| STAR’s Tim Hallman on the QGP Debate: What’s the Matter? |
If
physicists had a choice, they’d probably all live at or near the
beginning of the universe. String theorists and their ilk
would live closest to the moment of creation, but those nuclear
physicists studying such concepts as the long-sought quark-gluon plasma
would not be far behind. The QGP, as it’s known, is thought to be the
soupy state of the universe after the quarks and gluons began to
condense from the energy of the Big Bang but before they were bound
inexorably into the neutrons and protons that make up the universe as we
know it today. And because the QGP is theoretically accessible in
earthly accelerators—particularly the Relativistic Heavy Ion Collider,
or RHIC, at Brookhaven National Laboratory—this has made it one of the
hottest topics in physics.
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"There is no question that we’ve indeed produced a new state of matter, and that’s extremely exciting,” says Timothy J. Hallman of the STAR Collaboration, Brookhaven National Laboratory, New York |
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Photo: Manuello
Paganelli |
RHIC collides gold nuclei together at energies that simulate the
temperature just after the Big Bang, and it’s in these collisions that
physicists expect to see the ephemeral signs of the QGP. This has made
one collaboration in particular, STAR (Solenoidal Tracker At RHIC), led
by Brookhaven’s Tim Hallman, one of the most highly cited research
groups in the field. In late 2005, STAR placed five reports in the Hot
Papers collection of the hottest current research. In the last decade,
seven STAR papers have been cited over 100 times each, including the
collaboration’s seminal 2001 paper, "Elliptic flow in AU + AU
collisions at root s(NN)-130 GeV", published in Physical Review
Letters (see accompanying table), with nearly 250 citations—remarkable
numbers for a comparatively small discipline like nuclear physics.
Hallman himself, the STAR spokesman, now 54, received his bachelor’s
degree in 1974 from Muhlenberg College in Pennsylvania, proceeding on to
Johns Hopkins
University, where he earned his Ph.D. in physics in 1982. Hallman
worked at Hopkins first as a post-doc and then a research scientist
until 1991, when he took a position with UCLA to work as a research
physicist on the STAR collaboration. Since 1996, Hallman has been a
staff scientist at Brookhaven, where he has worked continuously with
STAR on the QGP search.
Hallman
spoke to Science Watch from his office at Brookhaven.

RHIC and the STAR
collaboration have both been in the works for 15 years. How has the
perception of the QGP and the goal of the RHIC collaborations changed
over the years?
The underlying assumption has always been that in the very first
moments of the universe, when the universe was at extremely high
temperatures, matter didn’t exist as it does in our world. The
conjecture is that at sufficiently high temperatures, matter will
break down into its fundamental constituents: quarks and gluons. This
is the state known as a quark-gluon plasma. Around 25 years ago,
visionary people like T.D. Lee at Columbia University began to
postulate that one way to access, or create in the laboratory,
conditions similar to those that existed in the early universe was to
collide heavy nuclei together at the speed of light. That idea grew,
through a number of meetings, into the proposal for the Relativistic
Heavy Ion Collider facility. RHIC started running in 2000 and since
then there have been several very striking discoveries that suggest we
have indeed produced a new state of matter, but this in turn has
recently led to a debate about what it is we’ve actually discovered.
What’s the basis of the debate?
Back in the day when all this was being formed as a direction for
nuclear science in the U.S., people discussed the possible discovery
of a QGP, perhaps without defining it completely or worrying about the
definition too much. It was envisioned to be a state of matter in
which quarks and gluons would deconfine from the hadrons in
which they are normally constrained. So, for some people, and this is
certainly true for some of the people in the STAR collaboration, the
real thrust of the program, as it was articulated back in this
formative stage, was to discover the QGP. Other people would say that
the real goal was to discover a new state of matter without specifying
the detailed properties. So this debate heated up about a year ago,
and it continues at a somewhat lower pitch today.
