Not every scientific discovery is heralded by a
clear cry of "Eureka!" A case in point is the study of an exotic state of
matter known as a quark-gluon plasma (QGP), in which hundreds of ordinary
protons and neutrons melt together and form a fiery soup of free-roaming
quarks and gluons. The universe consisted of such a quark stew 10
microseconds after the big bang, about 15 billion years ago.
Seven experiments have been gathering data for the past six years at
CERN, the European laboratory for particle physics near Geneva. Although
the accumulated evidence is not as direct and clear-cut as had been hoped
for when the program began, scientists conducting the experiments felt
sufficiently confident to make their February 10 announcement. "We now
have compelling evidence that a new state of matter has been created,"
said CERN theorist Ulrich Heinz. And that state, he continued, "features
many of the characteristics" predicted for a quark-gluon plasma.
Most modern high-energy particle physics experiments smash together the
smallest convenient particles--electrons or protons--because the simpler
the protagonists, the cleaner the data. The CERN experiments, in contrast,
use relative behemoths: lead nuclei composed of 208 protons and neutrons.
These nuclei are hurled at almost the speed of light at a thin foil, also
made of lead. On occasion, one of the projectiles strikes a target
nucleus, producing a spray of thousands of particles that travel on to the
experimental detectors. From these particles, physicists try to determine
whether the collision momentarily created a seething fireball of debris,
hot and dense enough to set quarks loose.
Quarks, glued together by particles aptly named gluons, are the basic
constituents of matter, making up the familiar protons and neutrons as
well as more exotic creatures seen only in cosmic rays and particle
accelerators. Ordinarily, quarks are locked away inside their parent
particles by a phenomenon called confinement. Individual quarks carry a
kind of charge that is somewhat analogous to electric charge but comes in
three varieties called colors.
Confinement requires that quarks group together in sets of three whose
colors blend to make "white" or in pairs of quark and antiquark whose
colors similarly cancel out. Separating the component quarks of a particle
takes a large amount of energy, and instead of exposing their bare color
charges to the world, the energy generates new quarks and antiquarks,
which pair up with any potential lone quarks to keep their colors
balanced. This pairing process kicks in when a quark gets farther than
about a femtometer (10–15 meter) from its companions--the approximate size
of particles such as protons and neutrons.
In the CERN experiments, when the two lead nuclei collide, the
interactions between their component protons and neutrons generate a swarm
of new particles out of the available collision energy. At lower energies,
most of these particles will be new hadrons, particles made up of confined
quarks and antiquarks. At sufficiently high energy densities, however, the
newly generated particles are so tightly packed together that confinement
stops being relevant; each quark has numerous companions within a
femtometer. Instead of being a hot swarm of numerous hadrons colliding
together and reacting, the fireball becomes one large cloud of quarks and
gluons. The tremendous energy and pressure of the quark-gluon plasma
causes it to explode outward. The temperature and density fall and soon
become too low to sustain the plasma state. The quarks then rapidly pair
off again, forming colorless hadrons. The fireball, now composed of
hadrons, continues expanding and cooling, and ultimately the hadrons fly
on to the detectors
Physicists have been eager to create the QGP in part because it
provides clues about the origin of the universe. The process of the quark
fireball cooling to form hadrons (and later to form atoms) mimics what
happened during the big bang. Our understanding of the universe's
expansion has been tested by experiment back to the third minute, when
ordinary atomic nuclei formed; with the quark-gluon plasma, "we have
extended our knowledge back to 10 microseconds after the big bang," says
Reinhard Stock of the University of Frankfurt, who led one of the CERN
experiments. The explosive pressure at that time was comparable, he
remarks, to the weight of "150 solar-masses acting on an area the size of
a fingernail." (Apocalyptists take note: the presumed creation of the QGP
did not create a mini–black hole or other Earth-destroying phenomenon, as
some press reports suggested it might last year.)
