UC Davis
Physics REU Program, Summer 2008
Candidates for galaxy clusters that pass (left) or fail (right)
visual checks. See Tom Johnson's writeup, below.
Students' names link to their final papers.
Condensed Matter Experiment
Kasey Kelly (Kenyon College; advisor Rena
Zieve) studied avalanches when grains composed of welded
spherical ball bearings are confined to a single layer in a rotating tumbler.
The motivation was to understand how earlier work by other students may have
been affected by warping of the container walls. Kasey found two signatures
that indicated warping. The first was a decrease in the apparent density of the
grains, since they could take up less space within the plane of the tumbler
by twisting slightly out of that plane. Since the density varies with the exact
arrangement of grains, observing density changes requires many avalanches.
Kasey's second signature solved this problem by relying on individual
configurations. She calculated histograms of the separations of pairs of
ball bearings. One would expect a first peak located at the ball diameter,
corresponding to any ball bearings that touch each other. Kasey found that
as the tumbler becomes less two-dimensional, this first peak splits into
three parts. Her work enables us to test quickly for warping in our further
measurements.
At a nanometer length scale, surfaces are far from smooth. Complicated
energetics determine whether one atomic species deposited on another material
grows in clumps, spreads smoothly, or some combination. Even without clumping,
the deposited material may be thicker in certain regions than others and form
steps. The steps have their own dynamics of migration and recombination. James Morad (Solano Community College; advisor Shirley
Chiang) used scanning tunneling microscopy (STM) and low-energy
electron microscopy (LEEM) to study surface structure when a small amount of
gold, corresponding to a few atomic layers, is adsorbed onto a germanium
sample. The work had two thrusts: obtaining a clean germanium surface as a
starting point, and later observing the structure formed by gold layers.
Sample cleaning involved bombarding with argon ions to blast any contaminant
atoms off the surface and then annealing at high temperature to remove any
craters formed on the surface. Although the procedure was not perfected during
the summer and some craters typically remained, James was able to observe a
series of atomic steps once gold was deposited. James has transfered to UC
Davis and is continuing his work during the school year.
Jason Veatch (University of Evansville; advisor
Rena
Zieve) studied the effect of uniaxial pressure on CeCoIn5 at low
temperatures, measuring how pressure shifts the superconducting transition
temperature. Jason's contribution was to extract useful data from a run where
we had no working thermometer at the sample. By comparing signals on warming
and cooling, Jason found the thermal time constant linking the sample to the
refrigerator. He then wrote a program to compute the sample's temperature
based on the refrigerator's temperature history. In a related project, Jason
set up CeIrIn5 samples for pressure cell measurements by polishing the
crystals and making low-resistance contacts for resistance measurements. This
material is unusual in that the transition to superconductivity as measured by
resistance appears at a significantly higher temperature than when the
transition is detected in heat capacity or magnetic susceptibility, and we
plan to monitor the temperature discrepancy under pressure.
Condensed Matter Theory
In a crystal, the electron orbitals of neighboring atoms overlap, leading to
interactions among the electrons and new orbitals that extend through the
crystal. The electron-electron interactions can give rise to phenomena such as
superconductivity or magnetic order. One of the simplest models that captures
some of these behaviors is the Hubbard Model, which considers the ability of
electrons to ``hop" from one location to a neighboring site and also an interaction energy
from having two electrons at the same site. When the two-dimensional Hubbard
Model has on average one electron per site, the result is antiferromagnetism:
magnetic order where electronic spins alternate direction and produce no bulk
magnetic moment. Shauna Story (University of
Arizona; advisor Richard
Scalettar) used Quantum Monte Carlo to test how
antiferromagnetism disappears as a lattice is diluted by having sites removed.
Site removal reduces the number of nearest neighbors and hence the electron
hopping; eventually it leads to disconnected sites with no possible
interactions.
Computational Complex Systems
Jake Ellowitz (Clark University;
advisor
Jim Crutchfield)
studied information sharing in simulations of reinforcement-based learning.
In the simulations, the problem was for robots to collide with walls as little
as possible while traveling through a room. The robots first had to discover
where the walls were, through trial-and-error. The robots can shorten
the learning process by communicating with each other. Jake accumulated
quantitative data on how information sharing affected learning, as
a function of both the likelihood of sharing and the density of robots.
For high densities, collective behavior of the robots emerges.
Biological Physics
Misfolded proteins are responsible for diseases from cystic fibrosis to
Alzheimer's. In many cases, misfolding leads to aggregation of proteins.
