Mysterious Source of High-Energy Cosmic Radiation Discovered

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Nov. 19, 2008

Steve Cole 
Headquarters, Washington 
202-358-0918 
stephen.e.cole@xxxxxxxx 

RELEASE: 08-301

MYSTERIOUS SOURCE OF HIGH-ENERGY COSMIC RADIATION DISCOVERED

WASHINGTON -- Scientists announced Wednesday the discovery of a 
previously unidentified nearby source of high-energy cosmic rays. The 
finding was made with a NASA-funded balloon-borne instrument high 
over Antarctica. 

Researchers from the Advanced Thin Ionization Calorimeter (ATIC) 
collaboration, led by scientists at Louisiana State University, Baton 
Rouge, published the results in the Nov. 20 issue of the journal 
Nature. The new results show an unexpected surplus of cosmic ray 
electrons at very high energy -- 300-800 billion electron volts -- 
that must come from a previously unidentified source or from the 
annihilation of very exotic theoretical particles used to explain 
dark matter. 

"This electron excess cannot be explained by the standard model of 
cosmic ray origin," said John P. Wefel, ATIC project principal 
investigator and a professor at Louisiana State. "There must be 
another source relatively near us that is producing these additional 
particles." 

According to the research, this source would need to be within about 
3,000 light years of the sun. It could be an exotic object such as a 
pulsar, mini-quasar, supernova remnant or an intermediate mass black 
hole. 

"Cosmic ray electrons lose energy during their journey through the 
galaxy," said Jim Adams, ATIC research lead at NASA's Marshall Space 
Flight Center in Huntsville, Ala. "These losses increase with the 
energy of the electrons. At the energies measured by our instrument, 
these energy losses suppress the flow of particles from distant 
sources, which helps nearby sources stand out." 

The scientists point out, however, that there are few such objects 
close to our solar system. 

"These results may be the first indication of a very interesting 
object near our solar system waiting to be studied by other 
instruments," Wefel said. 

An alternative explanation is that the surplus of high energy 
electrons might result from the annihilation of very exotic particles 
put forward to explain dark matter. In recent decades, scientists 
have learned that the kind of material making up the universe around 
us only accounts for about five percent of its mass composition. 
Close to 70 percent of the universe is composed of dark energy (so 
called because its nature is unknown). The remaining 25 percent of 
the mass acts gravitationally just like regular matter, but does 
little else, so it is normally not visible. 

The nature of dark matter is not understood, but several theories that 
describe how gravity works at very small, quantum distances predict 
exotic particles that could be good dark matter candidates. 

"The annihilation of these exotic particles with each other would 
produce normal particles such as electrons, positrons, protons and 
antiprotons that can be observed by scientists," said Eun-Suk Seo, 
ATIC lead at the University of Maryland, College Park. 

The 4,300-pound ATIC experiment was designed to be carried to an 
altitude of about 124,000 feet above Antarctica using a helium-filled 
balloon about as large as the interior of the New Orleans Superdome. 
The goal was to study cosmic rays that otherwise would be absorbed 
into the atmosphere. 

ATIC is an international collaboration of researchers from Louisiana 
State University, the University of Maryland, Marshall Space Flight 
Center, Purple Mountain Observatory in China, Moscow State University 
in Russia and the Max-Planck Institute for Solar System Research in 
Germany. ATIC is supported in the United States by NASA and flights 
are conducted under the auspices of the Balloon Program Office at 
NASA's Wallops Flight Facility in Virginia by the staff of the 
Columbia Scientific Balloon Facility. Antarctic logistics are 
provided by the National Science Foundation. 

For information on NASA's scientific balloon program, visit: 










http://sites.wff.nasa.gov/code820/ 


For information about NASA and agency programs, visit: 



http://www.nasa.gov 

	
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