Predictions of Spectral Parameters by Several Inflationary Universe Models in Light of the Planck Results

被引:21
作者
Gron, Oyvind [1 ]
机构
[1] Oslo & Akershus Univ, Fac Technol Art & Design, Coll Appl Sci, NO-0130 Oslo, Norway
关键词
cosmology; inflationary models; spectral parameters; Planck measurements; HYBRID NATURAL INFLATION; PERTURBATION SPECTRA; FIELD INFLATION; WARM INFLATION; SLOW-ROLL; CHAOTIC INFLATION; STANDARD MODEL; RECONSTRUCTION; CONSTRAINTS; ORIGIN;
D O I
10.3390/universe4020015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I give a review of predictions of values of spectral parameters for a large number of inflationary models. The present review includes detailed deductions and information about the approximations that have been made, written in a style that is suitable for text book authors. The Planck data have the power of falsifying several models of inflation as shown in the present paper. Furthermore, they fix the beginning of the inflationary era to a time about 10(-36) s, and the typical energy of a particle at this point of time to 10(16) GeV, only a few orders of magnitude less than the Planck energy, and at least 12 orders of magnitude larger than the most energetic particle produced by CERN's particle accelerator, LHC. This is a phenomenological review with contents as given in the list below. It includes systematic presentations of the different types of slow roll parameters that have been in use, and also of the N-formalism.
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页数:163
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