Learn about the dawn of gravitational wave astronomy through this course. The course aims to provide an understanding of gravitational waves, their historical perspective, and their detection. Students will learn about black holes, neutron stars, pulsars, and the measurement of gravitational waves. The course covers the technology and methods used in detecting gravitational waves, such as LIGO observatories, test masses, laser systems, and vibration isolation systems. The intended audience for this course includes individuals interested in astronomy, astrophysics, and the latest advancements in the field of gravitational wave astronomy.
Overview
Syllabus
Introduction
Welcome
Introductions
Andrew Cuomo
Peter Ward
Gravitational Waves
Historical Perspective
Black Holes
Einstein
Sun
Neutron Stars
Pulsars
Black Hole
Joe Weber
Holson Taylor
Einsteins ambivalence
Detection of gravitational waves
Measuring gravitational waves
Why is it so hard
Quantum Uncertainty
LIGO
Hanford Observatory
Test Mass
Beam Tubes
Vacuum Chambers
Mirror
Vibration Isolation System
Laser System
Timelap
Global Network of Detectors
Multiple Detectors
Binary Neutron Star Merger
What are Neutron Stars
Taught by
NYU Tandon School of Engineering
Tags
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Reviews
5.0 rating, based on 1 Class Central review
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I must say, it was an utterly captivating experience that left me awestruck. The lecturer not only elucidated the complex concepts surrounding gravitational waves but also infused the session with a palpable sense of excitement and wonder.
