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• W4384204559 abstract "In this paper, we carry out a systematic study of the prospect of testing general relativity with the inspiral signals of black hole binaries that could be detected with TianQin. The study is based on the parameterized post-Einsteinian (ppE) waveform, so that many modified gravity theories can be covered simultaneously. We consider black hole binaries with total masses ranging from $10rm M_odotsim10^7 M_odot$ and ppE corrections at post-Newtonian (PN) orders ranging from $-4$PN to $2$PN. Compared to the current ground-based detectors, TianQin can improve the constraints on the ppE phase parameter $beta$ by orders of magnitude. For example, the improvement at the $-4$PN and $2$PN orders can be about $13$ and $3$ orders of magnitude (compared to the results from GW150914), respectively. Compared to future ground-based detectors, such as ET, TianQin is expected to be superior below the $-1$PN order, and for corrections above the $-0.5$PN order, TianQin is still competitive near the large mass end of the low mass range $[10 rm M_odot, ,10^3 rm M_odot],$. Compared to the future space-based detector LISA, TianQin can be competitive in the lower mass end as the PN order is increased. For example, at the $-4$PN order, LISA is always superior for sources more massive than about $30rm M_odot,$, while at the $2$PN order, TianQin becomes competitive for sources less massive than about $10^4rm M_odot$. We also study the scientific potentials of detector networks involving TianQin, LISA and ET, and discuss the constraints on specific theories such as the dynamic Chern-Simons theory and the Einstein-dilaton Gauss-Bonnet theory." @default.
• W4384204559 created "2023-07-14" @default.
• W4384204559 creator A5011509922 @default.
• W4384204559 creator A5034005804 @default.
• W4384204559 creator A5050571932 @default.
• W4384204559 creator A5084257939 @default.
• W4384204559 date "2023-07-13" @default.
• W4384204559 modified "2023-10-05" @default.
• W4384204559 title "Testing general relativity with TianQin: The prospect of using the inspiral signals of black hole binaries" @default.
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• W4384204559 doi "https://doi.org/10.1103/physrevd.108.024030" @default.

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