The quark gluon plasma (QGP) is known as primordial deconfined nuclear matter occupied in the early universe ~10 microsecond after the Big Bang. The QGP can be created in high-energy nuclear collisions and found to behave as an almost perfect fluid. In this lecture, a framework of relativistic hydrodynamics is reviewed aiming at description of space-time evolution of the QGP in high-energy nuclear collisions. The topics include: conservation law, definition of frames, ideal and viscous hydrodynamics.
The purpose of this lecture is to learn basic aspects of high-energy nuclear collisions and relativistic hydrodynamics.
Quark gluon plasma, high-energy nuclear collisions, relativistic hydrodynamics
✔ 専門力 | 教養力 | コミュニケーション力 | 展開力(探究力又は設定力) | 展開力(実践力又は解決力) |
The lecture is given using slides and handwritten notes.
授業計画 | 課題 | |
---|---|---|
第1回 | Introduction to high-energy nuclear collisions | given in the lecture |
第2回 | Conservation law and frame | given in the lecture |
第3回 | Ideal hydrodynamics 1: Equation of motion | given in the lecture |
第4回 | Ideal hydrodynamics 2: Entropy conservation and sound velocity | given in the lecture |
第5回 | Dissipative hydrodynamics 1: Constitutive equations | given in the lecture |
第6回 | Dissipative hydrodynamics 2: Equation of motion | given in the lecture |
第7回 | Dissipative hydrodynamics 3: Causal dissipative hydrodynamics | given in the lecture |
第8回 | Dynamics of core and corona in high-energy nuclear collisions | given in the lecture |
Not specified
Lecture notes will be distributed.
Some assigned problems should be solved after the lectures.
It is required that the students have basic knowledge on quantum physics.
Some assigned problems should be solved after the lectures.