- Docente: Luca Ciotti
- Credits: 6
- SSD: FIS/05
- Language: Italian
- Teaching Mode: Traditional lectures
- Campus: Bologna
- Corso: Second cycle degree programme (LM) in Astrophysics and cosmology (cod. 8018)
Learning outcomes
Working knowledge of the gravitational phenomena (potential theory,
violent relaxation, phase mixing, equilibria, stability, tidal
fields, merging, Boltzman and Jeans equations) from open clusters
to galaxy clusters scale. Epicyclic theory, introduction to the
density wave theory for stellar disks.
Course contents
I] GENERALS
Potential theory and Green fuctions (Cartesian, spherical, and
cylindrical coordinates) by means of orthogonal functions. First,
second and third Newton theorems. Co-area theorem. Ellipsoidal
Coordinates - Gravitational potential of disk galaxies and
elliptical galaxies. Collisionless Boltzmann equation
and Fokker-Planck equation. Jeans equations and the problem
of self-consistency.
II] COLLISIONAL SYSTEMS: Gravitational evaporation - gravothermal
catastrophe and gravothermal oscillations. Dynamical evolution of
globular clusters.
III] COLLISIONLESS SYSTEMS: Epicyclic approximation and Oort
constants. Density waves - Jeans theorem: King models, galaxy
models and dark matter halos.
IV] EVOLUTIONARY PHENOMENA: Violent relaxation, phase mixing and
gravitational collapse. Tidal fields: tidal shocks, tidal
heating, tidal captures - Dynamical friction - Merging.
Readings/Bibliography
Selected arguments from:
'Dynamics of galaxies' (G. Bertin, Cambridge University
Press)
'Galactic Dynamics' (J. Binney, S. Tremaine Princeton University
Press)
'Galactic Astronomy' (J. Binney, M. Merrifield Princeton
University Press)
'Dynamical evolution of globular clusters' (L. Spitzer Princeton
University Press)
'Theory of rotating stars' (J.L. Tassoul, Princeton University
Press)
'Lecture notes on stellar dynamics' (L. Ciotti Scuola Normale
Superiore Pisa)
Teaching methods
Class lectures, discussion of influential research papers on
international journals
Assessment methods
Final oral examination. The examination is 45 minutes long, at the blackboard, organized in 3 sections (each 15 minutes long). In the first part the student illustrates a selected subject (the aim is to verify the presentation abilities of a well studied argument). In the second part the student is asked to solve a simple exercise (test of numerical abilities, and of a back-to-the-envelope estimate). In the third and last part a random argument from the program is discussed (test of the global preparation).
Teaching tools
Lecture notes. Selected chapters from technical books.
Office hours
See the website of Luca Ciotti