Detection of gravitational waves

Reports on Progress in Physics

Volumn 63, Issue 9, 2000, Pages 1317-1427

  Ju, L ^a   Blair, D G ^a   Zhao, C ^a  

^a UNIVERSITY OF WESTERN AUSTRALIA   (Australia)

Author keywords

[No Author keywords available]

Indexed keywords

GRAVITY WAVE;

EID: 0033808572     PISSN: 00344885     EISSN: None     Source Type: Journal    
DOI: 10.1088/0034-4885/63/9/201     Document Type: Review

References (326)

1. Observations of post-Newtonian timing effects in the binary pulsar PSR 1913 + 16
2. Discovery of a pulsar in a binary system
3. Detection and generation of gravitational waves
4. Evidence for discovery of gravitational radiation
5. Anisotropy and polarization in the gravitational-radiation experiments
6. Gravitational radiation
7. Interferometer detection of gravitational waves
8. An introduction to the theory of gravitational radiation
9. Calibration of gravitational radiation antenna by dynamic Newton field
10. Evaluation and preliminary measurement of the interaction of a dynamical gravitational near field with a cryogenic gravitational wave antenna
11. Possibility of detection gravitational waves from millisecond pulsars by resonant bar antennas
12. Sources of gravitational waves and prospects for their detection
13. Hydrodynamics of coalescing binary neutron stars: Ellipsoidal treatment
14. Gravitational radiation from nonaxisymmetric instability in a rotating star
15. Gravitational radiation from colliding black holes
16. Gravitational radiation from rapidly rotating nascent neutron stars
17. The rate of neutron star binary mergers in the universe: Minimal predictions for gravity wave detectors
18. Neutron star and black hole binaries in the galaxy
19. The merger rate of neutron star and black hole binaries
20. Formation of double neutron star systems and asymmetric supernova explosions
21. LIGO: The laser interferometer gravitational-wave observatory
22. VIRGO: Very wide band interferometric gravitational wave antenna
23. Truncated icosahedral gravitational wave antenna
24. Resonant bar detectors for gravitational waves
25. Gravitational waves from galactic centres
26. Low-frequency gravitational waves from supermassive black holes
27. Galaxy mergers and implications for massive black hole binary coalescence
28. Estimating the detectable rate of capture of stellar mass black holes by massive central black holes in normal galaxies
29. M/sub V/=M/sub V(log P, log T/sub e/) calibrations for W ursae Majoris systems
30. 4 s
31. Gravitational radiation and rotation of accreting neutron stars
32. Black hole mergers in the universe
33. Galaxy formation in an intergalactic medium dominated by explosions
34. Detection of massive forming galaxies at redshifts z > 1
35. High-redshift star formation in the Hubble deep field revealed by a submillimetre-wavelength survey
36. A cosmological background of gravitational waves produced by supernovae in the early universe
37. The cosmic background of supernova-generated gravitational radiation
38. Gravitational wave background from a cosmological population of core-collapse supernovae
39. Stochastic background of gravitational waves generated by a cosmological population of young, rapidly rotating neutron stars
40. Sensitivity of the laser interferometer gravitational wave observatory to a stochastic background, and its dependence on the detector orientations
41. Further experimental tests of relativistic gravity using the binary pulsar PSR 1913+16
42. Gravitational radiation
43. Multidirectional, multipolarization antenna for scalar and tensor gravitational radiation
44. A multimode antenna for the detection of short pulses of gravitational radiation
45. Wide-band bar detectors of gravitational radiation
46. Comparative performance of two-, three- and four-mode gravitational radiation detectors
47. Characterizing multi-mode resonant-mass gravitational wave detectors
48. On the detection of low frequency gravitational waves
49. Solar coronal plasma in Doppler measurements
50. LISA orbit and stability
51. The gravitational wave detector Nautilus operation at T = 0.1 K
52. Operation of the Allegro detector at LSU
53. Parametric interaction of the electric and acoustic fields in a sapphire monocrystal transducer with a microwave readout
54. Experimental study of spherical resonators at very low temperatures
55. Very low temperature measurements of quality factors of copper alloys for resonant gravitational wave antennae
