Class Central is learner-supported. When you buy through links on our site, we may earn an affiliate commission.

YouTube

Cosmological Perturbation Theory - Lecture 2

International Centre for Theoretical Sciences via YouTube

Overview

Save Big on Coursera Plus. 7,000+ courses at $160 off. Limited Time Only!
Delve into the intricacies of cosmological perturbation theory in this comprehensive lecture by David Wands from the International Centre for Theoretical Sciences. Explore key concepts such as metric perturbations, gravitational waves, and vector perturbations. Gain a deep understanding of scalar metric perturbations and their geometrical interpretation. Examine gauge dependence, linear gauge transformation rules, and various gauge-invariant variables. Learn about different gauges including longitudinal, comoving-orthogonal, uniform-density, and spatially-flat. Investigate energy-momentum conservation and the relationships between gauge-invariant variables. Conclude with a Q&A session to reinforce your understanding of these advanced cosmological concepts.

Syllabus

Cosmological perturbation theory
Lecture 2
Metric perturbations
Gravitational waves
Vector perturbations
Scalar metric perturbations
Geometrical interpretation
Vector perturbations
Gravitational waves
Gauge dependence
Linear gauge transformation rules
Linear gauge transformation rules
Gauge-invariant variables
Longitudinal gauge/Conformal Newtonian
Linear gauge transformation rules
Comoving-orthogonal gauge
Uniform-density gauge
Uniform-alpha-density gauge
Spatially-flat gauge
Energy-momentum conservation
Relating gauge-invariant variables
Q&A

Taught by

International Centre for Theoretical Sciences

Reviews

Start your review of Cosmological Perturbation Theory - Lecture 2

Never Stop Learning.

Get personalized course recommendations, track subjects and courses with reminders, and more.

Someone learning on their laptop while sitting on the floor.