Infinitesimal Einstein deformations of nearly Kähler metrics
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- by Andrei Moroianu and Uwe Semmelmann PDF
- Trans. Amer. Math. Soc. 363 (2011), 3057-3069 Request permission
Abstract:
It is well known that every 6-dimensional strictly nearly Kähler manifold $(M,g,J)$ is Einstein with positive scalar curvature $\operatorname {scal}>0$. Moreover, one can show that the space $E$ of co-closed primitive $(1,1)$-forms on $M$ is stable under the Laplace operator $\Delta$. Let $E(\lambda )$ denote the $\lambda$-eigenspace of the restriction of $\Delta$ to $E$. If $M$ is compact, and has normalized scalar curvature $\operatorname {scal}=30$, we prove that the moduli space of infinitesimal Einstein deformations of the nearly Kähler metric $g$ is naturally isomorphic to the direct sum $E(2)\oplus E(6)\oplus E(12)$. From Moroianu, Nagy, and Semmelmann (2008), the last summand is itself isomorphic with the moduli space of infinitesimal nearly Kähler deformations.References
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Additional Information
- Andrei Moroianu
- Affiliation: CMLS, École Polytechnique, UMR 7640 du CNRS, 91128 Palaiseau, France
- Email: am@math.polytechnique.fr
- Uwe Semmelmann
- Affiliation: Mathematisches Institut, Universität zu Köln, Weyertal 86-90, D-50931 Köln, Germany
- Address at time of publication: Department of Mathematics, University of Stuttgart, Pfaffenwaldring 57, D-70569 Stuttgart, Germany
- Email: uwe.semmelmann@math.uni-koeln.de, uwe.semmelmann@mathematik.uni-stuttgart.de
- Received by editor(s): June 10, 2008
- Received by editor(s) in revised form: March 30, 2009
- Published electronically: January 26, 2011
- © Copyright 2011
American Mathematical Society
The copyright for this article reverts to public domain 28 years after publication. - Journal: Trans. Amer. Math. Soc. 363 (2011), 3057-3069
- MSC (2010): Primary 58H15, 58E30, 53C10, 53C15
- DOI: https://doi.org/10.1090/S0002-9947-2011-05064-6
- MathSciNet review: 2775798