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.
- Received 11 June 1997
DOI:https://doi.org/10.1103/PhysRevLett.79.3121
©1997 American Physical Society