English

Quantum fields in the static de Sitter universe

High Energy Physics - Theory 2020-10-14 v2 General Relativity and Quantum Cosmology

Abstract

We construct explicit mode expansions of various tree-level propagators in the Rindler -- de Sitter universe, also known as the static (or compact) patch of the de Sitter spacetime. We construct in particular the Wightman functions for thermal states having a generic temperature TT. We give a fresh simple proof that the only thermal Wightman propagator that respects the de Sitter isometry is the restriction to the Rindler -- de Sitter wedge of the propagator for the Bunch--Davies state. It is the thermal state with T=(2π)1T = (2 \pi)^{-1} in the units of de Sitter curvature. We show that propagators with T(2π)1T\ne(2\pi)^{-1} are only time translation invariant and have extra singularities on the boundary of the static patch. We also construct the expansions for the so-called alpha-vacua in the static patch and discuss the flat limit.

Keywords

Cite

@article{arxiv.2005.13952,
  title  = {Quantum fields in the static de Sitter universe},
  author = {E. T. Akhmedov and K. V. Bazarov and D. V. Diakonov and U. Moschella},
  journal= {arXiv preprint arXiv:2005.13952},
  year   = {2020}
}

Comments

20 pages, 2 figures, 1 appendix

R2 v1 2026-06-23T15:52:56.460Z