NASA Satellite Glimpses Universe's First Trillionth of a Second

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March 16, 2006

Grey Hautaluoma 
Headquarters, Washington 
(202) 358-0668 

Susan Hendrix 
Goddard Space Flight Center, Greenbelt, Md. 
(301) 286-7745 

RELEASE: 06-097

NASA SATELLITE GLIMPSES UNIVERSE'S FIRST TRILLIONTH OF A SECOND

Scientists peering back to the oldest light in the universe have new 
evidence to support the concept of inflation. The concept poses the 
universe expanded many trillion times its size in less than a 
trillionth of a second at the outset of the big bang. 

This finding, made with NASA's Wilkinson Microwave Anisotropy Probe 
(WMAP), is based on three years of continuous observations of the 
cosmic microwave background (CMB), the afterglow light produced when 
the universe was less than a million years old. 

WMAP polarization data allow scientists to discriminate between 
competing models of inflation for the first time. This is a milestone 
in cosmology. "We can now distinguish between different versions of 
what happened within the first trillionth of a second of the 
universe," said WMAP Principal Investigator Charles Bennett of the 
Johns Hopkins University in Baltimore. "The longer WMAP observes, the 
more it reveals about how our universe grew from microscopic quantum 
fluctuations to the vast expanses of stars and galaxies we see 
today." 

Previous WMAP results focused on the temperature variations of this 
light, which provided an accurate age of the universe and insights 
into its geometry and composition. The new WMAP observations give not 
only a more detailed temperature map, but also the first full-sky map 
of the polarization of the CMB. This major breakthrough will enable 
scientists to obtain much deeper insight into what happened within 
the first trillionth of a second of the universe. The WMAP results 
have been submitted to the Astrophysical Journal and are posted at 

http://wmap.gsfc.nasa.gov/results 

Big bang physics describes how matter and energy developed over the 
last 13.7 billion years. WMAP's observation of the blanket of cool 
microwave radiation that permeates the universe shows patterns that 
mark the seeds of what grew into stars and galaxies. The patterns are 
tiny temperature differences within this extraordinarily uniform 
light. WMAP discerns temperature fluctuations at levels finer than a 
millionth of a degree. 

WMAP can resolve features in the cosmic microwave background based on 
polarization, or the way light is changed by the environment through 
which it passes. For example, sunlight reflecting off of a shiny 
object is polarized. Comparing the brightness of broad features to 
compact features in the microwave background, or afterglow light, 
helps tell the story of the infant universe. One long-held prediction 
was the brightness would be the same for features of all sizes. In 
contrast, the simplest versions of inflation predict the relative 
brightness decreases as the features get small, a trend seen in the 
new data. 

"This is brand new territory," said WMAP team member Lyman Page of 
Princeton University in Princeton, N.J. "The polarization data will 
become stronger as WMAP continues to observe the microwave 
background. WMAP's new results heighten the urgency of seeking out 
inflation's gravitational wave sign. If gravitational waves are seen 
in future measurements, that would be solid evidence for inflation." 

With a richer temperature map and the new polarization map, WMAP data 
favor the simplest versions of inflation. Generically, inflation 
posits that, at the outset of the big bang, quantum fluctuations - 
short-lived bursts of energy at the subatomic level - were converted 
by the rapid inflationary expansion into fluctuations of matter that 
ultimately enabled stars and galaxies to form. The simplest versions 
of inflation predict that the largest-sized fluctuations will also be 
the strongest. The new results from WMAP favor this signature. 

Inflation theory predicts that these same fluctuations also produced 
primordial gravitational waves whose distortion of space-time leaves 
a signature in the CMB polarization. This will be an important goal 
of future CMB measurements which, if found, would provide a stunning 
confirmation of inflation. 

"Inflation was an amazing concept when it was first proposed 25 years 
ago, and now we can support it with real data," said WMAP team member 
Gary Hinshaw of NASA's Goddard Space Flight Center in Greenbelt, Md. 

WMAP, a partnership between Goddard and Princeton, was launched on 
June 30, 2001. The WMAP team includes researchers in U.S. and 
Canadian universities and institutes. For images and information on 
the Web about WMAP, visit: 

http://www.nasa.gov/vision/universe/wmap_pol.html 

	
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