Mean-field phase transitions in TGFT quantum gravity
arXiv:2211.12768 · doi:10.1103/PhysRevLett.130.141501
Abstract
Controlling the continuum limit and extracting effective gravitational physics are shared challenges for quantum gravity approaches based on quantum discrete structures. The description of quantum gravity in terms of tensorial group field theory (TGFT) has recently led to much progress in its application to phenomenology, in particular cosmology. This application relies on the assumption of a phase transition to a nontrivial vacuum (condensate) state describable by mean-field theory, an assumption that is difficult to corroborate by a full renormalization group flow analysis due to the complexity of the relevant TGFT models. Here we demonstrate that this assumption is justified due to the specific ingredients of realistic quantum geometric TGFT models: combinatorially non-local interactions, matter degrees of freedom and Lorentz group data together with the encoding of micro-causality. This greatly strengthens the evidence for the existence of a meaningful continuum gravitational regime in group-field and spin-foam quantum gravity, the phenomenology of which is amenable to explicit computations in a mean-field approximation.
Revised version in line with the publication in PRL
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Cited by in corpus (11)
- Scalar Cosmological Perturbations from Quantum Entanglement within Lorentzian Quantum Gravity
- QFT with Tensorial and Local Degrees of Freedom: Phase Structure from Functional Renormalization
- Scalar Cosmological Perturbations from Quantum Gravitational Entanglement
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- Hilbert space formalisms for group field theory
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- Phase transitions in TGFT: Landau-Ginzburg analysis of the causally complete Lorentzian Barrett-Crane model