56. On the use of the finite elements method to design the structures of mechanical isolation to resonant mass antennas
57. Wiener filters for gravitational-wave antennas: Characteristics and application
58. Near shore ocean wave measurement using a very low frequency folded pendulum
59. The fast matched filter for gravitational-wave analysis
60. Long term performance of the cryogenic resonant-mass gravitational wave antenna, NIOBE
61. A data analysis approach for detecting gravitational waves from PSR 0437-4715
62. Report on two years of the UWA gravitational radiation antenna
63. Low resonant frequency resonant detectors
64. On the detection of monochromatic and stochastic gravitational waves with resonant gravitational wave detectors
65. Sources of gravitational radiation for detectors of the 21st century
66. On a theorem of irreversitable thermodynamics
67. Theory of the detection of short bursts of gravitational radiation
68. Ultimate sensitivity limit of a resonant gravitational wave antenna using a linear motion detector
69. On the measurement of a weak classical force coupled to a quantum-mechanical oscillator I. Issues of principle
70. Analysis of quantum-nondemolition measurement
71. Sapphire test-masses for measuring the standard quantum limit and achieving quantum non-demolition
72. Calculation of the absorption cross section for a cylindrical gravitational-wave antenna
73. Parametric back action effects in a high-Q cryogenic sapphire transducer
74. Approaching the quantum 'limit' for force detection
75. Surpassing the amplifier limit for force detection
76. Phase-sensitive parametric motion transducer
77. Development of an optical transducer
78. An optical transduction chain for the AURIGA detector
79. Superconducting tunable-diaphragm transducer for sensitive acceleration measurements
80. Long-term operation of the Rome explorer cryogenic gravitational wave detector
81. Niobium gravitational radiation antenna with superconducting parametric transducer
82. Development of a multi-mode transducer using a double SQUID preamplifier for the ALLEGRO detector
83. High dynamic range measurements of an all metal isolator using a sapphire transducer
84. Sensor and suspensions for a low-temperature gravitational wave antenna
85. Can a resonant-mass gravitational-wave detector have wideband sensitivity?
86. Nodal point supported gravitational wave antennas
87. First search of gravitational wave bursts with a network of detectors
88. Gravitational-wave stochastic background detection with resonant-mass detectors
89. Detection of cosmic rays by NAUTILUS
90. Analogical device for a rough localization of gravitational-wave sources
91. Choice of optimal orientation of one or two cylindrical gravitational antennas
92. Antenna pattern for four gravitational wave antennas
93. Antenna patterns of interferometric detectors of gravitational waves I. Linearly polarized waves
94. On the efficiency of the coincidence search in gravitational wave experiments
95. Background noise reduction in gravitational wave detectors through use of an amplitude ratio filter
96. On the design of ultralow temperature spherical gravitational wave detectors
97. Proposed gravitational wave observatory based on solid elastic spheres
98. Coalescing binaries and spherical gravitational wave detectors
99. Eigenfrequencies and quality factors of vibration of aluminium alloy spherical resonators
100. Testing theories of gravity with a spherical gravitational wave detector
101. Gravitational-wave stochastic background detection with resonant-mass detectors
102. Spherical gravitational wave antennas and the truncated icosahedral arrangement
103. Spherical resonant-mass gravitational wave detectors
104. Signal to noise analysis for a spherical gravitational wave antenna instrumented with multiple transducers
105. Limits on the sensitivity of spherical gravitational wave detectors and on the accuracy of reconstructed signals
106. Detecability of gravitational wave events by spherical resonant-mass antennas
107. What can we learn about gravitational wave physics with an elastic spherical antenna?
108. Sapphire dielectric resonator transducers
109. Sensitivity and optimization of a high-Q sapphire dielectric motion sensing transducer
110. Parametric transducers for the advanced cryogenic resonant-mass gravitational wave detectors
111. Local array of high frequency antennas
