Energy in first order 2+1 gravity
Alejandro Corichi, Irais Rubalcava-Garcia

TL;DR
This paper investigates the energy definitions in 2+1 dimensional gravity using first order formalism, revealing that different consistent actions lead to either zero or negative energy for Minkowski spacetime.
Contribution
It introduces two gauge-invariant actions in first order formalism for 3D gravity, showing their relation to previous energy results and the dependence on action choice.
Findings
The natural extension of 4D Palatini gravity yields zero energy for Minkowski space.
A gauge-invariant action relates to Marolf-Patiño energy expression.
Minkowski spacetime can have zero or negative energy depending on the action used.
Abstract
We consider =0 three dimensional gravity with asymptotically flat boundary conditions. This system was studied by Ashtekar and Varadarajan within the second order formalism -with metric variables- who showed that the Regge-Teitelboim formalism yields a consistent Hamiltonian description where, surprisingly, the energy is bounded from below and from above. The energy of the spacetime is, however, determined up to an arbitrary constant. The natural choice was to fix that freedom such that Minkowski spacetime has zero energy. More recently, Marolf and Pati\~no started from the Einstein-Hilbert action supplemented with the Gibbons-Hawking term and showed that, in the 2+1 decomposition of the theory, the energy is shifted from the Ashtekar-Varadarajan analysis in such a way that Minkowski spacetime possesses a negative energy. In this contribution we consider the first order…
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