Is this why you still haven’t actually, officially
announced the discovery of a quark-gluon plasma?
|
Highly Cited Papers by the STAR Collaboration, including T.J. Hallman, Published Since 1995
(Ranked by total citations)
| Rank |
Paper |
Citations |
| 1 |
K.H.
Ackermann, et al., "Elliptic flow in Au +
Au collisions at root sNN=130 GeV,"
Phys. Rev. Lett., 86(3): 402-7, 2001. |
239 |
| 2 |
C.
Adler, et al., "Disappearance of
back-to-back high-pT hadron correlations
in central Au + Au collisions at root sNN=200
GeV," Phys. Rev. Lett., 90(8): 082302,
2003. |
164 |
| 3 |
C.
Adler, et al., "Centrality dependence of
high-pT hadron suppression in Au + Au
collisions at root sNN=130 GeV,"
Phys. Rev. Lett., 89(20): 202301, 2002. |
161 |
| 4 |
J.
Adams, et al., "Transverse-momentum and
collision-energy dependence of high-pT
hadron suppression in Au + Au collisions at
ultrarelativistic energies," Phys. Rev. Lett.,
91(17): 172302, 2003. |
137 |
| 5 |
C.
Adler, et al., "Pion interferometry of root
sNN=130 GeV Au + Au collisions at RHIC,"
Phys. Rev. Lett., 87(8): 082301, 2001. |
129 |
|
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Yes. The question is whether we should make "the big
announcement" of the discovery of the QGP or "the big
announcement" that we’ve discovered a new state of matter and
say that it represents the full success of what we originally set out
to do. Within STAR, our view, as embodied in a white paper, was that
we’re really seeking the QGP and we have a specific definition of
that. And there are definitely some specific questions that need to be
answered before we can say with any certainty that that’s what we’ve
discovered. We’ve been a little bit conservative in this sense,
certainly to the frustration of some people who want us to go beyond
that.
But you have discovered something new?
There is no question that we’ve indeed produced a new state of
matter, and that’s extremely exciting.
So can you tell us what you’re seeing and why it doesn’t
satisfy the full requirement of a QGP?
There are certain key parts of our definition, and we’re trying
to be precise. Our official definition, as phrased in technical jargon
in our bible here, is that the QGP is a (locally) thermally
equilibrated state of matter in which quarks and gluons are deconfined
from hadrons so that the colored degrees of freedom become manifest
over nuclear rather than merely nucleonic volumes. In other words,
instead of protons, which we know have quarks and gluons in them, we’re
trying to demonstrate that we have a volume of matter in which quarks
and gluons exist—deconfined—over the size of a gold nucleus,
rather than merely in the protons and neutrons themselves. There are a
few key things you need to show to prove that this is what you’ve
got, and now we have some major pieces of experimental evidence. One
is the measurement of something called elliptic flow. The other is
called jet quenching.
Okay. Can you describe these in a way that we can
understand?
The first is a measure of the asymmetry in how particles are
produced in the collision. And we see what we expect to see there.
That’s strong evidence that the matter in the particles colliding is
what we call locally thermally equilibrated, which means the pieces
interact with each other strongly and collectively share the energy
from the collision.
Jet quenching is another very striking observation. Because quarks
can’t exist in nature "undressed," which means without
being bound to other quarks or anti-quarks, when you collide these
particles and two quarks hit each other, they go off in different
directions and immediately decay into a spray of particles called a
jet. These jets result from the hard scattering of two quarks, or a
quark and a gluon, or two gluons. And we know from lots of work at
other facilities that when we collide two protons, we should expect to
see jets of matter going sideways some known percentage of the time.
It’s predicted, though, that in a quark-gluon plasma, the
interaction of the particles when they exit the plasma might influence
what we see. If one of the scattered quarks or gluons had to go
through this QGP goop, it might be so strongly impacted that we wouldn’t
see a jet of particles coming out on that side. So that’s what we
call jet quenching, and that was also observed. When we collide two
nuclei of gold together, they have 197 protons and neutrons in each
one, but inside each of these particles are quarks and gluons, so we’re
colliding swarms of quarks and gluons, and we look for these jets of
particles going out sideways; we expect to see one on one side and a
balancing jet on the other. But what we observe, with a much higher
probability than we’d expect, is a jet coming out one side of the
collision but no recognizable jet of particles balancing it out on the
other side. We’ve shown that there is still energy coming out of the
other side—the energy has to be conserved. But because of the
interaction with this new state of matter, there’s much greater
dissipation, and so it’s not readily recognizable as a jet of
particles.
