On the initial regime of pre-big bang cosmology

被引:3
|
作者
Gasperini, M. [1 ,2 ]
机构
[1] Univ Bari, Dipartimento Fis, Via G Amendola 173, I-70126 Bari, Italy
[2] Ist Nazl Fis Nucl, Sez Bari, Via E Orabona 4, I-70125 Bari, Italy
关键词
cosmological perturbation theory; cosmology with extra dimensions; STRING COSMOLOGY; PERTURBATIONS; PHENOMENOLOGY; ANISOTROPIES; CONSTRAINTS; INFLATION;
D O I
10.1088/1475-7516/2017/09/001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The production of a background of super-horizon curvature perturbations with the appropriate (red) spectrum needed to trigger the cosmic anisotropies observed on large scales is associated, in the context of pre-big bang inflation, with a phase of growing string coupling. The extension towards the past of such a phase is not limited in time by the dynamical backreaction of the quantum perturbations of the cosmological geometry and of its sources. A viable, slightly red spectrum of scalar perturbations can thus be the output of an asymptotic, perturbative regime which is well compatible with an initial string-vacuum state satisfying the postulate of "Asymptotic Past Triviality".
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页数:10
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