Ligo gravity
[DOCX File]Instructions for the Preparation of a
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LIGO - Laser Interferometer Gravity Wave Observatory. COS - Core Optics Support. IOO - Input Optics. DRD - Design Requirements Document. SRD - Science Requirements Document. RM - Recycling Mirror. BS - Beam Splitter. ITMx, ITMy - Input Test Mass in the interferometer ‘X’ or ‘Y’ arm. ETMx, ETMy - End Test Mass in the interferometer ‘X ...
LIGO - Wikipedia
(P5, C1) One of the key aspects of Advanced LIGO is having the two sites at opposite sides of the United States (see Figure 3a). It takes light 10 ms to travel directly between these sites (and as gravitational waves travel at the speed of light as well, this is true of gravitational waves too).
[DOCX File]B. P. Abbott et al. (LIGO Scientific Collaboration and ...
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The Laser Interferometer Gravitational-Wave Observatory (LIGO) is an ongoing project to measure the gravitational radiation predicted by general relativity. According to Albert Einstein’s theory of general relativity, gravity can be thought of as a curvature of space-time. Einstein’s theory predicts that when massive stellar objects are ...
[DOC File]General Relativity - Department of Physics
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LIGO interferometers generate about 10 megabytes of data per second, which is almost one terabyte data per day [21]. And LIGO interferometers are highly distributed in thousands of kilometers away. To handle such large-scale real-time data, LIGO gravitational wave data analysis system has the following characteristics. Data reduction.
[DOC File]Laser Interferometer Gravitational Wave Observatory
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LIGO is a pair of interferometers (one in Washington and one in Louisiana). The length of one arm of the interferometer is 4 km! Despite this, the experimental groups must look for changes in the arm length distance as a gravitational waves passes on the order of m, …
[DOC File]Laser Interferometer Gravitational Wave Observatory
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LIGO-T970071-02, Core Optics Support Design Requirements Document, Michael R. Smith. LIGO-T970074-00, Secondary Light Noise Sources in LIGO, Jordan Camp . Advanced LIGO LIGO-T000092-02-D. 2. Laser Interferometer Gravitational Wave Observatory. ETMM. ITMx. PRM. SRM. ITMy. BS
The Effect of Transverse Shifts on the LIGO interferometer
LIGO Vacuum Compatibility, Cleaning Methods and Procedures, LIGO-E960022-00-D. ASC Optical Lever Design Requirement Document, LIGO-T950106-01-D. LIGO-E000007-00. LIGO Naming Convention (LIGO-E950111-A-E) LIGO Project System Safety Management Plan LIGO-M950046-F. LIGO EMI Control Plan and Procedures (LIGO-E960036)
[DOC File]Laser Interferometer Gravitational Wave Observatory
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The gravity waves can be detected and recorded with mobile phone inertial sensors. (It is a challenge however to mockup the LIGO-Virgo results as the membrane has …
[DOC File]Paper Title (use style: paper title)
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On February 11, scientists at the Laser Interferometer Gravitational-Wave Observatory (LIGO) [ which is jointly run by the California Institute of Technology (Caltech) and the Massachusetts Institute of Technology(MIT)] publicly announced the detection of gravity waves, first predicted by Albert Einstein in his Theory of General Relativity (1915).
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