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DATE: 29 April 2019, 16:00 to
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Introduction
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Unseen at last: the black hole in M87
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Michell / Laplace calculation
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M87 is a galaxy with ten times as many stars as our own Milky Way
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A lens forms an image by collecting the waves from all points on its aperture
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1 parsec = 3.26 light years
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Angular resolution needed to see the black hole
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Very Long Baseline interferometry
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Best "picture" of M87 before the EHT image
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Broken Lens equivalent to EHT
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From 'Einstein Centenary Symposium' 1980
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Now, here, you see, it takes all the running you can do, to keep in the same place
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Accretion on to a black hole
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Conserving angular momentum and dissipating energy : rubbing two rings together
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Photon orbits near a black hole
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Status and prospects
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Q&A
Description:
Explore the groundbreaking discovery of the black hole at the center of galaxy M87 in this comprehensive lecture by Rajaram Nityananda. Delve into the three key aspects that led to this achievement: the behavior of matter and light near black holes, their role in galactic center phenomena, and the advanced techniques enabling unprecedented angular resolution. Learn about the Michell/Laplace calculation, Very Long Baseline interferometry, and the principles of accretion onto black holes. Gain insights into the challenges of imaging such distant objects and the significance of this discovery for our understanding of the universe. The lecture concludes with a discussion on the current status and future prospects of black hole research, followed by an engaging Q&A session.

Unseen at Last - The Black Hole in M87 by Rajaram Nityananda

International Centre for Theoretical Sciences
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