Abstract
Abstract
When tetrad (metric) fields are not invertible, the standard canonical formulation of
gravity cannot be adopted as it is. Here we develop a Hamiltonian theory of gravity for
noninvertible tetrad. In contrast to Einstein gravity, this phase is found to exhibit three
local degrees of freedom. This reflects a discrete discontinuity in the limit of a vanishing
tetrad determinant. For the particular case of vanishing lapse, the Hamiltonian constraint
disappears from the classical theory upon fixing the torsional gauge-freedom. Any state
functional invariant under the internal gauge rotations and spatial diffeomorphisms is a formal solution of the associated quantum theory. The formulation here provides a Hamiltonian
basis to analyze gravity theory around a physical singularity, which corresponds to a zero of
the tetrad determinant in curved spacetime.
Subject
Astronomy and Astrophysics
Cited by
1 articles.
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