The Holst Spin Foam Model via Cubulations
Aristide Baratin, Cecilia Flori, Thomas Thiemann

TL;DR
This paper introduces a new spin foam model based on cubulations of spacetime, derived from the Holst action, offering a different structure and potential advantages over traditional simplicial models in quantum gravity.
Contribution
It proposes a novel spin foam model using cubulation instead of triangulation, directly from the Holst action, and interprets it as a generating functional for physical n-point functions.
Findings
The model's amplitudes differ from standard spin foam models.
Tetrad n-point functions exhibit a Wick-like structure.
Restriction to simple representations depends on the gauge choice.
Abstract
Spin foam models are an attempt for a covariant, or path integral formulation of canonical loop quantum gravity. The construction of such models usually rely on the Plebanski formulation of general relativity as a constrained BF theory and is based on the discretization of the action on a simplicial triangulation, which may be viewed as an ultraviolet regulator. The triangulation dependence can be removed by means of group field theory techniques, which allows one to sum over all triangulations. The main tasks for these models are the correct quantum implementation of the Plebanski constraints, the existence of a semiclassical sector implementing additional "Regge-like" constraints arising from simplicial triangulations, and the definition of the physical inner product of loop quantum gravity via group field theory. Here we propose a new approach to tackle these issues stemming directly…
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