GRAVITATIONAL WAVES AND THEIR DETECTION

机译：引力波及其检测

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Direct detection of gravitational waves is one of the great challenges of contemporary experimental physics. Gravitational waves constitute a powerful testing ground for theories of gravity and provide unique information about the coherent bulk motion of the matter in the Universe. After more then 40 years from the beginning of the experimental search for cosmic gravitational waves, several detectors are today monitoring the strongest potential sources in our Galaxy and in the local group We report here the principles of operation and the main techinques adopted by resonant-mass and interferometric detectors.

机译：直接检测引力波是当代实验物理学的巨大挑战之一。引力波构成了重力理论的强大测试场，并提供有关宇宙中问题的相干散装运动的独特信息。经过40年来从实验搜索宇宙引力波开始时，今天几个探测器都在我们的星系和本地群体中监控最强大的潜在来源，我们在此报告了操作原则和共振群体所采用的主要技术和干涉探测器。

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《School on Non-Accelerator Astroparticle Physics》|2005年||共20页
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EUGENIO COCCIA;
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1. LIGO Experiments Cannot Detect Gravitational Waves by Using Laser Michelson Interferometers—Light’s Wavelength and Speed Change Simultaneously When Gravitational Waves Exist Which Make the Detections of Gravitational Waves Impossible for LIGO Experiments [J] . Xiaochun Mei, Zhixun Huang, Policarpo Yōshin Ulianov, Journal of Modern Physics . 2016,第13期

机译：LIGO实验无法使用激光迈克尔逊干涉仪检测引力波-当引力波存在时，光的波长和速度会同时变化，这使得LIGO实验无法检测到引力波
2. How beaming of gravitational waves compares to the beaming of electromagnetic waves: impacts to gravitational wave detection [J] . Andrew L. Miller, Thulsi Wickramasinghe Journal of Physics: Conference Series . 2016,第1期

机译：引力波的发射与电磁波的发射相比如何：对引力波检测的影响
3. How beaming of gravitational waves compares to the beaming of electromagnetic waves: impacts to gravitational wave detection [J] . Andrew L. Miller, Thulsi Wickramasinghe Journal of Physics: Conference Series . 2016,第1期

机译：引力波的发射与电磁波的发射相比如何：对引力波检测的影响
4. Gravitational Waves: Detectors to Detections [C] . Barry C. Barish International Conference on Big Scientific Data Management . 2019

机译：引力波：探测器检测
5. Constraining the r-mode saturation amplitude from a hypothetical detection of r-mode gravitational waves from a newborn neutron star: Detection strategies and machine learning algorithms. [D] . Mitidis, Andonis. 2015

机译：通过假设检测来自新生中子星的r模式引力波来约束r模式饱和幅度：检测策略和机器学习算法。
6. Toward the detection of gravitational waves under non-Gaussian noises II. Independent component analysis [O] . Soichiro MORISAKI, Jun’ichi YOKOYAMA, Kazunari EDA, 2016

机译：走向非高斯噪声下的引力波检测II。独立成分分析
7. LIGO Experiments Cannot Detect Gravitational Waves by Using Laser Michelson Interferometers—Light’s Wavelength and Speed Change Simultaneously When Gravitational Waves Exist Which Make the Detections of Gravitational Waves Impossible for LIGO Experiments [O] . Xiaochun Mei, Zhixun Huang, Policarpo Yōshin Ulianov, 2016

机译：Ligo实验不能通过使用激光迈克尔逊干涉仪 - 光的波长和速度同时检测引力波，当存在重力波的引力波是不可能进行利焦实验的重力

GRAVITATIONAL WAVES AND THEIR DETECTION

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