Gravity from Dirac Eigenvalues
arXiv:gr-qc/9708041 · doi:10.1142/S0217732398000541
Abstract
We study a formulation of euclidean general relativity in which the dynamical variables are given by a sequence of real numbers , representing the eigenvalues of the Dirac operator on the curved spacetime. These quantities are diffeomorphism-invariant functions of the metric and they form an infinite set of ``physical observables'' for general relativity. Recent work of Connes and Chamseddine suggests that they can be taken as natural variables for an invariant description of the dynamics of gravity. We compute the Poisson brackets of the 's, and find that these can be expressed in terms of the propagator of the linearized Einstein equations and the energy-momentum of the eigenspinors. We show that the eigenspinors' energy-momentum is the Jacobian matrix of the change of coordinates from the metric to the 's. We study a variant of the Connes-Chamseddine spectral action which eliminates a disturbing large cosmological term. We analyze the corresponding equations of motion and find that these are solved if the energy momenta of the eigenspinors scale linearly with the mass. Surprisingly, this scaling law codes Einstein's equations. Finally we study the coupling to a physical fermion field.
An enlarged and improved version which will be pubblished in Mod. Phys. Lett. A
References in corpus (2)
Cited by in corpus (13)
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