So what does that tell you, and why isn’t that enough to
establish that what you’ve got is this long-sought QGP?
If we use the theory to interpret this suppression of jets, or jet
quenching, what we come to understand is that matter is produced that
has an energy density 50 to 100 times that of normal nuclear matter.
That’s indirect proof that this matter is almost certainly not
composed of protons and neutrons, and that the "degrees of
freedom" are those of quarks and gluons. It’s indirect evidence
of deconfinement. And so these two measurements almost get us there,
but there is a further refinement. In effect, we’ve proven that the
system is thermally equilibrated at an early time and we’ve proven,
at least indirectly, that there is deconfinement and that the degrees
of freedom are those of quarks and gluons, but we haven’t proven
that we have all of these simultaneously. There’s one little further
push we have to make, and that’s what we’re working on now. We’re
studying it by measuring particles that contain heavy quarks, known as
charm and bottom quarks.
In the papers that have come out, you’ve made much of
this notion of a perfect liquid, as opposed to a QGP. What does that
mean?
It’s clear to everyone that something very exciting has been
accomplished at RHIC—that we’ve discovered this new state of
matter and it has some very intriguing properties. One such property
is that, unlike the original expectations, the constituents of this
matter are not weakly coupled, as they would be in gas, but seem to be
very strongly coupled and very strongly interacting, as would be the
case in a liquid. A plasma can be a liquid or a gas, so it doesn’t
mean it’s not a QGP. We just have to find out where it falls on the
continuum between the two, and that depends on the ratio of the
potential energy of the constituents to their kinetic energy. Our
plasma at RHIC seems to be closer to a liquid than a gas. But there’s
another facility that will do similar studies when it comes online in
a year or so, the Large Hadron Collider at CERN, which will have
significantly higher energies, a factor that some people think will
make the matter the LHC produces somewhat closer to being a gas than a
liquid.
Do you feel the pressure to make a definitive
announcement of a discovery one way or the other, before the LHC can
possibly beat you to it?
Our business is competitive by its nature. Certainly we think we’re
very close at Brookhaven, and we want to let people know about our big
successes as soon as we feel the case is strong enough. We think that
will be before the LHC turns on. We think it’s close.
In the heat of all this controversy, RHIC and
Brookhaven have had funding problems and have gotten help from an
unlikely source. Can you tell us about that?
Well, our country has a lot of challenges right now, and how we
fund all the priorities is a very challenging task. We feel that
nuclear science and RHIC are a high priority, but RHIC recently got
hit by a couple of realities. One was that because of the need to
balance priorities, funding for RHIC went down in the budget this
year. That, by itself, we could probably deal with, although not
without some really deep cuts. But the other critical factor is our
power costs. We had a long-standing agreement on what power would cost
us, but that agreement expired. Now we’re renegotiating, and the
price of electricity has jumped by close to a factor of two. That and
the reduced budget made it so that we weren’t going to have enough
weeks of running time to make a run worthwhile. Then, toward the end
of last year, we had an up-turn in the situation. I don’t really
know the details, but the gist of it is that several members of the
board that helps manage Brookhaven, led by board member Jim Simons of
Renaissance Technologies, an investment company, organized a $13
million contribution. Simons used to be a mathematician here at SUNY
Stony Brook. This contribution, combined with the DOE funding that was
already there, will allow us to have a very significant run this year.
At the moment, things are looking reasonably positive.
Science
Watch®, May/June 2006, Vol. 17, No. 3
Citing URL:
http://www.sciencewatch.com/may-june2006/sw_may-june2006_page3.htm |
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