WASHINGTON, (UPI) -- Using a sensitive telescope hung
beneath a giant helium
balloon, an international team of scientists say they have determined
the universe is flat and
expanding forever.
Their report, which appears in Thursday's journal Nature,
is based on the most detailed picture
yet of the early universe at a time before the birth of the first stars,
when it was just hundreds of
thousands of years old and far more compact. The researchers say with
their work, they have
greatly updated and sharpened the focus of an image of the early universe.
A far more blurry
image of the early universe released nearly a decade ago was described
by one researcher as
peering at the face of God.
The data taken by the BOOMERANG experiment shed light,
researchers say, on the curvature
of the universe, the nature of matter and energy in intergalactic space
and whether the universe
will expand forever or collapse into a "Big Crunch."
"These are literally snapshots of what the universe looked
like when it was just a few hundred
thousand years old, fully a thousand times smaller and hotter than it
is today" said Andrew
Lange of the California Institute of Technology during a press conference
Wednesday.
"What BOOMERANG measures is the heat left over from the
Big Bang," Lange said, one of
the principal investigators in the international research team.
The experiment's Italian co-leader, Paolo de Bernardis
of the University of Rome, said the
BOOMERANG data may solve several problems, including the total amount
of matter and
energy in the universe.
The BOOMERANG telescope -- sensitive to microwaves --
circumnavigated Antarctica at a
height of about 24 miles (38 kilometres) for 10 days in December, 1998.
The scientific results
will also appear in Physical Review Letters, as well as in Nature.
The sensitive telescope studied the cosmic microwave
background radiation, which is believed
to be the glow of the universe when it was only 300,000 years old, before
the birth of the first
star. Part of the static seen on an unused television channel is caused
by the cosmic microwave
background.
Among the results claimed by the research team:
--The universe is flat, in the sense that light beams
through intergalactic space that were initially
parallel would remain parallel and would never meet or diverge.
--The universe went through a dramatic expansion in size
-- called "inflation" -- a split-second
after the Big Bang.
--The universe is expanding and will never recollapse into a "Big Crunch."
University of Chicago theorist Michael Turner said his
reaction to the study was, "Wow, wow
and wow." The first wow, he said, is that the universe is flat, the second
is that inflation
occurred and the third is that, "This is just the beginning. BOOMERANG
is beginning to test
what I think we will call the new cosmology."
The results of the BOOMERANG experiment are likely to
relegate some theories of how the
universe formed to the scrap heap, according to Canadian team member Richard
Bond, a
theoretician whose mathematical models of the early universe have played
a central role in the
research.
"We can now take the information and compare it to a
vast library of theories," said Bond, of
the Canadian Institute for Advanced Research and the Canadian Institute
for Theoretical
Astrophysics at the University of Toronto.
Among the discards, he said, will be any theory that
doesn't include inflation -- a rapid
expansion of the early universe that was first proposed as a way to explain
the relative
uniformity of the universe we now see.
The new data don't mean inflation is proved, said astrophysicist
Wayne Hu of the Institute for
Advanced Studies at Princeton University, but they are good evidence for
the idea. "This was a
test for the inflation theory," he said -- a test the theory passed.
Inflation theory predicted that much of the microwave
variation would be on a small scale. Hu
said -- about one degree across, as seen from Earth, and that is precisely
what the
BOOMERANG experiment showed.
Turner, though, said he thinks, "we're across the threshold" on proof of inflation.
The BOOMERANG data also appears to settle another long-standing
problem: whether the
universe has enough matter so that its expansion will someday stop, to
be followed by a long
collapse into a fiery "Big Crunch."
A flat universe, Turner said, can only exist if there is not enough matter to cause it to recollapse.
De Bernardis said, "We compared our data to (theoretical
models of various curved universes)
and found that the best model is a flat one."
That discovery, combined with the finding last year that
the universe is expanding more quickly
than expected, allows researchers to calculate how much matter and energy
there is in the
universe, he said.
About 5 percent of the universe is normal matter and
energy, he said. Another 30 percent is
dark matter, which is undetectable except by gravity. And the rest is
what he called "dark
energy," a still-mysterious form of energy that is driving the speed-up
of the universe's
expansion.
The cosmic microwave background, or CMB, was discovered
by accident in 1965. It was the
first really solid evidence that the Big Bang really did occur.
Modern theory says that for the first 300,000 years after
the Big Bang, the universe was so hot
that ordinary matter couldn't form and light particles could not travel
; it was an opaque,
super-hot, dense fluid. Waves in that fluid, driven by gravity, created
spots that were hotter than
others.
Then, as the fluid cooled, there came a point where matter
formed, light could travel, and the
universe as we know it could start to form. But, much as we can still
feel the heat of a fire even
though it has gone out, the heat of the fluid left a glow that is still
with us as the cosmic
microwave background.
Variations in that glow, according to Barth Netterfield
of the University of Toronto, the leader
of the Canadian BOOMERANG contingent, are "the oldest picture of the universe
you could
ever take."
The first microwave experiment to capture the public's
attention was the COBE satellite, whose
striking image of the universe was made to look like a red and blue Easter
egg.
The team behind COBE -- short for COsmic Background Explorer
-- reported their data in
1992, with the principal investigator, George Smoot, saying the images
were like looking at the
face of God.
The face of God, however, was blurry: COBE's picture
of the microwave background could
only see variations that were larger than seven degrees across, as seen
from Earth. By contrast,
the moon, which is much nearer, looks to be about half a degree across.
The BOOMERANG telescope can see variations that are one-sixth
of a degree across -- a
dramatic increase in sensitivity, Netterfield said.
"To be able to measure this with such precision is just
unreal," said Bond. "It's an amazing and
daunting thing."
BOOMERANG stands for Balloon Observations of Millimetric
Extragalactic Radiation and
Geomagnetics. The research team included members from the United States,
Italy, Canada,
and the United Kingdom.