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From
•>>March 2005
Rainer J. Fries answers
a few questions about this month's fast moving front in the
field of Physics.
Field: Physics
Article: Hadron production in heavy ion collisions: Fragmentation and recombination from a dense parton phase - art. no. 044902
Authors: Fries,
RJ;Muller, B;Nonaka, C;Bass, SA
Journal: PHYS REV C, 6804: (4) 4902-4902, OCT 2003
Addresses: Duke Univ, Dept Phys, Durham, NC 27708 USA.
Duke Univ, Dept Phys, Durham, NC 27708 USA.
Brookhaven Natl Lab, RIKEN, BNL Res Ctr, Upton, NY 11973 USA.
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Why
do you think your paper is highly cited?
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“In this work we propose a new way to describe the hadronization of a quark gluon plasma.”
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With the advent of our paper the so-called baryon puzzles at
the Relativistic Heavy Ion Collider (RHIC) could be solved. At
present our paper provides the most comprehensive description of
hadron spectra at RHIC so far. It further provides very direct
evidence that quark degrees of freedom are present during the
collision through a quark counting rule for an observable called
elliptic flow. This was met with great excitement, since most
signals of the phase transition are only indirect and hard to
interpret.
Does
it describe a new discovery or a new methodology that's useful to
others?
Several groups are working with the same idea and try to
refine our understanding of high energy nuclear collisions.
Because of its simplicity I expect quark recombination to be a
very useful tool for the further analysis of data from RHIC and
future experiments, like the Large Hadron Collider at CERN. The
first goal of RHIC was to prove that a quark gluon plasma is
created. The quark counting rule that can be understood with
quark recombination is a major step toward that claim.
Could
you summarize the significance of your paper in layman's terms?
In this work we propose a new way to describe the
hadronization of a quark gluon plasma. A few microseconds after
the Big Bang, the universe was extremely hot. The temperature
was roughly (~ 1,000,000,000,000 K), more than 1,000 times
hotter than in the interior of the sun. Under such conditions
all matter dissolves into the most fundamental building blocks.
Even atomic nuclei, protons, and neutrons can no longer exist,
but evaporate into quarks and gluons. When the universe expanded
and cooled to a certain critical temperature, a phase transition
occurred at which the quarks and gluons were freezing out and
creating bound states, the known hadrons. The protons and
neutrons among these hadrons eventually formed the nuclei of all
the chemical elements observed in the universe. The phase
transition to the quark gluon plasma is studied at the
Relativistic Heavy Ion Collider (RHIC) at Brookhaven National
Lab on Long Island. This machine smashes gold ions into each
other with extreme energies (about 40 TeV per collision). Part
of this energy is converted into heat. For a very short time,
roughly 10^(-23) seconds, the temperature peaks above the phase
transition temperature and a quark gluon plasma is created. We
try to study the properties of this high-temperature phase by
analyzing the particles created in the collision. Our paper
describes the hadronization process through a recombination of
quarks into bound states (the hadrons). Several observations at
the Relativistic Heavy Ion Collider could not be understood with
conventional wisdom, e.g., through an angle of 90 degrees from
the beam axis as many protons as pions are seen with large
momentum (several GeV/c), while one expected to see a ratio of
roughly 1:4. In our paper we explain how protons (consisting of
3 quarks) are boosted to larger momentum by a factor of 3, while
pions (consisting of 1 quark and 1 antiquark) are only boosted
by a factor of 2, which cancels the inherent suppression of
protons.
How
did you become involved in this research?
I first started working on problems related to high-energy
nuclear collisions while working on my Ph.D. in Regensburg,
Germany. I got involved full-time with RHIC physics during my
stay as a postdoc at Duke University, where this paper was
written in collaboration with Berndt Muller, Chiho Nonaka, and
Steffen A. Bass.
Dr. Rainer J. Fries
Research Associate, Nuclear Theory Group
School of Physics and Astronomy
University of Minnesota
Minneapolis, MN, USA
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