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20232026
most citedThe abundance of dark matter haloes down to Earth mass

17 citations · 41 across the 9 of their papers we have counts for

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6 papers · 1 filter

astro-ph.CO2026

Prospects for probing dark matter with filamentary 21cm emission

Yizhou Liu, Yingjie Jing, Haoran Shi +1

The cosmic web contains most of the matter in the Universe, and its filamentary structure is closely related to the properties of dark matter. Compared with the cold dark matter (C…

astro-ph.CO2026

The dark matter halo mass function in the cosmology at all times and over all scales -- from planetary to galaxy cluster masses

Haonan Zheng, Sownak Bose, Carlos S. Frenk +7

The dark matter halo mass function is one of the most fundamental predictions of structure formation theory and cosmological simulations. We present the full halo mass function in…

astro-ph.CO2026

Halo abundance and clustering in cosmologies with massive and asymmetric neutrinos

Yizhou Liu, Wangzheng Zhang, Shihong Liao +1

Neutrinos are the most abundant fermions in the Universe and influence the formation of large-scale structure through both their non-zero masses and a possible chemical potential w…

astro-ph.CO2026

Distinguishing the nature of dark matter by mapping cosmic filaments from Lyman-alpha emission

Yizhou Liu, Liang Gao, Shihong Liao +3

The standard CDM cosmological model predicts that cosmic filaments are highly clumpy, whereas warm dark matter -- invoked to address small-scale challenges in CDM -- produces…

astro-ph.CO2025

Particle loads for cosmological simulations with equal-mass dark matter and baryonic particles

Shihong Liao, Yizhou Liu, Haonan Zheng +5

Traditional cosmological hydrodynamical simulations usually assume equal-numbered but unequal-mass dark matter and baryonic particles, which can lead to spurious collisional heatin…

astro-ph.CO2023★ 11 cited

JWST high redshift galaxy observations have a strong tension with Planck CMB measurements

Deng Wang, Yizhou Liu

JWST high redshift galaxy observations predict a higher star formation efficiency than the standard cosmology does, which poses a new tension to CDM. We find that the situation…