Results 31 to 40 of about 4,299 (279)
TESTING RELATIVISTIC GRAVITY AND DETECTING GRAVITATIONAL WAVES IN SPACE [PDF]
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
REVIEW OF GRAVITATIONAL WAVE DETECTIONS: DYNAMICAL SPACE [PDF]
This is a review of the numerous successful gravitational wave detections and the implications for the nature of space and time. The prevailing space time paradigm in physics was founded on the putative “null” results of the Michelson-Morley (MM) 1887 interferometer experiment to detect light speed anisotropy and which resulted in two different new ...
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Automatic amplitude control for phasemeter of spaceborne laser interferometry
Laser interferometry of the space gravitational wave antenna needs to demodulate the gravitational wave signal by a phasemeter with high phase readout precision.
Hao-Jie Li +6 more
doaj +1 more source
Space missions to detect the cosmic gravitational-wave background [PDF]
22 pages, 7 figures, IOP style, References ...
Cornish, Neil J., Larson, Shane L.
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The space gravitational wave detection mission has put forward multiple performance requirements for micro-newton thrusters, such as “fast response, high resolution, and low noise”. In order to solve the problem that the traditional open-loop
Hongbo Zhou +4 more
core +1 more source
Laser acquisition experimental demonstration for space gravitational wave detection missions
The laser acquisition-pointing technique is one of the most important techniques for space gravitational wave detection missions, like the Taiji program and the LISA (Laser Interferometer Space Antenna) program. The laser acquisition system suppresses the laser deviation angle to 1 µrad at the receiving aperture.
Ruihong, Gao +5 more
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In space laser interferometer gravitational wave (G. W.) detection missions, the stability of the laser beam pointing direction has to be kept at 10 nrad/root Hz.
李玉琼 +5 more
core +1 more source
We study the observation of a stochastic gravitational-wave background (SGWB) made by a pulsar-timing array in the spherical harmonic space of the observable. The observable is a timing residual which is the time-averaged redshift fluctuation of a pulsar
Liu, Guo-Chin;Ng, Kin-Wang
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Phase transition gravitational waves from pseudo-Nambu-Goldstone dark matter and two Higgs doublets
We investigate the potential stochastic gravitational waves from first-order electroweak phase transitions in a model with pseudo-Nambu-Goldstone dark matter and two Higgs doublets.
Zhao Zhang +5 more
doaj +1 more source
Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
On 11 February 2016, the LIGO and Virgo scientific collaborations announced the first direct detection of gravitational waves, a signal caught by the LIGO interferometers on 14 September 2015, and produced by the coalescence of two stellar-mass black ...
Mario Spera +2 more
doaj +1 more source

