Hadrons at Accelerators and Astrophysics Observables
PH2301 is a semester module in English language at which is offered in winter semester.
If not stated otherwise for export to a non-physics program the student workload is given in the following table.
|Total workload||Contact hours||Credits (ECTS)|
|150 h||60 h||5 CP|
Responsible coordinator of the module PH2301 is Laura Fabbietti.
Content, Learning Outcome and Preconditions
We will focus on the experimental test of the strong Interaction in the non-perturbative regime ( Low Energy QCD)
and explore the connections to astrophysics with examples from modern and contemporary experiments.
In the first semester, we will focus on the pillars of the strong interactions and treat:
* Chiral Symmetry Breaking (CSB) and possible Restauration (CSR)
CSB is linked to the origin of the hadron mass and experimentally very challenging to explore.
A historical review of the attempts and state of the art of the results will be discussed.
* Hadron properties in the nuclear medium and link to CSR
Hadron properties within nuclear matter at different densities are on one hand connected to the search of CSR but on the other end relevant for the description of objects such as neutron stars. The key experiments will be studied
* Meson-Nucleon and Meson-Nucleus Interaction
* Hyperon-Nucleon interaction
The behaviour of hadrons in matter depend on the two-body and three-body interactions. The experimental method
used to access them will be discussed
* Scattering experiments, pionic and kaonic atoms
* Hadronic Resonances and Exotic bound state in low energy QCD
* Link to dense and cold system as Neutron Stars
At the end of the course, the link to the physics of neutrons stars will be made and
then further expanded in the second module of the course during the sommer
Modern experiments at different accelerator facilities to study low energy QCD processes involving hadrons and their interaction with nuclear matter under different temperature and density conditions will be presented. A complete overview of the observables and the techniques to extract the latter from experiments with accelerated beam up to few GeV will be provided.
The focus will be on Hadron properties within nuclear matter and in particular we will learn how this can be connected to a possible observation of chiral symmetry restauration. Another rather hot topic in our field is the tests with terrestrial experiments of diferent hypotheses for the content of neutron stars. The state of the art of this kind of research will be discussed as well.
Nuclear, Particle and Astrophysics Lecture, Expert or Intro
Courses, Learning and Teaching Methods and Literature
Courses and Schedule
|VO||2||Hadrons at Accelerators and Astrophysics Observables||Fabbietti, L.||
Tue, 10:00–12:00, PH 2024
|UE||2||Exercise to Hadrons at Accelerators and Astrophysics Observables||
Responsible/Coordination: Fabbietti, L.
|dates in groups|
Learning and Teaching Methods
The course will be based on scientific articles, mainly experimental works, that will be explained and discussed.
The articles treated during the course will be distributed during each lessons to the students.
Slides with all the exposed material will also be made available to the students.
Explenatory examples will be presented at the blackboard.
Book: The structure of the Nucleon
A. W. Thomas and W. Weise
Hadrons in strongly interacting matter
Stefan Leupold, Volker Metag, Ulrich Mosel (Giessen U.). Jul 2009. 80 pp.
Published in Int.J.Mod.Phys. E19 (2010) 147-224