Is dark matter made of mirror matter? Evidence from cosmological data

被引:11
作者
Ciarcelluti, Paolo [1 ]
Wallemacq, Quentin [1 ]
机构
[1] Univ Liege, IFPA, Dep AGO, B-4000 Liege, Belgium
关键词
Cosmology; Cosmic microwave background; Large scale structure; Dark matter; EARLY UNIVERSE COSMOLOGY; DAMA/LIBRA SIGNAL; ABUNDANCE;
D O I
10.1016/j.physletb.2013.12.057
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present new fast numerical simulations of cosmic microwave background and large scale structure in the case in which the cosmological dark matter is made entirely or partly made of mirror matter. We consider scalar adiabatic primordial perturbations at linear scales in a flat Universe. The speed of the simulations allows us for the first time to use Markov Chain Monte Carlo analyses to constrain the mirror parameters. A Universe with pure mirror matter can fit very well the observations, equivalently to the case of an admixture with cold dark matter. In both cases, the cosmological models estimate the presence of a consistent amount of mirror dark matter, 0.06 less than or similar to Omega(mirror)h(2) less than or similar to 0.12. (C) 2013 The Authors. Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:62 / 66
页数:5
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