Logo

TASI Lectures: Introduction to Cosmology

Small book cover: TASI Lectures: Introduction to Cosmology

TASI Lectures: Introduction to Cosmology
by

Publisher: arXiv
Number of pages: 82

Description:
These proceedings summarize lectures that were delivered as part of the 2002 and 2003 Theoretical Advanced Study Institutes in elementary particle physics (TASI) at the University of Colorado at Boulder. They are intended to provide a pedagogical introduction to cosmology aimed at advanced graduate students in particle physics and string theory.

Home page url

Download or read it online for free here:
Download link
(690KB, PDF)

Similar books

Book cover: Particle Physics Aspects of Modern CosmologyParticle Physics Aspects of Modern Cosmology
by - arXiv
Modern cosmology has created a tight link between particle physics / field theory and a wealth of new observational data on the structure of the Universe. These notes focus on some aspects concerning the connection between theory and observations.
(16134 views)
Book cover: The Shape of the UniverseThe Shape of the Universe
by - viXra
A special solution of the Maxwell equations is presented, which disposes of the properties the Higgs-field must have, if it should not violate already secured perceptions and observations. If both fields are identical remains to be seen at this time.
(13136 views)
Book cover: Dark Energy: Observational Evidence and Theoretical ModelsDark Energy: Observational Evidence and Theoretical Models
by - Akademperiodyka
The book elucidates the current state of the dark energy problem and presents the results of the authors, who work in this area. It describes the observational evidence for the existence of dark energy, the methods of constraining of its parameters.
(12914 views)
Book cover: Cosmic Microwave Background Anisotropies up to Second OrderCosmic Microwave Background Anisotropies up to Second Order
by - arXiv
These notes present the computation of the system of Boltzmann equations describing the evolution of the photon, baryon and cold dark matter fluids up to second order in perturbation theory. They follow the time evolution of the CMB anisotropies.
(11702 views)