The Trans-Planckian Problem for Inflationary Cosmology Revisited

dc.creatorBrandenberger, Robert
dc.creatorZhang, Xinmin
dc.date2009-03-12
dc.date2009-03-15
dc.date.accessioned2026-07-07T12:52:09Z
dc.date.available2026-07-07T12:52:09Z
dc.descriptionWe consider an inflationary universe model in which the phase of accelerated expansion was preceded by a non-singular bounce and a period of contraction which involves a phase of deceleration. We follow fluctuations which exit the Hubble radius in the radiation-dominated contracting phase as quantum vacuum fluctuations, re-enter the Hubble radius in the deflationary period and re-cross during the phase of inflationary expansion. Evolving the fluctuations using the general relativistic linear perturbation equations, we find that they exit the Hubble radius during inflation not with a scale-invariant spectrum, but with a highly red spectrum with index $n_s = -3$. We also show that the back-reaction of fluctuations limits the time interval of deflation. Our toy model demonstrates the importance for inflationary cosmology both of the trans-Planckian problem for cosmological perturbations and of back-reaction effects . Firstly, without understanding both Planck-scale physics and the phase which preceded inflation, it is a non-trivial assumption to take the perturbations to be in their local vacuum state when they exit the Hubble radius at late times. Secondly, the back-reaction effects of fluctuations can influence the background in an important way.
dc.description8 pages, 2 figures, 2 references added
dc.identifierhttps://arxiv.org/abs/0903.2065
dc.identifierhttp://arxiv.org/abs/0903.2065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223211
dc.subjectHigh Energy Physics - Theory
dc.subjectCosmology and Nongalactic Astrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe Trans-Planckian Problem for Inflationary Cosmology Revisited
dc.typetext

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