Dark matter and dark energy in the Universe: Astrophysical reasons and theoretical models

被引：3

作者：

Apunevych, S. ^{[1
]}

Kulinich, Yu. ^{[1
]}

Novosyadlyj, B. ^{[1
]}

Pelykh, V. ^{[2
]}

机构：

[1] Ivan Franko Natl Univ Lviv 8, Astron Observ, UA-79005 Lvov, Ukraine

[2] Pidstryhach Inst Appl Problems Mech & Math 3 B, UA-76060 Lvov, Ukraine

来源：

KINEMATICS AND PHYSICS OF CELESTIAL BODIES | 2009年 / 25卷 / 02期

关键词：

HUBBLE-SPACE-TELESCOPE; COSMOLOGICAL CONSEQUENCES; GLOBULAR-CLUSTERS; POWER SPECTRUM; SCALE; CONSTRAINTS; SUPERSYMMETRY; AGE; DISCOVERIES; PARAMETERS;

D O I：

10.3103/S0884591309020019

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The general review on the problem of dark matter and dark energy in observable Universe is given. The problem is treated from the point of view of research fields on the boundary of which this fundamental task is situated, namely, the astrophysics and theoretical physics. We emphasize that interdisciplinary nature of "dark sector" of Universe problem can assist in its resolution. The paper does not describe the history of the question, but is centred on revealing the main trends and perspectives.

引用

页码：55 / 72

页数：18

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