Kathy
Does the Cosmos Have a Direction?
by R. Cowen
East side, west side, all around the cosmos:
No matter which way an
observer looks, the vast reaches of space
appear the same. Indeed,
direction is meaningless in the simplest
version of the Big Bang model,
which holds that the primordial universe
expanded uniformly, like a
perfectly spherical balloon.
An alignment in the cosmos? The red line running
between the constellations
Aquila and Sextans, with Earth at its center,
indicates a special direction
in space. The polarization of radio waves
emitted by galaxy A, which lies
nearly parallel to this axis, rotates more
(blue corkscrew) on the journey
towards Earth than does the polarization
of radio waves from galaxy B
(green), which lies in a nearly perpendicular
direction. (Illustration:
Nodland)
A controversial report now challenges that
long-held tenet. An analysis of
the polarization of radio waves emitted by
distant galaxies suggests that
the universe may have a preferred direction
after all.
"This work defies the notion that there is
no up or down in space," says
Borge Nodland of the University of Rochester
(N.Y.). He and John P. Ralston
of the University of Kansas in Lawrence describe
their analysis in the
April 21 Physical Review Letters.
The results of the study, if verified, could
have startling consequences.
One possibility is that the Big Bang gave
rise to a nonuniform distribution
of matter and a somewhat lopsided expansion.
Alternatively, the interaction
of electromagnetic radiation with some kind
of exotic, unknown elementary
particle might produce a preferred direction
in space.
Several cosmologists dismiss the study out
of hand. They argue that the
report represents a premature effort by two
theorists searching for a
subtle effect among a disparate set of observations
gathered in the 1970s
and 1980s by radio astronomers using a variety
of telescopes. Many of the
observations predate high-resolution, multiple-array
radio telescopes.
However, Philipp P. Kronberg of the University
of Toronto, who studies
polarization and some years ago disproved
a similar claim about the
universe (SN: 8/7/82, p. 84), says that the
new work appears to be on a
sound footing.
In their study, theoretical physicists Nodland
and Ralston reviewed the
measured polarization of radio waves emitted
by 160 distant galaxies. The
original observations were designed to measure
Faraday rotation, a
well-documented effect in which intergalactic
magnetic fields rotate the
angle of polarization of waves traveling
through them. But the physicists
say they have found an extra twist.
Galaxies that lie along a particular direction
in space show significantly
greater polarization of their radio waves
than do galaxies in any other
direction.
>From Earth, this axis runs toward the constellation
Sextans in one
direction and the constellation Aquila in
the other. The effect is more
pronounced among the more distant galaxies
in the sample, the researchers
note.
"I really think this is much ado about nothing,"
says cosmologist Michael
S. Turner of the University of Chicago and
the Fermi National Accelerator
Laboratory in Batavia, Ill. "The number one
rule in astronomy is that you
can't reanalyze someone else's data to look
for an effect that [the
observations] were not designed to measure."
Kronberg disagrees. "They have seen a statistically
significant effect, and
it raises a flag that there is something
of fundamental interest here, and
it ought to be rechecked, as they say in
their paper."
Turner emphasizes that the existence of a
special direction in space does
not violate Einstein's theory of general
relativity, which allows for a
multitude of nonuniform universes. David
N. Spergel of Princeton University
says the finding appears to be at odds with
measurements of the cosmic
microwave background, the whisper of radiation
left over from the Big Bang.
The tiny fluctuations in that uniform background
would seem to be
inconsistent with a lopsided cosmos, he says.
References:
Nodland, B., and J.P. Ralston. 1997. Indication
of anisotropy in
electromagnetic propagation over cosmological
distances. Physical Review
Letters 78(April 21):1.
Sources:
Borge Nodland
Department of Physics and Astronomy
University of Rochester
Rochester, NY 14627