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| Photo: Fred Ullrich, Fermilab |
Particles and prairie. For many
people, these words are synonymous
with Fermilab.
In the 1970s, when founding
director Robert Wilson led the
construction of the Tevatron
particle accelerator, Robert Betz
launched in the center of its
four-mile ring one of the earliest
and most ambitious prairie
reconstruction projects in the
state of Illinois.
Betz, who died on April 5,
was a professor of biochemistry
at Northeastern Illinois
University. He was one of the
first people to recognize the
importance of saving the native
prairie ecosystem. Known as "Professor Prairie," he traveled
across the Midwest to identify
and catalog "cemetery prairies,"
the last remnants of original
prairie that grew on pioneer cemeteries
and escaped development.
At Fermilab, he used his
knowledge and worked with
grounds crews and volunteers
to turn farmland back into the
original tallgrass prairie.
"There is a chain of people
who have inspired this region, for
which I would list [Henry David]
Thoreau, [John] Muir, Aldo
Leopold, May Watts, and then
Dr. Betz," said Stephen Packard,
director of Audubon of the
Chicago Region, speaking at the
Betz memorial symposium in
July. "It was visionary of Dr. Betz
early in his life to look around
and say, ‘There is still nature
here that is important to save.'"
Early on, Betz recognized
the importance of burns for
the well-being of the prairie. With
persistence and a big smile on
his face, he set out to convince
other scientists of the benefits
of prairie burns. Today, burns
are a standard tool to maintain
prairies and to control invasive
plants. While prairie plants with
their long roots survive the
fire, non-native plants succumb
to the heat.
More than 30 years after the
start of the Fermilab prairie
reconstruction project, the lab
is home to 1100 acres of prairie,
about 270 species of birds and
more than 50 species of butterflies,
thanks to the vision of
Professor Prairie.
Kurt Riesselmann
Supercomputers can play chess,
map DNA, and aid in the study
of dark energy. But recently they
were unleashed on a bold new
frontier: optimizing the production
of potato chips.
Imagine a conveyor belt carrying
a neat row of saddleshaped
Pringles-brand potato
chips. As the belt moves at
high speed, the air rushing past
the chips can lift them up and
send them sailing off the production
line.
"This is fundamentally a problem
of air-flow over the potato
chip," says Richard Herman,
chancellor of the University of
Illinois at Urbana-Champaign.
"Much like air-flow over the wing
of a plane, this is a problem in
computational fluid dynamics."
Herman, a mathematician,
presented the problem in June
at the 2007 National User
Facility Organization meeting at
Lawrence Berkeley National
Laboratory as an example of
public/private partnerships to
improve national competitiveness.
After analyzing the problem
using high-performance computers,
Proctor & Gamble redesigned
the chips and adjusted
the speed of the production
line so fewer chips go flying,
Herman says.
So if you really can't eat just
one, don't worry. Thanks to
supercomputers, there are more
chips per potato reaching chip
enthusiasts worldwide.
Lauren Younis
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| Photo courtesy of MoNA |
In the olden days, farmers would
travel for miles through the
American countryside to help
neighbors raise a barn.
A similar bustle was under
way in early July on the Michigan
plains, though the focus was
nuclear physics instead of farming.
College students–mostly
from the Midwest, but some
from as far away as California—converged on the National
Superconducting Cyclotron
Laboratory to help the lab's graduate
students and staff move the
modular neutron array (MoNA).
The box-shaped array,
assembled primarily by undergraduate
students and used
to detect neutrons, is composed
of 144 plastic bars, each two
meters long. It was moved to a
more spacious vault as part
of a major reconfiguration of the
lab, which is at Michigan State
University.
Each bar had to be hauled
by hand, and most of the hands
belonged to undergraduates.
"It was kind of like an assembly
line," reflected Tova Yoast-Hull, a junior from Kenyon
College in Ohio. "Except the
parts don't move down the
line–the people do." Pairs of
students lugged each 40-pound
bar down 70 meters of hallway.
Most challenging, however,
were the six wires running
from each bar, totaling 864
cables that had to be detached
and meticulously reconnected
at the proper terminals. All told,
the move and reinstallation
involved 27 people from 10 colleges,
and took about a week.
