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An Integrated GPR B-Scan Preprocessing Model Based on Image Enhancement for Detecting Subsurface Pipes. [PDF]
Sensors (Basel)Shi Z +5 more
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Core Payload of the Space Gravitational Wave Observatory: Inertial Sensor and Its Critical Technologies. [PDF]
Sensors (Basel)Wang S +10 more
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Towards Tsunami Early-Warning with Distributed Acoustic Sensing: Expected Seafloor Strains Induced by Tsunamis. [PDF]
Pure Appl GeophysBecerril C +7 more
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Galaxy Tomography with the Gravitational Wave Background from Supermassive Black Hole Binaries
Chen Y.
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General Relativity and its Applications, 2006
Gravitational waves may reach the Earth in different forms which depend on the nature of the emitting source: they may be short bursts, outcome of a catastrophic event like the gravitational collapse or the coalescence of a binary system; they may be continuous, weak wavetrains emitted by a non axially symmetric, rotating neutron star or by binary ...
V. Ferrari
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Gravitational waves may reach the Earth in different forms which depend on the nature of the emitting source: they may be short bursts, outcome of a catastrophic event like the gravitational collapse or the coalescence of a binary system; they may be continuous, weak wavetrains emitted by a non axially symmetric, rotating neutron star or by binary ...
V. Ferrari
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Evidence for different gravitational-wave sources in the NANOGrav dataset
Physical Review D, 2021 Ligong Bian, Jing Liu, Xing-Yü Yang
exaly +2 more sources
Accurate precision cosmology with redshift unknown gravitational wave sources
Physical Review D, 2021 International audienceGravitational waves can provide an accurate measurement of the luminosity distance to the source but cannot provide the source redshift unless the degeneracy between mass and redshift can be broken.
Suvodip Mukherjee +2 more
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Detection of astrophysical gravitational wave sources by TianQin and LISA
Science China Physics Mechanics and Astronomy, 2023TianQin and LISA are space-based laser interferometer gravitational wave (GW) detectors planned to be launched in the mid-2030s. Both detectors will detect low-frequency GWs around 10−2 Hz; however, TianQin is more sensitive to frequencies above this ...
Alejandro Torres-Orjuela +7 more
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