activity
20192026
most citedConstraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

126 citations · 835 across the 28 of their papers we have counts for

collaborators

28 papers

gr-qc2026

Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection

Tian-Yang Sun, Yue Niu, Chun-Yan Jiang +3

Gravitational-wave astronomy has opened a direct observational window onto compact-object dynamics, strong-field gravity, and cosmology. Among the transient sources accessible thro…

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

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

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.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.CO2026

Simultaneous determination of Hubble constant and cosmic baryon density: Forecasts for the synergy between FRBs and emerging probes

Peng-Ju Wu, Bo-Yang Zhang, Ji-Guo Zhang +3

Two of the most pressing challenges in cosmology are the persistent discrepancy in measurements of the Hubble constant, referred to as the Hubble tension, and the deficit of baryon…

astro-ph.CO2025★ 5 cited

How Dark Sector Equations of State Govern Interaction Signatures

Peng-Ju Wu, Ming Zhang, Shang-Jie Jin

Using late-Universe observations, we demonstrate that freeing dark energy and dark matter equations of state (EoS) dramatically alters the inferred strength and direction of their…

astro-ph.CO2025★ 1 cited

Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies

Ya-Nan Du, Ji-Yu Song, Yichao Li +4

Gravitational-wave (GW) events are generally believed to originate in galaxies and can thus serve, like galaxies, as tracers of the universe's large-scale structure. In GW observat…

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…

astro-ph.CO2025★ 49 cited

Probing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data

Tian-Nuo Li, Guo-Hong Du, Yun-He Li +4

There is a possibility of interaction between dark energy and dark matter, and this interaction may also undergo a sign change during the evolution of the universe. In this paper,…

gr-qc2024★ 2 cited

Search for exotic gravitational wave signals beyond general relativity using deep learning

Yu-Xin Wang, Xiaotong Wei, Chun-Yue Li +6

The direct detection of gravitational waves by LIGO has confirmed general relativity (GR) and sparked rapid growth in gravitational wave (GW) astronomy. However, subtle post-Newton…

astro-ph.CO2024★ 126 cited

Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

Tian-Nuo Li, Peng-Ju Wu, Guo-Hong Du +4

The recent results from the first year baryon acoustic oscillations (BAO) data released by the Dark Energy Spectroscopic Instrument (DESI), combined with cosmic microwave backgroun…

astro-ph.CO2024★ 3 cited

Enhancing dark siren cosmology through multi-band gravitational wave synergetic observations

Yue-Yan Dong, Ji-Yu Song, Shang-Jie Jin +2

Multi-band gravitational-wave (GW) standard siren observations are poised to herald a new era in the study of cosmic evolution. These observations offer higher signal-to-noise rati…

gr-qc2023★ 21 cited

Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow

Tian-Yang Sun, Chun-Yu Xiong, Shang-Jie Jin +3

Glitches represent a category of non-Gaussian and transient noise that frequently intersects with gravitational wave (GW) signals, exerting a notable impact on the processing of GW…

astro-ph.CO2023★ 39 cited

Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation

Tian-Nuo Li, Shang-Jie Jin, Hai-Li Li +2

Gravitational wave (GW) standard siren observations provide a rather useful tool to explore the evolution of the Universe. In this work, we wish to investigate whether dark sirens…

astro-ph.CO2023★ 25 cited

A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short -ray bursts

Tao Han, Shang-Jie Jin, Jing-Fei Zhang +1

In the third-generation (3G) gravitational-wave (GW) detector era, the multi-messenger GW observation for binary neutron star (BNS) merger events can exert great impacts on explori…

astro-ph.CO2023★ 15 cited

Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO

Shang-Jie Jin, Rui-Qi Zhu, Ji-Yu Song +3

The 2.5-generation (2.5G) ground-based gravitational wave (GW) detectors LIGO Voyager and NEMO are expected to be operational in the late 2020s and early 2030s. In this work, we ex…

astro-ph.CO2023★ 51 cited

The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens

Shang-Jie Jin, Ye-Zhu Zhang, Ji-Yu Song +2

In the coming decades, the space-based gravitational-wave (GW) detectors such as Taiji, TianQin, and LISA are expected to form a network capable of detecting millihertz GWs emitted…

gr-qc2023★ 10 cited

Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning

Yu-Xin Wang, Shang-Jie Jin, Tian-Yang Sun +2

Recent developments in deep learning techniques have offered an alternative and complementary approach to traditional matched filtering methods for the identification of gravitatio…

astro-ph.CO2023★ 32 cited

Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations

Shang-Jie Jin, Shuang-Shuang Xing, Yue Shao +2

Gravitational waves (GWs) from the compact binary coalescences can be used as standard sirens to explore the cosmic expansion history. In the next decades, it is anticipated that w…

astro-ph.CO2022★ 42 cited

Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models

Shang-Jie Jin, Rui-Qi Zhu, Ling-Feng Wang +3

The multi-messenger gravitational-wave (GW) observation for binary neutron star merger events could provide a rather useful tool to explore the evolution of the universe. In partic…

gr-qc2022★ 43 cited

Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation

Shang-Jie Jin, Tian-Nuo Li, Jing-Fei Zhang +1

Using the measurements of tidal deformation in the binary neutron star (BNS) coalescences can obtain the information of redshifts of gravitational wave (GW) sources, and thus actua…

astro-ph.CO2022★ 41 cited

A path to precision cosmology: synergy between four promising late-universe cosmological probes

Peng-Ju Wu, Yue Shao, Shang-Jie Jin +1

In the next decades, it is necessary to forge new late-universe cosmological probes to precisely constrain the Hubble constant and the equation of state of dark energy simultaneous…

astro-ph.CO2021★ 57 cited

How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?

Shang-Jie Jin, Ling-Feng Wang, Peng-Ju Wu +2

In the next decades, the gravitational-wave (GW) standard siren observations and the neutral hydrogen 21-cm intensity mapping (IM) surveys, as two promising cosmological probes, wi…