The course aims to provide a phenomenological derivation of the Standard Cosmological Model, using critical observations and concepts from classical and modern physics. The goal is to provide students with a solid foundation for understanding the large-scale structure and evolution of the universe and to pursue a career in space physics. The course also offers a general knowledge of cosmological phenomena and methods, suitable for students interested in other areas of physics as well.
The course aims to discuss the main observations that have led to the formulation of the Standard Cosmological Model, emphasizing their critical aspects and their impact on particle physics and theories of gravity.
During the course, students will develop knowledge regarding the most relevant astronomical observations for cosmology. These include the surface brightness of the night sky, the recession velocity of galaxies, the cosmic microwave background and its anisotropies, gamma-ray background, optical spectra of distant quasars, the 21 cm radiation, X-ray emission from galaxy clusters, Type Ia supernovae, the spatial distribution of galaxies in the cosmos, their peculiar velocities, and various manifestations of gravitational lensing.
In parallel, students will acquire the necessary concepts that, when combined into a coherent framework, will allow them to develop the Standard Cosmological Model. This includes Friedmann's equations, equations of state for fluids, energy and curvature, cosmological redshift, Universe models, the Big Bang theory, dark matter, the cosmological constant, thermal history, equivalence, decoupling, recombination, reionization, cosmological nucleosynthesis, cosmic inflation, gravitational instability, statistical analysis tools for large-scale structure, and galaxy bias.
At the end of the course, the developed concepts will be used to discuss a recent publication on one of the cutting-edge research topics in cosmology.
There are no pre-requisites for this course. However, we warmly suggest to have attended the course "Intriduction to Astrophysics and Cosmology" during the Laurea Triennale.
Lectures will be conducted in a frontal format, using slides and ancillary materials provided through AulaWeb.
Lezioni frontali con utilizzo di slide e materiale fornito tramite AulaWeb.
Ricevimento: During and after the course: free (S805 al DIFI) by prior appointment via email: enzo.franco.branchini@unige.it
ENZO FRANCO BRANCHINI (President)
MARCO RAVERI
SILVANO TOSI (President Substitute)
September 2024
Standard oral exam on the blackboard. Questions on two topics indicated by the candidate.
The exam consists of an oral test that includes questions from the committee on two topics chosen by the students. On average, the exam lasts about 40 minutes per student. The questions aim to assess the level of knowledge and mastery of the topics developed by the students, as well as the clarity of exposition and the appropriate use of language in the discipline, in order to determine the final evaluation.
Students who have valid certification of physical or learning disabilities on file with the University and who wish to discuss possible accommodations or other circumstances regarding lectures, coursework and exams, should speak both with the instructor and with Professor Sergio Di Domizio (sergio.didomizio@unige.it), the Department’s disability liaison.
