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The results of present lattice QCD calculations are illustrated in Figure
which shows the temperature dependence of the Wilson loop L and
the quark condensate
along with the corresponding generalised susceptibilities
.
The quantity L is a measure of the free quark energy and thereby
of the color mobility or color deconfinement. The sharp jump from very
small values (low quark mobility) to large values occurs at the critical
temperature corresponding to the deconfinement phase transition. At exactly
the same position the quark condensate, a measure for the quark mass acquired
by spontaneous breaking of the chiral symmetry in low temperature QCD,
drops steeply. These calculations indicate that quarks and, hence, hadrons
loose their mass (except for the small current quark masses) at a critical
temperature Tc, a process called chiral symmetry restoration,
and simultaneously acquire a finite free energy in the medium, resulting
in a finite mobility corresponding to deconfinement. This interpretation
is supported by a concurrent steep jump in the energy density (not illustrated).
The susceptibilities shown as the red curves in Figure
are a measure of the fluctuations that characteristically are maximal in
the vicinity of a phase transition. To put the critical temperature on
an absolute energy scale requires calibration of the lattice results by
tying them e.g. to a physical hadron mass. The best calibration to date
fixes the critical temperature to 150 MeV. Including systematic errors,
the temperature range for Tc inferred from lattice QCD
is between 150 MeV and at most 200 MeV, as indicated in Figure
by the arrow. All lattice QCD results obtained so far are valid for a system
of vanishing baryon number density (baryochemical potential
= 0). To extend the knowledge of the hadron gas - quark-gluon plasma boundary
into the domain of finite baryon number one needs to employ QCD inspired
models (blue line in Figure
).
Energy densities of about the required magnitude are indeed reached in
the initial phase of central Pb+Pb collisions at the SPS together with
baryon densities of up to 5 times nuclear matter density. However, the
lattice calculations describe a stationary state whereas nuclear collisions
are a typical example of a rapidly evolving system. Of equal importance
as energy density are therefore lifetime and equilibration times in nuclear
collisions. A very intense theoretical discussion is currently devoted
to the question if thermal relaxation time scales are sufficiently small
compared to the expansion time scale. However, the final answer concerning
the creation of an equilibrated strongly interacting medium, of either
partonic or a hadronic nature, can only be settled by experiment. To fully
explore the high-density regime simulations of the collision show that
beam energies of a few tens of GeV per nucleon are optimal. Maximum densities
are reached when the colliding nuclei still barely stop each other. A study
of the chiral and deconfinement phase transitions along the density axis
is complementary to studies at high energy density i.e. high temperature
and is equally important for a full understanding of the nature of these
phase transitions.