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'Bubbles' of broken symmetry in quark soup

Date:
February 15, 2010
Source:
DOE/Brookhaven National Laboratory
Summary:
Scientists report the first hints of profound symmetry transformations in the hot soup of quarks, antiquarks and gluons produced in most energetic collisions. These new results thus suggest the opportunity to test some crucial features of symmetry-altering bubbles speculated to have played important roles in the evolution of the infant universe.

Scientists at the Relativistic Heavy Ion Collider report the first hints of profound symmetry transformations in the hot soup of quarks, antiquarks, and gluons produced in RHIC's most energetic collisions.
Credit: Image courtesy of DOE/Brookhaven National Laboratory

Scientists at the Relativistic Heavy Ion Collider (RHIC), a 2.4-mile-circumference particle accelerator at the U.S. Department of Energy's Brookhaven National Laboratory, report the first hints of profound symmetry transformations in the hot soup of quarks, antiquarks, and gluons produced in RHIC's most energetic collisions. In particular, the new results, reported in the journal Physical Review Letters, suggest that "bubbles" formed within this hot soup may internally disobey the so-called "mirror symmetry" that normally characterizes the interactions of quarks and gluons.

"RHIC's collisions of heavy nuclei at nearly light speed are designed to re-create, on a tiny scale, the conditions of the early universe. These new results thus suggest that RHIC may have a unique opportunity to test in the laboratory some crucial features of symmetry-altering bubbles speculated to have played important roles in the evolution of the infant universe," said Steven Vigdor, Brookhaven's Associate Laboratory Director for Nuclear and Particle Physics, who oversees research at RHIC.

Physicists have predicted an increasing probability of finding such bubbles, or local regions, of "broken" symmetry at extreme temperatures near transitions from one phase of matter to another. According to the predictions, the matter inside these bubbles would exhibit different symmetries -- or behavior under certain simple transformations of space, time, and particle types -- than the surrounding matter. In addition to the symmetry violations probed at RHIC, scientists have postulated that analogous symmetry-altering bubbles created at an even earlier time in the universe helped to establish the preference for matter over antimatter in our world.

RHIC's most energetic collisions create the kind of extreme conditions that might be just right for producing such local regions of altered symmetry: A temperature of several trillion degrees Celsius, or about 250,000 times hotter than the center of the Sun, and a transition to a new phase of nuclear matter known as quark-gluon plasma. Furthermore, as the colliding nuclei pass near each other, they produce an ultra-strong magnetic field that facilitates detecting effects of the altered symmetry.

Now, early data from RHIC's STAR detector hint at a violation in what is known as mirror symmetry, or parity. This rule of symmetry suggests that events should occur in exactly the same way whether seen directly or in a mirror, with no directional dependence. But STAR has observed an asymmetric charge separation in particles emerging from all but the most head-on collisions at RHIC: The observations suggest that positively charged quarks may prefer to emerge parallel to the magnetic field in a given collision event, while negatively charged quarks prefer to emerge in the opposite direction. Because this preference would appear reversed if the situation were reflected through a mirror, it appears to violate mirror symmetry.

"In all previous studies of systems governed by the strong force among quarks and gluons, it has been found to very high precision that events and their mirror reflections occur at exactly the same rate, with no directional dependence," Vigdor said. "So this observation at STAR is truly intriguing."

At RHIC, the parity-violating bubbles are formed in a random way, possibly with oppositely oriented charge separation in bubbles at different locations. Averaged over many events there would appear to be no parity violation, even though there were violations locally in each event. Although allowed by quantum chromodynamics (QCD), the underlying theory that describes the strong nuclear force, such local strong parity violation has never been detected directly.

"The key to observing the effect in high-energy nuclear collisions is to study correlations among the particles emerging from the collision," said Nu Xu of Lawrence Berkeley National Laboratory, the spokesperson for the STAR collaboration.

The theory suggests that particles with the same sign of electric charge should tend to be emitted from such local parity-violating regions in the same direction, either both parallel, or both anti-parallel, to the magnetic field arising in the collision, whereas unlike-sign particles should be emitted in opposite directions.

"We have observed a correlation among emitted charged particles of the predicted type, with the degree of directional preference increasing as the collisions vary from head-on to more grazing," Xu said.

STAR data also suggest the local breaking of another form of symmetry, known as charge-parity, or CP, invariance. According to this fundamental physics principle, when energy is converted to mass or vice-versa according to Einstein's famous E=mc2 equation, equal numbers of particles and oppositely charged antiparticles must be created or annihilated. If CP symmetry had not been broken at some very early time in the evolution of our universe, the particles and antiparticles created in equal numbers in the Big Bang would subsequently have annihilated one another in pairs, leaving no matter to form the stars, planets, and people that now populate our world.

While some small violations of CP symmetry have been found in previous laboratory experiments, those violations are far too weak to account for the amount of matter remaining in the universe today. Likewise, the signs of possible local CP violation at STAR cannot explain the global predominance of matter in today's world, but they may offer insight into how such symmetry violations occur.

"The features observed at STAR are qualitatively consistent with predictions of symmetry-breaking domains in hot quark matter," said Vigdor. "Confirmation of this effect and understanding how these domains of broken symmetry form at RHIC may help scientists understand some of the most fundamental puzzles of the universe, and will be a subject of intense study in future RHIC experiments."

"For example," he said, "we will want to see if the signal disappears, as predicted, at lower collision energies, where the produced matter is no longer hot enough to make the transition to the quark-gluon plasma phase. These future studies will further check the early work, will test more mundane possible explanations for the observed effects, and will explore a wide range of related phenomena."

Research at RHIC is funded primarily by the U.S. Department of Energy's Office of Science and by various national and international collaborating institutions.

Video.


Story Source:

The above story is based on materials provided by DOE/Brookhaven National Laboratory. Note: Materials may be edited for content and length.


Cite This Page:

DOE/Brookhaven National Laboratory. "'Bubbles' of broken symmetry in quark soup." ScienceDaily. ScienceDaily, 15 February 2010. <www.sciencedaily.com/releases/2010/02/100215101018.htm>.
DOE/Brookhaven National Laboratory. (2010, February 15). 'Bubbles' of broken symmetry in quark soup. ScienceDaily. Retrieved September 23, 2014 from www.sciencedaily.com/releases/2010/02/100215101018.htm
DOE/Brookhaven National Laboratory. "'Bubbles' of broken symmetry in quark soup." ScienceDaily. www.sciencedaily.com/releases/2010/02/100215101018.htm (accessed September 23, 2014).

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