Tests and Problems of the Standard Model in Cosmology

被引：35

作者：

Lopez-Corredoira, Martin ^{[1
,2
]}

机构：

[1] Inst Astrofis Canarias, Tenerife 38205, Spain

[2] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain

来源：

FOUNDATIONS OF PHYSICS | 2017年 / 47卷 / 06期

关键词：

Cosmology; Observational cosmology; Origin formation and abundances of the elements; Dark matter; Dark energy; Superclusters and large-scale structure of the Universe; MICROWAVE BACKGROUND TEMPERATURE; MODIFIED NEWTONIAN DYNAMICS; PROBE WMAP OBSERVATIONS; LARGE-SCALE STRUCTURE; DIGITAL SKY SURVEY; HIERARCHICAL FRACTAL COSMOLOGY; BIG-BANG NUCLEOSYNTHESIS; QUASI-STELLAR OBJECTS; LINEAR COMBINATION METHOD; SELF CREATION COSMOLOGY;

D O I：

10.1007/s10701-017-0073-8

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The main foundations of the standard CDM model of cosmology are that: (1) the redshifts of the galaxies are due to the expansion of the Universe plus peculiar motions; (2) the cosmic microwave background radiation and its anisotropies derive from the high energy primordial Universe when matter and radiation became decoupled; (3) the abundance pattern of the light elements is explained in terms of primordial nucleosynthesis; and (4) the formation and evolution of galaxies can be explained only in terms of gravitation within a inflation + dark matter + dark energy scenario. Numerous tests have been carried out on these ideas and, although the standard model works pretty well in fitting many observations, there are also many data that present apparent caveats to be understood with it. In this paper, I offer a review of these tests and problems, as well as some examples of alternative models.

引用

页码：711 / 768

页数：58

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