Diana Qiu (Yale University; advisor Daniel Cox)
examined configurations of the tumor suppressing protein p53. A protein
consists of a chain of amino acids, folded into a pattern that often involves
common structures such as helices. Computers are not yet fast enough to
determine how proteins fold. Instead, Diana ``threaded" the known amino acid
sequence for p53 onto a helix, with some flexibility in the spacing between
amino acids. Interactions among amino acids determine the energy of a
threading; for example, it may be favorable for one amino acid to lie
directly above another, exactly one turn of the helix apart. Diana looked
for potentially low-energy configurations, which she used as starting points in
a molecular dynamics code. The computer simulation let protein molecules
evolve in time, and helix structures that persisted for a few nanoseconds
were judged stable. Diana did find a stable helix structure. Results for
interacting proteins were less conclusive, perhaps because the length of
threaded helix was short.
Emily Ricks (University of Virginia;
advisor Xiangdong
Zhu) worked on the Oblique-Incidence Reflectivity
Difference (OI-RD) microscope that Professor Zhu's group is developing.
OI-RD detects chemical interactions through polarization changes
in reflected light. The technique has potential for high throughput.
It is also non-invasive and cannot itself affect the reactions,
unlike the commonly used fluorescent tagging. Emily set up a library
of several hundred small molecules in an array of tiny wells, while
keeping the molecules ordered in an intuitive way that can reduce errors
in positioning the different chemicals or in reading the results.
Emily also had to adapt the standard procedures for printing these
arrays since some of the equipment used was designed for fluorescence
measurements, which have somewhat different requirements than OI-RD.
Elementary Particle Experiment
Kathryn Marable (Brandeis University; advisors Bob Svoboda and Mani
Tripathi) worked on two separate projects. One related to
data analysis from the CACTUS telescope, which primarily observed the nearby
Draco cluster. Draco is about 95\% dark matter. If dark matter particles
coming from Draco interact with the earth's atmosphere, they can create brief
pulses of Cerenkov radiation. Having a thorough understanding of the detector
is crucial to the experiment. Kathryn installed and debugged a new piece of
simulation code for modelling the detector. In separate work, she also
designed and prototyped electronics for controlling photomultiplier tubes.
This latter work was for the LUX experiment, an attempt to view dark matter
through its interactions with an underwater tank of xenon.
The LUX experiment searches for dark matter through its interactions with
xenon. To reduce background noise, the xenon is surrounded by a large tank of
water. Energetic particles, such as muons, that enter the tank will produce
Cerenkov radiation in the water. Matching the time of the Cerenkov burst and
a signal from the inner xenon can eliminate certain events as spurious. Carlos Rojo (Rice University; advisors Bob Svoboda and Mani
Tripathi) worked on setting up photomultiplier tubes within the
water bath to detect Cerenkov radiation. The difficulty is in sealing the tube
casings to prevent water damage. To mimic the lengthy time periods the
sealings will have to hold during an actual experiment, Carlos heated the
casings over two weeks. The 3M polypropylene adhesive he chose did appear
sufficiently water-tight.
UC Davis particle physicists have worked for years on the Compact Muon
Solenoid (CMS), a detector at the Large Hadron Collider (LHC). Although
the hardware portion was completed several years ago, other work
continues: modeling how the detector will behave when LHC is
turned on later this year, and developing analysis tools. Matt Sanders (Washington and Lee University;
advisor John
Conway investigated how a Higgs particle that decayed via four
muons might appear at LHC. He wrote macros in ROOT to reconstruct the
initial Higgs energy from the muon information. By comparing results from
his algorithm and from a different calculation designed by another researcher,
Matt was able to verify that both methods functioned as desired.
Nuclear Physics
The huge accelerators for experimental particle physics boost light
particles such as electrons, protons, and positrons to almost the speed
of light before colliding them together. However, heavy ions such as
gold nuclei can produce even more energetic collisions. Their extra
mass more than compensates for their slower speeds. Analyzing a
gold-gold collision is immensely complicated, in part because
it is truly multiple near-simultaneous events involving
individual nucleons. Matt
Caulfield (Stevens Institute of Technology; advisors Manuel Calderon de la Barca
Sanchez and Daniel
Cebra) wrote a Glauber model simulation to extract hidden
information about heavy-ion collisions, such as the closest approach
of the ion centers during the event and the number of nucleons that
actively collide. Assuming a certain distribution for the nucleons
within the nucleus, Matt computed a distribution for the number of
charged hadrons that would be observed from collisions. The ultimate goal
is to be able to reconstruct properties of the nucleon collisions from
the data.
Cosmology
Over a period of six years, the Deep Lens Survey gathered optical data from five
regions of space. The "depth" of the survey comes because of the long
observation time, which averages out noise and allows distant, faint objects
to be seen. Although measurements ceased several years ago, analysis of the
data continues. Tom Johnson (Colorado College;
advisor Dave
Wittman) worked on distinguishing galaxy clusters. As very
large-scale structure, these clumps of galaxies can be used to study how the
mass distribution in the universe originated and evolved. Tom searched for
parts of the images where several neighboring pixels indicated more than
average numbers of galaxies. After comparing his list of galaxy cluster
candidates to lists generated through other algorithms, he examined remaining
candidates individually. In the end he found 58 previously unidentified
possible clusters, which will be used in further analysis efforts.
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