
We investigate the theoretical description of quantum many-body systems out of thermal equilibrium. By combining advanced numerical simulations with (semi-) analytical methods, we decode the complex, real-time dynamics of matter under extreme conditions—such as the early stages of ultrarelativistic heavy-ion collisions and the formation of the Quark-Gluon Plasma (QGP).
Key pillars of our research include:
Further Reading:
J. Roth, Y. Ye, S. Schlichting, L. von Smekal arXiv:2603.17874

We develop comprehensive theoretical frameworks to model the entire spacetime evolution of ultrarelativistic heavy-ion collisions, tracing the system from the initial impact to the final freeze-out of hadrons. A core focus of our work is the "bottom-up" thermalization scenario, where we map how early-stage glasma fields transition into a chemically equilibrated Quark-Gluon Plasma. By connecting first-principles QCD dynamics with experimental observables, we also how to constrain the initial geometry and transport properties of the plasma in both large and small collision systems.
Review:
Further Reading:

Strong interaction matter is expected to possess a critical point at finite net-baryon density, where it undergoes a second-order phase transition. Similarly, in the chiral limit of vanishing light-quark masses the transition between the hadronic phase with broken chiral symmetry and the chirally symmetric phase at vanishing net-baryon density in all likelihood also becomes of second order, which may have an imprint on the properties of real-world QCD, where the light quark masses are small. Near these critical points, static and dynamic properties of strong-interaction matter exhibit universal behavior, which can be characterized in terms of critical exponents and universal scaling functions.
Further Reading:

We investigate high-energy scattering processes in Quantum Chromodynamics (QCD) across a wide range of collision systems, encompassing proton-proton (p+p), proton-nucleus (p+A), nucleus-nucleus (A+A), and electron-nucleus (e+A) collisions. Our focus is the regime where rapid gluon growth leads to non-linear recombination and gluon saturation. Using the Color Glass Condensate (CGC) effective field theory, we study how this saturated state sets the universal initial conditions for high-energy interactions. Our work explores the impact of non-linear QCD dynamics on key experimental observables, such as forward particle production and particle correlations, providing clean insights into the nuclear wave function that are vital for both current hadron colliders and future e+A programs. Furthermore, we develop advanced numerical and analytical frameworks to track how these highly occupied gluon fields decorrelate and evolve immediately after the initial impact, bridging the gap between saturation physics and pre-equilibrium plasma dynamics.
Review:
Further Reading:

Highly energetic particles created at the early stages of heavy ion collisions act as tomographic probes of the QGP. These jets traverse the medium and lose energy through interactions, a phenomenon known as jet quenching, allowing us to extract fundamental properties such as transport coefficients.
Further Reading:

sschlichting@physik.uni-bielefeld.de
The medal is awarded to theoretical physicists who are under the age of 40 and whose research in the field of theoretical high-energy nuclear physics has achieved important international recognition and impact. The decision on awarding the medal is taken by an international committee.
Type: Verleihung Status: validiert Year: 2022The medal and prize money of 2000 US dollars are awarded to theoretical physicists who are under the age of 40 and whose research in the field of theoretical high-energy nuclear physics has achieved important international recognition and impact.
Type: Verleihung Status: validiert Year: 2022

Dr. Baochi Fu


Jie Zhu

Min An



Jens Hügel



PhD Theses (Doktorarbeiten)
M.Sc. Theses
B.Sc. Theses
Since July 2017, the CRC/TRR 211 has been investigating the most extreme states of matter in the Universe. The researchers explore what happens when ordinary matter is heated to extremely high temperatures and subjected to enormous pressure. Under such conditions, protons and neutrons dissolve into their constituents – quarks and gluons. These states occur in neutron-star mergers, in heavy-ion collisions at particle accelerators, and in the early Universe shortly after the Big Bang.