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Traceability of laser interferometric length measurements
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Year: 1988 Publisher: Gaithersburg, MD : U.S. Dept. of Commerce, National Institute of Standards and Technology,

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An overview of gravitational waves : theory, sources and detection
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ISBN: 9813141751 9789813141759 Year: 2017 Publisher: New Jersey: World scientific,

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"This book describes detection techniques used to search and analyse gravitational waves (GW). It covers the whole domain of GW detection, starting from the theory and ending with the experimental techniques (both present and future) used to detect them. The theoretical sections of the book address the theory of GW in the general relativity followed by the theory of GW detection. The different sources of GW are described as well as the methods used to analyse them and to extract the physical parameters of the sources. With the recent announcement of gravitational wave detection and the first results from LISA Pathfinder, this book will allow non-specialists to understand the present status of the field and the future of gravitational wave detection"--

Third international symposium on precision mechanical measurements.
Authors: --- --- --- --- --- et al.
ISBN: 0819463515 Year: 2006 Publisher: Bellingham Society of photo-optical instrumentation engineers

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Continuous "system-level" scale for comparing laser gain media
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Year: 2008 Publisher: Adelphi, MD : Army Research Laboratory,

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First International conference on vibration measurements by laser techniques : advances and applications
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ISBN: 0819416975 Year: 1994 Publisher: Bellingham SPIE International society for optical engineering

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Advanced gravitational wave detectors
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ISBN: 9781139231978 1139231979 9781139046916 1139046918 9780521874298 0521874297 9781139233514 1139233513 1107225868 9781107225862 1280393742 9781280393747 9786613571663 6613571660 1139232738 9781139232739 1139230506 9781139230506 1139229060 9781139229067 Year: 2012 Publisher: Cambridge, UK ; New York : Cambridge University Press,

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After decades of research, physicists now know how to detect Einstein's gravitational waves. Advanced gravitational wave detectors, the most sensitive instruments ever created, will be almost certain of detecting the births of black holes throughout the Universe. This book describes the physics of gravitational waves and their detectors. The book begins by introducing the physics of gravitational wave detection and the likely sources of detectable waves. Case studies on the first generation of large scale gravitational wave detectors introduce the technology and set the scene for a review of the experimental issues in creating advanced detectors in which the instrument's sensitivity is limited by Heisenberg's uncertainty principle. The book covers lasers, thermal noise, vibration isolation, interferometer control and stabilisation against opto-acoustic instabilities. This is a valuable reference for graduate students and researchers in physics and astrophysics entering this field.


Book
Present and Future of Gravitational Wave Astronomy
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ISBN: 303655226X 3036552251 Year: 2022 Publisher: MDPI - Multidisciplinary Digital Publishing Institute

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The first detection on Earth of a gravitational wave signal from the coalescence of a binary black hole system in 2015 established a new era in astronomy, allowing the scientific community to observe the Universe with a new form of radiation for the first time. More than five years later, many more gravitational wave signals have been detected, including the first binary neutron star coalescence in coincidence with a gamma ray burst and a kilonova observation. The field of gravitational wave astronomy is rapidly evolving, making it difficult to keep up with the pace of new detector designs, discoveries, and astrophysical results. This Special Issue is, therefore, intended as a review of the current status and future directions of the field from the perspective of detector technology, data analysis, and the astrophysical implications of these discoveries. Rather than presenting new results, the articles collected in this issue will serve as a reference and an introduction to the field. This Special Issue will include reviews of the basic properties of gravitational wave signals; the detectors that are currently operating and the main sources of noise that limit their sensitivity; planned upgrades of the detectors in the short and long term; spaceborne detectors; a data analysis of the gravitational wave detector output focusing on the main classes of detected and expected signals; and implications of the current and future discoveries on our understanding of astrophysics and cosmology.


Book
Quantum Enhancement of a 4 km Laser Interferometer Gravitational-Wave Detector
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ISBN: 9783319176864 3319176854 9783319176857 3319176862 Year: 2015 Publisher: Cham : Springer International Publishing : Imprint: Springer,

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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.

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