Quantum Gravity Extension of the Inflationary Scenario

被引:179
|
作者
Agullo, Ivan [1 ]
Ashtekar, Abhay
Nelson, William
机构
[1] Penn State, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
基金
美国国家科学基金会;
关键词
Early universe - Energy density - Loop quantum gravity - Orders of magnitude - Planck scale - Quantum field theory - Quantum gravity;
D O I
10.1103/PhysRevLett.109.251301
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Since the standard inflationary paradigm is based on quantum field theory on classical space-times, it excludes the Planck era. Using techniques from loop quantum gravity, the paradigm is extended to a self-consistent theory from the Planck scale to the onset of slow roll inflation, covering some 11 orders of magnitude in energy density and curvature. This preinflationary dynamics also opens a small window for novel effects, e.g., a source for non-Gaussianities, which could extend the reach of cosmological observations to the deep Planck regime of the early Universe. DOI: 10.1103/PhysRevLett.109.251301
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页数:5
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