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Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation
Han Wang, Ian Harry, Alexander Nitz +1
The measurement of eccentricity would provide strong constraints on the formation channel of stellar-mass binary black holes. However, current ground-based gravitational wave detec…
Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes
Shuai Liu, Yi-Ming Hu, Jian-dong Zhang +1
We study the prospect of using TianQin to detect stellar-mass binary black holes (SBBHs). We estimate the expected detection number as well as the precision of parameter estimation…
Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals
Hui-Min Fan, Yi-Ming Hu, Enrico Barausse +5
Systems consisting of a massive black hole and a stellar-origin compact object (CO), known as extreme-mass-ratio inspirals (EMRIs), are of great significance for space-based gravit…
Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries
Shun-Jia Huang, Yi-Ming Hu, Valeriya Korol +6
We explore the prospects of detecting of Galactic double white dwarf (DWD) binaries with the space-based gravitational wave (GW) observatory TianQin. In this work, we analyze both…
Science with the TianQin observatory: Preliminary results on massive black hole binaries
Hai-Tian Wang, Zhen Jiang, Alberto Sesana +8
We investigate the prospects of detecting gravitational waves from coalescing massive black hole binaries in the Universe with the TianQin observatory, a space-based gravitational…
Gravitational waves induced by the asymmetric jets of gamma-ray bursts
Shuang Du, Xiao-Dong Li, Yi-Ming Hu +2
We study the gravitational wave (GW) production induced by the asymmetric jets of gamma-ray bursts (GRBs). The asymmetric jets result in a recoil force acted on the central compact…
Hearing the birth of the lightest intermediate mass black holes with the second generation gravitational wave detectors
Yun-Feng Liang, Yuan-Zhu Wang, Hao Wang +6
Intermediate mass black holes (IMBHs) with a mass between and times that of the sun, which bridges the {mass gap between the} stellar-mass black holes and the sup…
Neutron star-black hole coalescence rate inferred from macronova/kilonova observations
Xiang Li, Yi-Ming Hu, Zhi-Ping Jin +2
Neutron starblack hole (NSBH) coalescences are widely believed to be promising gravitational wave sources in the era of advanced detectors of LIGO/Virgo but such binaries hav…
GRB/GW association: Long-short GRB candidates, time-lag, measuring gravitational wave velocity and testing Einstein's equivalence principle
Xiang Li, Yi-Ming Hu, Yi-Zhong Fan +1
Short-duration gamma-ray bursts (SGRBs) are widely believed to be powered by the mergers of compact binaries, such as binary neutron stars or possibly neutron star-black hole binar…
Maximising the detection probability of kilonovae associated with gravitational wave observations
Man Leong Chan, Yi-Ming Hu, Chris Messenger +2
Estimates of the source sky location for gravitational wave signals are likely span areas ranging up to hundreds of square degrees or more, making it very challenging for most tele…
Glitch or Anti-Glitch: a Bayesian View
Yi-Ming Hu, Matthew Pitkin, Ik Siong Heng +1
The sudden spin-down in the rotation of magnetar 1E 2259+586 observed by Archibald et al. (2013) was a rare event. However this particular event, referred to as an anti-glitch, was…