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1
Introduction
2
Welcome
3
Presentation
4
Stars
5
White Dwarfs
6
Neutron Stars
7
Black Holes
8
General Relativity
9
Spacetime
10
Two Black Holes
11
Einsteins Equations
12
Ray Weiss
13
Interferometry 101
14
Layout
15
How Extreme is LIGO
16
Stellar Graveyard
17
The Binary Neutron Star
18
Gravitational Waves vs Telescopes
19
LIGO Measurements
20
LIGO Hacking
21
RealTime Computing
22
The Trick
23
Simple Software
24
Electronics
25
Fast Shutter
26
Vibration
27
Damping
28
CryoBaffle dampers
29
Acoustic Mode dampers
30
Squeeze Light
31
Quantum Noise
32
Squeezed Vacuum
33
Questions
34
Runaway amplification
35
Waveform
36
Realtime
37
Geology
38
Electronics shielding
39
Quantum squeezing
40
Laser
Description:
Explore the cutting-edge world of gravitational wave detection in this 58-minute Hackaday Remoticon keynote presentation by Dr. Keith Thorne. Delve into the intricate workings of the Laser Interferometer Gravitational-Wave Observatory (LIGO), the most precise measurement device ever created, capable of detecting motion 1/10,000 the diameter of a proton. Learn about the extreme engineering challenges involved in building and operating LIGO, including cooling mirrors to 77 nano-Kelvins and hacking the Linux kernel for real-time digital control. Discover how the LIGO team uses innovative techniques like "squeezed light" to overcome quantum mechanical limitations and improve detection sensitivity. Gain insights into astrophysical phenomena such as white dwarfs, neutron stars, and black holes, and understand how LIGO's measurements compare to traditional telescopes. Explore the fascinating intersection of physics, engineering, and computer science that makes gravitational wave detection possible, and get answers to questions about realtime computing, electronics shielding, and quantum squeezing in this comprehensive overview of one of science's most ambitious projects. Read more

The Extreme Instruments of Astrophysics - LIGO

Hackaday
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