Primordial inhomogeneities spectra in mixed dark matter models with non-zero cosmological constant

被引:0
|
作者
Kahniashvili, T
Novosyadlyj, B
Valdarnini, R
机构
[1] LVOV IVAN FRANKO STATE UNIV, ASTRON OBSERV, UA-290005 LVOV, UKRAINE
[2] SCH ADV INT STUDIES, I-340013 TRIESTE, ITALY
来源
HELVETICA PHYSICA ACTA | 1996年 / 69卷 / 03期
关键词
D O I
暂无
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The transfer functions of power spectra for mixed (cold + hot) dark matter models with a cosmological constant are calculated. Under the assumption of the post-inflationary Harrison-Zeldovich spectrum some characteristics of the large scale structure of the Universe are calculated and compared with observable ones.
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页码:219 / 224
页数:6
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