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20 February 2018, 14:00 to
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Introduction
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In Brightest Day and Blackest Night
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Questions that children scientists often ask:
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Cosmic Time
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97 percent of the Universe is Invisible "Dark"
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Black Holes! from Outer Space!!
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Gravitational Waves
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How the Michelson Interferometer Works:
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LIGO Observatories in the U.S.
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The Michelson Interferometer
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Sensitivity Evolution of GW Detectors
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Sensitivity Evolution of LIGO Detectors
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Power
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Quadruple Suspensions
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Optics: 40 kg Silica
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LIGO Louisiana Control Room
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LIGO Hanford Control Room
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Simulating Extreme Spacetimes SXS Project
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Masses in the Stellar Graveyard
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What's next for LIGO?
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LIGO India
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some Future Challenges: for LIGO-India
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Caltech Relativity group 1974
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GWS??
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2704 BATSE Gamma-Ray Bursts
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Q&A
Description:
Explore the groundbreaking field of gravitational wave astronomy in this 1-hour 7-minute lecture by Rana Adhikari at the International Centre for Theoretical Sciences. Delve into the detection of gravitational waves predicted by Einstein, and learn how the LIGO project uses ultra-sensitive laser interferometers to measure spacetime distortions from black hole collisions billions of years ago. Discover the challenges of measuring motions smaller than a proton, the evolution of gravitational wave detectors, and the future of LIGO, including the LIGO-India project. Gain insights into cosmic time, dark matter, black holes, and the workings of interferometers. The lecture concludes with a Q&A session, offering a comprehensive overview of this cutting-edge area of physics and cosmology.

In Brightest Day and Blackest Night by Rana Adhikari

International Centre for Theoretical Sciences
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