Why CMB physics?
by Massimo Giovannini
Publisher: arXiv 2007
Number of pages: 179
Description:
The aim of these lectures is to introduce some basic problems arising in gravitation and modern cosmology. All along the discussion the guiding theme is provided by the phenomenological and theoretical properties of the Cosmic Microwave Background (CMB).
Download or read it online for free here:
Download link
(2MB, PDF)
Similar books
Neutrinos and the Starsby Georg Raffelt - arXiv
The role of neutrinos in stars is introduced for students with little prior astrophysical exposure. We begin with neutrinos as an energy-loss channel in ordinary stars and how stars provide information on neutrinos and possible other particles.
(11119 views)
Introduction to Cosmologyby David H Lyth - arXiv
These notes form an introduction to cosmology with special emphasis on large scale structure, the cmb anisotropy and inflation. In some places a basic familiarity with particle physics is assumed, but otherwise no special knowledge is needed.
(17584 views)
Dense Matter in Compact Starsby Andreas Schmitt - arXiv
Cold and dense nuclear and quark matter can be found in the interior of compact stars. The author gives a pedagogical introduction to microscopic calculations based on phenomenological models, effective theories, and perturbative QCD.
(15582 views)
Supernova Remnants: The X-ray Perspectiveby Jacco Vink - arXiv
Supernova remnants are beautiful astronomical objects that are also of high scientific interest, because they provide insights into supernova explosion mechanisms, and because they are the likely sources of Galactic cosmic rays.
(12586 views)