Fwd: WMAP Reveals Neutrinos, End of Dark Ages, First Second of Universe
Henk Elegeert
hmje at HOME.NL
Sat Mar 8 08:52:19 CET 2008
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---------- Forwarded message ----------
From: NASA News <hqnews at mediaservices.nasa.gov>
Date: Fri 07 Mar 2008 17:00:01 EST
Subject: WMAP Reveals Neutrinos, End of Dark Ages, First Second of Universe
To: NASA News <hqnews at mediaservices.nasa.gov>
March 7, 2008
J.D. Harrington
Headquarters, Washington
202-358-5241
j.d.harrington at nasa.gov
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 at jhu.edu
Kitta MacPherson
Princeton University, Princeton, N.J.
609-258-5729
kittamac at princeton.edu
Rebecca Johnson
University of Texas at Austin McDonald Observatory
512-475-6763
rjohnson at astro.as.utexas.edu
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
-end-
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