paper

Complex Chern-Simons Theory with and An Improved Spinfoam Model with Cosmological Constant

arXiv:2504.06427

Abstract

This paper presents an improvement to the four-dimensional spinfoam model with cosmological constant (-SF model) in loop quantum gravity. The original -SF model, defined via Chern-Simons theory on graph-complement 3-manifolds, produces finite amplitudes and reproduces curved 4-simplex geometries in the semi-classical limit. However, extending the model to general simplicial complexes necessitated ad hoc, non-universal phase factors in face amplitudes, complicating systematic constructions. We resolve this issue by redefining the vertex amplitude using a novel set of phase space coordinates that eliminate the extraneous phase factor, yielding a universally defined face amplitude. Key results include: (1) The vertex amplitude is rigorously shown to be well-defined for Chern-Simons levels , compatible with semi-classical analysis (). (2) The symplectic structure of the Chern-Simons phase space is modified to accommodate holonomies, relaxing quantization constraints to . (3) Edge amplitudes are simplified using constraints aligned with colored tensor models, enabling systematic gluing of 4-simplices into complexes dual to colored graphs. (4) Stationary phase analysis confirms consistency of critical points with prior work, recovering Regge geometries with curvature determined by . These advancements streamline the spinfoam amplitude definition, facilitating future studies of colored group field theories and continuum limits of quantum gravity. The results establish a robust framework for 4D quantum gravity with non-zero , free of previous ambiguities in face amplitudes.

23+4 pages, 5 figures; v2: typos corrected