Zahlavi

Ultra-Relativistic Heavy Ion Collisions

Contemporary nuclear physics is highly interested in properties of strongly interacting matter under extreme conditions similar to those present in the early Universe shortly after the Big Bang. In a laboratory, we simulate the Big Bang conditions in collisions of ultra-relativistic heavy nuclei, which compress and heat the usual nuclear matter and transform it to a new state called the Quark-Gluon Plasma (QGP). In this new state quarks and gluons, the elementary constituents of protons and neutrons in nuclei, escape their confinement and are freed for a very short instant. The subsequent expansion of this high-density nuclear matter state decreases its temperature and quarks and gluons merge back to form observable hadrons. In our institute, experimental study of such extreme states of strongly interacting matter has a long tradition. In the 1990s, we first participated in the WA98 experiment built in the West Area of the Super Proton Synchrotron (SPS) at the European Laboratory for Nuclear Research, CERN. In 1997, we joined the CERES/NA45 experiment operated in the North Area of the SPS. Since the mid-90s, we have participated in preparations of the ALICE experiment which was at that time in its preparatory phase and became operational in 2009 at the Large Hadron Collider (LHC) at CERN. Since 2000, in parallel to our activities at CERN, our ultra-relativistic heavy-ion group is also actively involved in the STAR experiment situated at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory in the USA.