Hamiltonian formulation of gravity as a spontaneously-broken gauge theory of the Lorentz group
Mehraveh Nikjoo, Tom Zlosnik

TL;DR
This paper develops a Hamiltonian formulation of gravity as a spontaneously-broken gauge theory of the complexified Lorentz group, revealing how the parameter 1 influences the number of propagating degrees of freedom and connecting to chiral asymmetry.
Contribution
It introduces a novel Hamiltonian framework for gauge-theoretic gravity models with a free parameter 1, analyzing how this parameter affects degrees of freedom and symmetry breaking.
Findings
For 1 7 0, no local degrees of freedom propagate.
For 1 7 1 7 1, three complex degrees of freedom propagate.
At 1 = 1 7 1, the theory reduces to General Relativity in a symmetry-broken regime.
Abstract
A number of approaches to gravitation have much in common with the gauge theories of the standard model of particle physics. In this paper, we develop the Hamiltonian formulation of a class of gravitational theories that may be regarded as spontaneously-broken gauge theories of the complexified Lorentz group with the gravitational field described entirely by a gauge field valued in the Lie algebra of and a `Higgs field' valued in the group's fundamental representation. The theories have one free parameter which appears in a similar role to the inverse of the Barbero-Immirzi parameter of Einstein-Cartan theory. However, contrary to that parameter, it is shown that the number of degrees of freedom crucially depends on the value of . For non-zero values of , it is shown that three complex degrees of freedom propagate on general backgrounds, and…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
