1992/09/15 by Antoine Folacci · 2 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Noncommutative and Quantum Gravity Theories #Quantum Electrodynamics and Casimir Effect #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.46.2553
published as Phys.Rev.D46:2553-2559,1992 · This paper has been published under the title "Zero modes, euclideanization and quantization" [Phys. Rev. D46, 2553 (1992)]
openalex publication_date 1992/09/15 · arxiv created 2009/11/11 · arxiv updated 2010/04/21 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
We consider the massless scalar field on the four-dimensional sphere S4. Its classical action S=(1)/(2)\ensuremath∫S4dV(\ensuremath∇\ensuremathφ)2 is degenerate under the global invariance \ensuremathφ\ensuremath→\ensuremathφ+const. We then quantize the massless scalar field as a gauge theory by constructing a Becchi-Rouet-Stora-Tyutin-invariant quantum action. The corresponding gauge-breaking term is a nonlocal one of the form SGB=(\frac12\ensuremathαV)(\ensuremath∫S4dV\ensuremathφ)2 where \ensuremathα is a gauge parameter and V is the volume of S4. It allows us to correctly treat the zero-mode problem. The quantum theory is invariant under O(5), the symmetry group of S4, and the associated two-point functions have no infrared divergence. The well-known infrared divergence which appears by taking the massless limit of the massive scalar field propagator is therefore a gauge artifact. By contrast, the massless scalar field theory on de Sitter space dS4, the Lorentzian version of S4, is not invariant under the symmetry group of that spacetime O(1,4). Here, the infrared divergence is real. Therefore, the massless scalar quantum field theories on S4 and dS4 cannot be linked by analytic continuation. In this case, because of zero modes, the Euclidean approach to quantum field theory does not work. Similar consideration also apply to massive scalar field theories for exceptional values of the mass parameter.