CERN researchers cite several lines of evidence that strongly indicate
they created the quark-gluon plasma. first are the relative numbers of
various hadrons, which indicate the temperature and energy density that
must have prevailed when they formed. The result is consistent with the
levels theoretically required to produce a plasma. The energy density is
about seven times that of ordinary nuclear matter, and the fireball is
expanding at 55 percent of the speed of light when the hadrons "freeze
out" of it.
The next observed effect is enhancement of strangeness, which refers to
a type of quark. Altogether there are six different species, or "flavors,"
of quark, going by the whimsical names of up, down, strange, charm, bottom
and top. The lion's share of ordinary matter is composed of the
lightweight up and down quarks: two ups and one down quark make a proton;
one up and two downs, a neutron. Strange particles, produced in particle
physics experiments, contain at least one strange quark or antiquark.
Strange quarks are heavier than ups and downs, making them more
difficult to produce. In the early 1980s theorists predicted that they
should be unusually abundant in the QGP, where energy levels are so high
that strange quark-antiquark pairs are produced essentially as easily as
pairs of ups and downs are. The CERN experiments saw several features of
enhanced strangeness. When conditions were ripe for a plasma, overall
strangeness was two times higher, and a particle called omega, containing
three strange quarks, occurred 15 times more often. Such extra enhancement
of "multistrange" particles is characteristic of a plasma.
Whereas strangeness is enhanced in a QGP, certain charm particles,
containing the next heavier variety of quark, are suppressed, as predicted
in 1986. Attention focuses on the J/psi meson, which consists of a charm
quark and a charm antiquark. Charm quarks are so massive that these
charm-anticharm pairs can be produced only during the initial extremely
high energy proton-neutron collisions and not during the subsequent
fireball. How many of the pairs remain together to be detected as J/psi
mesons depends on whether they had to endure a QGP: a hot, seething plasma
separates a charm quark from its partner charm antiquark, so they end up
detected as a different species of hadron. The observed pattern of J/psi
suppression in the CERN experiments "rules out the available conventional
[explanations] based on confined matter," asserts Louis Kluberg of the
Laboratory of High Energy Nuclear Physics in Palaiseau, France.
All this evidence comes down on the side of a quark-gluon plasma. Why,
then, in the words of Heinz, is this evidence "not enough to prove beyond
reasonable doubt" that a quark-gluon plasma has been created?
The problem is that the evidence is indirect, involving detection of
particles produced when the plasma changes back to ordinary hadrons. If
there were a complete and consistent dynamical theory that described the
collisions, such indirectness might be less of a concern. But such a
theory does not exist: theorists must resort to various approximation
schemes and computer models, incorporating guesses about which processes
are most significant to try to re-create the observed data. Indeed, some
theorists will now be playing devil's advocate, doing their darnedest to
concoct a model involving only hadron collisions that can explain all the
CERN data
A way to shortcut such efforts is to obtain untainted evidence
directly from the plasma--by studying particles that do not
interact strongly with quarks and gluons and so can escape from the QGP
while it is still a plasma. They would carry direct signals of the extant
conditions. For example, the formation of a QGP should greatly increase
the number of photons emitted. Alas, CERN's photon data are inconclusive,
almost swamped by the large background of photons that are explicable
without a QGP. "There are intriguing indications of direct photons, but
they are marginal," Heinz says.
Such direct evidence will have to wait for the Relativistic Heavy Ion
Collider, or RHIC (pronounced "rick"), at Brookhaven National Laboratory
in Upton, N.Y., which will start examining head-on collisions of two beams
of gold ions in the summer [see "A Little Big Bang," by Madhusree
Mukerjee, SCIENTIFIC AMERICAN, March 1999]. The usable collision
energies will be 10 times those of CERN's program, which ought to produce
a QGP with a higher temperature and longer lifetime, allowing much clearer
direct observations. RHIC's plasma should be well above the transition
point between a QGP and ordinary hadronic matter, allowing numerous more
advanced studies of the plasma's properties, not merely an uncertain
demonstration that it exists at all.
In 2005, CERN's Large Hadron Collider will come on-line and slam ions
at 30 times the energy level of RHIC. "We have now scratched the surface,"
Heinz says. The higher energies of RHIC and the Large Hadron Collider are
needed to "complete the picture."