Syracuse Joins the Search by Gary Ruderman
The first chancellor of Syracuse University allowed his cow to graze on
campus.
But from those pastoral roots, the university has grown to be leader in the
development of science and technology in New York state.
In the 1980s, Syracuse launched one of the state’s first Centers for Advanced
Technology–the CASE Center—to revitalize local economic growth through
technology. Last year, New York state was the second-largest sponsor, after
the federal government, of research at the university.
“Syracuse spins off a lot of businesses from its CASE Center, and the
Syracuse Research Corp. attracts quite a lot of very smart people,” observed
U.S. Representative James T. Walsh (R-NY, 25th District). Walsh chairs the
House Appropriations Committee’s subcommittee on Veterans Affairs,
Housing and Urban Development, and Independent Agencies. The
subcommittee funds basic research for NASA, the Environmental
Protection Agency and the National Science Foundation.
The university is also on the forefront of physics research.
For the first time, Syracuse University professors and
students are collaborating in a Fermilab experiment, a
search to validate CP violations. With Fermilab’s Joel Butler
and a team of 175 scientists and students from institutions
around the word, the Syracuse team will lead the most
exhaustive study of heavy quarks and B-quark physics
in an experiment planned for 2007. The BTeV (B-physics
at the Tevatron collider) approval document credited the
experiment with “great potential to discover new physics.”
Among the physics faculty at Syracuse University are Marina Artuso,
Tomasz Skwarnicki, and Sheldon Stone, co-leader of the BTeV experiment
at Fermilab. Their expertise—building and interpreting results from the Ring
Imaging Cherenkov Counter (RICH)—is a crucial element of BTeV. Syracuse
is responsible for building the RICH counter and has recently been joined by
a new assistant professor, Steve Blusk. The Syracuse team is also working
on building the pixel detector at the heart of the experiment.
The Syracuse group has been working with RICH counters since they were
developed in the 1990s. In the mid-1990s, Stone worked at Fermilab to test
the RICH counter for the CLEO experiment at
Cornell University, part of Syracuse’s 22-year
particpation in CLEO.
“Detectors can’t be reused,” Stone said, “since
the geometry of each experiment differs and the
technology changes and advances so quickly.”
For example, clearing out data from the
RICH Counter for the CLEO experiment took
2.5 microseconds; BTeV has the capability to clear
out the detector in just 132 nanoseconds. The
group finished construction of the CLEO III RICH in
August 2000, and has been taking data since then.
The BTeV experiment has four main parts: dipole
magnet, pixel detector, trigger and RICH detector.
The dipole magnet is centered on the interaction
region, inside of which is a silicon pixel detector
that tracks the particles and is coupled to a
“trigger.” The computerized trigger looks at each
of the estimated 7.5 million beam crossings a
second and decides which are most interesting to
investigate. Downstream of the pixels are other
tracking detectors followed by the RICH, an
electromagnetic calorimeter made from PbWO4
(lead tungstate) crystals and iron plates to detect
muons. Crystal calorimeters are another specialty
of Stone, who led the construction of the first such
device in a magnetic field, for CLEO II.
The goal of BTeV is to conduct the most extensive
study ever undertaken of CP violation in the decays
of particles containing B-quarks.
“BTeV is the most important experiment that a
high-energy physicist would be interested in,”
said Chaouki Boulahouache, a Syracuse University
graduate student earning his Ph.D. in August 2002.
Boulahouache is working on parts of the BTeV
pixel detector with Marina Artuso, his advisor.
The 50x400-micron pixel detector is in the center
of the 12-meter-long experiment.
For Orlokh Dorjkhaidav, another of the five
graduate students on the Syracuse team, BTeV
is a full-time summer job and a 20-hour-a-week
job during the school year.
“Syracuse is not that big of a city so you study
and study,” said Dorjkhaidav, a native of Mongolia.
He is working on the hybrid photon detector that
transforms light to electrical signals for analysis.
Joel Butler, of the lab’s Experimental Physics
Projects Department, and head of the BTeV
Research and Development Group, is co-leader
of the experiment with Stone. Stone focuses on
heavy quarks; Butler has worked for many years
on photoproduction of charmed particles.
