activity
20222025
most citedGravitational Wave Astronomy With TianQin

56 citations · 112 across the 16 of their papers we have counts for

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Showing 2024Show all

8 papers · 1 filter

astro-ph.GA2024★ 2 cited

Signal-to-noise Ratio Analytic Formulae of the Inspiral Binary Black Holes in TianQin

Hong-Yu Chen, Han Wang, En-Kun Li +1

Binary black holes are one of the important sources for the TianQin gravitational wave project. Our research has revealed that, for TianQin, the signal-to-noise ratio of inspiral b…

gr-qc2024

Mapping Anisotropies in the Stochastic Gravitational-Wave Background with TianQin

Zhi-Yuan Li, Zheng-Cheng Liang, En-Kun Li +2

In the milli-Hertz frequency band, stochastic gravitational-wave background can be composed of both astronomical and cosmological sources, both can be anisotropic. Numerically depi…

astro-ph.GA2024★ 56 cited

Gravitational Wave Astronomy With TianQin

En-Kun Li, Shuai Liu, Alejandro Torres-Orjuela +50

The opening of the gravitational wave window has significantly enhanced our capacity to explore the universe's most extreme and dynamic sector. In the mHz frequency range, a divers…

gr-qc2024

Unveiling a multi-component stochastic gravitational-wave background with the TianQin + LISA network

Zheng-Cheng Liang, Zhi-Yuan Li, En-Kun Li +2

Space-borne detectors, including TianQin and Laser Interferometry Space Antenna (LISA), are tasked with simultaneously observing the Galactic foreground, astrophysical and cosmolog…

gr-qc2024★ 6 cited

Dealing with data gaps for TianQin with massive black hole binary signal

Lu Wang, Hong-Yu Chen, Xiangyu Lyu +2

Space-borne gravitational wave detectors like TianQin might encounter data gaps due to factors like micrometeoroid collisions or hardware failures. Such events will cause discontin…

gr-qc2024

Revisiting Stochastic Gravitational-wave Background in the Strong Signal Case

Zheng-Cheng Liang, Zhi-Yuan Li, En-Kun Li +2

Weak-signal limit is often used in estimating stochastic gravitational-wave background (SGWB) intensities. This approximation fails and the signal-to-noise ratio (SNR) can be much…

astro-ph.CO2024

An Opacity-Free Method of Testing the Cosmic Distance Duality Relation Using Strongly Lensed Gravitational Wave Signals

Shun-Jia Huang, En-Kun Li, Jian-dong Zhang +4

The cosmic distance duality relation (CDDR), expressed as DL(z) = (1 + z)2DA(z), plays an important role in modern cosmology. In this paper, we propose a new method of testing CDDR…

astro-ph.GA2024★ 1 cited

Bayesian parameter estimation of massive black hole binaries with TianQin-LISA

Jie Gao, Yi-Ming Hu, En-Kun Li +2

This paper analyses the impact of various parameter changes on the estimation of parameters for massive black hole binary (MBHB) systems using a Bayesian inference technique. Sever…