The objective is to introduce the audience to the field of relativistic fluid dynamics and to its applications in high-energy and gravitational physics.
The BIP consists of one week of lectures and tutorials, followed by team projects pursued by the students at their home institutions. Follow-up sessions will be organized to guide the students through their projects.
Physics
Bachelor students; Master students; PhD students.
6
English
25th-29th May 2026
West University of Timișoara (main building)
May – July 2026
Students will work in teams of 2-4 on the projects chosen at the end of the physical component.
Universitatea de Vest din Timișoara, Romania (Lect. Univ. Dr. Victor E. Ambruș, victor.ambrus@e-uvt.ro)
P1. Goethe Univerity, Frankfurt am Main, Germany (PD Dr. Hendrik van Hees, hees@itp.uni-frankfurt.de);
P2. University of Florence, Italy (Prof. Dr. Francesco Becattini, becattini@fi.infn.it) ;
P3. Bielefeld University, Germany (Prof. Dr. Sören Schlichting, schlichting@physik.uni-bielefeld.de);
P4. University of Catania, Italy (Prof. Dr. Vincenzo Greco, vincenzo.greco@dfa.unict.it)
1. Course syllabus (covered during physical component):
a) Basics of Relativistic hydrodynamics (Dr. Masoud Shokri, Goethe U)
This activity introduces the key concepts and the main equations of relativistic hydrodynamics, starting from a brief introduction to special relativity, tensors and covariant conservation equations; and leading to the modern formulation of relativistic hydrodynamics of perfect (ideal) and real (dissipative) fluids.
b) Hydrodynamics in astrophysics
This activity introduces the basics of fluid flows in general relativity, as well as the coupling to external electromagnetic fields, in the frame of the theory of relativistic magneto-hydrodynamics, with a focus on astrophysical applications, such as neutron star mergers.
c) Numerical methods for Relativistic fluid dynamics
This activity discusses the technical aspects behind solving the hydrodynamics equations on a computer, such as finite-volume methods, approximate Riemann solvers, propagation characteristics, with illustrations by state of the art hydrodynamics codes.
d) Mesoscopic formulation of fluid dynamics
This activity This activity describes fluids at a mesoscopic level (i.e., using momentum space distributions), connecting the kinetic theory to the hydrodynamic equations.
e) Hydrodynamics as an effective field theory
This activity demonstrates the tight connection between the fundamental framework of quantum field theory and the hydrodynamic description of relativistic fluids and plasmas.
f) Hydrodynamics in heavy ion collisions
This activity summarizes the main achievements of hydrodynamics in identifying the quark-gluon plasma as a new state of matter formed in ultra high-energy nuclear collisions, addressing the current limitations of hydrodynamics and perspectives to overcome them in the case of small systems.
2. Virtual component
The students form teams and each team selects a project from a list of proposals. During the virtual component, the students meet with the tutors assigned for the specific project to receive guidance. During the last session, the students defend their project in front of a panel formed by the tutor and the lecturer for the corresponding component.
Please fill in the registration form.