Conformal geometrodynamics regained: gravity from duality
arXiv:1310.1699 · doi:10.1016/j.aop.2015.02.017
Abstract
There exist several ways of constructing general relativity from `first principles': Einstein's original derivation, Lovelock's results concerning the exceptional nature of the Einstein tensor from a mathematical perspective, and Hojman-Kuchař-Teitelboim's derivation of the Hamiltonian form of the theory from the symmetries of spacetime, to name a few. Here I propose a different set of first principles to obtain general relativity in the canonical framework without presupposing spacetime in any way. I first require consistent propagation of scalar spatially covariant constraints. I find that up to a certain order in derivatives (four spatial and two temporal), there are large families of such consistently propagated constraints. Then I look for pairs of such constraints that can gauge-fix each other and form a theory with two dynamical degrees of freedom per \emph{space} point. This demand singles out the ADM Hamiltonian either in i) CMC gauge, with arbitrary (finite, non-zero) speed of light, and an extra term linear in York time, or ii) a gauge where the Hubble parameter is conformally harmonic.
15 pages, 1 figure. Stronger results than previous version
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Cited by in corpus (10)
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- Cosmology in time asymmetric extensions of general relativity
- Cosmological signatures of time-asymmetric gravity
- Extending the rigidity of general relativity
- Linking shape dynamics and loop quantum gravity
- Local(ish) gravity theories in conformal superspace