By
MATTHEW FORDAHL
AP Science Writer
APRIL 02, 2000 - The
invisible and so far unidentified dark matter that accounts for 90 percent
of the universe could soon be brought to light as scientists develop
sensitive detectors capable of sniffing out tiny particles predicted by
theory but not yet proven to exist.
Teams of researchers are
racing to build the devices even though they might be hunting for
something that occurs only in the minds of theoretical physicists. If so,
a generation of theories can be tossed out.
But if the weakly
interacting massive particles WIMPs are detected, the finding
could solve fundamental mysteries of the universe: how it formed after the
Big Bang, the nature of its structure and whether it will all end in a Big
Crunch.
"It
will certainly be one of the great discoveries in the history of
science,'' said physicist Joel Primack of the University of California,
Santa Cruz. "It will be a window on a completely different aspect of
the universe.''
Astronomers have known for
70 years that visible matter is only a small part of the universe.
Something that exerts a strong gravitational tug, for instance, causes the
outer stars of a spiral galaxy to revolve faster than they should, given
what is visible.
Other dark matter
possibilities have been ruled out. Dead stars, large planets and black
holes, once thought to be leading candidates, are now considered unlikely.
Weighty but ghostly WIMPs are currently the prime suspects.
Physicists theorize that the
tiny particles originated during the Big Bang, but they only interact
weakly with the protons and neutrons of the visible universe. If real, 10
trillion WIMPs may be zipping through every 2 pounds of matter here on
Earth every second.
A dozen experiments
worldwide are based on the assumption that occasionally a WIMP might smack
into normal matter. But the challenge has been to differentiate them from
other particles that zip through the cosmos.
Scientists announced the
first results from new ultracold detectors last month, ironically while
all but debunking the findings of Italian researchers who claimed they
possibly found the elusive particles.
The Italian Dark Matter
Experiment, or DAMA, used detectors that emit flashes of light whenever a
particle collides with sodium iodide atoms. Researchers theorized that the
number of hits would increase in June and decrease in December, as the
Earth moves faster or slower through a theoretical cloud of the
hypothetical particles.
Sure enough, the detectors
buried a mile underground registered a small increase in bombardments.
Though DAMA's experiment
could differentiate possible WIMPs from charged particles, it could not
distinguish the elusive mystery matter from ordinary neutrons. The fact
that it's a mile underground shields it from most but not all stray
neutrons.
"There's
no way to tell what's triggering it,'' said Primack, who was a co-author
of a paper first suggesting WIMPs might be cold dark matter. "That's
why I call it an unsophisticated detector.''
A more discriminating
detector cooled to near absolute zero and buried 30 feet beneath Stanford
University registered hits like the Italian experiment, but its more
detailed findings showed the events were most likely caused by ordinary
neutrons.
"The
important aspect of the current results is that we have pushed that
technology through to the forefront of the field,'' said Stanford's Blas
Cabrera, a principal investigator of the Cryogenic Dark Matter Search.
"In a sense, it's a bit unfortunate that there's a focus on this
direct comparison with the DAMA results.''
Rather than just registering
hits, the American team is able to make two specific measurements the
amount of heat released and the amount of electricity that is discharged.
"For
every event, getting two different kinds of information lets you see a
much clearer picture of what is causing the event,'' Primack said.
Ten U.S. universities worked
to develop, test and run the device that soon will be moved to an
abandoned iron mine in northern Minnesota, where it will be shielded by
4,300 feet of rock and earth. Sensitivity is expected to increase by a
factor of 100 when the $12 million, six-year project gets under way.
"This
is a very difficult measurement,'' said Tony Spadafora, associate director
of the Center for Particle Astrophysics at UC Berkeley. "You're
looking for a new hypothetical effect and you have to eliminate known
backgrounds.''
At least five other similar
cryogenic experiments are being built or are planned around the world.
Other researchers are focusing on creating the particles with high-speed
accelerators.
If found, the weight of
WIMPs estimated to be 50 times heavier than a proton would help
physicists determine the mass of the universe, a figure that could mean
the difference between a cosmos that expands forever or collapses on
itself.
But confirmation also would
validate a popular and elegant theory that predicts a yet-to-be-found
partner for every known particle. WIMPs may be the lightest and most
stable supersymmetric particle, said Katherine Freese of the University of
Michigan.
"If
you discover the dark matter, you've not only discovered a major
astrophysical question what is the universe made of but also are
getting at trying to understand the nature of fundamental physics, the
nature of particles,'' she said.
And because WIMPs are not
the ordinary particles that make up people, planets and stars, it would
make everything that is known today a very small minority member of the
cosmos.
"What's
fascinating, if we're right, is that most of the stuff of the universe is
other than the protons and neutrons that we're used to,'' Spadafora said.
"The implication is that most of the universe is something else. This
is the ultimate Copernican revolution.'' |