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We compare simulated galaxy distributions in the cold ΛCDM and warm ΛWDM dark matter models. The ΛWDM model adds one parameter to the ΛCDM model, namely the cut-off wavenumber kfs of linear density perturbations. The challenge is to measure kfs. This study focuses on “smoothing lengths” π/kfs in the range from 12 Mpc to 1 Mpc. The simulations reveal two distinct galaxy populations at any given redshift z: hierarchical galaxies that form bottom up starting at the transition mas?Mfs, and stripped down galaxies that lose mass to neighboring galaxies during their formation, are near larger galaxies, often have filamentary distributions, and seldom fill voids. We compare simulations with observations, and present four independent measurements of kfs, and the mass mh of dark matter particles, based on the redshift of first galaxies, galaxy mass distributions, and rotation curves of spiral galaxies.
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篇名 Simulations and Measurements of Warm Dark Matter Free-Streaming and Mass
来源期刊 天文学与天体物理学国际期刊(英文) 学科 地球科学
关键词 DARK MATTER MASS WARM DARK MATTER Free-Streaming GALAXY MASS Distribution Spiral GALAXY Adiabatic Invariant
年,卷(期) twxyttwlxgjqkyw_2019,(4) 所属期刊栏目
研究方向 页码范围 368-392
页数 25页 分类号 P15
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DARK
MATTER
MASS
WARM
DARK
MATTER
Free-Streaming
GALAXY
MASS
Distribution
Spiral
GALAXY
Adiabatic
Invariant
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天文学与天体物理学国际期刊(英文)
季刊
2161-4717
武汉市江夏区汤逊湖北路38号光谷总部空间
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333
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0
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