Cover image for Gravitational-Wave Physics and Astronomy : An Introduction to Theory, Experiment and Data Analysis.
Gravitational-Wave Physics and Astronomy : An Introduction to Theory, Experiment and Data Analysis.
Title:
Gravitational-Wave Physics and Astronomy : An Introduction to Theory, Experiment and Data Analysis.
Author:
Creighton, Jolien D. E.
ISBN:
9783527636051
Personal Author:
Edition:
1st ed.
Physical Description:
1 online resource (391 pages)
Contents:
Gravitational-Wave Physics and Astronomy -- Contents -- Preface -- List of Examples -- Introduction -- References -- 1 Prologue -- 1.1 Tides in Newton's Gravity -- 1.2 Relativity -- 2 A Brief Review of General Relativity -- 2.1 Differential Geometry -- 2.1.1 Coordinates and Distances -- 2.1.2 Vectors -- 2.1.3 Connections -- 2.1.4 Geodesics -- 2.1.5 Curvature -- 2.1.6 Geodesic Deviation -- 2.1.7 Ricci and Einstein Tensors -- 2.2 Slow Motion in Weak Gravitational Fields -- 2.3 Stress-Energy Tensor -- 2.3.1 Perfect Fluid -- 2.3.2 Electromagnetism -- 2.4 Einstein's Field Equations -- 2.5 Newtonian Limit of General Relativity -- 2.5.1 Linearized Gravity -- 2.5.2 Newtonian Limit -- 2.5.3 Fast Motion -- 2.6 Problems -- References -- 3 Gravitational Waves -- 3.1 Description of Gravitational Waves -- 3.1.1 Propagation of Gravitational Waves -- 3.2 Physical Properties of Gravitational Waves -- 3.2.1 Effects of Gravitational Waves -- 3.2.2 Energy Carried by a Gravitational Wave -- 3.3 Production of Gravitational Radiation -- 3.3.1 Far- and Near-Zone Solutions -- 3.3.2 Gravitational Radiation Luminosity -- 3.3.3 Radiation Reaction -- 3.3.4 Angular Momentum Carried by Gravitational Radiation -- 3.4 Demonstration: Rotating Triaxial Ellipsoid -- 3.5 Demonstration: Orbiting Binary System -- 3.6 Problems -- References -- 4 Beyond the Newtonian Limit -- 4.1 Post-Newtonian -- 4.1.1 System of Point Particles -- 4.1.2 Two-Body Post-Newtonian Motion -- 4.1.3 Higher-Order Post-Newtonian Waveforms for Binary Inspiral -- 4.2 Perturbation about Curved Backgrounds -- 4.2.1 Gravitational Waves in Cosmological Spacetimes -- 4.2.2 Black Hole Perturbation -- 4.3 Numerical Relativity -- 4.3.1 The Arnowitt-Deser-Misner (ADM) Formalism -- 4.3.2 Coordinate Choice -- 4.3.3 Initial Data -- 4.3.4 Gravitational-Wave Extraction -- 4.3.5 Matter -- 4.3.6 Numerical Methods -- 4.4 Problems.

