Detecting gravitational wave with an interferometric seismometer array on lunar nearside

Li, Junlang; Liu, Fangfei; Pan, Yuan; Wang, Zijian; Cao, Mengdi; Wang, Mengyao; Zhang, Fan; Zhang, Jinhai; Zhu, Zong-Hong

doi:10.1007/s11433-023-2179-9

Cited by 12 publications

(2 citation statements)

References 81 publications

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“…The detection of the gravitational waves by Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo [32] and the first picture of the black hole by Event Horizon Telescope (EHT) [33] label that we have entered the multi-messenger astronomy. The study on the gravitational waves and black hole shadows have been attracted a lot of attentions [34][35][36][37][38][39][40][41]. For the gravitational waves of a binary black hole merger system, there are three parts: inspiral, merger, and ringdown.…”

Section: Jcap07(2024)008mentioning

confidence: 99%

Quasinormal modes and greybody factor of a Lorentz-violating black hole

Guo,

Tan,

Liu

2024

J. Cosmol. Astropart. Phys.

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Recently, a static spherically symmetric black hole solution was found in gravity nonminimally coupled a background Kalb-Ramond field. The Lorentz symmetry is spontaneously broken when the Kalb-Ramond field has a nonvanishing vacuum expectation value. In this work, we focus on the quasinormal modes and greybody factor of this black hole. The master equations for the perturbed scalar field, electromagnetic field, and gravitational field can be written into a Schrödinger equation. We use three methods to solve the quasinormal frequencies in the frequency domain. The results agree well with each other. The time evolution of a Gaussian wave packet is studied. The quasinormal frequencies fitted from the time evolution data agree well with that of frequency domain. The greybody factor is calculated by Wentzel-Kramers-Brillouin (WKB) method. The effect of the Lorentz-violating parameter on the quasinormal modes and greybody factor are also studied.

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Section: Jcap07(2024)008mentioning

confidence: 99%

Quasinormal modes and greybody factor of a Lorentz-violating black hole

Guo,

Tan,

Liu

2024

J. Cosmol. Astropart. Phys.

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“…Following opportunities to submit mission ideas to NASA and ESA calls, three new concepts were proposed in 2020: the Lunar GW Antenna (LGWA) [5], the Lunar Seismic and Gravitational Antenna (LSGA) [6] and the Gravitational-wave Lunar Observatory for Cosmology (GLOC) [7], soon followed by a study of a concept similar to GLOC called LION [8]. Another concept similar to LGWA was recently proposed using a different sensor technology [9]. The LGWA and LSGA concepts exploit the response of the Moon to GWs, while GLOC and LION work like the Virgo/LIGO detectors on Earth [10,11].…”

Section: Introductionmentioning

confidence: 99%

Opportunities and limits of lunar gravitational-wave detection

Cozzumbo,

Mestichelli,

Mirabile

et al. 2024

Phil. Trans. R. Soc. A.

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A new era of lunar exploration has begun with participation of all major space agencies. This activity brings opportunities for revolutionary science experiments and observatories on the Moon. The idea of a lunar gravitational-wave detector was already proposed during the Apollo programme. The key characteristic of the Moon is that it is seismically extremely quiet. It was also pointed out that the permanently shadowed regions at the lunar poles provide ideal conditions for gravitational-wave detection. In recent years, three different detector concepts were proposed with varying levels of technological complexity and science potential. In this paper, we confront the three concepts in terms of their observational capabilities based on a first more detailed modelling of instrumental noise. We identify important technological challenges and potential show-stoppers. This article is part of a discussion meeting issue ‘Astronomy from the Moon: the next decades (part 2)’.

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Perceiving deci-Hertz gravitational waves over the Moon

Shao

2023

Sci. China Phys. Mech. Astron.

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Detecting gravitational wave with an interferometric seismometer array on lunar nearside

Cited by 12 publications

References 81 publications

Quasinormal modes and greybody factor of a Lorentz-violating black hole

Quasinormal modes and greybody factor of a Lorentz-violating black hole

Opportunities and limits of lunar gravitational-wave detection

Perceiving deci-Hertz gravitational waves over the Moon

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