A Deformation Theory of Self-Dual Einstein Spaces
C. G. Torre

TL;DR
This paper develops a deformation theory for self-dual Einstein spaces, analyzing the local structure of their moduli space via elliptic complexes and revealing conditions for discreteness and dimensionality based on the cosmological constant.
Contribution
It introduces a new elliptic complex framework to study the moduli space of self-dual Einstein connections and characterizes its properties depending on the cosmological constant.
Findings
Moduli space is discrete for positive cosmological constant.
Moduli space can be a manifold with dimension given by the Atiyah-Singer index theorem for negative cosmological constant.
Linearization leads to an elliptic complex governing local properties.
Abstract
The self-dual Einstein equations on a compact Riemannian 4-manifold can be expressed as a quadratic condition on the curvature of an (spin) connection which is a covariant generalization of the self-dual Yang-Mills equations. Local properties of the moduli space of self-dual Einstein connections are described in the context of an elliptic complex which arises in the linearization of the quadratic equations on the curvature. In particular, it is shown that the moduli space is discrete when the cosmological constant is positive; when the cosmological constant is negative the moduli space can be a manifold the dimension of which is controlled by the Atiyah-Singer index theorem.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Geometric Analysis and Curvature Flows