Eddy White, a senior from
the University of Notre Dame in
Indiana, found the work enlightening. "Having so much hands-on
experience with equipment,
you really learn how it works,"
he said.
The lone postdoctoral
researcher involved in the move,
Artemis Spyrou, reminisced
about the long hours she spent
assembling machinery in the
lab during her graduate school
days in Greece, where three
people managed all the equipment. "It's always fun to do
teamwork," she said. In her case,
there was a bonus: The only
other graduate student in her
group at the time, George
Perdikakis, became her husband.
Annie Jia, National
Superconducting Cyclotron
Laboratory
A video of busy students assembling
MoNA is available. Click here to see video.
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| Photo: Fred Ullrich, Fermilab |
When Aaron Chou heard about
an experiment in Italy that suggested the existence of an
exotic particle as a candidate
for dark matter, he was intrigued
enough to go looking for it.
His first stop: the Fermilab
cafeteria.
"The Fermilab cafeteria is a
wonderful place to talk to people
and ask around for available
equipment," says Chou, a postdoctoral
researcher at the lab.
Working the lab grapevine,
Chou (left, photo at bottom)
and William Wester, a scientist
in Fermilab's Particle Physics
Division, scrounged enough
parts to build their experiment
on a shoestring budget. They
borrowed a high-powered laser
and scavenged a spare Tevatron
magnet that could be operated
at the existing Fermilab Magnet
Test Facility, and kept the cost
to about $30,000.
Their project, called GammeV
(named for particle searches in
the gamma ray to milli-electronvolt
energy range), follows up
on an experiment called PVLAS
at Legnaro National Laboratory
in Italy two years ago that
suggested the existence of the
ultralight particle.
The new experiment involves
sending pulses of high-powered
laser light through an opening
in a magnet and toward a mirror.
Normally, scientists would
expect no photons, or light particles,
to show up on the other
side of the mirror. But if the new
ultralight particle exists, some
of the photons will convert into
the proposed particle, travel
through the mirror, and then
convert back into photons,
which scientists would detect
on the other side. It would
appear that light was passing
straight through a wall.
Though scientists are skeptical
of the suggested particle's
existence, the results from
Legnaro need to be checked,
says Chou, who strayed from
his usual area of research–cosmology–
to help put the project
together. "It's unlikely but not
impossible that the result is
correct. If it is, it would be one
of the most astounding discoveries
of this century," he says.
"Such a discovery could fundamentally
change the direction
of future experimental research
in particle physics. The potential
scientific impact and the
low cost of the experiment make
this a no-brainer. It's the type of
experiment you just have to do."
Amelia Williamson
Most particle physicists spend
at least a few hours a day
looking at a computer screen.
In their free time, however,
many prefer the "silver screen."
At Fermilab, the International
Film Society fills this need
each month by presenting films
from around the world. A
showing of Wes Anderson's
off-beat comedy The Life
Aquatic with Steve Zissou kicked off the society's new
season this summer.
The origins of the film society
go back to 1971. The
group's most important goal is "to provide a relaxed atmosphere
where we can interact
with our colleagues and be
entertained by a good movie,"
says scientist Tania Moulik,
who chairs the society.
"Many films provide a window
to different cultures, promoting
understanding and
providing a ground for common
discussion among viewers
from diverse cultures," she says–
especially important in a large,
international community such
as Fermilab's.
The public is invited as well,
and people stay to discuss a
film after its showing. This season,
offerings range from the
Charlie Chaplin classic The
Great Dictator to the contemporary Donnie Darko.
So, lean back and enjoy
the show. Just don't ask for popcorn:
Fermilab's Ramsey
Auditorium is a food-free
environment.
J. Bryan Lowder
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AtenciÓn, ACHTUNG, ATTENTION
The symmetry challenge:
Where has your symmetry been?
Our readers live in all parts of the globe, from Alaska to Wyoming; from Argentina to Zimbabwe. But
when a copy of symmetry lands in a mailbox, that's often not the end of its journey. We have
heard stories of symmetry being read in some quite surprising places, including hiking trails and
nude beaches.