Butler explained that at the beginning of the
universe—less than a second after the Big Bang—
there developed a slight excess of quarks over
antiquarks. As the universe cooled, the quarks and
antiquarks annihilated in photons, “but the slight
residual of quarks became us…”, meaning the
universe and its inhabitants. The Tevatron gives
experimenters the largest number of B-particles
and the biggest range of things to look at since the
beginning of the universe. B-quarks are produced
in only 0.1 percent of all Tevatron collisions.
A Fermilab scientist since 1979, Butler has
been working on building BTeV for eight years
“and I’m very enthusiastic. The technology is new
and exciting. We are breaking ground in particle
identification, tracking and computing. The physics
that comes out of it is very exciting.”
Butler added that BTeV has a National Science
Foundation grant to pursue and refine fault
tolerance computing—making decisions on which
particles are “interesting.” Fault tolerance has
promising future business applications, Butler said.
The first test of BTeV’s RICH detector is slated
for next spring. “BTeV’s taken a huge amount of
time,” said Stone, “and we’re still waiting for the
Department of Energy” to take further action.
The experimenters anticipate the $110 million
project being funded by the end of 2002, with
the experiment beginning late in 2007. But there
are no specific appropriation plans on the table,
although the recent HEPAP Subpanel on Long-
Range Planning for U.S. High-Energy Physics
emphasized that “it is important that we participate
in some” B-physics experiments in the US, with
the possibilities including “a dedicated hadronic
B experiment at the Fermilab Tevatron.”
Waiting isn’t easy, but the history of the university
offers a lesson in resilience.
Syracuse University was originally Genesee
College, founded in Ohio by the Methodist
Episcopal Church. It moved to a 50-acre farmland
area in central New York State in 1870 promoting
“equal education for men and women,” according
to the university’s history pages. Three years later
Syracuse University moved out of rented space
and dedicated its first building, the $136,000
Hall of Languages. True to the area’s rural nature,
the first Chancellor allowed his cow to graze on
campus.
In 1874, Syracuse offered the nation’s first
bachelor of fine arts degree. The school continued
to grow until World War I when 1,000 students
were drafted and overall enrollment fell more
than 30 percent.
The Great Depression meant a 10-percent salary
cut for professors as well the elimination of the
school’s 20-year-old college of agriculture, the
only private agricultural school in the country. Just
before World War II, the enrollment soared from
5,600 to 16,000. With the construction of more
than 20 new buildings, the school’s assets rose to
$200 million from $15 million. By 1946 Syracuse
welcomed 9,664 returning veterans, tripling the
school’s enrollment. Today, enrollment is more
than 18,000 full-time undergraduate and graduate
students.
The institution has a host of famous grads.
The College of Arts and Sciences counts writers
Joyce Carol Oates, William Safire and Stephen
Crane as alumni. Among prominent physicists,
Rubin Braunstein, co-inventor of the light-emitting
diode, is a graduate, as are Joel Lebowitz of
Rutgers, Harvey Scher of the Weizman Institute
and Dongqi Li of Argonne National Lab. Mark Reed
of Yale, a widely quoted source on nanoelectronics
and molecular electronics, received his Ph.D. at
Syracuse. George Campbell, who specialized in
particle physics, is now president of Cooper Union
College. Eileen Collins and F. Story Musgrave have
achieved milestones as NASA astronauts. Collins
was the first female to pilot and command the
space shuttle. Musgrave went on six space flights,
and worked outside the shuttle to repair the Hubble
Space Telescope in 1993.
In sports, Syracuse has produced two of the
premier running backs in football history: Jim
Brown, who went on to National Football League
stardom with the Cleveland Browns; and Ernie
Davis, the first African-American to win the
Heisman Trophy as the nation’s outstanding
college football player in 1961. Since 1980, the
Syracuse football team has played in the Carrier
Dome, the fifth-largest domed stadium in the U.S.,
and the first constructed in the Northeast region.
With its innovative roof of fiberglass fabric, the
dome dominating the Syracuse skyline could serve
to symbolize the university’s commitment to
science and technology leadership.
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