QFT and topology in two dimensions: -symmetry and the de Sitter universe
arXiv:2002.12084 · doi:10.1007/s00023-021-01030-7
Abstract
We study bosonic Quantum Field Theory on the double covering of the 2-dimensional de Sitter universe, identified to a coset space of the group . The latter acts effectively on and can be interpreted as it relativity group. The manifold is locally identical to the standard the Sitter spacetime ; it is globally hyperbolic, geodesically complete and an inertial observer sees exactly the same bifurcate Killing horizons as in the standard one-sheeted case. The different global Lorentzian structure causes however drastic differences between the two models. We classify all the -inveriant two-point functions and show that: 1) there is no Hawking-Gibbons temperature; 2) there is no covariant field theory solving the Klein-Gordon equation with mass less than , i.e. the complementary fields go away.
arXiv comment43 pages, 1 figure
References in corpus (11)
- Cosmic Topology
- Microlocal Analysis and Interacting Quantum Field Theories: Renormalization on Physical Backgrounds
- Two-point Functions and Quantum Fields in de Sitter Universe
- Analyticity properties and thermal effects for general quantum field theory on de Sitter space-time
- de Sitter tachyons and related topics
- A remark on alpha vacua for quantum field theories on de Sitter space
- Propagators and Gaussian effective actions in various patches of de Sitter space
- Heating up an environment around black holes and inside de Sitter space
- Topological surprises in de Sitter QFT in two-dimensions
- A note on canonical quantization of fields on a manifold
- Quantum fields on curved spacetimes and a new look at the Unruh effect