QFT, String Temperature and the String Phase of De Sitter Space-time
M. Ram'on Medrano, N. S'anchez

TL;DR
This paper explores the relationship between quantum field theory and string theory in de Sitter space, introducing a dual transform linking classical and quantum string lengths, and analyzing the back reaction effects leading to two curvature phases.
Contribution
It introduces a dual transform connecting QFT and string theory in de Sitter space and analyzes the back reaction, revealing two distinct curvature phases sustained by strings.
Findings
The string temperature in de Sitter space is the dual of the QFT-Hawking-Gibbons temperature.
De Sitter space admits two curvature solutions: classical low curvature and quantum high curvature.
A maximal curvature value exists due to string back reaction, supporting a stringy phase.
Abstract
The density of mass levels \rho(m) and the critical temperature for strings in de Sitter space-time are found. QFT and string theory in de Sitter space are compared. A `Dual'-transform is introduced which relates classical to quantum string lengths, and more generally, QFT and string domains. Interestingly, the string temperature in De Sitter space turns out to be the Dual transform of the QFT-Hawking-Gibbons temperature. The back reaction problem for strings in de Sitter space is addressed selfconsistently in the framework of the `string analogue' model (or thermodynamical approach), which is well suited to combine QFT and string study.We find de Sitter space-time is a self-consistent solution of the semiclassical Einstein equations in this framework. Two branches for the scalar curvature R(\pm) show up: a classical, low curvature solution (-), and a quantum high curvature solution…
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