On networks of space-based gravitational-wave detectors

Fuente: arXiv
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Main Authors: Cai, Rong-Gen, Guo, Zong-Kuan, Hu, Bin, Liu, Chang, Lu, Youjun, Ni, Wei-Tou, Ruan, Wen-Hong, Seto, Naoki, Wang, Gang, Wu, Yue-Liang
Format: Preprint
Published: 2023
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author Cai, Rong-Gen
Guo, Zong-Kuan
Hu, Bin
Liu, Chang
Lu, Youjun
Ni, Wei-Tou
Ruan, Wen-Hong
Seto, Naoki
Wang, Gang
Wu, Yue-Liang
author_facet Cai, Rong-Gen
Guo, Zong-Kuan
Hu, Bin
Liu, Chang
Lu, Youjun
Ni, Wei-Tou
Ruan, Wen-Hong
Seto, Naoki
Wang, Gang
Wu, Yue-Liang
contents The space-based laser interferometers, LISA, Taiji and TianQin, are targeting to observe milliHz gravitational waves (GWs) in the 2030s. The joint observations from multiple space-based detectors yield significant advantages. In this work, we recap the studies and investigations for the joint space-based GW detector networks to highlight: 1) the high precision of sky localization for the massive binary black hole (BBH) coalescences and the GW sirens in the cosmological implication, 2) the effectiveness to test the parity violation in the stochastic GW background observations, 3) the efficiency of subtracting galactic foreground, 4) the improvement in stellar-mass BBH observations. We inspect alternative networks by trading off massive BBH observations and stochastic GW background observation.
format Preprint
id arxiv_https___arxiv_org_abs_2305_04551
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle On networks of space-based gravitational-wave detectors
Cai, Rong-Gen
Guo, Zong-Kuan
Hu, Bin
Liu, Chang
Lu, Youjun
Ni, Wei-Tou
Ruan, Wen-Hong
Seto, Naoki
Wang, Gang
Wu, Yue-Liang
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
The space-based laser interferometers, LISA, Taiji and TianQin, are targeting to observe milliHz gravitational waves (GWs) in the 2030s. The joint observations from multiple space-based detectors yield significant advantages. In this work, we recap the studies and investigations for the joint space-based GW detector networks to highlight: 1) the high precision of sky localization for the massive binary black hole (BBH) coalescences and the GW sirens in the cosmological implication, 2) the effectiveness to test the parity violation in the stochastic GW background observations, 3) the efficiency of subtracting galactic foreground, 4) the improvement in stellar-mass BBH observations. We inspect alternative networks by trading off massive BBH observations and stochastic GW background observation.
title On networks of space-based gravitational-wave detectors
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2305.04551