Astronomers continue the search for antimatter
Finding antimatter may be more difficult than previously thought.
Provided by the Chandra X-ray Center, Cambridge, Massachusetts
October 31, 2008
Scientists are on the hunt for evidence of antimatter left over from the very early universe. New results using data from NASA's Chandra X-ray Observatory and Compton Gamma Ray Observatory suggest the search may have become even more difficult.
Elementary particles make up antimatter. Each has the same mass as its corresponding matter counterparts — protons, neutrons, and electrons — but the opposite charges and magnetic properties. When matter and antimatter particles collide, they annihilate each other and produce energy.
According to the Big Bang model, the universe was awash in particles of both matter and antimatter shortly after the Big Bang. Most of this material annihilated, but because there was slightly more matter than antimatter — less than one part per billion — only matter was left behind, at least in the local universe.
Black holes and pulsars power relativistic jets that scientists believe produce trace amounts of antimatter, but they've found no evidence for antimatter remaining from the infant universe.
How could any primordial antimatter have survived? Scientists believe there was an extraordinary period just after the Big Bang, called inflation, when the universe expanded exponentially in just a fraction of a second.
"If clumps of matter and antimatter existed next to each other before inflation, they may now be separated by more than the scale of the observable universe, so we would never see them meet," said Gary Steigman of Ohio State University, who conducted the study. "But they might be separated on smaller scales, such as those of superclusters or clusters, which is a much more interesting possibility."
In that case, collisions between two galaxy clusters, the largest gravitationally bound structures in the universe, might show evidence for antimatter. X-ray emission shows how much hot gas is involved in such a collision. If some of the gas from either cluster has antimatter particles, then there will be annihilation and gamma rays will accompany X rays.
Steigman used data obtained by Chandra and Compton to study the Bullet Cluster, an area where two large galaxy clusters crashed into one another at extremely high velocities. At a relatively close distance, and with a favorable side-on orientation as viewed from Earth, the Bullet Cluster provides an excellent test site to search for the signal for antimatter.
"This is the largest scale over which this test for antimatter has ever been done," said Steigman, whose paper was published in the October 2 issue of The Journal of Cosmology and Astroparticle Physics. "I'm looking to see if there could be any clusters of galaxies which are made of large amounts of antimatter."
The observed amount of X rays from Chandra and the non-detection of gamma rays from the Compton data show the antimatter fraction in the Bullet Cluster is less than three parts per million.
Moreover, simulations of the Bullet Cluster merger show these results rule out any significant amounts of antimatter over scales of about 65 million light-years, an estimate of the original separation of the two colliding clusters.
"The collision of matter and antimatter is the most efficient process for generating energy in the universe, but it just may not happen on very large scales," said Steigman. "But, I'm not giving up yet as I'm planning to look at other colliding galaxy clusters that have recently been discovered."
Finding antimatter in the universe could tell scientists about how long the period of inflation lasted.
"Success in this experiment, although a long shot, would teach us a lot about the earliest stages of the universe," said Steigman.
Steigman placed tighter constraints on the presence of antimatter on smaller scales by looking at single galaxy clusters that do not involve such large, recent collisions.