Han M, Liu H, Qu D, Vidotto F, Zhang C (2025)
Publication Type: Journal article
Publication year: 2025
Book Volume: 111
Article Number: 086012
Journal Issue: 8
DOI: 10.1103/PhysRevD.111.086012
We study homogenous and isotropic quantum cosmology using the spinfoam formalism of loop quantum gravity (LQG). We define a coupling of a scalar field to the 4-dimensional Lorentzian Engle-Pereira-Rovelli-Livine (EPRL) spinfoam model. We employ the numerical method of complex critical points to investigate the model on two different simplicial complexes: the triangulations of a single hypercube and two connected hypercubes. We find nontrivial implications for the effective cosmological dynamics. In the single-hypercube model, the numerical results suggest an effective Friedmann equation with a scalar density that contains higher-order derivatives and a scalar potential. The scalar potential plays a role similar to a positive cosmological constant and drives an accelerated expansion of the universe. The double-hypercubes model resembles a symmetric cosmic bounce, and a similar effective Friedmann equation emerges with higher-order derivative terms in the effective scalar density, whereas the scalar potential becomes negligible.
APA:
Han, M., Liu, H., Qu, D., Vidotto, F., & Zhang, C. (2025). Cosmological dynamics from covariant loop quantum gravity with scalar matter. Physical Review D, 111(8). https://doi.org/10.1103/PhysRevD.111.086012
MLA:
Han, Muxin, et al. "Cosmological dynamics from covariant loop quantum gravity with scalar matter." Physical Review D 111.8 (2025).
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