90 citations · 393 across the 12 of their papers we have counts for
12 papers
Two-Dimensional Pulsar Distance Inference from Nanohertz Gravitational Waves
Si-Ren Xiao, Ji-Yu Song, Yue Shao +3
Pulsar timing arrays (PTAs) are limited in localizing nanohertz continuous gravitational waves (CGWs) by uncertainties in pulsar distances. We introduce a method to infer pulsar di…
Nanohertz gravitational waves from a quasar-based supermassive black hole binary population model as dark sirens
Si-Ren Xiao, Yue Shao, Ling-Feng Wang +4
Recently, several pulsar timing array (PTA) projects have detected evidence of the existence of a stochastic gravitational wave background (SGWB) in the nanohertz frequency band, p…
Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
Ji-Yu Song, Ling-Feng Wang, Yichao Li +4
Gravitational waves (GWs) from compact binary coalescences encode the absolute luminosity distances of GW sources. Once the redshifts of GW sources are known, one can use the dista…
Probing the interaction between dark energy and dark matter with future fast radio burst observations
Ze-Wei Zhao, Ling-Feng Wang, Ji-Guo Zhang +2
Interacting dark energy (IDE) scenario assumes that there exists a direct interaction between dark energy and cold dark matter, but this interaction is hard to be tightly constrain…
Prospects for constraining interacting dark energy cosmology with gravitational-wave bright sirens detected by future SKA-era pulsar timing arrays
Bo Wang, Dong-Ze He, Ling-Feng Wang +2
We explore the constraints on cosmological parameters in interacting dark energy (IDE) models described by energy transfer rates and , using s…
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…
Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
Ling-Feng Wang, Yue Shao, Si-Ren Xiao +2
Ultra-low-frequency gravitational waves (GWs) generated by individual inspiraling supermassive black hole binaries (SMBHBs) at the centers of galaxies may be detected by pulsar tim…
A forecast of using fast radio burst observations to constrain holographic dark energy
Xing-Wei Qiu, Ze-Wei Zhao, Ling-Feng Wang +2
Recently, about five hundred fast radio bursts (FRBs) detected by CHIME/FRB Project have been reported. The vast amounts of data would make FRBs a promising low-redshift cosmologic…
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…
Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
Ling-Feng Wang, Jie-Hao Zhang, Dong-Ze He +2
Measurements of time-delay cosmography of lensed quasars can provide an independent probe to explore the expansion history of the late-time Universe. In this paper, we employ the t…
Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
Ling-Feng Wang, Xuan-Neng Zhang, Jing-Fei Zhang +1
We investigate the impacts of the gravitational-wave (GW) standard siren observation of the Einstein Telescope (ET) on constraining the total neutrino mass. We simulate 1000 GW eve…
A closer look at interacting dark energy with statefinder hierarchy and growth rate of structure
Jing-Lei Cui, Lu Yin, Ling-Feng Wang +2
We investigate the interacting dark energy models by using the diagnostics of statefinder hierarchy and growth rate of structure. We wish to explore the deviations from CDM and…