An online resource for the course 402-0833-00L given
within the MSc curriculum of the Institute for Theoretical Physics, ETH Zurich
This course aims to be a review of modern Cosmology, and in particular, of those aspects of modern Cosmology that provide information to Particle Physics.
Cosmology has become, in recent years, a much more quantitative scientific endeavour than it used to be, thanks to the wealth of observational information coming from modern satellite telescopes,like Hubble, Cobe, Planck et al. There is now an equivalent to the Standard Model for Cosmology, a basic narrative of the evolution of the Universe in the past as well as in the future.
This narrative, mostly a product of last one hundred years, puts constraints to fundamental theories of nature that strive to extend the Standard Model (henceforth abbreviated to SM) of particle physics. In fact we have reached the point where the most compelling evidence that there exist other fundamental particles beyond those of the SM (and gravitons) comes from cosmological observations that indicate the existence of Dark Matter.
It is therefore becoming increasingly important for a particle physicist to understand what is the Standard Theory of Cosmology, what are its successes and which constraints are imposed by those successes on fundamental particle theories, as well as which are the open questions that the study of the Universe poses on us.
The material in this lecture can be found at any introductory book on Cosmology or the Early Universe. For concise versions seewhile a very accessible introduction, without many details, but with the basic concepts elucidated can be found in
- Rubakov and Gobrunov: sec. 2.2,3.1,3.2,4.1
- Weinberg: sec. 1.5
- Zee: VIII.1,VIII.2
The Matter density vs Dark Energy density discussion can be found atbut similar material is, once again, present in all GR books in the references.
- Zee: VIII.2
- Weinberg, 3.1 and 3.2 are excellent accounts of thermal evolution and BBN, with many further details than we talked about in class.
- Dolgov & Bambi ch. 10
- Weinberg ch. 2 & 7
- Gorbunov & Rubakov ch. 6
- [All about instantons]Instantons in QCD
- [For thermal field theory enthusiasts]Basics of Thermal Field Theory, by Laine and Vuorinen
- [Easier to follow]Baryogenesis,J.M.Cline
- [EW Baryogenesis specifically]Electroweak Baryogenesis, by Morrissey and Ramsey-Musolf
- [Brief but with all the links to literature]Matter and Antimatter in the Universe, by Canetti, Drewes and Shaposhnikov
- Leptogenesis in the Universe, by Fong, Nardi, Riotto
- [Neutrino-less double beta decay future experiments]Neutrinoless Double-Beta Decay: Status and Prospects, by Dolinski, Poon and Rodejohann
Bothhave a good discussion of the material. I based most of the lecture on the excellent which is contains many topics beyond the lecture (and the course) and is a very good source for those interested in doing research in DM models.
- Weinberg: ch 3.4
- Gorbunov and Rubakov: ch. 9
The slides shown at class can be found here.
Two good reviews are For a recent review by the pioneer of Chaotic Inflation, Andrei Linde see For an (advanced level) review focused on density perturbations see
I based some of the discussion in class onAlso, have a look on the apropriately named You might also want to read the classic, (and greatly enjoyable), if a bit dated, paper by Weinberg (1989), the one which all anthropic wars cite,
- Bambi and Dolgov, ch. 11
Most of the discussion in the class and much more is contained in
39+1 questions for the exam can be found here.