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The metric in the superspace of Riemannian metrics and its relation to gravity
General Relativity and Quantum Cosmology · Submitted 1 Sep 2001
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Just one of this class has the property to bring the lagrangian of General Relativity into the form of a classical particle's motion.
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The abstract, sentence by sentence
The space of all Riemannian metrics is infinite-dimensional. Nevertheless a great deal of usual Riemannian geometry can be carried over. The superspace of all Riemannian metrics shall be endowed with a class of Riemannian metrics; their curvature and invariance properties are discussed. Just one of this class has the property to bring the lagrangian of General Relativity into the form of a classical particle's motion. The signature of the superspace metric depends in a non-trivial manner on the signature of the original metric, we derive the corresponding formula. Our approach is a local one: the essence is a metric in the space of all symmetric rank-two tensors, and then the space becomes a warped product of the real line with an Einstein space.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The space of all Riemannian metrics is infinite-dimensional. | background 1.00 | 0.09 | 0.03 | asserted 1.00 |
| s1 | Nevertheless a great deal of usual Riemannian geometry can be carried over. | background 0.96 | 0.11 | 0.06 | asserted 0.98 |
| s2 | The superspace of all Riemannian metrics shall be endowed with a class of Riemannian metrics; their curvature and invariance properties are discussed. | contribution 0.96 | 0.62 | 0.15 | asserted 0.84 |
| s3 | Just one of this class has the property to bring the lagrangian of General Relativity into the form of a classical particle's motion. | result 0.96 | 0.71 | 0.47 | asserted 1.00 |
| s4 | The signature of the superspace metric depends in a non-trivial manner on the signature of the original metric, we derive the corresponding formula. | result 0.99 | 0.92 | 0.16 | asserted 1.00 |
| s5 | Our approach is a local one: the essence is a metric in the space of all symmetric rank-two tensors, and then the space becomes a warped product of the real line with an Einstein space. | method 0.84 | 0.84 | 0.18 | asserted 1.00 |
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Original abstract
The space of all Riemannian metrics is infinite-dimensional. Nevertheless a great deal of usual Riemannian geometry can be carried over. The superspace of all Riemannian metrics shall be endowed with a class of Riemannian metrics; their curvature and invariance properties are discussed. Just one of this class has the property to bring the lagrangian of General Relativity into the form of a classical particle's motion. The signature of the superspace metric depends in a non-trivial manner on the signature of the original metric, we derive the corresponding formula. Our approach is a local one: the essence is a metric in the space of all symmetric rank-two tensors, and then the space becomes a warped product of the real line with an Einstein space.
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2 arXiv papers cite this in 2 sentences
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Cites it as background 1 paper
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For example, in quantum field theory $E$ is a spinor bundle on $M$ (see [ref] ), in gauge field theory $E$ is a bundle of connections on a principal bundle over $M$ (see [ref] ), and in general relativity $E$ is the bundle of Riemannian metrics on $M$ (see [ref] ).
Euler-Lagrange equations for functionals defined on Fr\'echet manifolds · Introduction · 0.98
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