What unusual places have you gone with a copy of the magazine in your suitcase or backpack?
Send your story, perhaps with a photo of you and the magazine, to letters@symmetrymagazine.org with subject line "Travel," or mail it to the address on our contact page. We will publish the best stories and
photos in an upcoming issue.

Photo illustration by Sanbox Studio
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Particle sudoku
Did you find last month's sudoku tough? Word
from our readers is that the puzzle in the Jun/Jul
07 issue of symmetry was much more difficult
than a regular sudoku. Reader and Fermilab
retiree Phil Martin, Sequim, Wash., wrote,
"Awesome sudoku! Can we look forward to more
in the future?"
To put those of you who are still stuck out of
your misery, we provide the solution to the right.
A larger-print version is online.
The solution to the puzzle is unique. Every one
of the Standard Model's 16 elementary particle
types appears in each row, column, and 4x4
sub-square. If you managed to complete the
puzzle or found any nifty tricks to solve it, let us
know at letters@symmetrymagazine.org.
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With regard to your story on dark energy (May 2007): Please explain the amount of known energy
there is in the universe. If there is a small percentage of known matter, what is the percentage of
known energy?
Richard Blaine, Savannah River Site, Aiken, South Carolina
Michael Turner, University of Chicago, replies:
That's a wonderful question. For energy in the universe, here are the "known knowns:"
- Cosmic microwave background (CMB) radiation, the echo of the big bang:
0.005% of the total matter/energy density of the universe
- Direct light from all the stars that have ever lived (due to redshifting this peaks near the infrared):
0.0001%
- Re-radiated light (by dust) from all the stars that have ever lived: 0.0001%
- Kinetic energy of all matter: 0.00003%
- Cosmic rays (particles believed to be accelerated by exploding stars with energies up to at least
1020 eV): at most 0.000005%
By far, the bulk of the known energy is the CMB radiation. The biggest known unknown, of course,
is the dark energy, accounting for 73% of the all the matter/energy. And at this stage, it is too early
to rule out unknown unknowns that may account for up to 10% of all the matter/energy.
Within our own Milky Way galaxy, cosmic-ray particles (mostly protons) trapped by the galaxy's
magnetic field have an energy density comparable to the CMB. However, outside the Milky Way
the energy density contained in cosmic rays is expected to be much less.
While reading symmetry (May 2007), I came across an article about Katie and Adam Yurkewicz moving
from Fermilab, Batavia, to CERN, Switzerland. I was floored when I realized that the home they
were leaving (424 Blaine St) is the home I grew up in. I attended grades 1-4 in the small school
building right across the street. I lived there until I got married. My father (the then-owner) lived
downstairs and my wife and I and our first child lived in the upstairs apartment for a number of years
after I got out of the army in 1968. My sister and her husband lived in the apartment before we
did. I did a double take when I saw the picture of the moving truck parked in front of the house. We
drive past the house every now and then, but I had no idea who lived there.
Small world, isn't it?
Kim Carlson, President, Savannah Community Association, Aurora, Illinois
Many readers of symmetry are undoubtedly familiar with the Dan Brown novel Angels and Demons,
which is staged partially at CERN. One of the characters, physicist Vittoria Vetra, is described as "CERN's resident guru of Hatha yoga."
If any physicist may rightly aspire to having been a "resident guru of Hatha yoga," it might be me.
For decades, CERN has had an active Yoga Club that provides yoga classes on site, but to my
knowledge, I am the only physicist who has taught Hatha yoga regularly at CERN.
Ever since I was trained as a yoga teacher in the 1970s, wherever I find myself for an extended
period of time, I arrange a free Hatha yoga class. I have offered such classes at Kent, Ohio;
Anchorage, Alaska; Berlin, Germany; New York City; Tsukuba, Japan (at the KEK laboratory); and
presently in Davis, California.
At CERN in the 1980s, I taught once a week for about four years on the second floor of Restaurant
No. 2. My students included other physicists who were avid runners, who saw yoga as a way to
increase flexibility.
Richard Breedon, University of California, Davis
Letters can be submitted via letters@symmetrymagazine.org
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