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Quark Matter




Phases of matter whose degrees of freedom include
Quark s and Gluon s. These phases occur at extremely high
temperatures and densities, billions of times higher than
can be produced in equilibrium in laboratories.
Under such extreme conditions, the familiar
structure of matter, with quarks arranged into Nucleon s and
nucleons bound into Nuclei and surrounded by Electrons , is
completely disrupted, and the quarks roam freely.
This is analogous to the way that the crystal
structure of ice is disrupted by heating or compression, and melts
into a liquid of more elementary constituents (water molecules).

In the Standard Model of particle physics, the strongest force is
the Strong Interaction , which is described by the theory of
Quantum Chromodynamics (QCD). At ordinary temperatures or
densities this force just Confines the quarks into
composite particles ( Hadrons ) of size
around 10-15m = 1 Femtometer = 1 fm
(corresponding to the QCD energy scale
ΛQCD≈200 MeV)
and its effects are not noticeable at longer
distances. However, when the temperature reaches the
QCD energy scale (T of order 1012K)
or the density rises to the point where the
average inter-quark separation is less than 1 fm, (quark Chemical Potential μ around 400 MeV) the hadrons are melted into their
constituent quarks, and the strong interaction becomes the dominant
feature of the physics. Such phases are called quark matter or QCD
matter.




OCCURRENCE IN NATURE


  • The Big Bang . At very early times, when the universe was only a few tens of microseconds old, the temperature was so high that all matter took the form of a hot phase of quark matter called the Quark-gluon Plasma (QGP).

  • Compact stars ( Neutron Stars ). A neutron star is much cooler than 1012 K, but it is compressed by its own weight to such high densities that is is reasonable to surmise that quark matter may exist in the interior.

  • Strangelets. These are hypothetical lumps of quark matter that might populate interstellar space. They only exist if nuclear matter is metastable against decay into quark matter: this is generally regarded as a fairly radical hypothesis.

  • Heavy-ion collisions. Physicists can product small short-lived regions of space whose energy density is comparable to that of the 20-microsecond-old universe. This is achieved by colliding heavy nuclei at high speeds. Extremely powerful accelerators are needed, such as RHIC at Brookhaven National Laboratory in the USA, or the future LHC at CERN in Switzerland/France. There is good evidence that the quark-gluon plasma has been produced at RHIC (Müller, 2005).



THERMODYNAMICS


The context for understanding the thermodynamics of quark matter is
the Standard Model of particle physics, which contains six different
Flavors of quarks, as well as
Lepton s like Electron s and Neutrino s. These
interact via the Strong Interaction , Electromagnetism , and
also the Weak Interaction which allows one flavor of quark to turn
into another. Electromagnetic interactions occur between particles
that carry electrical charge; strong interactions occur between
particles that carry Color Charge .

The correct thermodynamic treatment of quark matter depends on the
physical context. For large quantities that exist for long periods
of time (the "thermodynamic limit"), we must take into account the fact that
the only conserved charges in the standard model are quark
number (equivalent to Baryon number), electric charge, the eight color
charges, and lepton number. Each of these can have an associated
chemical potential. However, large volumes of matter must be electrically and
color-neutral, which determines the electric and color charge chemical
potentials. This leaves a three-dimensional phase space,
parameterized by quark chemical
potential, lepton chemical potential, and temperature.

In compact stars quark matter would occupy cubic kilometers and
exist for millions of years, so the thermodynamic limit is
appropriate. However, the neutrinos
escape, violating lepton number, so the phase space for
quark matter in compact stars only has two
dimensions, temperature (T) and quark number chemical potential μ
(see next section). A strangelet is not in the thermodynamic
limit of large volume, so it is like an exotic nucleus: it may carry
electric charge.
A heavy-ion collision is in neither the thermodynamic
limit of large volumes nor long times. Putting aside questions of whether
it is sufficiently equilibrated for thermodynamics to be applicable,
there is certainly not enough time for weak interactions to occur, so flavor
is conserved, and there are independent chemical potentials for all six
quark flavors. The initial conditions
(the Impact Parameter of the collision, the number of up and down quarks
in the colliding nuclei, and the fact that they contain no quarks of
other flavors) determine the chemical potentials.


PHASE DIAGRAM