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Quantum Enhancement of a 4 km Laser Interferometer Gravitational-Wave Detector b

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Specificaties

Objectstaat
Nieuw: Een nieuw, ongelezen en ongebruikt boek in perfecte staat waarin geen bladzijden ontbreken of ...
ISBN-13
9783319367026
Type
NA
Publication Name
NA
ISBN
9783319367026
Book Title
Quantum Enhancement of a 4 km Laser Interferometer Gravitational-Wave Detector
Book Series
Springer Theses Ser.
Publisher
Springer International Publishing A&G
Item Length
9.3 in
Publication Year
2016
Format
Trade Paperback
Language
English
Illustrator
Yes
Author
Sheon S. Y. Chua
Genre
Science
Topic
Physics / Quantum Theory, Physics / Optics & Light, Physics / Relativity, Gravity
Item Weight
130.3 Oz
Item Width
6.1 in
Number of Pages
Xx, 220 Pages

Over dit product

Product Identifiers

Publisher
Springer International Publishing A&G
ISBN-10
3319367021
ISBN-13
9783319367026
eBay Product ID (ePID)
239660413

Product Key Features

Book Title
Quantum Enhancement of a 4 km Laser Interferometer Gravitational-Wave Detector
Number of Pages
Xx, 220 Pages
Language
English
Topic
Physics / Quantum Theory, Physics / Optics & Light, Physics / Relativity, Gravity
Publication Year
2016
Illustrator
Yes
Genre
Science
Author
Sheon S. Y. Chua
Book Series
Springer Theses Ser.
Format
Trade Paperback

Dimensions

Item Weight
130.3 Oz
Item Length
9.3 in
Item Width
6.1 in

Additional Product Features

Number of Volumes
1 vol.
Table Of Content
Preface.- Acknowledgements.- Introduction.- Gravitational Waves and the Quest for their Direct Detection.- Quantum Optics and Light.- Quantum Noise in Gravitational -Wave Detectors and Applied Squeezed States.- Squeezed State Generation for Gravitational-wave Detection.- The Doubly Resonant, Travelling- Wave Squeezed Light Source.- Backscatter Tolerance of a travelling-wave Optical Parametric Oscillator.- Overview of the LIGO Squeezed Light Injection Experiment.- Squeezing-enhancement of a 4km LIGO gravitational-wave detector.- Backscattered-light Impact in a Squeezing-enhanced Gravitational-Wave Detector.- Results Summary, Recommendations and Future Work.- Quantum noise and squeezing in Dual-recycled Michelson Interferometers.- Initial analysis and repair of the Enhanced LIGO H1 Output Mode Cleaner.- Supplementary Information for the Backscatter-light Experiments at LIGO.
Synopsis
Preface.- Acknowledgements.- Introduction.- Gravitational Waves and the Quest for their Direct Detection.- Quantum Optics and Light.- Quantum Noise in Gravitational -Wave Detectors and Applied Squeezed States.- Squeezed State Generation for Gravitational-wave Detection.- The Doubly Resonant, Travelling- Wave Squeezed Light Source.- Backscatter Tolerance of a travelling-wave Optical Parametric Oscillator.- Overview of the LIGO Squeezed Light Injection Experiment.- Squeezing-enhancement of a 4km LIGO gravitational-wave detector.- Backscattered-light Impact in a Squeezing-enhanced Gravitational-Wave Detector.- Results Summary, Recommendations and Future Work.- Quantum noise and squeezing in Dual-recycled Michelson Interferometers.- Initial analysis and repair of the Enhanced LIGO H1 Output Mode Cleaner.- Supplementary Information for the Backscatter-light Experiments at LIGO., The work in this thesis was a part of the experiment of squeezed light injection into the LIGO interferometer. The work first discusses the detailed design of the squeezed light source which would be used for the experiment. The specific design is the doubly-resonant, traveling-wave bow-tie cavity squeezed light source with a new modified coherent sideband locking technique. The thesis describes the properties affecting the squeezing magnitudes and offers solutions which improve the gain. The first part also includes the detailed modeling of the back-scattering noise of a traveling Optical Parametric Oscillator (OPO). In the second part, the thesis discusses the LIGO Squeezed Light Injection Experiment, undertaken to test squeezed light injection into a 4km interferometric gravitational wave detector. The results show the first ever measurement of squeezing enhancement in a full-scale suspended gravitational wave interferometer with Fabry-Perot arms. Further, it showed that the presence of a squeezed-light source added no additional noise in the low frequency band. The result was the best sensitivity achieved by any gravitational wave detector. The thesis is very well organized with the adequate theoretical background including basics of Quantum Optics, Quantum noise pertaining to gravitational wave detectors in various configurations, along with extensive referencing necessary for the experimental set-up. For any non-experimental scientist, this introduction is a very useful and enjoyable reading. The author is the winner of the 2013 GWIC Theses Prize.
LC Classification Number
QC178

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