Logo

Introduction to Early Universe Cosmology

Small book cover: Introduction to Early Universe Cosmology

Introduction to Early Universe Cosmology
by

Publisher: arXiv
Number of pages: 70

Description:
A central topic in these lectures is the 'theory of cosmological perturbations', the theory which describes the generation of inhomogeneities in the very early universe and their evolution until the current time. The theory is applied to three classes of models of the very early universe.

Home page url

Download or read it online for free here:
Download link
(600KB, PDF)

Similar books

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.
(11717 views)
Book cover: Big Bang Nucleosynthesis and Physics Beyond the Standard ModelBig Bang Nucleosynthesis and Physics Beyond the Standard Model
by - arXiv
We first present a pedagogical account of relativistic cosmology and primordial nucleosynthesis, discussing both theoretical and observational aspects, and then examine such constraints in detail, in particular those pertaining to new particles.
(14177 views)
Book cover: Cosmology and AstrophysicsCosmology and Astrophysics
by - arXiv.org
In these lectures I review the present status of the so-called Standard Cosmological Model, based on the hot Big Bang Theory and the Inflationary Paradigm. I will make special emphasis on the recent developments in observational cosmology ...
(11192 views)
Book cover: Cosmology for Particle PhysicistsCosmology for Particle Physicists
by - arXiv
We begin with a recapitulation of General Relativity, and the Standard Model of Cosmology. This is followed by lectures on inflation, density perturbations, study of hot and cold relics decoupled from the remaining constituents, and baryon asymmetry.
(17696 views)