PřF:F8290 Cosmology - Course Information
F8290 Cosmology
Faculty of ScienceSpring 2008
- Extent and Intensity
- 2/1. 2 credit(s) (plus extra credits for completion). Type of Completion: k (colloquium).
- Teacher(s)
- doc. Mgr. Josef Klusoň, Ph.D., DSc. (lecturer)
prof. RNDr. Michal Lenc, Ph.D. (lecturer)
doc. Mgr. Josef Klusoň, Ph.D., DSc. (seminar tutor)
prof. RNDr. Michal Lenc, Ph.D. (seminar tutor) - Guaranteed by
- prof. RNDr. Michal Lenc, Ph.D.
Department of Theoretical Physics and Astrophysics – Physics Section – Faculty of Science
Contact Person: prof. RNDr. Michal Lenc, Ph.D. - Timetable
- Mon 13:00–14:50 F3,03015, Mon 15:00–15:50 F3,03015
- Course Enrolment Limitations
- The course is also offered to the students of the fields other than those the course is directly associated with.
- fields of study / plans the course is directly associated with
- Theoretical Physics and Astrophysics (programme PřF, N-FY) (2)
- Theoretical Physics and Astrophysics (programme PřF, N-FY, specialization Astrofyzika)
- Theoretical Physics and Astrophysics (programme PřF, N-FY, specialization Teoretická fyzika)
- Syllabus
- 1. Introduction to General Relativity 2. Introduction to Cosmology 2.1 More general form of matter 3. Horizons 4. Matter 4.1 The Cosmic Microwave Background 4.2 The Cosmological Constant Problem 4.3 Dark Energy 5. Early Times in the Standard Cosmology 5.1 Describing Matter 5.2 Particles in Equilibrium 6. Thermal relics 6.1 Baryogenesis 6.2 Baryon Number Violation 7. Field theory and potential 7.1 The Lagrangian 7.2 Internal symmetry 7.2.1 Coninuos and discrete symmetries 7.2.2 Spontaneously broken symmetry and VEVS 7.2.3 Explicitly broken global symmetries 7.2.4 The restoration of a spontaneously broken internal symmetry 7.2.5 Quantum corrections to the potential 7.2.6 Gauge coupling unification and the Planck scale 7.2.7 The oneloop correction 5 7.3 Nonpertubative effects 7.4 Flatness requirements on the treelevel potential 8. Inflation Cosmology 8.1 Unified Theories of Elementary Particles and Inflationary Universe Scenario 8.1.1 Scalar field and Symmetry breaking 9. Chaotic inflation 10. Problems of the standard BigBang model 11. Inflation as a solution 11.1 The General Idea of Inflation 11.2 Slowly Rolling Scalar Fields 11.3 Attractor Solutions in Inflation 11.4 Solving the problems of standard cosmology 11.5 Reheating and Preheating 11.6 The Beginnings of Inflation 12. Quantum fluctuations 13. String theory and Cosmology 14. VafaTseytlin cosmology 14.1 String theory dualities 14.2 BV model 15. Pre big bang cosmology 15.1 Scale factor duality 16. Witten-Ovrut cosmology
- Language of instruction
- Czech
- Further Comments
- The course is taught annually.
- Enrolment Statistics (Spring 2008, recent)
- Permalink: https://is.muni.cz/course/sci/spring2008/F8290