Non-Standard Cosmological Models and The Trans-Planckian Censorship Conjecture

被引:16
|
作者
Torabian, Mahdi [1 ]
机构
[1] Sharif Univ Technol, Dept Phys, Azadi Ave, Tehran 111559161, Iran
来源
关键词
inflation; non-standard cosmology; swampland; trans-Planckian censorship;
D O I
10.1002/prop.201900092
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The trans-Planckian censorship conjecture (TCC) puts an upper bound on the life-time of de Sitter spacetimes. It has immediate consequences for inflationary cosmology. In the standard paradigm, the universe has experienced a single stage of inflation and follows a thermal history. Then, the TCC puts an upper bound on the Hubble parameter during inflation H-inf around 0.1 GeV. Consequently, it implies a severe fine-tuning in initial condition for inflation and non-detection of primordial gravitational waves. In this note, we study non-standard cosmological paradigms with non-thermal history and/or multiple stages of inflations. It is motivated by string theory compactifications and axiverse scenarios in which the modulus/axion fields are effective in the early universe. In early matter domination the TCC bound on H-inf can be raised up to 3 orders of magnitude. In multiple inflationary scenarios the upper bound on the observable inflation can be raised up 10(14) GeV to touch the Planck 2018 bound.
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页数:5
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