A general approach for testing non-cold dark matter at small cosmological scales

被引：7
|
作者：
Murgia, R. [1 ,2 ]
机构：
[1] SISSA, Via Bonomea 265, I-34136 Trieste, Italy
[2] INFN, Sez Trieste, Via Bonomea 265, I-34136 Trieste, Italy
来源：
8TH YOUNG RESEARCHER MEETING, 2017 | 2018年 / 956卷
关键词：
HALO FORMATION; ALPHA FOREST; TOO BIG; GALAXIES; PHYSICS; MILKY; FAIL;
D O I：
10.1088/1742-6596/956/1/012005
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
We present a general approach for modelling the small-scale suppression in the linear matter power spectrum induced by the presence of non-cold dark matter. We show that the new parametrisation accurately describes a large variety of non-thermal scenarios, removing the need to individually test each of them. We discuss the first astrophysical constraints on its free parameters and we outline the next steps for pursuing a full statistical data analysis.
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页数：6
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