Deficit angles in 4D spinfoam with a cosmological constant: de Sitter-ness, anti–de Sitter-ness and more

Muxin Han and Qiaoyin Pan
Phys. Rev. D 109, 084040 – Published 15 April 2024

Abstract

This paper investigates the critical behaviors of the 4-dimensional spinfoam model with cosmological constant for a general 4-dimensional simplicial complex as the discretization of spacetime. We find that, at the semiclassical regime, the spinfoam amplitude is peaked at the real critical points that correspond to zero deficit angles (modulo 4πZ/γ) hinged by internal triangles of the 4-complex. Since the 4-simplices from the model are of constant curvature, the discrete geometry with zero deficit angle manifests a de Sitter (dS) spacetime or an anti–de Sitter (AdS) spacetime depending on the sign of the cosmological constant fixed by the boundary condition. The non-(A)dS spacetimes emerge from the complex critical points by an analytic continuation to complex configurations.

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  • Received 29 January 2024
  • Accepted 11 March 2024

DOI:https://doi.org/10.1103/PhysRevD.109.084040

© 2024 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Muxin Han1,2,* and Qiaoyin Pan1,†

  • 1Department of Physics, Florida Atlantic University, 777 Glades Road, Boca Raton, Florida 33431, USA
  • 2Institut für Quantengravitation, Universität Erlangen-Nürnberg, Staudtstrasse 7/B2, 91058 Erlangen, Germany

  • *hanm@fau.edu
  • qpan@fau.edu

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Vol. 109, Iss. 8 — 15 April 2024

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