Energy density in expanding universes as seen by an Unruh detector

Björn Garbrecht and Tomislav Prokopec
Phys. Rev. D 70, 083529 – Published 25 October 2004

Abstract

We consider the response of an Unruh detector to scalar fields in an expanding spacetime. When combining transition elements of the scalar field Hamiltonian with the interaction operator of detector and field, one finds at second order in time-dependent perturbation theory a transition amplitude, which actually dominates in the ultraviolet over the first order contribution. In particular, the detector response faithfully reproduces the particle number implied by the stress energy of a minimally coupled scalar field, which is inversely proportional to the energy of a scalar mode. This finding disagrees with the contention that in de Sitter space, the response of the detector drops exponentially with particle energy and therefore indicates a thermal spectrum.

  • Figure
  • Received 6 July 2004

DOI:https://doi.org/10.1103/PhysRevD.70.083529

©2004 American Physical Society

Authors & Affiliations

Björn Garbrecht* and Tomislav Prokopec

  • Institut für Theoretische Physik, Universität Heidelberg, Philosophenweg 16, D-69120 Heidelberg, Germany

  • *Electronic address: B.Garbrecht@ThPhys.Uni-Heidelberg.De
  • Electronic address: T.Prokopec@ThPhys.Uni-Heidelberg.De

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Issue

Vol. 70, Iss. 8 — 15 October 2004

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