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950621s1994 si a b 001 0 eng d |
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|a 95132527
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|a 9810218206
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|a (ICU)BID20273316
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|a (OCoLC)31810611
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|a MdBSTS
|c MdBSTS
|d IU
|d DLC
|d OrLoB-B
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|a eng
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|a lccopycat
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|a QC179
|b .S28 1994
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| 100 |
1 |
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|a Saulson, Peter R.
|0 http://id.loc.gov/authorities/names/n95033134
|1 http://viaf.org/viaf/71492681
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| 245 |
1 |
0 |
|a Fundamentals of interferometric gravitational wave detectors /
|c Peter R. Saulson.
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| 260 |
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|a Singapore ;
|a River Edge, N.J. :
|b World Scientific,
|c c1994.
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| 300 |
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|a xvi, 299 p. :
|b ill. ;
|c 23 cm.
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| 336 |
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|a text
|b txt
|2 rdacontent
|0 http://id.loc.gov/vocabulary/contentTypes/txt
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| 337 |
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|a unmediated
|b n
|2 rdamedia
|0 http://id.loc.gov/vocabulary/mediaTypes/n
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| 338 |
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|a volume
|b nc
|2 rdacarrier
|0 http://id.loc.gov/vocabulary/carriers/nc
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| 504 |
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|a Includes bibliography (p. [283]-294) and index.
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| 505 |
0 |
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|g 1.
|t The Search for Gravitational Waves.
|t The Importance of the Search.
|t A Bit of History.
|t The Practice of Gravitational Wave Detection.
|t A Guide for the Reader --
|g 2.
|t The Nature of Gravitational Waves.
|t Waves in General Relativity.
|t The Michelson-Morley Experiment.
|t A Schematic Detector of Gravitational Waves.
|t Description of Gravitational Waves in Terms of Force --
|g 3.
|t Sources of Gravitational Waves.
|t Physics of Gravitational Wave Generation.
|t In the Footsteps of Heinrich Hertz?
|t Observation of Gravitational Wave Emission.
|t Astronomical Sources of Gravitational Waves --
|g 4.
|t Linear Systems, Signals and Noise.
|t Characterizing a Time Series.
|t Linear Systems.
|t The Signal-to-Noise Ratio --
|g 5.
|t Optical Readout Noise.
|t Photon Shot Noise.
|t Radiation Pressure Noise.
|t Shot Noise in Classical and Quantum Mechanics.
|t The Remarkable Precision of Interferometry --
|g 6.
|t Folded Interferometer Arms.
|t Herriott Delay Line.
|t Beam Diameter and Mirror Diameter.
|t Fabry-Perot Cavities.
|t A Long Fabry-Perot Cavity.
|t Hermite-Gaussian Beams.
|t Scattered Light in Interferometers.
|t Comparison of Fabry-Perot Cavities with Delay Lines.
|t Optical Readout Noise in Folded Interferometers.
|t Transfer Function of a Folded Interferometer.
|t To Fold, or Not to Fold? --
|g 7.
|t Thermal Noise.
|t Brownian Motion.
|t Brownian Motion of a Macroscopic Mass Suspended in a Dilute Gas.
|t The Fluctuation-Dissipation Theorem.
|t Remarks on the Fluctuation-Dissipation Theorem.
|t The Quality Factor, Q.
|t Thermal Noise in a Gas-Damped Pendulum.
|t Dissipation from Internal Friction in Materials.
|t Special Features of the Pendulum.
|t Thermal Noise of the Pendulum's Internal Modes --
|g 8.
|t Seismic Noise and Vibration Isolation.
|t Ambient Seismic Spectrum.
|t Seismometers.
|t Vibration Isolators.
|t Myths About Vibration Isolation.
|t Isolation in an Interferometer.
|t Stacks and Multiple Pendulums.
|t Q: High or Low?
|t A Gravitational "Short Circuit" Around Vibration Isolators.
|t Beyond Passive Isolation --
|g 9.
|t Design Features of Large Interferometers.
|t How Small Can We Make a Gravitational Wave Interferometer?
|t Noise from Residual Gas.
|t The Space-Borne Alternative --
|g 10.
|t Null Instruments.
|t Some virtues of nullity.
|t The Advantages of Chopping.
|t The Necessity to Operate a Gravitational Wave Interferometer as an Active Null Instrument --
|g 11.
|t Feedback control systems.
|t The Loop Transfer Function.
|t The Closed Loop Transfer Function.
|t Designing the Loop Transfer Function.
|t Instability.
|t The Compensation Filter.
|t Active Damping: A Servo Design Example.
|t Feedback to Reduce Seismic Noise over a Broad Band --
|g 12.
|t An Interferometer as an Active Null Instrument.
|t Fringe-Lock in a Non-Resonant Interferometer.
|t Shot Noise in a Modulated Interferometer.
|t Rejection of Laser Output Power Noise.
|t Locking the Fringe.
|t Fringe Lock for a Fabry-Perot Cavity.
|t A Simple Interferometer with Fabry-Perot Arms.
|t Beyond the Basic Interferometer --
|g 13.
|t Resonant Mass Gravitational Wave Detectors.
|t Does Form Follow Function?
|t The Idea of Resonant Mass Detectors.
|t A Bar's Impulse Response and Transfer Function.
|t Resonant Transducers.
|t Thermal Noise in a Bar.
|t Bandwidth of Resonant Mass Detectors.
|t A Real Bar.
|t Quantum Mechanical Sensitivity "Limit"
|t Beyond the Quantum "Limit"? --
|g 14.
|t Detecting Gravitational Wave Signals.
|t The Signal Detection Problem.
|t Probability Distribution of Time Series.
|t Coincidence Detection.
|t Optimum Orientation.
|t Local Coincidences.
|t Searching for Periodic Gravitational Waves.
|t Searching for a Stochastic Background --
|g 15.
|t Gravitational Wave Astronomy.
|t Gravitational Wave Astronomy.
|t Gravitational Wave Source Positions.
|t Interpretation of Gravitational Waveforms.
|t Previous Gravitational Wave Searches --
|g 16.
|t Prospects.
|t A Prototype Interferometer.
|t LIGO.
|t Proposed Features of 4 km Interferometers.
|
| 650 |
|
0 |
|a Gravitational waves.
|0 http://id.loc.gov/authorities/subjects/sh85056562
|
| 650 |
|
0 |
|a Gravity waves.
|0 http://id.loc.gov/authorities/subjects/sh85056572
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| 650 |
|
0 |
|a Interferometers.
|0 http://id.loc.gov/authorities/subjects/sh85067257
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| 650 |
|
7 |
|a Gravitational waves.
|2 fast
|0 http://id.worldcat.org/fast/fst00946882
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| 650 |
|
7 |
|a Interferometers.
|2 fast
|0 http://id.worldcat.org/fast/fst00976233
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| 901 |
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|a ToCBNA
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| 903 |
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|a HeVa
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| 929 |
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|a cat
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| 999 |
f |
f |
|i d570882f-1475-57e5-92b8-7407a948b8a6
|s ac7510a0-6f5e-518a-9094-14d5c3225a39
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| 928 |
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|t Library of Congress classification
|a QC179.S280 1994
|l JCL
|c JCL-Sci
|i 2837001
|
| 927 |
|
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|t Library of Congress classification
|a QC179.S280 1994
|l JCL
|c JCL-Sci
|e CRERAR
|b 42707802
|i 3288413
|
