Overview
This course aims to educate learners on the observation of gravitational waves from a binary black hole merger. The learning outcomes include understanding the properties of the source, the significance of the discovery, and the future implications of gravitational-wave astronomy. The course teaches concepts such as gravitational waves, strain, signal processing, parameter estimation, and numerical simulations. The teaching method involves lectures and discussions on the LIGO detectors, advanced technologies, and the process of detecting gravitational waves. This course is intended for individuals interested in astrophysics, gravitational-wave astronomy, and the latest advancements in the field.
Syllabus
Introduction
Welcome
Gravitational Waves
The Goal of LIGO
What is a Gravitational Wave
What is a Strain
Strains from Astrophysical Sources
Strength of Gravitational Waves
Experimental Challenge
Michelson Interferometer
Gravitational Wave Detector
Advanced LIGO Detector
Sound
GW 5914
Chirp Mass
Signal Processing
Parameter Estimation
Numerical Simulation
Implications
Localization
Binary Neutron Stars
The Future
The Village
The Search Results
Taught by
APS Physics