Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-05-14
Astronomy and Astrophysics
Astrophysics
LaTex, 4 pages, 2 .ps figures. To appear in the Proceedings of the Euro Conference Rencontres de Moriond: The Cosmological Mod
Scientific paper
We investigate inflation driven by the evolution of highly excited quantum states within the framework of out of equilibrium field dynamics. The self-consistent evolution of these quantum states and the scale factor is studied analytically and numerically. It is shown that the time evolution of these quantum states lead to two consecutive stages of inflation under conditions that are the quantum analogue of slow-roll. The evolution of the scale factor during the first stage has new features that are characteristic of the quantum state. During this initial stage the quantum fluctuations in the highly excited band build up an effective homogeneous condensate with a non-perturbatively large amplitude as a consequence of the large number of quanta. The second stage of inflation is similar to the usual classical chaotic scenario but driven by this effective condensate. The excited quantum modes are already superhorizon in the first stage and do not affect the power spectrum of scalar perturbations. Thus, this novel scenario provides a field theoretical justification for chaotic scenarios driven by a classical homogeneous scalar field of large amplitude.
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