activity
20242026
most citedDynamical Dark Energy in the Crosshairs: A Joint Analysis with DESI, Pantheon plus, and TDCOSMO Constraints

26 citations · 78 across the 13 of their papers we have counts for

collaborators

14 papers

physics.gen-ph2026

Revisiting the Hubble Tension with DESI DR2 Baryon Acoustic Oscillation Observations and Machine Learning Methods

Chenfa Zheng, Shuo Cao, Wuzheng Guo +4

One of the key unresolved questions in modern cosmology is the Hubble tension, which arises from the inconsistency between determinations of the Hubble constant () based on ne…

astro-ph.CO2026

Probing Dark Matter Substructure with Wave-Optics Distortions of Strongly Lensed LISA Gravitational Waves

Tonghua Liu, Kai Liao, Marek Biesiada +1

Strong lensing changes the phase of a gravitational-wave signal as well as its amplitude and arrival time. We study whether this phase information can distinguish between three dar…

astro-ph.CO2026

Finite-Core Signatures in LISA-Band Wave-Optics Lensing by Low-Mass Dark Matter Halos

Dejiang Li, Tonghua Liu, Kai Liao +3

LISA-band gravitational waves from massive binary black holes can be diffractively lensed by low-mass dark matter halos and subhalos, so their frequency-dependent amplification can…

astro-ph.CO2026

Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors

Youkai Li, Kai Liao, Mingqi Sun +4

As plans for the construction of third-generation gravitational wave (GW) detectors advance, research into strongly lensed GWs has become increasingly critical. It is anticipated t…

astro-ph.IM2025

Identifying Microlensing by Compact Dark Matter through Diffraction Patterns in Gravitational Waves with Machine Learning

Ao Liu, Tonghua Liu, Dejiang Li +5

Gravitational wave lensing, particularly microlensing by compact dark matter (DM), offers a unique avenue to probe the nature of dark matter. However, conventional detection method…

astro-ph.IM2025★ 3 cited

Identification of Strongly Lensed Gravitational Wave Events Using Squeeze-and-Excitation Multilayer Perceptron Data-efficient Image Transformer

Dejiang Li, Tonghua Liu, Ao Liu +4

With the advancement of third-generation gravitational wave detectors, the identification of strongly lensed gravitational wave (GW) events is expected to play an increasingly vita…

astro-ph.CO2025★ 10 cited

Torsion cosmology in the light of DESI, supernovae and CMB observational constraints

Tonghua Liu, Xiaolei Li, Tengpeng Xu +2

In this work, we investigate a torsion-based cosmological model within the Einstei-Cartan framework, constrained by the latest combined datasets including DESI DR2 BAO, PantheonPlu…

astro-ph.CO2025★ 26 cited

Dynamical Dark Energy in the Crosshairs: A Joint Analysis with DESI, Pantheon plus, and TDCOSMO Constraints

Tonghua Liu, Xiaolei Li, Jieci Wang

In this work, we perform a comprehensive joint analysis of three representative dark energy models - , the Chevallier-Polarski-Linder (CPL) parametrization, and the Gene…

astro-ph.CO2025★ 3 cited

Revisiting the Hubble constant, sound horizon and cosmography from late-time Universe observations

Zhiwei Yang, Tonghua Liu, Xiaolei Li

The Hubble tension has become one of the central problems in cosmology. In this work, we determine the Hubble constant and sound horizon by using the combination of Bar…

astro-ph.CO2025

Advancing Cosmological Parameter Estimation and Hubble Parameter Reconstruction with Long Short-Term Memory and Efficient-Kolmogorov-Arnold Networks

Jiaxing Cui, Marek Biesiada, Ao Liu +3

In this work, we propose a novel approach for cosmological parameter estimation and Hubble parameter reconstruction using Long Short-Term Memory (LSTM) networks and Efficient-Kolmo…

astro-ph.CO2024★ 15 cited

Determination of cosmic curvature independent of the sound horizon and using BOSS/eBOSS and DESI DR1 BAO observations

Tonghua Liu, Shengjia Wang, Hengyu Wu +1

We present an improved model-independent method for determining the cosmic curvature using the observations of Baryon Acoustic Oscillations (BAOs) and the Hubble parameter. The pur…

astro-ph.CO2024

A model-independent determination of the sound horizon using recent BAO measurements and strong lensing systems

Tonghua Liu, Shuo Cao, Jieci Wang

We propose an improved method to determine the sound horizon in a cosmological model-independent way by using the latest observations of BAO measurements from DES, BOSS/eBOSS, and…

astro-ph.CO2024★ 2 cited

Model independent calibration for sound horizon combining observations of supernovae and transversal BAO measurements

Tonghua Liu, Xinyi Zhong, Jieci Wang +1

The sound horizon is a key theoretical prediction of the cosmological model that depends on the speed of sound and the rate of expansion in the early universe, before matter and ra…

gr-qc2024★ 19 cited

Optimal quantum strategy for locating Unruh channels

Qianqian Liu, Tonghua Liu, Cuihong Wen +1

From the perspective of quantum information theory, the effect of Unruh radiation on a two-level accelerated detector can be modeled as a quantum channel. In this work, we employ t…