Results 251 to 260 of about 15,075 (298)

Exploring the extremes: The cosmic laboratory. [PDF]

Innovation (Camb)
Huang Y, He S, Ge L, Li Z, Mao Y, Liu J.
europepmc   +1 more source

Emergence of Calabi-Yau manifolds in high-precision black-hole scattering. [PDF]

Nature
Driesse M, Jakobsen GU, Klemm A, Mogull G, Nega C, Plefka J, Sauer B, Usovitsch J.   +7 more
europepmc   +1 more source

Research on Interferometric Tilt Sensor for Vibration Isolation Platform. [PDF]

Sensors (Basel)
Bai W, Feng W, Wang P, Zhang Z, Zhao G.
europepmc   +1 more source

Extracting overlapping gravitational-wave signals of Galactic compact binaries: A mini review. [PDF]

Fundam Res
Niu R, Zhao W.
europepmc   +1 more source

Reducing Risks in Petrochemical Plants Through the Integration of Existing and Emerging Gas Leak Detection Technologies. [PDF]

Sensors (Basel)
Lee JH, Lim SY, Lee JJ, Shin H, Kim Y, Kim I.   +5 more
europepmc   +1 more source

Signatures of correlation of spacetime fluctuations in laser interferometers. [PDF]

Nat Commun
Sharmila B, Vermeulen SM, Datta A.
europepmc   +1 more source

Low Temperature and Gravitation Wave Detectors

, 2014
The success of a precision experiment is often associated to the use of low temperature techniques. In particular, when the thermal noise is a barrier for improving the experiment sensitivity, the cryogenics is crucial for beating this limitation. This strategy was applied in the case of the resonant gravitational wave detectors (GW) and now it is ...
RICCI, Fulvio
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Resonant detectors for gravitational waves

Advances in Space Research, 2000
Abstract For the first time a number of cryogenic resonant bar detectors of gravitational waves — ALLEGRO, AURIGA, EXPLORER, NAUTILUS, NIOBE — are on the air, in a continuous search for impulsive events. We present their capabilities, the foreseen upgrades and their role in a future global network with interferometric detectors.
L. Baggio, M. Cerdonio, V. Crivelli Visconti, L. Taffarello, J. Zendri, Prodi, Giovanni Andrea, L. Conti, Mezzena, Renato, Vitale, Stefano, M. Bonaldi, P. Falferi, V. Martinucci, A. Ortolan, G. Vedovato, P. Fortini   +14 more
openaire   +3 more sources

Stabilized lasers for advanced gravitational wave detectors

Laser and Photonics Reviews, 2010
Second-generation interferometric gravitational wave detectors require high-power lasers with approximately 200 W of output power in a linear polarized, single-frequency, fundamental-mode laser beam.
B Willke
exaly   +3 more sources

The Virgo Gravitational Wave Detector

Frontiers in Optics 2009/Laser Science XXV/Fall 2009 OSA Optics & Photonics Technical Digest, 2009
The interferometer spectral-density of resolution is 6 x 10-231/ √HZ at 250 Hz.. We show the performances of mirror surfaces and coatings, laser frequency and amplitude stabilizations, interferometer control. We discuss advanced Virgo optical-technologies.
openaire   +2 more sources