Observables of the Euclidean Supergravity
arXiv:gr-qc/9707030 · doi:10.1103/PhysRevLett.79.3121
Abstract
The set of constraints under which the eigenvalues of the Dirac operator can play the role of the dynamical variables for Euclidean supergravity is derived. These constraints arise when the gauge invariance of the eigenvalues of the Dirac operator is imposed. They impose conditions which restrict the eigenspinors of the Dirac operator.
Revised version, some misprints in the ecuations (11), (13) and (17) corrected. The errors in the published version will appear cortected in a future erratum
References in corpus (1)
Cited by in corpus (12)
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- Noncommutative Finsler Geometry, Gauge Fields and Gravity
- Nonholonomic Clifford Structures and Noncommutative Riemann--Finsler Geometry
- Euclidean Supergravity in Terms of Dirac Eigenvalues
- On Local Constraints of D=4 Supergravity in Terms of Dirac Eigenvalues
- Constraints on spacetime manifold in Euclidean supergravity in terms of Dirac eigenvalues
- On The Symplectic Two-Form of Gravity in Terms of Dirac Eigenvalues
- Toward Supergravity Spectral Action
- On the Dirac Eigenvalues as Observables of the on-shell N=2 D=4 Euclidean Supergravity