Cited by 23Noncommutative and Quantum Gravity TheoriesCosmology and Gravitation TheoriesRelativity and Gravitational Theory

Perturbing a quantum gravity condensate

Open access
Gielen, Steffen·2015·Physical Review D

Abstract

In a recent proposal using the group field theory approach, a spatially homogeneous (generally anisotropic) universe is described as a quantum gravity condensate of ``atoms of space,'' which allows the derivation of an effective cosmological Friedmann equation from the microscopic quantum gravity dynamics. Here we take a first step towards the study of cosmological perturbations over the homogeneous background. We consider a state in which a single ``atom'' is added to an otherwise homogeneous condensate. Backreaction of the perturbation on the background is negligible and the background dynamics can be solved separately. The dynamics for the perturbation takes the form of a quantum cosmology Hamiltonian for a ``wave function,'' depending on background and perturbations, of the product form usually assumed in a Born-Oppenheimer approximation. We show that the perturbation we consider corresponds to a spatially homogeneous metric perturbation, and for this case derive the usual procedures in quantum cosmology from fundamental quantum gravity.

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  • First steps have been taken to extend GFT condensate cosmology to homogeneous metric perturbations and to inhomogeneous geometries reconstructed from the statistical distribution over homogeneous geometries provided by the condensate density.

    “Some first steps have also been taken in the extension of GFT condensate cosmology to the study of cosmological perturbations, restricted to homogeneous metric perturbations [44], and to inhomogeneous geometries reconstructed from the statistical distribution over homogeneous geometries provided by the condensate density [39].”

    From The universe as a quantum gravity condensate (2017) · cites this paper as [44]

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  • Boundary spin network states correspond to discrete quantum 3-geometries and transition amplitudes between them are given by spin foam amplitudes.

    “In the latter, boundary spin network states correspond to discrete quantum 3-geometries [12] and transition amplitudes in between two such boundary states are given by appropriate spin foam amplitudes [13].”

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Research works printed but not linked: 17

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Authors
Gielen, S.
Affiliations
Perimeter Institute (CA)
Corresponding author
Gielen, Steffen
Venue
Physical Review D
Published
2015-02-20
Volume
91
Issue
4
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W2145322946
Cited by
23
References
1
Citations by year
2021: 1 · 2019: 3 · 2018: 2 · 2017: 6 · 2016: 7 · 2015: 4
FWCI
3.99
Type
journal article
Language
en
Open access
Locations
  • Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
  • White Rose Research Online (University of Leeds, The University of Sheffield, University of York) (acceptedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • Repository@Nottingham (University of Nottingham) (submittedVersion, cc-by)
  • arXiv (Cornell University)
Funders
  • Seventh Framework Programme (622339)
  • Government of Canada
  • Ministry of Research and Innovation
Topics
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
Keywords
group field theory, cosmological perturbations, Born-Oppenheimer approximation, quantum cosmology, metric perturbations, Friedmann equations, anisotropic cosmology

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