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Titlebook: Advanced Interferometers and the Search for Gravitational Waves; Lectures from the Fi Massimo Bassan Book 2014 Springer International Publi

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發(fā)表于 2025-3-21 16:11:22 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
期刊全稱(chēng)Advanced Interferometers and the Search for Gravitational Waves
期刊簡(jiǎn)稱(chēng)Lectures from the Fi
影響因子2023Massimo Bassan
視頻videohttp://file.papertrans.cn/146/145803/145803.mp4
發(fā)行地址Coverage of all experimental aspects of the search for gravitational radiation with optical interferometers.Description of the technological developments underlying the evolution of advanced interfero
學(xué)科分類(lèi)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Advanced Interferometers and the Search for Gravitational Waves; Lectures from the Fi Massimo Bassan Book 2014 Springer International Publi
影響因子The search for gravitational radiation with optical interferometers is gaining momentum worldwide. Beside the VIRGO and GEO gravitational wave observatories in Europe and the two LIGOs in the United States, which have operated successfully during the past decade, further observatories are being completed (KAGRA in Japan) or planned (ILIGO in India). The sensitivity of the current observatories, although spectacular, has not allowed direct discovery of gravitational waves. The advanced detectors (Advanced LIGO and Advanced Virgo) at present in the development phase will improve sensitivity by a factor of 10, probing the universe up to 200 Mpc for signal from inspiraling binary compact stars. This book covers all experimental aspects of the search for gravitational radiation with optical interferometers. Every facet of the technological development underlying the evolution of advanced interferometers is thoroughly described, from configuration to optics and coatings and from thermal compensation to suspensions and controls. All key ingredients of an advanced detector are covered, including the solutions implemented in first-generation detectors, their limitations, and how to overcome
Pindex Book 2014
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發(fā)表于 2025-3-21 23:14:10 | 只看該作者
Advice for Technology and Security Leadershe main types of thermal noise affecting gravitational wave detectors. In the last part of the chapter a special emphasis is given to the thermal noise due to dissipation in the mirrors optical coatings.
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https://doi.org/10.1007/978-3-540-49342-6hind the super attenuator chains developed in Virgo to reduce the seismic noise. In the second part, we illustrate the techniques to suspend the mirror reducing the thermal noise in the detection bandwidth, according to the theory illustrated in Chap. ..
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Applying Your Skills to Cybersecuritybrication process of the optics, will play a crucial role. High precision beam shaping of the CO. laser beam and high sensitivity wavefront sensors will be implemented to face these challenges, moving the thermal compensation system toward adaptive optical systems.
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發(fā)表于 2025-3-22 19:59:09 | 只看該作者
0067-0057 developments underlying the evolution of advanced interferoThe search for gravitational radiation with optical interferometers is gaining momentum worldwide. Beside the VIRGO and GEO gravitational wave observatories in Europe and the two LIGOs in the United States, which have operated successfully
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發(fā)表于 2025-3-23 00:23:42 | 只看該作者
Jim Graham,Marolo Alfaro,James Blatzd open the way to gravitational wave astronomy. The legacy of first-generation detectors is discussed before giving an overview of the technology challenges that have been faced to make advanced detectors possible. The various aspects outlined here are then discussed in more detail in the subsequent chapters of the book.
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