Distortion of extra dimensions in the inflationary multiverse

被引:0
|
作者
Rubin, Sergey G. [1 ,2 ]
Fabris, Julio C. [1 ,3 ,4 ]
机构
[1] Natl Res Nucl Univ MEPhI Moscow Engn Phys Inst, Kashirskoe shosse 31, Moscow 115409, Russia
[2] Kazan Fed Univ, NI Lobachevsky Inst Math & Mech, Kremlevskaya St 18, Kazan 420008, Russia
[3] Univ Fed Espirito Santo, Nucleo Cosmo Ufes, BR-29075910 Vitoria, ES, Brazil
[4] Univ Fed Espirito Santo, Dept Fis, BR-29075910 Vitoria, ES, Brazil
关键词
Extra dimensions; inflation; fluctuations; multiverse;
D O I
10.1142/S0218271823400023
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The observable inflation is a final step in a slow evolution of our space. The latter occurs starting from the Planck scale, so that eventually a huge number of causally disconnected regions of space (pocket universes) will appear. The Multiverse thus formed consists of similar universes and, therefore, does not fulfill its mission. Here, we discuss the way to improve the situation. We study the effect of the quantum fluctuations at high energies on the shape of compact extra dimensions which turn out to be specific to each pocket universe. Low-energy physical parameters depend on extra dimensional metric. Therefore, the low-energy physics is different in different pocket universes. The numerical estimation of the probability of finding a particular metric is based on the model of compact two-dimensional extra space.
引用
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页数:14
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