking consequence we find that the symmetric Einstein metric on the Grassmannian $\mathrm{Gr}_{2}(\mathbb{C}^{n+2})$ for $n$ odd is rigid.

Journal of the Mathematical Society of JapanVol. 77(2)
University of Stuttgart (DE), Institute for Basic Science (KR)
Openalex Percentile: Top 95%
Geometric Analysis and Curvature Flows
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