Control of the gravitational wave interferometric detector advanced Virgo /
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| Author / Creator: | Diaz, Julia Casanueva, author. |
|---|---|
| Imprint: | Cham, Switzerland : Springer, 2018. |
| Description: | 1 online resource |
| Language: | English |
| Series: | Springer theses Springer theses. |
| Subject: | |
| Format: | E-Resource Book |
| URL for this record: | http://pi.lib.uchicago.edu/1001/cat/bib/11679050 |
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| 100 | 1 | |a Diaz, Julia Casanueva, |e author. | |
| 245 | 1 | 0 | |a Control of the gravitational wave interferometric detector advanced Virgo / |c Julia Casanueva Diaz. |
| 264 | 1 | |a Cham, Switzerland : |b Springer, |c 2018. | |
| 300 | |a 1 online resource | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
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| 490 | 1 | |a Springer theses | |
| 500 | |a "Doctoral thesis accepted by the University of Paris-Sud, Orsay, France." | ||
| 504 | |a Includes bibliographical references. | ||
| 588 | 0 | |a Online resource; title from PDF title page (SpringerLink, viewed August 2, 2018). | |
| 505 | 0 | |a Intro; Supervisor's Foreword; Abstract; Acknowledgements; Contents; Abbreviations; 1 Introduction; 1.1 Introduction; References; 2 Gravitational Waves; 2.1 Gravitational Waves; 2.2 Sources of Gravitational Waves; 2.2.1 Neutron Stars; 2.2.2 Compact Binary Coalescence; 2.2.3 Bursts; 2.2.4 Stochastic Background; 2.3 GW150914: First Detection; References; 3 Ground Based Gravitational Wave Detectors; 3.1 Detection Principle; 3.2 Interferometer Sensitivity; 3.2.1 Shot Noise; 3.2.2 Improving the Sensitivity; 3.2.3 Limiting Noises; 3.2.4 Homodyne Detection Versus Frontal Modulation; References | |
| 505 | 8 | |a 4 Advanced Virgo4.1 OSD: Optical Simulation and Design; 4.2 TCS: Thermal Compensation System; 4.3 SUSP: Suspensions; 4.4 INJ: Injection; 4.5 DET: Detection; 4.6 ISC: Interferometer Sensing and Control; 4.7 DAQ: Data Acquisition; References; 5 Fabry-Perot Cavities in Advanced Virgo; 5.1 Basic Properties; 5.1.1 Types of Cavity; 5.2 Dynamical Effects; 5.3 Gaussian Optics; 5.3.1 Generalities and Definitions; 5.3.2 Higher Order Modes; 5.3.3 Stability of a Resonator; 5.4 Longitudinal Motion Control; 5.4.1 Feedback Control Loops; 5.4.2 Length Sensing: PDH Technique | |
| 505 | 8 | |a 5.4.3 Lock Acquisition: Guided Lock5.5 Angular Motion Control; 5.5.1 Alignment Coordinates; 5.5.2 Automatic Alignment; 5.6 Summary; References; 6 Power Recycled Interferometer; 6.1 PRITF Optical Configuration; 6.1.1 Electric Field Equations in Dark Fringe: Carrier; 6.1.2 Sidebands Behaviour: Schnupp Asymmetry and PRC Length; 6.1.3 Summary: Working Point; 6.2 Longitudinal Control; 6.2.1 Final State: Sensing and Driving; 6.2.2 PRC Stability Versus Alignment: 131 MHz; 6.2.3 Lock Acquisition Strategy: Variable Finesse; 6.2.4 Step 3: Recombined Configuration; 6.2.5 Step 4: PR Alignment | |
| 505 | 8 | |a 6.2.6 Towards Dark Fringe: MICH Offset Reduction6.2.7 Summary: Longitudinal Control Sensing; 6.3 SSFS: Second Stage of Frequency Stabilization; 6.3.1 SSFS Architecture; 6.3.2 SSFS Commissioning: CARM to MC; 6.3.3 Impact of HOMs on the Optical TF; 6.4 Angular Control; 6.4.1 Sensing and Driving; 6.5 Summary; References; 7 Advanced Virgo Commissioning; 7.1 Commissioning Timeline; 7.2 Steps 1 and 2: Arm Cavities Control; 7.2.1 Velocity and Finesse Measurements; 7.2.2 Guided Lock Implementation; 7.2.3 Error Signal Calibration; 7.2.4 Angular Control; 7.3 Step 3: Recombined; 7.3.1 MICH Loop | |
| 505 | 8 | |a 7.3.2 CARM/DARM Loops7.3.3 Second Stage of Frequency Stabilization; 7.4 Step 4: PR Alignment; 7.4.1 PRCL Loop; 7.4.2 MICH Driving Matrix; 7.4.3 Longitudinal Loops After the PR Alignment; 7.4.4 Alignment Using Quadrant Photodiodes; 7.5 Towards Dark Fringe; 7.5.1 Optical Gain Evolution; 7.5.2 Recycling Gain; 7.5.3 Alignment; 7.6 Dark Fringe; References; 8 Conclusion; Reference | |
| 520 | |a This book focuses on the development and implementation of the longitudinal, angular and frequency controls of the Advanced Virgo detector, both from the simulation and experimental point of view, which contributed to Virgo reaching a sensitivity that enabled it to join the LIGO-Virgo O2 run in August 2017. This data taking was very successful, with the first direct detection of a binary black hole merger (GW170814) using the full network of three interferometers, and the first detection and localization of a binary neutron star merger (GW170817). The second generation of gravitational wave detector, Advanced Virgo, is capable of detecting differential displacements of the order of 10?21m. This means that it is highly sensitive to any disturbance, including the seismic movement of the Earth. For this reason an active control is necessary to keep the detector in place with sufficient accuracy. | ||
| 650 | 0 | |a Gravitational waves. |0 http://id.loc.gov/authorities/subjects/sh85056562 | |
| 650 | 0 | |a Interferometry. |0 http://id.loc.gov/authorities/subjects/sh85067258 | |
| 650 | 7 | |a SCIENCE |x Physics |x Quantum Theory. |2 bisacsh | |
| 650 | 7 | |a Mensuration & systems of measurement. |2 bicssc | |
| 650 | 7 | |a Gravity. |2 bicssc | |
| 650 | 7 | |a Laser technology & holography. |2 bicssc | |
| 650 | 7 | |a Astronomy, space & time. |2 bicssc | |
| 650 | 7 | |a Gravitational waves. |2 fast |0 (OCoLC)fst00946882 | |
| 650 | 7 | |a Interferometry. |2 fast |0 (OCoLC)fst00976235 | |
| 655 | 4 | |a Electronic books. | |
| 776 | 0 | 8 | |i Print version: |a Diaz, Julia Casanueva. |t Control of the gravitational wave interferometric detector advanced Virgo. |d Cham, Switzerland : Springer, 2018 |z 331996013X |z 9783319960135 |w (OCoLC)1040615745 |
| 830 | 0 | |a Springer theses. |0 http://id.loc.gov/authorities/names/no2010186160 | |
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| 928 | |t Library of Congress classification |a QC179 |l Online |c UC-FullText |u https://link.springer.com/10.1007/978-3-319-96014-2 |z Springer Nature |g ebooks |i 12555228 | ||