Essential Cosmological Perturbation Theory by David Wands
Offered By: International Centre for Theoretical Sciences via YouTube
Course Description
Overview
Syllabus
Essential cosmological perturbation theory
ACG
cosmological standard model
probes of cosmological perturbations
COMPOSITION OF THE COSMOS TODAY
Friedmann's dynamic cosmology
waves in an expanding universe Sp + 3Hop +Cs / 22 8p =
cosmological perturbation theory
understanding metric perturbations
waves in an expanding universe
Metric perturbations
Gravitational waves e.g., ogij o q +
Vector perturbations
Scalar metric perturbations
Linear gauge transformation rules Coordinate change: time-slicing: -+ T+STT, X
Gauge dependence
Linear gauge transformation rules Coordinate change:
FRW cosmology preferred coordinates for homogeneous and
Linear perturbation dynamics:
adiabatic perturbations uniform-density and
ON formalism for primordial density fluctuations
more information in higher-order correlators...
models for origin of cosmic structure passive models single field
conclusions
Vector perturbations
Taught by
International Centre for Theoretical Sciences
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