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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 language | English |
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Article number | 133 |
Number of pages | 24 |
Journal | Journal of High Energy Physics |
Volume | 2017 |
Issue number | 1 |
DOIs | |
Publication status | Published - 30 Jan 2017 |
Keywords
- Classical Theories of Gravity
- Field Theories in Higher Dimensions
- Field Theories in Lower Dimensions
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Dive into the research topics of 'Massive scalar field evolution in de Sitter'. Together they form a unique fingerprint.Projects
- 1 Finished
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DARKHORIZONS: Dark Matter and the Early Universe in the LHC Era
Fairbairn, M. & Kilpatrick, J.
1/09/2015 → 28/02/2021
Project: Research