Advanced Gravitational Wave Detectors
D. G. Blair
Cambridge University Press, Feb 16, 2012 - Science - 321 pages
After decades of research, physicists now know how to detect Einstein's gravitational waves. Advanced gravitational wave detectors, the most sensitive instruments ever created, will be almost certain of detecting the births of black holes throughout the Universe. This book describes the physics of gravitational waves and their detectors. The book begins by introducing the physics of gravitational wave detection and the likely sources of detectable waves. Case studies on the first generation of large scale gravitational wave detectors introduce the technology and set the scene for a review of the experimental issues in creating advanced detectors in which the instrument's sensitivity is limited by Heisenberg's uncertainty principle. The book covers lasers, thermal noise, vibration isolation, interferometer control and stabilisation against opto-acoustic instabilities. This is a valuable reference for graduate students and researchers in physics and astrophysics entering this field.
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Part 2 Current laser interferometer detectors three case studies
Part 3 Technology for advanced gravitationalwave detectors
Part 4 Technology for third generation gravitational wave detectors
achieved acoustic modes actuators advanced detectors Advanced LIGO amplitude angular antenna arm cavities Astrophys band bandwidth beam splitter binary black hole carrier Classical and Quantum coalescence coating coupling cryogenic degrees of freedom density detection detection band detuning displacement energy equation Fabry–Perot factor feedback filtering fluctuations frequency range fused silica gravitational wave detectors GW detectors input instability laser interferometer LCGT length Lett light power lock loss low frequency measurement mechanical Michelson mode cleaner modulation motion neutron stars observatory optical cavities optical power oscillator output parameters pendulum phase phase quadrature photodiode Phys polarisation power recycling pulsar Q-factor Quantum Gravity quantum noise radiation pressure readout recycling cavity recycling mirror reduce resonant sensitivity shadow sensors shot noise sidebands signal recycling sources stabilisation stage substrate supernova suspension techniques temperature test mass thermal lensing thermal noise vacuum Virgo waveform wavelength