
For several years, physicists at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory (BNL), USA, have studied an unusual state of matter called the quark–gluon plasma, which they believe mimics the hot, dense particle soup that existed immediately after the big bang.
Now, the PHENIX collaboration at RHIC reports findings about a particle called the J/ø meson that will help physicists distinguish the properties of the quark–gluon plasma (QGP) from those of normal matter1.
To create a QGP, physicists crash gold nuclei together at close to the speed of light. This provides enough energy to break apart the protons and neutrons in the nuclei into their constituent quarks and gluons, which mediate the force between quarks. In this energetic mash up, a host of short-lived particles can form, including mesons, which are made up of a quark and an anti-quark.
When collisions of gold nuclei yield fewer J/ø mesons than expected from theoretical predictions, it indicates that a QGP has formed. Suppressed meson production can occur because the QGP weakens the binding force between the two quarks in the J/ø particle. The PHENIX collaboration’s detector (Fig. 1) counts the number of J/ø mesons created in collisions by detecting the electrons and muons—particles with the same charge, but more mass, than electrons—produced from J/ø decays.
Effects other than the formation of the QGP, however, can also suppress the yield of J/ø particles, which makes interpreting gold–gold collisions “ambiguous”, says Yasuyuki Akiba, a scientist at the RIKEN BNL Research Center and a member of the PHENIX collaboration.
To isolate these other effects, the PHENIX team analyzed data taken in 2003 and 2008 from collisions between deuterium—a proton and neutron—and gold, since these collisions cannot form a QGP. Even in the absence of a QGP, the team found the production of J/ø particles was more suppressed than expected at the highest relative velocities between the deuterium and the gold collisions. “Conventional models cannot describe the data,” says Akiba.
The team thinks the unexplained suppression may be related to how the apparent density of gluons in the gold nuclei, which determines the rate of J/ø production, varies with the speed of the deuterium.
More analysis is needed to determine whether this explanation is correct, but this work “gives a precise baseline that will be very useful for separating the quark–gluon plasma effects in gold–gold collisions,” says Akiba.
The corresponding author for this highlight is based at the Experimental Group, RIKEN BNL Research Center
gro-pr | Source: Research asia research news
Further information: www.riken.jp
www.researchsea.com
Further Reports about: anti-quark > BNL > Gluons > high-energy collision experiments > meson particles > Open Book Accounting > PHENIX > Quarks > Relativistic Heavy Ion Collider
More articles from Physics and Astronomy:
Electricity without losses
18.05.2012 | Universität Konstanz
Herschel Space Observatory study reveals galaxy-packed filament
18.05.2012 | McGill University
The first evidence in X-rays of a supernova shock wave breaking through a cocoon of gas around the star has been found.
This discovery may help explain why some supernova explosions are more powerful than others.
This supernova is called SN 2010jl and is found in a galaxy about 160 million light years from Earth.
SN 2010jl was first spotted by astronomers on November 3, 2010, and probably exploded about a month before that.
Observations with NASA's Chandra X-ray Observatory have provided the first X-ray evidence of a supernova shock wave breaking through a cocoon of gas surrounding the star that exploded. This discovery may help astronomers understand why some supernovas are much more powerful than others.
On November 3, 2010, a supernova was ...
An international research team led by Gerd Weigelt from the Max-Planck-Institut für Radioastronomie in Bonn reports on high-resolution studies of an active galactic nucleus.
The use of near-infrared interferometry allowed the team to resolve a ring-shaped dust distribution (generally called "dust torus") in the inner region of the nucleus of the active galaxy NGC 3783. This method is able to achieve an angular resolution equivalent to the resolution of a telescope with a diameter ...
Some populations of tiger snakes stranded for thousands of years on tiny islands surrounding Australia have evolved to be giants, growing to nearly twice the size of their mainland cousins. Now, new research in The American Naturalist suggests that the enormity of these elapids was driven by the need to have big-mouthed babies.
Mainland tiger snakes, which generally max out at 35 inches (89 cm) long, patrol swampy areas in search of frogs, their dietary staple. When sea levels rose around 10,000 years ago, some tiger snakes found themselves marooned on islands that would become dry and frog-free. With their favorite food gone, ...
HITS astrophysicists discover a new heating source in cosmological structure formation
So far, astrophysicists thought that super-massive black holes can only influence their immediate surroundings. A collaboration of scientists at the Heidelberg Institute for Theoretical Studies (HITS) and in Canada and the US now discovered that diffuse gas in the universe can absorb luminous gamma-ray emission from black holes, heating it ...
After ten years of development, the new German solar telescope GREGOR will start operating at the Spanish Observatorio del Teide of the Instituto de Astrofísica de Canarias on Tenerife. It is the largest solar telescope in Europe and number three worldwide.
It will provide the German and the international community of solar physicists with new and better instrumentation which will enable them to investigate our home star in unprecedented detail.
Studying the Sun is a key to understand the physical processes on and in the majority of stars. Moreover, there is ...
New technique reveals unseen information in DNA code
18.05.2012 | Life Sciences
Biologists Produce Potential Malarial Vaccine from Algae
18.05.2012 | Life Sciences
Listening to Chickens Could Improve Poultry Production
18.05.2012 | Agricultural and Forestry Science
10.05.2012 | Event News
WWU hosts Germany’s Biggest Giftedness Congress
09.05.2012 | Event News
Neuroscientists Discuss Latest Research Results in Potsdam
08.05.2012 | Event News