Results 21 to 30 of about 7,690,788 (272)
Rapid search for massive black hole binary coalescences using deep learning
Physics Letters B, 2023 The coalescences of massive black hole binaries are one of the main targets of space-based gravitational wave observatories. Such gravitational wave sources are expected to be accompanied by electromagnetic emissions. Low latency detection of the massive
Wen-Hong Ruan +3 more
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A joint search for gravitational wave bursts with AURIGA and LIGO [PDF]
, 2008 The first simultaneous operation of the AURIGA detector* and the LIGO observatory* was an opportunity to explore real data, joint analysis methods between two very different types of gravitational wave detectors: resonant bars and interferometers.
Cantley, C. A. +5 more
core +2 more sources
Search for gravitational-wave bursts in LIGO data from the fourth science run [PDF]
, 2007 The fourth science run of the LIGO and GEO 600 gravitational-wave detectors, carried out in early 2005, collected data with significantly lower noise than previous science runs.
Abbott, B. +4 more
core +2 more sources
Applied Sciences, 2022 Space-based gravitational wave detection programs, such as the Laser Interferometer Space Antenna (LISA) or Taiji program, obtain gravitational wave signals by measuring the change in the distance between three satellites by laser.
Zhiwei Chen +4 more
doaj +1 more source
Gravitational wave detection in space [PDF]
International Journal of Modern Physics D, 2016 Gravitational Wave (GW) detection in space is aimed at low frequency band (100[Formula: see text]nHz–100[Formula: see text]mHz) and middle frequency band (100[Formula: see text]mHz–10[Formula: see text]Hz). The science goals are the detection of GWs from (i) Supermassive Black Holes; (ii) Extreme-Mass-Ratio Black Hole Inspirals; (iii) Intermediate ...
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Configuration Stability Analysis for Geocentric Space Gravitational-Wave Observatories
Aerospace, 2022 Long-term configuration stability is essential for a space-based gravitational-wave observatory, which can be affected by orbit insertion errors. This paper investigated the stability of a geocentric gravitational-wave observatory from the view of the ...
Xingyu Zhou, Feida Jia, Xiangyu Li
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Aerospace, 2023 Since deep space exploration tasks, such as space gravitational wave detection, put forward increasingly higher requirements for the satellite platform, the scale and complexity of the satellite management unit (SMU) software are also increasing, and the
Lu Li +5 more
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Concepts and status of Chinese space gravitational wave detection projects [PDF]
Nature Astronomy, 2021 Gravitational wave (GW) detection in space probes GW spectrum that is inaccessible from the Earth. In addition to LISA project led by European Space Agency, and the DECIGO detector proposed by the Japan Aerospace Exploration Agency, two Chinese space-based GW observatories -- TianQin and Taiji -- are planned to be launched in the 2030s.
Yungui Gong, Jun Luo, Bin Wang
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Applied Sciences, 2023 We present a low-intensity noise single-frequency Yb-doped all-fiber amplifier oriented to space-borne gravitational wave detection. Relative intensity noise (RIN) below −70 dBc/Hz @ 1 mHz~1 Hz was achieved by virtue of feedback-loop-based intensity ...
Zaiyuan Wang +5 more
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TESTING RELATIVISTIC GRAVITY AND DETECTING GRAVITATIONAL WAVES IN SPACE [PDF]
Gravitation and Astrophysics, 2010 8 pages, 1 figure, invited presentation for the Ninth Asia-Pacific International Conference on Gravitation and Astrophysics (ICGA9), Wuhan, June 28-July 3, 2009; for the proceedings to be published by World ...
openaire +2 more sources