112. Two stage superconducting quantum interference device amplifier in a high-Q gravitational wave transducer
113. NIOBE: Improved noise temperature performance and background noise suppression
114. Future prospects for the University of Western Australia's cryogenic resonant-mass gravitational wave detector
115. On the detection of low frequency gravitational waves
116. Photon-noise-limited laser transducer for gravitational antenna
117. Wideband interferometric gravitational radiation antenna
118. Wide-band laser interferometer gravitational-radiation experiment
119. Noise behaviour of the Garching 30-meter prototype gravitational-wave detector
120. The Glasgow 10 m prototype laser interferometric gravitational wave detector
121. Improved sensitivity in a gravitational wave interferometer and implications for LIGO
122. Recycling in laser-interferometric gravitational-wave detectors
123. Optimization of long-baseline optical interferometers for gravitational-wave detection
124. Resonant sideband extraction: A new configuration for interferometric gravitational wave detectors
125. An experimental demonstration of resonant sideband extraction for laser-interferometric gravitational wave detectors
126. External modulation technique for sensitive interferometric detection of displacement
127. Demonstration of light recycling in a Michelson interferometer with Fabry-Perot cavities
128. Demonstration of a power-recycled Michelson interferometer with Fabry-Perot arms by frontal modulation
129. Power recycling in the Garching 30 m prototype interferometer for gravitational-wave detection
130. High power phase measurements limited by quantum noise and application to detection of gravitational waves
131. Broadband and tuned signal recycling with a simple Michelson interferometer
132. Experimental demonstration of dual recycling for interferometric gravitational wave detectors
133. Experimental demonstration of a suspended dual recycling interferometer for gravitational wave detection
134. The VIRGO project: A wide band antenna for gravitational wave detection
135. GEO 600: A 600 m laser interferometric gravitational wave antenna
136. 300-m laser interferometer gravitational wave detector (TAMA 300)
137. A method to bolt out scattered light effects and its application to a gravitational wave detector
138. A Michelson interferometer using delay line
139. Sagnac interferometer for gravitational-wave detection
140. Polarization-based balanced heterodyne detection method in a Sagnac interferometer for precision phase measurement
141. Experimental demonstration of resonant sideband extraction with a Sagnac interferometer
142. Frequency response of Michelson- and Sagnac-based interferometers
143. Concepts for extending the ultimate sensitivity of interferometric gravitational wave detectors using non-transmissive optics with diffractive or holographic coupling
144. High power laser and novel optics for laser interferometric gravitational wave detectors
145. All-reflective Michelson, Sagnac, and Fabry-Perot interferometers based on grating beam splitters
146. Quantum-mechanical radiation-pressure fluctuations in an interferometer
147. Quantum-mechanical noise in an interferometer
148. Recycling in laser interferometric gravitational-wave detectors
149. An overview of recycling in laser interferometric gravitational wave detectors
150. Proposal for a 600 m laser-interferometric gravitational wave antenna
151. Optical problems in interferometric gravitational wave antennas
152. Birefringence-induced losses in interferometers
153. Aspect of the suspension system for GEO 600
154. A double pendulum vibration isolation system for a laser interferometric gravitational wave antenna
155. Triple-pendulum vibration isolation system for a laser interferometer
156. Active control of a balanced two-stage pendulum vibration isolation system and its application to laser interferometric gravity wave detectors
157. Performance of a gas spring harmonic oscillator
158. First results from the Pisa seismic noise super-attenuator for low frequency gravitational wave detection
159. Seismic vibration mechanical filters for the gravitational waves detector VIRGO
160. Passive and active seismic isolation for gravitational radiation detectors and other instruments
161. Vibration isolation for broadband gravitational wave antennas
162. Performance of an analogue phase follower
163. One-mile equivalent length interferometric pendulum for seismic noise reduction
