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.

引用

页数：6

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