activity
20172026
most citedTesting the effect of on tension using a Gaussian Process method

52 citations · 154 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2026

Hierarchical Gaussian-process reconstruction of late-time expansion with DESI BAO and compressed Planck priors

Yu-Hao Mu, Zhihuan Zhou, Enkun Li

We reconstruct the late-time expansion history with a hierarchical Gaussian process (GP) that co-samples the kernel hyperparameters together with $(\Hzero,\Om,\Ok,ω_b h^2…

astro-ph.CO2026

Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements

Zhihuan Zhou, Zhuang Miao, Sheng Bi +2

We identify a geometric obstruction to resolving the Hubble tension by combining early-time sound-horizon reduction with late-time smooth dark energy. Within CDM, the BAO--SN ma…

astro-ph.CO2023★ 9 cited

Cosmological Constraints on Thermal Friction of Axion Dark Matter

Gang Liu, Yuhao Mu, Zhihuan Zhou +1

In this paper, we investigate the process in which axion dark matter undergoes thermal friction, resulting in energy injection into dark radiation, with the aim of mitigating the H…

astro-ph.CO2023★ 14 cited

Kinetically Coupled Scalar Fields Model and Cosmological Tensions

Gang Liu, Zhihuan Zhou, Yuhao Mu +1

In this paper, we investigate the kinetically coupled early dark energy (EDE) and scalar field dark matter to address cosmological tensions. The EDE model presents an intriguing th…

astro-ph.CO2023★ 4 cited

A Measurement of Hubble Constant Using Cosmographic Approach from Fast Radio Bursts and SNe Ia

Jiaze Gao, Zhihuan Zhou, Minghui Du +3

The Hubble constant is a crucial parameter in cosmology. However, different cosmic observations have resulted in varying posterior results for , leading to what is k…

astro-ph.CO2023★ 22 cited

Alleviating Cosmological Tensions with a Coupled Scalar Fields Model

Gang Liu, Zhihuan Zhou, Yuhao Mu +1

In this paper, we investigate the interaction between early dark energy (EDE) and scalar field dark matter, proposing a coupled scalar fields model to address the Hubble tension an…

astro-ph.CO2022★ 5 cited

Equality scale-based and sound horizon-based analysis of the Hubble tension

Zhihuan Zhou, Yuhao Mu, Gang Liu +2

The Hubble horizon at matter-radiation equality () and the sound horizon at the last scattering surface () provides interesting consistency check for th…

astro-ph.CO2022★ 6 cited

Limit on the dark matter mass from its interaction with photons

Zhihuan Zhou, Gang Liu, Yuhao Mu +1

In this work, we explore the phenomenology of generalized dark matter (GDM) which interacts with photons (). We assume that DM establishes elastic scattering with when it ha…

astro-ph.CO2021★ 24 cited

Can phantom transition at restore the Cosmic concordance?

Zhihuan Zhou, Gang Liu, Yuhao Mu +1

The tension among inferences of Hubble constant () is found in a large array of datasets combinations. Modification to the late expansion history is the most direct solution t…

astro-ph.CO2019★ 52 cited

Testing the effect of on tension using a Gaussian Process method

En-Kun Li, Minghui Du, Zhi-Huan Zhou +2

Using the redshift space distortion (RSD) data, the tension is studied utilizing a parameterization of growth rate . Here, is derive…

astro-ph.CO2017★ 18 cited

Probing the Neutrino Mass Hierarchy beyond CDM Model

En-Kun Li, Hongchao Zhang, Minghui Du +2

Taking the neutrino oscillation data into consideration, a dimensionless parameter is adopted to parameterize the three neutrino mass eigenstates and the n…