Radiation flashes may help crack cosmic mystery
Faint, fleeting blue flashes of radiation emitted by particles that travel faster than the speed of light through the atmosphere may help scientists solve one of the oldest mysteries in astrophysics.
For nearly a century, scientists have wondered about the origin of cosmic rays鈥攕ubatomic particles of matter that stream in from outer space. 鈥淲here exactly, we don鈥檛 know,鈥� said Scott Wakely, Assistant Professor in 萌妹社区ics at the University of Chicago. 鈥淭hey鈥檙e raining down on the atmosphere of the Earth, tens of thousands of particles per second per square meter.鈥�
Recent results from the Pierre Auger Cosmic Ray Observatory suggest that the highest-energy cosmic rays may come from the centers of active galaxies. But the vast majority of the cosmic rays seen at Earth originate from its own galaxy, from sources that are still unknown. Tracking down these sources is crucial to developing a comprehensive understanding of the phenomenon, scientists say.
The University of Chicago鈥檚 Enrico Fermi suggested more than 50 years ago a process that, in its modern form, could allow the shock waves of exploding stars to propel most cosmic rays to their high energies. The idea remains popular, but unverified.
Wakely now has a $625,000 grant from the National Science Foundation to develop an instrument that might reveal important new data about the nature and origin of cosmic rays. Working in collaboration with Simon Swordy, the James Franck Professor in 萌妹社区ics at Chicago, they plan to make detailed measurements of Cerenkov radiation, which cosmic rays emit when they travel faster than the speed of light through the atmosphere.
While many people believe that nothing moves faster than light, 鈥渨hat鈥檚 actually the case is nothing can go faster than light can go in a vacuum,鈥� Wakely explained. But light moves slower in air and water than it does in a vacuum.
鈥淪o it鈥檚 possible that you get a particle which goes through the atmosphere faster than light does. And when that happens, you get the equivalent of a sonic boom, but with electromagnetic radiation. And that light boom is called Cerenkov radiation.鈥�
Wakely and Swordy are particularly interested in measuring the energy and mass of cosmic rays. But the density of molecules in the atmosphere stands in the way. When high-energy charged particles hit the top of the atmosphere, it鈥檚 like smashing into 30 feet of water. The individual particles break into a shower of smaller pieces, frustrating attempts to measure them directly.
Incoming cosmic-ray particles trigger two flashes of Cerenkov radiation. The first occurs when the original particle enters into the atmosphere, but the resulting shower of secondary particles also emits Cerenkov light. In a 2001 article published in Astroparticle 萌妹社区ics, the University of Utah鈥檚 David Kieda, along with Swordy and Wakely, proposed a ground-based 鈥渄irect Cerenkov technique.鈥� The idea was to record both flashes of Cerenkov light.
Many experiments are designed to record the second flash of Cerenkov light. These include a collaboration called VERITAS (Very Energetic Radiation Imaging Telescope Array System), to which Swordy and Wakely belong. But no one had ever looked for that first Cerenkov flash until Kieda, Swordy and Wakely pointed out that it should be there.
The first scientists to see direct Cerenkov light belong to a European group that operate the High Energy Stereoscopic System (HESS), an array of telescopes in the African nation of Namibia. 鈥淭hey showed that even with non-optimum equipment, you could actually do something useful,鈥� Wakely said. 鈥淲ith equipment designed to do this properly, we can do even better.鈥�
The idea behind direct Cerenkov detection was to combine the precision of balloon-borne cosmic-ray instruments with the far greater detection area afforded by ground-based arrays like VERITAS and HESS. 鈥淭his is something that鈥檚 never been possible before,鈥� Wakely said.
Low-energy cosmic rays are pervasive. But as their energy increases, their frequency drops dramatically. Scientists try to work around this obstacle by building extensive detector arrays on the ground. Another strategy: fly their instruments on high-altitude, helium-filled balloons into the atmosphere, where fewer air molecules get in the way.
Both methods involve trade-offs. 鈥淏alloon-borne experiments are small, but exquisite in their detail,鈥� Wakely said, while ground-based experiments are huge but offer poor resolution.
Most cosmic rays are protons or other types of charged particles. But some of them consist of the nuclei of iron atoms or other heavy elements. An iron nucleus traveling at nearly the speed of light produces approximately 700 times more light than a single proton.
鈥淲e came up with this idea because we had done both direct measurements of cosmic-ray nuclei before they interact in the atmosphere鈥攐n balloons and spacecraft鈥攁nd also work with air shower detection at ground level,鈥� Swordy said.
Source: University of Chicago
