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."



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