References -- 5 Sources of Gravitational Radiation -- 5.1 Sources of Continuous Gravitational Waves -- 5.2 Sources of Gravitational-Wave Bursts -- 5.2.1 Coalescing Binaries -- 5.2.2 Gravitational Collapse -- 5.2.3 Bursts from Cosmic String Cusps -- 5.2.4 Other Burst Sources -- 5.3 Sources of a Stochastic Gravitational-Wave Background -- 5.3.1 Cosmological Backgrounds -- 5.3.2 Astrophysical Backgrounds -- 5.4 Problems -- References -- 6 Gravitational-Wave Detectors -- 6.1 Ground-Based Laser Interferometer Detectors -- 6.1.1 Notes on Optics -- 6.1.2 Fabry-Pérot Cavity -- 6.1.3 Michelson Interferometer -- 6.1.4 Power Recycling -- 6.1.5 Readout -- 6.1.6 Frequency Response of the Initial LIGO Detector -- 6.1.7 Sensor Noise -- 6.1.8 Environmental Sources of Noise -- 6.1.9 Control System -- 6.1.10 Gravitational-Wave Response of an Interferometric Detector -- 6.1.11 Second Generation Ground-Based Interferometers (and Beyond) -- 6.2 Space-Based Detectors -- 6.2.1 Spacecraft Tracking -- 6.2.2 LISA -- 6.2.3 Decihertz Experiments -- 6.3 Pulsar Timing Experiments -- 6.4 Resonant Mass Detectors -- 6.5 Problems -- References -- 7 Gravitational-Wave Data Analysis -- 7.1 Random Processes -- 7.1.1 Power Spectrum -- 7.1.2 Gaussian Noise -- 7.2 Optimal Detection Statistic -- 7.2.1 Bayes's Theorem -- 7.2.2 Matched Filter -- 7.2.3 Unknown Matched Filter Parameters -- 7.2.4 Statistical Properties of the Matched Filter -- 7.2.5 Matched Filter with Unknown Arrival Time -- 7.2.6 Template Banks of Matched Filters -- 7.3 Parameter Estimation -- 7.3.1 Measurement Accuracy -- 7.3.2 Systematic Errors in Parameter Estimation -- 7.3.3 Confidence Intervals -- 7.4 Detection Statistics for Poorly Modelled Signals -- 7.4.1 Excess-Power Method -- 7.5 Detection in Non-Gaussian Noise -- 7.6 Networks of Gravitational-Wave Detectors -- 7.6.1 Co-located and Co-aligned Detectors.

7.6.2 General Detector Networks -- 7.6.3 Time-Frequency Excess-Power Method for a Network of Detectors -- 7.6.4 Sky Position Localization for Gravitational-Wave Bursts -- 7.7 Data Analysis Methods for Continuous-Wave Sources -- 7.7.1 Search for Gravitational Waves from a Known, Isolated Pulsar -- 7.7.2 All-Sky Searches for Gravitational Waves from Unknown Pulsars -- 7.8 Data Analysis Methods for Gravitational-Wave Bursts -- 7.8.1 Searches for Coalescing Compact Binary Sources -- 7.8.2 Searches for Poorly Modelled Burst Sources -- 7.9 Data Analysis Methods for Stochastic Sources -- 7.9.1 Stochastic Gravitational-Wave Point Sources -- 7.10 Problems -- References -- 8 Epilogue: Gravitational-Wave Astronomy and Astrophysics -- 8.1 Fundamental Physics -- 8.2 Astrophysics -- References -- Appendix A Gravitational-Wave Detector Data -- A.1 Gravitational-Wave Detector Site Data -- A.2 Idealized Initial LIGO Model -- References -- Appendix B Post-Newtonian Binary Inspiral Waveform -- B.1 TaylorT1 Orbital Evolution -- B.2 TaylorT2 Orbital Evolution -- B.3 TaylorT3 Orbital Evolution -- B.4 TaylorT4 Orbital Evolution -- B.5 TaylorF2 Stationary Phase -- References -- Index.
Abstract:
This most up-to-date, one-stop reference combines coverage of both theory and observational techniques, with introductory sections to bring all readers up to the same level. Written by outstanding researchers directly involved with the scientific program of the Laser Interferometer Gravitational-Wave Observatory (LIGO), the book begins with a brief review of general relativity before going on to describe the physics of gravitational waves and the astrophysical sources of gravitational radiation. Further sections cover gravitational wave detectors, data analysis, and the outlook of gravitational wave astronomy and astrophysics.
Local Note:
Electronic reproduction. Ann Arbor, Michigan : ProQuest Ebook Central, 2017. Available via World Wide Web. Access may be limited to ProQuest Ebook Central affiliated libraries.
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