Available:*
Library | Item Barcode | Call Number | Material Type | Item Category 1 | Status |
---|---|---|---|---|---|
Searching... | 30000010328420 | QB117 A38 2012 | Open Access Book | Book | Searching... |
On Order
Summary
Summary
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.
Table of Contents
Part I An Introduction to Gravitational Wave Astronomy and Detectors |
1 Gravitational wavesD. G. Blair and L. Ju and C. Zhao and E. J. Howell |
2 Sources of gravitational wavesD. G. Blair and E. J. Howell |
3 Gravitational wave detectorsD. G. Blair and L. Ju and C. Zhao and H. Miao and E. J. Howell and P. Barriga |
4 Gravitational wave data analysisB. S. Sathyaprakash and B. F. Schutz |
5 Network analysisL. Wen and B. F. Schutz |
Part II Current Laser Interferometer Detectors: Three Case Studies |
6 The Laser Interferometer Gravitational-Wave ObservatoryP. Fritschel |
7 The VIRGO detectorS. Braccini |
8 GEO 600H. Lück and H. Grote |
Part III Technology for Advanced Gravitational Wave Detectors |
9 Lasers for high optical power interferometersB. Willke and M. Frede |
10 Thermal noise, suspensions and test massesL. Ju and G. Harry and B. Lee |
11 Vibration isolation |
Part 1 Seismic isolation for advanced LIGOB. Lantz |
Part 2 Passive isolationJ-C. Dumas |
12 Interferometer sensing and controlP. Barriga |
13 Stabilizing interferometers against high optical power effectsC. Zhao and L. Ju and S. Gras and D. G. Blair |
Part IV Technology for Third Generation Gravitational Wave Detectors |
14 Cryogenic interferometersJ. Degallaix |
15 Quantum theory of laser-interferometer GW detectorsH. Miao and Y. Chen |
16 ET. A third generation observatoryM. Punturo and H. Lück |
Index |