Primordial Non-Gaussianity

被引：7
|
作者：
Celoria, M. [1 ,2 ]
机构：
[1] Gran Sasso Sci Inst, Via F Crispi 7, I-67100 Laquila, Italy
[2] Abdus Salaam Int Ctr Theoret Phys, ICTP, Str Costiera 11, I-34151 Trieste, Italy
来源：
GRAVITATIONAL WAVES AND COSMOLOGY | 2020年 / 200卷
关键词：
HALO MASS FUNCTION; N-BODY SIMULATIONS; SCALE-DEPENDENT BIAS; 3-POINT CORRELATION-FUNCTION; EXCURSION SET APPROACH; LUMINOUS RED GALAXIES; NONLINEAR EVOLUTION; POWER SPECTRUM; DARK ENERGY; BISPECTRUM;
D O I：
10.3254/ENFI200009
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Here we review the present status of modelling of and searching for primordial non-Gaussianity of cosmological perturbations. After introducing the models for non-Gaussianity generation during inflation, we discuss the search for non-Gaussian signatures in the Cosmic Microwave Background and in the Large-Scale Structure of the Universe.
引用
收藏
页码：179 / 215
页数：37
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