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Primordial perturbations and precision cosmology from the Cosmic Microwave Background

Primordial perturbations and precision cosmology from the Cosmic Microwave Background

Primordial perturbations and precision cosmology from the Cosmic Microwave Background. Antony Lewis CITA, University of Toronto. http://cosmologist.info. Outline. Introduction and current data Parameter estimation General primordial perturbations Current constraints

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505 views • 42 slides
Primordial perturbations and precision cosmology from the Cosmic Microwave Background

Primordial perturbations and precision cosmology from the Cosmic Microwave Background

Primordial perturbations and precision cosmology from the Cosmic Microwave Background. Antony Lewis CITA, University of Toronto. http://cosmologist.info. Outline. Introduction and current data Parameter estimation General primordial perturbations Current constraints

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429 views • 42 slides
Primordial perturbations and precision cosmology from the Cosmic Microwave Background

Primordial perturbations and precision cosmology from the Cosmic Microwave Background

Primordial perturbations and precision cosmology from the Cosmic Microwave Background. Antony Lewis CITA, University of Toronto. http://cosmologist.info. Evolution of the universe. Opaque. Transparent. Hu & White, Sci. Am., 290 44 (2004).

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183 views • 18 slides
Semi-Numerical Simulations of

Semi-Numerical Simulations of

Semi-Numerical Simulations of. HII Bubble Growth During. Reionization. August 14, 2008. Patrick Ho, SULI Program. Mentor: Marcelo Alvarez, SLAC KIPAC. Reionization. Recombination (z ~ 1100). Key phase transition in cosmological history: HI becomes HII.

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274 views • 17 slides
Inflationary Theory of Primordial Cosmological Perturbation

Inflationary Theory of Primordial Cosmological Perturbation

Inflationary Theory of Primordial Cosmological Perturbation. Project for General Relativity (Instructor: Prof.Whiting) Sohyun Park. Brief introduction about the title. It is firmly established by observation that our universe is homogeneous and isotropic on large scales (~ 100Mpc).

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243 views • 13 slides

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