activity
20242026
most citedConstraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

126 citations · 382 across the 35 of their papers we have counts for

collaborators

36 papers

math.CO2026

A chain theorem for planar PM-compact bricks

Yaxian zhang, Qiuli Li, Fuliang Lu

A connected graph is matching covered if it contains at least one edge and every edge belongs to some perfect matching of . A matching covered graph is a brick if it is 3-co…

astro-ph.CO2026★ 6 cited

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-CDM Interpretations, and Tensions

Tian-Nuo Li, Guo-Hong Du, Hao Wang +3

Recent baryon acoustic oscillation measurements from DESI provide important new clues for reassessing whether the standard CDM model offers a sufficient description of the late-…

astro-ph.CO2026

Exploring the Cosmic Dawn through the 21 cm Forest and High-redshift Radio Sources with the SKA

Junsong Cang, Benedetta Ciardi, Barun Maity +12

The 21~cm forest, seen as absorption features in the spectra of distant radio sources, is produced by intervening neutral hydrogen and offers a direct probe of the neutral intergal…

astro-ph.CO2026

Constraints on the Sum of Neutrino Masses from ACT DR6 and DESI DR2 Considering Isocurvature Initial Conditions

Hongsheng Hou, Sai Wang, Zhi-Chao Zhao +1

We present a robust assessment of cosmological constraints on the sum of neutrino masses () when relaxing the standard assumption of purely adiabatic primordial initial c…

astro-ph.CO2026

Synergy between CSST and future gravitational-wave detectors: Probing primordial black holes by cross-correlating dark sirens with galaxies

Ya-Nan Du, Ji-Yu Song, Jing-Fei Zhang +1

Gravitational-wave (GW) events and galaxies both trace the cosmic matter distribution, but the mergers of astrophysical black holes and primordial black holes (PBHs) are expected t…

astro-ph.CO2026

Neutrino mass constraints in interacting dark energy models after DESI DR2

Hui Li, Guo-Hong Du, Tian-Nuo Li +4

Recent DESI observations indicate a deviation from the CDM model, showing a preference for dynamical dark energy and thereby relaxing the upper limit on the neutrino mass within…

astro-ph.CO2026

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data

Guo-Hong Du, Tian-Nuo Li, Lu Yin +4

In the JWST and DESI era, the JWST high-redshift galaxy observations and DESI baryon acoustic oscillation (BAO) measurements severely challenge the standard CDM model, while the…

astro-ph.CO2026

Multi-band cross-correlation dark sirens: enhancing cosmological parameter and gravitational-wave bias constraints

Ji-Yu Song, Ya-Nan Du, Yue-Yan Dong +2

Multi-band gravitational-wave (GW) observation, combining space-borne and ground-based detectors across different frequency bands, can improve the sky localization of compact binar…

gr-qc2026

Robust parameter inference for Taiji via time-frequency contrastive learning and normalizing flows

Tian-Yang Sun, Bo Liang, Ji-Yu Song +6

Transient noise artifacts, commonly referred to as glitches, pose a major challenge to parameter inference for space-based gravitational-wave (GW) observations. We develop a glitch…

gr-qc2026

Scalarizations of magnetized Reissner-Nordström black holes induced by parity-violating and parity-preserving interactions

Hao-Jie Lin, Tao Zhu, Jing-Fei Zhang +1

We study spontaneous scalarization of a scalar field in the magnetized Reissner--Nordström spacetime induced by parity-violating and parity-preserving interactions, represented by…

cond-mat.stat-mech2026

Nonequilibrium crossover in the supercritical region from quench dynamics

Zi-Qiang Zhao, Zhang-Yu Nie, Jing-Fei Zhang +1

Distinguishing different subphases in the supercritical region is an important issue in statistical physics and condensed matter physics. Traditional approaches rely mainly on stat…

gr-qc2026

Unifying topological, geometric, and complex classifications of black hole thermodynamics

Shi-Hao Zhang, Shao-Wen Wei, Jing-Fei Zhang +1

Black hole thermodynamics has recently witnessed three distinct classification schemes: based on local geometric properties of the temperature function, global topological invarian…

gr-qc2026

Assessing the robustness of amortized simulation-based inference to transient noise in gravitational-wave ringdowns