164. An active vibration isolation system for inertial reference and precision measurement
165. Low-frequency active vibration isolation system
166. Integrated structural damping and control system design for high-order flexible systems
167. Extending the VIRGO gravitational wave detection band down to a few Hz: Metal blade springs and magnetic antisprings
168. Test on a low-frequency inverted pendulum system
169. The inverted pendulum as a probe of anelasticity
170. An inverted pendulum preisolator stage for the VIRGO suspension system
171. Reducing low-frequency residual motion in vibration isolation to the nanometre level
172. Performance of an ultra low-frequency folded pendulum
173. Transfer function of an ultralow frequency vibration isolation system
174. Vibration isolation performance of an ultra-low frequency folded pendulum
175. Ultra-low frequency oscillator using a pendulum with crossed suspension wires
176. Transfer function of a crossed wire pendulum isolation system
177. A long-period conical pendulum for vibration isolation
178. Ultra-low frequency pre-isolation in three dimensions
179. An improvement in the VIRGO super attenuator for interferometric detection of gravitational wave: The sue of a magnetic antispring
180. Seismic noise filters, vertical resonance frequency reduction with geometrical anti-springs: A feasibility study
181. Thermal noise in mechanical experiments
182. Ultrahigh Q pendulum suspensions for gravitational wave detectors
183. Materials problems in the construction of long-period pendulums
184. Mechanical loss in fibres for low noise pendulums
185. Thermal noise in the test mass suspensions of a laser interferometer gravitational-wave detector prototype
186. Suspensions losses in the pendula of laser interferometer gravitational-wave detectors
187. The LIGO 40 m prototype laser interferometer gravitational wave detector
188. Aspect of the thermal motion of a mass suspended as a pendulum by wires
189. Suspension last stages for the mirrors of the VIRGO interferometric gravitational wave antenna
190. Prospect for gravitational wave detection with laser interferometer detectors
191. Mechanical loss factors of material and suspension systems for advanced gravitational wave detectors
192. Isolation of test masses in the advanced laser interfeormetric gravitational wave antennae
193. On the thermal noise from the violin modes of the test mass suspension in the gravitational wave antennae
194. An investigation of limitations to quality factor measurements of suspended masses due to resonances in the suspension wires
195. Brownian motion of a mass suspended by an anelastic wire
196. Experiments and techniques for the detection of gravitational and pulsed electromagnetic radiation from astrophysical sources
197. The quality factor of niobium flexure pendulums
198. Mirror thermal noise in interferometric gravitational-wave detectors
199. Thermally excited vibration isolations of the mirrors of laser interferometer gravitational-wave detectors
200. An investigation of some mechanical properties of materials for test masses in laser gravitational wave detectors
201. Monolithically suspended fused silica substrates with very high mechanical
202. Design and verification of low acoustic loss suspension system for measuring the Q-factor of a gravitational wave detector test mass
203. Mechanical quality factors of fused silica resonators
204. Oscillators for free mass gravitational antennas
205. Sapphire beamsplitters and test masses for advanced laser interferometer gravitational wave detectors
206. Mechanical losses associated with the technique of hydroxide-catalysis bonding of fused silica
207. Using sapphire test masses and niobium flexure suspension in laser interferometer gravitational wave detectors
208. First results on the electronic cooling of the Pisa seismic noise super-attenuator for gravitational wave detection
209. Vibration isolation for gravitational wave detection
210. Position control system for suspended masses in laser interferometer gravitational wave detectors
211. Normal mode suppression in all metal cantilever vibration isolators
212. Active control of a balanced two-stage pendulum vibration isolation system and its application to laser interferometric gravity wave detectors
213. Can piezoelectric accelerometers be used to actively damp the mechanical suspensions in laser interferometric gravitational wave detectors?
