Group field cosmology: a cosmological field theory of quantum geometry
arXiv:1201.4151 · doi:10.1088/0264-9381/29/10/105005
Abstract
Following the idea of a field quantization of gravity as realized in group field theory, we construct a minisuperspace model where the wavefunction of canonical quantum cosmology (either Wheeler-DeWitt or loop quantum cosmology) is promoted to a field, the coordinates are minisuperspace variables, the kinetic operator is the Hamiltonian constraint operator, and the action features a nonlinear and possibly nonlocal interaction term. We discuss free-field classical solutions, the quantum propagator, and a mean-field approximation linearizing the equation of motion and augmenting the Hamiltonian constraint by an effective term mixing gravitational and matter variables. Depending on the choice of interaction, this can reproduce, for example, a cosmological constant, a scalar-field potential, or a curvature contribution.
14 pages, 2 figures. v2: minor typos corrected, references added
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Cited by in corpus (30)
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- Quantum cosmology: a review
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- Quantum Cosmology from Group Field Theory Condensates: a Review
- Renormalization of Tensorial Group Field Theories: Abelian U(1) Models in Four Dimensions
- Critical evaluation of common claims in loop quantum cosmology
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- Super-Group Field Cosmology
- Minisuperspace models as infrared contributions
- Non-linear (loop) quantum cosmology
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- The interacting multiverse and its effect on the cosmic microwave background
- Third quantization of -type gravity
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- Constraints on Operator Ordering from Third Quantization
- Fourth Quantization
- Semiclassical solutions of generalized Wheeler-DeWitt cosmology
- Minisuperspace models of discrete systems
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- Weyl Curvature Hypothesis in light of Quantum Backreaction at Cosmological Singularities or Bounces
- Effective cosmology from one-body operators in group field theory