THE FOLLOWING RELEASE WAS RECEIVED FROM THE UNIVERSITY OF WASHINGTON,
IN SEATTLE, AND IS FORWARDED FOR YOUR INFORMATION.  (FORWARDING DOES
NOT IMPLY ENDORSEMENT BY THE AMERICAN ASTRONOMICAL SOCIETY.)  Steve
Maran, American Astronomical Society

FROM: Vince Stricherz
(206) 543-2580
[EMAIL PROTECTED]
(NOTE: researcher contact information at end)

For Immediate Release
July 27, 2004

NEW THEORY LINKS NEUTRINO'S SLIGHT MASS
TO ACCELERATING UNIVERSE EXPANSION

Two of the biggest physics breakthroughs during the last decade are the
discovery that wispy subatomic particles called neutrinos actually have a
small amount of mass and the detection that the expansion of the universe is
actually picking up speed.

Now three University of Washington physicists are suggesting the two
discoveries are integrally linked through one of the strangest features of
the universe, dark energy, a linkage they say could be caused by a
previously unrecognized subatomic particle they call the "acceleron."

Dark energy was negligible in the early universe, but now it accounts for
about 70 percent of the cosmos. Understanding the phenomenon could help to
explain why someday, long in the future, the universe will expand so much
that no other stars or galaxies will be visible in our night sky, and
ultimately it could help scientists discern whether expansion of the
universe will go on indefinitely.

In this new theory, neutrinos are influenced by a new force resulting from
their interactions with accelerons. Dark energy results as the universe
tries to pull neutrinos apart, yielding a tension like that in stretched
rubber band, said Ann Nelson, a UW physics professor. That tension fuels the
expansion of the universe, she said.

Neutrinos are created by the trillions in the nuclear furnaces of stars such
as our sun. They stream through the universe, and billions pass through all
matter, including people, every second. Besides a minuscule mass, they have
no electrical charge, which means they interact very little, if at all, with
the materials they pass through.

But the interaction between accelerons and other matter is even weaker,
Nelson said, which is why those particles have not yet been seen by
sophisticated detectors. However, in the new theory, accelerons exhibit a
force that can influence neutrinos, a force she believes can be detected by
a variety of neutrino experiments already operating around the world.

"There are many models of dark energy, but the tests are mostly limited to
cosmology, in particular measuring the rate of expansion of the universe.
Because this involves observing very distant objects, it is very difficult
to make such a measurement precisely," Nelson said.

"This is the only model that gives us some meaningful way to do experiments
on earth to find the force that gives rise to dark energy. We can do this
using existing neutrino experiments."

The new theory is advanced in a paper by Nelson; David Kaplan, also a UW
physics professor; and Neal Weiner, a UW research associate in physics.
Their work, supported in part by a grant from the U.S. Department of Energy,
is detailed in a paper accepted for publication in an upcoming issue of
Physical Review Letters, a journal of the American Physical Society.

The researchers say a neutrino's mass can actually change according to the
environment through which it is passing, in the same way the appearance of
light changes depending on whether it's traveling through air, water or a
prism. That means that neutrino detectors can come up with somewhat
different findings depending on where they are and what surrounds them.

But if neutrinos are a component of dark energy, that suggests the existence
of a force that would reconcile anomalies among the various experiments,
Nelson said. The existence of that force, made up of both neutrinos and
accelerons, will continue to fuel the expansion of the universe, she said.

Physicists have pursued evidence that could tell whether the universe will
continue to expand indefinitely or come to an abrupt halt and collapse on
itself in a so-called "big crunch." While the new theory doesn't prescribe a
"big crunch," Nelson said, it does mean that at some point the expansion
will stop getting faster.

"In our theory, eventually the neutrinos would get too far apart and become
too massive to be influenced by the effect of dark energy any more, so the
acceleration of the expansion would have to stop," she said. "The universe
could continue to expand, but at an ever-decreasing rate."

                            ###

For more information, contact Nelson at (206) 543-2027 or
[EMAIL PROTECTED]; Kaplan at (206) 685-3546 or
[EMAIL PROTECTED]; Weiner at (206) 854-7277 or
[EMAIL PROTECTED]

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