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1
Introduction
2
Welcome
3
Gravitational Waves
4
The Goal of LIGO
5
What is a Gravitational Wave
6
What is a Strain
7
Strains from Astrophysical Sources
8
Strength of Gravitational Waves
9
Experimental Challenge
10
Michelson Interferometer
11
Gravitational Wave Detector
12
Advanced LIGO Detector
13
Sound
14
GW 5914
15
Chirp Mass
16
Signal Processing
17
Parameter Estimation
18
Numerical Simulation
19
Implications
20
Localization
21
Binary Neutron Stars
22
The Future
23
The Village
24
The Search Results
Description:
Explore the groundbreaking discovery of gravitational waves from a binary black hole merger in this 42-minute lecture by Duncan Brown at the APS March Meeting 2016. Delve into the details of the first direct detection of gravitational waves by the Laser Interferometer Gravitational-Wave Observatory (LIGO) on September 14, 2015. Learn about the physics behind gravitational waves, the experimental challenges faced by LIGO, and the advanced technology used in the detectors. Understand the signal processing techniques and parameter estimation methods employed to analyze the observed waveform. Discover the implications of this historic observation for the field of gravitational-wave astronomy and explore future prospects, including the detection of binary neutron star mergers. Gain insights into the collaborative effort behind this monumental achievement and its significance in confirming Einstein's theory of general relativity.

The Observation of Gravitational Waves from a Binary Black Hole Merger

APS Physics
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