Logo

Introduction to Non-Baryonic Dark Matter

Small book cover: Introduction to Non-Baryonic Dark Matter

Introduction to Non-Baryonic Dark Matter
by

Publisher: arXiv
Number of pages: 51

Description:
These lectures on non-baryonic dark matter matter are divided into two parts. In the first part, I discuss the need for non-baryonic dark matter in light of recent results in cosmology, and I present some of the most popular candidates for non-baryonic dark matter. These include neutrinos, axions, neutralinos, WIMPZILLAs, etc. In the second part, I overview several observational techniques that can be employed to search for WIMPs (weakly interacting massive particles) as non-baryonic dark matter.

Home page url

Download or read it online for free here:
Download link
(1.7MB, PDF)

Similar books

Book cover: Mathematical Problems Of Radiative EquilibriumMathematical Problems Of Radiative Equilibrium
by - Cambridge University Press
Schwarzschild's work on absorption and diffusion in the sun's atmosphere rendered the theory of radiative equilibrium a definite chapter of mathematical astrophysics. Besides the known results the reader will also find discussions of other models.
(7108 views)
Book cover: Introduction to CosmologyIntroduction to Cosmology
by - 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.
(15857 views)
Book cover: Dense Matter in Compact StarsDense Matter in Compact Stars
by - 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.
(14123 views)
Book cover: An Introduction to Cosmic Rays and Gamma-Ray BurstsAn Introduction to Cosmic Rays and Gamma-Ray Bursts
by - arXiv
The author reviews the subjects of non-solar cosmic rays and long-duration gamma-ray bursts. This is a version of an introductory talk to high-energy physicists. Nothing besides the standard model is required to understand CRs of any energy.
(13071 views)