English

Massive scalar field evolution in de Sitter

General Relativity and Quantum Cosmology 2017-03-08 v3 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

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. 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.

Keywords

Cite

@article{arxiv.1607.00334,
  title  = {Massive scalar field evolution in de Sitter},
  author = {Tommi Markkanen and Arttu Rajantie},
  journal= {arXiv preprint arXiv:1607.00334},
  year   = {2017}
}

Comments

22 pages, 5 figures. v2: References added. v3: Expanded text, added references. Version accepted by JHEP

R2 v1 2026-06-22T14:40:59.717Z