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Cosmological Perturbation Theory Lecture 1
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History of the Universe
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ESA Planck CMB temperature map
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ESA Planck CMB polarization map
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Planck CMB angular power spectra
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ESA Planck CMB lensing map
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ESA Planck CMB temperature map
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COMPOSITION OF THE COSMOS TODAY
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outline:
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Key questions
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Planck CMB angular power spectra
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ESA Planck CMB temperature map
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Einstein's theory of gravity: General Relativity
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Friedmann's dynamic cosmology
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FLRW metric
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Breaking spatial symmetry
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Scalar perturbations
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Expanding equations order-by-order
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Perturbation equations order-by-order
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Fourier transform
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Statistical distribution
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Power spectrum
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Higher-order statistics
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Vector perturbations decompose
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Tensor perturbations
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Metric perturbations
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Perturbation equations order-by-order
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Fourier transform
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Expanding equations order-by-order
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Q&A
Description:
Delve into the foundations of cosmological perturbation theory in this comprehensive lecture by David Wands from the International Centre for Theoretical Sciences. Explore the history of the universe, analyze ESA Planck CMB maps and power spectra, and examine the composition of the cosmos today. Learn about Einstein's theory of general relativity, Friedmann's dynamic cosmology, and the FLRW metric. Investigate scalar, vector, and tensor perturbations, Fourier transforms, statistical distributions, and power spectra. Gain insights into expanding and perturbation equations order-by-order, higher-order statistics, and metric perturbations. Conclude with a Q&A session to reinforce understanding of these complex cosmological concepts.

Cosmological Perturbation Theory - Lecture 1

International Centre for Theoretical Sciences
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