Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2003-03-11
JCAP 0312:006,2003
Physics
High Energy Physics
High Energy Physics - Theory
10 two-column pages, 1 figure; uses RevTeX4
Scientific paper
10.1088/1475-7516/2003/12/006
In the presence of a short-distance cutoff, the choice of a vacuum state in an inflating, non-de Sitter universe is unavoidably ambiguous. The ambiguity is related to the time at which initial conditions for the mode functions are specified and to the way the expansion of the universe affects those initial conditions. In this paper we study the imprint of these uncertainties on the predictions of inflation. We parametrize the most general set of possible vacuum initial conditions by two phenomenological variables. We find that the generated power spectrum receives oscillatory corrections whose amplitude is proportional to the Hubble parameter over the cutoff scale. In order to further constrain the phenomenological parameters that characterize the vacuum definition, we study gravitational particle production during different cosmological epochs.
Armendariz-Picon Cristian
Lim Eugene A.
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