Location: ITP, Science Campus Riedberg, Max-von-Laue-Str. 1, room 02.116
Time: Thursday, January 24, 2013, 16:30-17:30 (plus
10min for discussion)
Contact: hees@fias.uni-frankfurt.de
Before experiments at the Relativistic Heavy Ion Collider started recreating little droplets of the matter that filled the microseconds-old universe, this stuff was thought to be a tenuous gas-like plasma. Now we know from experiments at RHIC and at the Large Hadron Collider that at these extreme temperatures nature serves up hot quark soup --- the hottest liquid in the universe and the liquid that flows with the least dissipation. The only other comparably liquid liquid is the coldest liquid in the universe, namely the fluid made of trapped fermionic atoms at microKelvin rather than TeraKelvin temperatures. These are two examples of strongly coupled fluids without any apparent quasiparticle description. I will describe how physicists are using RHIC and LHC experiments --- as well as calculations done using dualities between liquids and black holes discovered in string theory --- to discern the properties of hot quark soup. In this domain, string theory is answering questions posed by laboratory experiments. I will describe the opportunities and challenges for coming experiments at RHIC and the LHC, among them understanding how a liquid with no apparent particulate description emerges from quarks and gluons, searching for a critical point in the QCD phase diagram and, maybe, taking snapshots of QCD sphalerons.