Massive scalar field evolution in de Sitter

Tommi Markkanen*, Arttu Rajantie

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

24 Citations (Scopus)
168 Downloads (Pure)

Abstract

The behaviour of a massive, non-interacting and non-minimally coupled quantised scalar field in an expanding de Sitter background is investigated by solving the field evolution for an arbitrary initial state. In this approach there is no need to choose a vacuum in order to provide a definition for particle states, nor to introduce an explicit ultraviolet regularization. We conclude that the expanding de Sitter space is a stable equilibrium configuration under small perturbations of the initial conditions. Depending on the initial state, the energy density can approach its asymptotic value from above or below, the latter of which implies a violation of the weak energy condition. The backreaction of the quantum corrections can therefore lead to a phase of super-acceleration also in the non-interacting massive case.

Original languageEnglish
Article number133
Number of pages24
JournalJournal of High Energy Physics
Volume2017
Issue number1
DOIs
Publication statusPublished - 30 Jan 2017

Keywords

  • Classical Theories of Gravity
  • Field Theories in Higher Dimensions
  • Field Theories in Lower Dimensions

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