English

Stress tensor fluctuations in de Sitter spacetime

General Relativity and Quantum Cosmology 2010-06-15 v1 High Energy Physics - Theory

Abstract

The two-point function of the stress tensor operator of a quantum field in de Sitter spacetime is calculated for an arbitrary number of dimensions. We assume the field to be in the Bunch-Davies vacuum, and formulate our calculation in terms of de Sitter-invariant bitensors. Explicit results for free minimally coupled scalar fields with arbitrary mass are provided. We find long-range stress tensor correlations for sufficiently light fields (with mass m much smaller than the Hubble scale H), namely, the two-point function decays at large separations like an inverse power of the physical distance with an exponent proportional to m^2/H^2. In contrast, we show that for the massless case it decays at large separations like the fourth power of the physical distance. There is thus a discontinuity in the massless limit. As a byproduct of our work, we present a novel and simple geometric interpretation of de Sitter-invariant bitensors for pairs of points which cannot be connected by geodesics.

Keywords

Cite

@article{arxiv.0911.4870,
  title  = {Stress tensor fluctuations in de Sitter spacetime},
  author = {Guillem Pérez-Nadal and Albert Roura and Enric Verdaguer},
  journal= {arXiv preprint arXiv:0911.4870},
  year   = {2010}
}

Comments

35 pages, 4 figures

R2 v1 2026-06-21T14:16:00.047Z