WMAP Reveals Neutrinos, End of Dark Ages, First Second of Universe

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March 7, 2008

J.D. Harrington 
Headquarters, Washington 
202-358-5241 
j.d.harrington@xxxxxxxx

Robert Naeye/Rob Gutro
Goddard Space Flight Center, Greenbelt, Md.
301-286-4453/4044

Lisa De Nike
Johns Hopkins University, Baltimore, Md.
443-287-9960 
Lde@xxxxxxx

Kitta MacPherson
Princeton University, Princeton, N.J.
609-258-5729
kittamac@xxxxxxxxxxxxx

Rebecca Johnson
University of Texas at Austin McDonald Observatory
512-475-6763
rjohnson@xxxxxxxxxxxxxxxxxxx

RELEASE: 08-079

WMAP REVEALS NEUTRINOS, END OF DARK AGES, FIRST SECOND OF UNIVERSE

WASHINGTON - NASA released this week five years of data collected by 
the Wilkinson Microwave Anisotropy Probe (WMAP) that refines our 
understanding of the universe and its development. It is a treasure 
trove of information, including at least three major findings:


New evidence that a sea of cosmic neutrinos permeates the universe 
Clear evidence the first stars took more than a half-billion years to 
create a cosmic fog 
Tight new constraints on the burst of expansion in the universe's 
first trillionth of a second

"We are living in an extraordinary time," said Gary Hinshaw of NASA's 
Goddard Space Flight Center in Greenbelt, Md. "Ours is the first 
generation in human history to make such detailed and far-reaching 
measurements of our universe."

WMAP measures a remnant of the early universe - its oldest light. The 
conditions of the early times are imprinted on this light. It is the 
result of what happened earlier, and a backlight for the later 
development of the universe. This light lost energy as the universe 
expanded over 13.7 billion years, so WMAP now sees the light as 
microwaves. By making accurate measurements of microwave patterns, 
WMAP has answered many longstanding questions about the universe's 
age, composition and development.

The universe is awash in a sea of cosmic neutrinos. These almost 
weightless sub-atomic particles zip around at nearly the speed of 
light. Millions of cosmic neutrinos pass through you every second. 

"A block of lead the size of our entire solar system wouldn't even 
come close to stopping a cosmic neutrino," said science team member 
Eiichiro Komatsu of the University of Texas at Austin.

WMAP has found evidence for this so-called "cosmic neutrino 
background" from the early universe. Neutrinos made up a much larger 
part of the early universe than they do today.

Microwave light seen by WMAP from when the universe was only 380,000 
years old, shows that, at the time, neutrinos made up 10% of the 
universe, atoms 12%, dark matter 63%, photons 15%, and dark energy 
was negligible. In contrast, estimates from WMAP data show the 
current universe consists of 4.6% percent atoms, 23% dark matter, 72% 
dark energy and less than 1 percent neutrinos. 

Cosmic neutrinos existed in such huge numbers they affected the 
universe's early development. That, in turn, influenced the 
microwaves that WMAP observes. WMAP data suggest, with greater than 
99.5% confidence, the existence of the cosmic neutrino background - 
the first time this evidence has been gleaned from the cosmic 
microwaves.

Much of what WMAP reveals about the universe is because of the 
patterns in its sky maps. The patterns arise from sound waves in the 
early universe. As with the sound from a plucked guitar string, there 
is a primary note and a series of harmonics, or overtones. The third 
overtone, now clearly captured by WMAP, helps to provide the evidence 
for the neutrinos.

The hot and dense young universe was a nuclear reactor that produced 
helium. Theories based on the amount of helium seen today predict a 
sea of neutrinos should have been present when helium was made. The 
new WMAP data agree with that prediction, along with precise 
measurements of neutrino properties made by Earth-bound particle 
colliders.

Another breakthrough derived from WMAP data is clear evidence the 
first stars took more than a half-billion years to create a cosmic 
fog. The data provide crucial new insights into the end of the "dark 
ages," when the first generation of stars began to shine. The glow 
from these stars created a thin fog of electrons in the surrounding 
gas that scatters microwaves, in much the same way fog scatters the 
beams from a car's headlights.

"We now have evidence that the creation of this fog was a drawn-out 
process, starting when the universe was about 400 million years old 
and lasting for half a billion years," said WMAP team member Joanna 
Dunkley of the University of Oxford in the U.K. and Princeton 
University in Princeton, N.J. "These measurements are currently 
possible only with WMAP."

A third major finding arising from the new WMAP data places tight 
constraints on the astonishing burst of growth in the first 
trillionth of a second of the universe, called "inflation", when 
ripples in the very fabric of space may have been created. Some 
versions of the inflation theory now are eliminated. Others have 
picked up new support.

"The new WMAP data rule out many mainstream ideas that seek to 
describe the growth burst in the early universe," said WMAP principal 
investigator, Charles Bennett, of The Johns Hopkins University in 
Baltimore, Md. "It is astonishing that bold predictions of events in 
the first moments of the universe now can be confronted with solid 
measurements."

The five-year WMAP data were released this week, and results were 
issued in a set of seven scientific papers submitted to the 
Astrophysical Journal. For further information, see

http://wmap.gsfc.nasa.gov

Prior to the release of the new five-year data, WMAP already had made 
a pair of landmark finds. In 2003, the probe's determination that 
there is a large percentage of dark energy in the universe erased 
remaining doubts about dark energy's very existence. That same year, 
WMAP also pinpointed the 13.7 billion year age of the universe.

Additional WMAP science team institutions are: the Canadian Institute 
for Theoretical Astrophysics, Columbia University, University of 
British Columbia, ADNET Systems, University of Chicago, Brown 
University, and UCLA.

For related images to this story, please visit on the Web:

http://www.nasa.gov/topics/universe/features/wmap_five.html

	
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