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
Stellar Superfluidsby Dany Page, et al. - arXiv
Neutron stars provide a fertile environment for exploring superfluidity. It is not surprising that Cooper pairing occurs in dense matter since nucleon pairing is observed in nuclei as energy differences between even-even and odd-even nuclei.
(10524 views)
Elements of Astrophysicsby Nick Kaiser - University of Hawaii
These are the notes for an introductory graduate course. They are meant to be a 'primer' for students embarking on a Ph.D. in astronomy. The level is somewhat shallower than standard textbook courses, but quite a broad range of material is covered.
(17981 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.
(13484 views)
Astronuclear Physics: a Tale of the Atomic Nuclei in the Skiesby M. Arnould, S. Goriely - arXiv.org
A century ago, nuclear physics entered astrophysics, giving birth to a new field of science. The present Astronuclear Physics review focuses primarily on the facets of nuclear physics that are of relevance to astronomy and astrophysics.
(3244 views)