Hamiltonian group field theory with multiple scalar matter fields
Steffen Gielen, Axel Polaczek

TL;DR
This paper extends Hamiltonian group field theory to include multiple scalar matter fields, revealing how effective cosmological dynamics approximate classical general relativity and exhibit quantum corrections like bounce singularities.
Contribution
It introduces a Hamiltonian formulation for models with multiple scalar fields in group field theory, highlighting new features and technical challenges compared to single-field models.
Findings
Effective dynamics reduce to Friedmann equations at large volume
Quantum corrections lead to bounce singularities
Different matter fields are treated differently under generic conditions
Abstract
One approach to defining dynamics for quantum gravity in a naturally timeless setting is to select a suitable matter degree of freedom as a 'clock' before quantisation. This idea of deparametrisation was recently introduced in group field theory leading to a Hamiltonian formulation in which states or operators evolve with respect to the clock given by a free massless scalar field, similar to what happens in deparametrised models in quantum cosmology. Here we extend the construction of Hamiltonian group field theory to models with multiple scalar matter fields, encountering new features and technical subtleties compared with the previously studied case. We show that the effective cosmological dynamics for these more general models reduce to the Friedmann dynamics of general relativity with multiple scalar fields in the limit of large volume, if suitable (non-generic) initial conditions…
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