Loop Quantum Cosmology and Probability of Inflation

被引:0
作者
G. Vereshchagin
S. Bedić
机构
[1] piazza della Repubblica 10,ICRANet
[2] Physics Department,ICRA and University of Rome “Sapienza”
[3] National Academy of Sciences of Belarus,ICRANet
来源
Astronomy Reports | 2018年 / 62卷
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摘要
We study the measure on the set of initial conditions in remote past for Loop Quantum Cosmology with massive scalar field motivated by various choices of the measure present in the literature. The main finding of the paper is existence of an attractor at contracting phase of the universe, which, in addition to the well known attractor at expanding phase, predicts a very specific duration of inflationary stage with the number of e-foldings about 140.
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页码:959 / 964
页数:5
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