Structure formation with two periods of inflation: beyond PLaln ΛCDM

被引:5
作者
Enqvist, Kari [1 ,2 ]
Sawala, Till [1 ,2 ]
Takahashi, Tomo [3 ]
机构
[1] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland
[2] Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland
[3] Saga Univ, Dept Phys, Saga 8408502, Japan
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2020年 / 10期
关键词
inflation; physics of the early universe; power spectrum; DARK; PERTURBATIONS; SIMULATIONS; GALAXIES; BIG;
D O I
10.1088/1475-7516/2020/10/053
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss structure formation in models with a spectator field in small-field inflation which accommodate a secondary period of inflation. In such models, subgalactic scale primordial fluctuations can be much suppressed in comparison to the usual power-law Lambda CDM model while the large scale fluctuations remain consistent with current observations. We discuss how a secondary inflationary epoch may give rise to observable features in the small scale power spectrum and hence be tested by the structures in the Local Universe.
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收藏
页数:19
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