214. Low noise wideband accelerometer using an inductive displacement sensor
215. Ground tilt spectrum measured with a new high sensitivity rotational accelerometer
216. Low-noise RF capacitance bridge transducer
217. Interferometric detectors for gravitational radiation
218. External modulation technique for sensitive interferometric detection of displacements
219. External phase-modulation interferometry
220. Control of a 10 m delay line laser interferometer using the pre-modulation method
221. Demonstration of a power-recycles Michelson interferometer with Fabry-Perot arms by frontal modulation
222. Longitudinal control of an interferometer for the detection for the detection of gravitational waves
223. Signal separation technique for a power-recycled interferometric gravitational wave detector
224. An argon laser interferometer for the detection of gravitational radiation
225. Prototype Michelson interferometer with Fabry-Perot cavities
226. Quantum noise limited interferometer phase measurements
227. Interferometer with internal and external phase modulation
228. An optically recombined laser interferometer for gravitational wave detection
229. A digital approach to automatic control of a long-baseline interferometric antenna for gravitational wave detection
230. Automatic alignment of a Michelson interferometer
231. Digitally controlled interferometer prototype for gravitational wave detection
232. Laser phase and frequency stabilization using an optical resonator
233. Sub-hertz relative frequency stabilization of two-diode laser-pumped Nd:YAG lasers locked to a Fabry-Perot interferometer
234. Frequency-stabilized laser-diode-pumped Nd:YAG laser
235. Improved multistage wideband laser frequency stabilization
236. Ultrahigh-spectral-purity laser for the VIRGO project
237. Short-term frequency stabilization of diode-laser pumped Nd:YAG lasers using double pendulum suspended cavities
238. Optical mode cleaner with suspended mirrors
239. Test of an 18-m-long suspended mode cleaner cavity
240. Stimulated Brillouin scattering in monomode optical fibre
241. Suppression of stimulated Brillouin scattering in a fibre by changing the core radius
242. A mode selector to suppress fluctuations in laser beam geometry
243. A high accuracy method for the simulation of non-ideal optical cavity
244. Tolerance of dual recycling laser interferometer gravitational wave detectors to mirror tilt and curvature errors
245. The LIGO project: Project and plans
246. Fabrication and measurement of optics for gravitational wave detectors
247. Development of low-loss sapphire mirrors
248. Measurement of birefringence in a suspended sample of fused silica
249. Birefringence measurements of sapphire test masses for laser interferometer gravitational wave detector
250. Analytical models of thermal aberrations in massive mirrors heated by high power laser beams
251. Analytical models of transient thermoelastic deformations of mirrors heated by high power cw laser beams
252. Simulation of thermal effects in interferometric gravitational-wave detectors
253. Thermal lensing in recycling interferometric gravitational wave detectors
254. Optical absorption measurements in monocrystalline sapphire at 1 μm
255. Monolithic, unidirectional single-mode Nd:YAG ring laser
256. Amplitude and frequency stability of a diode pumped Nd:YAG laser operating at a single-frequency continuous-wave output power of 20 W
257. Frequency-stabilized, 10-W continuous-wave, laser-diode, end pumped, injection-locked, Nd:YAG laser
258. Design and characterization of a 5.5-W, CW, injection-locked fibre-coupled, laser-diode-pumped Nd:YAG miniture-slab laser
259. Intensity noise properties of injection locked lasers
260. Intensity noise dependence of Nd:YAG lasers on their diode-laser pump sources
261. Feedback control of the intensity noise of injection locked lasers
262. Suppression of the intensity noise in a diode-pumped eodymium: YAG nonplanar ring laser
263. 62-W CW TEM/sub 00/ Nd:YAG laser side-pumped by fibre-coupled diode lasers
264. 40-W CW, TEM00-mode, diode-laser-pumped, Nd:YAG miniature-slab laser
265. Versatile, efficient, diode-pumped miniature slab laser
266. LISA-new development in design
267. Fabry-Perot cavity gravity-wave detectors
268. The frequency response of interferometric gravitational wave detectors
269. Low resonant frequency cantilever spring vibration isolator for gravitational wave detectors