Emergence of a low spin phase in group field theory condensates
Steffen Gielen

TL;DR
This paper demonstrates that group field theory condensates naturally evolve into a low spin phase, reproducing classical Friedmann cosmology and linking quantum gravity models with loop quantum cosmology.
Contribution
It shows that GFT condensates reach a low spin phase with a dominant spin, leading to classical cosmological dynamics, strengthening the connection between GFT and LQC.
Findings
GFT condensates dynamically reach a low spin phase.
Total volume evolution follows classical Friedmann equations.
Dominant spin can be the lowest or next lowest value.
Abstract
Recent results have shown how quantum cosmology models can be derived from the effective dynamics of condensate states in group field theory (GFT), where 'cosmology is the hydrodynamics of quantum gravity': the classical Friedmann dynamics for homogeneous, isotropic universes, as well as loop quantum cosmology (LQC) corrections to general relativity have been shown to emerge from fundamental quantum gravity. We take one further step towards strengthening the link with LQC and show, in a class of GFT models for gravity coupled to a free massless scalar field and for generic initial conditions, that GFT condensates dynamically reach a low spin phase of many quanta of geometry, in which all but an exponentially small number of quanta are characterised by a single spin (i.e. by a constant volume per quantum). As the low spin regime is reached, GFT condensates expand to exponentially…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