Song-Tao Liu, Tian-Yang Sun, Yu-Xin Wang +4

Gravitational waves (GW) emitted by binary systems allow us to perform precision tests of general relativity in the strong field regime. Ringdown signals allow for probing black ho…

astro-ph.CO2026★ 5 cited

Measuring neutrino mass in light of ACT DR6 and DESI DR2

Lu Feng, Tian-Nuo Li, Guo-Hong Du +2

The recent release of high-precision cosmological data, particularly the small-scale cosmic microwave background (CMB) measurements from ACT and baryon acoustic oscillation (BAO) d…

astro-ph.CO2026

Three-band dark-siren cosmology with intermediate mass black hole binaries: Synergy of Taiji, LGWA, and the Einstein Telescope

Ji-Yu Song, Yue-Yan Dong, Shang-Jie Jin +3

Gravitational-wave (GW) dark sirens provide an independent probe of the cosmic expansion history. Their cosmological constraining power, however, depends critically on precise lumi…

astro-ph.CO2026★ 4 cited

Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing

Guo-Hong Du, Tian-Nuo Li, Tonghua Liu +2

General relativity (GR) faces challenges from cosmic acceleration and observational tensions, necessitating stringent tests at cosmological scales. In this work, we probe GR deviat…

astro-ph.IM2026

Factorized neural posterior estimation for rapid and reliable inference of parameterized post-Einsteinian deviation parameters in gravitational waves

Yong-Xin Zhang, Tian-Yang Sun, Chun-Yu Xiong +5

The direct detection of gravitational waves (GWs) by LIGO has confirmed general relativity (GR), but testing GR via GWs requires estimating parameterized post-Einsteinian (ppE) dev…

astro-ph.CO2025

Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra

Tian-Yang Sun, Tian-Nuo Li, He Wang +2

The cosmic microwave background power spectra are a primary window into the early universe. However, achieving interpretable compression and fast inference diagnostics under weak m…

astro-ph.CO2025★ 12 cited

Measuring neutrino masses with joint JWST and DESI DR2 data

Sheng-Han Zhou, Tian-Nuo Li, Guo-Hong Du +3

Early JWST observations reveal an unexpectedly abundant population of high-redshift candidate massive galaxies at , and recent DESI measurements show a preference for…

astro-ph.CO2025★ 24 cited

Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data

Tian-Nuo Li, Peng-Ju Wu, Guo-Hong Du +3

Recent observations of DESI hint that dark matter (DM) may not be cold but have a non-zero equation of state (EoS) parameter, and that dark energy (DE) may not be a cosmological co…

astro-ph.CO2025

Cosmological preference for a positive neutrino mass at 2.7: A joint analysis of DESI DR2, DESY5, and DESY1 data

Guo-Hong Du, Tian-Nuo Li, Peng-Ju Wu +2

Neutrinos and dark energy (DE) have entered a new era of investigation, as the latest DESI baryon acoustic oscillation measurements tighten the constraints on the neutrino mass and…

astro-ph.CO2025★ 8 cited

Testing the cosmic distance duality relation with baryon acoustic oscillations and supernovae data

Tian-Nuo Li, Guo-Hong Du, Peng-Ju Wu +3

One of the most fundamental relationships in modern cosmology is the cosmic distance duality relation (CDDR), which describes the relationship between the angular diameter distance…

astro-ph.CO2025★ 12 cited

Gravitational wave standard sirens: A brief review of cosmological parameter estimation

Shang-Jie Jin, Ji-Yu Song, Tian-Yang Sun +5

Gravitational wave (GW) observations are expected to serve as a powerful and independent probe of the expansion history of the universe. By providing direct and calibration-free me…

gr-qc2025★ 1 cited

Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope

Yue-Yan Dong, Ji-Yu Song, Jing-Fei Zhang +1

Gravitational-wave (GW) detection offers a novel approach to exploring intermediate-mass black holes (IMBHs). The GW signals from IMBH mergers mainly fall in the decihertz frequenc…