Perceiving deci-Hertz gravitational waves over the Moon

Shao, Lijing

doi:10.1007/s11433-023-2215-4

Sci. China Phys. Mech. Astron.

2023

DOI: 10.1007/s11433-023-2215-4

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Perceiving deci-Hertz gravitational waves over the Moon

Lijing Shao

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2024

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Cited by 3 publications

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Prospects for detecting neutron star–white dwarf mergers with decihertz gravitational-wave observatories

Kang,

Liu,

Zhu

et al. 2024

Monthly Notices of the Royal Astronomical Society

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Based on different neutron star–white dwarf (NS-WD) population models, we investigate the prospects of gravitational-wave (GW) detections for NS-WD mergers, with the help of early warnings from two space-borne decihertz GW observatories, DO-Optimal and DECIGO. We not only give quick assessments of the GW detection rates for NS-WD mergers with the two decihertz GW detectors, but also report systematic analyses on the characteristics of GW-detectable merger events using the method of Fisher matrix. With a sufficient one-day early-warning time, the yearly GW detection number for DO-Optimal is in the range of (1.5–1.9) × 103, while it is (3.3–4.6) × 104 for DECIGO. More importantly, our results show that most NS-WD mergers can be localized with an uncertainty of $\mathcal {O}(10^{-2})\, \mathrm{deg}^2$. Given the NS-WD merger as a possible origin for a peculiar long-duration gamma-ray burst, GRB 211211A, followed with kilonova-like emissions, we further suggest that the GW early-warning detection would allow future electromagnetic telescopes to get prepared to follow-up transients after some special NS-WD mergers. Based on our analyses, we emphasize that such a feasible ‘wait-for’ pattern can help to firmly identify the origin of GRB 211211A-like events in the future and bring excellent opportunities for the multimessenger astronomy.

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Prospects for detecting neutron star–white dwarf mergers with decihertz gravitational-wave observatories

Kang,

Liu,

Zhu

et al. 2024

Monthly Notices of the Royal Astronomical Society

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Research progress on clock noise suppression technique for space-borne gravitational wave detection

XU,

TAN,

SHAO

2024

Sci. Sin.-Phys. Mech. Astron.

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Identification and extraction of gravitational-wave signals of Galactic compact binaries

ShaoDong,

XueHao,

YiYang

et al. 2024

Sci. Sin.-Phys. Mech. Astron.

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Perceiving deci-Hertz gravitational waves over the Moon

Cited by 3 publications

References 5 publications

Prospects for detecting neutron star–white dwarf mergers with decihertz gravitational-wave observatories

Prospects for detecting neutron star–white dwarf mergers with decihertz gravitational-wave observatories

Research progress on clock noise suppression technique for space-borne gravitational wave detection

Identification and extraction of gravitational-wave signals of Galactic compact binaries

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