Nonlinear evolution of dark matter and dark energy in the Chaplygin-gas cosmology

被引：46
作者：
Bilic, N
Lindebaum, RJ
Tupper, GB
Viollier, RD
机构：
[1] Rudjer Boskovic Inst, Zagreb 10002, Croatia
[2] Univ KwaZulu Natal, Sch Chem & Phys Sci, ZA-3209 Scottsville, South Africa
[3] Univ Cape Town, Dept Phys, Inst Theoret Phys & Astrophys, ZA-7701 Rondebosch, South Africa
来源：
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2004年 / 11期
关键词：
dark matter; dark energy theory; cosmology of theories beyond the SM;
D O I：
10.1088/1475-7516/2004/11/008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The hypothesis that dark matter and dark energy are unified through the Chaplygin gas, an exotic fluid obeying p = -A/rho, is re-examined. Using generalizations of the spherical model which incorporate effects of the acoustic horizon we show that an initially perturbative Chaplygin gas evolves into a mixed system containing cold dark matter-like gravitational condensate.
引用
收藏
页码：121 / 131
页数：11
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