This file is automatically updated immediately after anyone submits a Call
for Contributed
Presentations. Here are the newly
registered presentations. Last editing update: March
27, 2008.
A=3, T=2, D=1, R=2,
S=15, O=1. Total=24 Return to Meeting Links
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T
O
T
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Baier, John
Carter, Tom
D'Cruz, Noella
Chamberlain, Jeff
Foster, Tom |
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D
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R
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Horner, Lenore
Horner, Lenore
Lindell, Rebecca
Lindell, Rebecca |
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Brown, Jacob
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Caceres, Gabriel
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Campbell, Sawyer
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Chott, Nic
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Garvin, Tim
S Goodin, Isaac |
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Grobe, Sebastian
S Kristoff,
James
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Linton, Ryan
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Lodes, Ryan
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Lovelace, Kara
S Norton, Matthew |
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Rolando, Daniel
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Stachyra, Michael
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Tockstein, Ryan
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Traynor, Thomas
S
Wischhusen, David |
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Active Learning
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John Baier,
johnbaier@isp.com or
john_baier@glenbard.org
Active Learning, Friday afternoon
Equipment needs: None
Comments: Please schedule me after 3:00 pm on Friday.
Inexpensive equipment for circuits and resonance. John
Baier, Glenbard South High School, Glen Ellyn, IL
61037.
Covers for one and two inch diameter four foot long fluorescent tubes
can be used to do resonance and the speed of sound. I will also show an
inexpensive way of using a 4x6 inch board with nails to do series,
parallel, and other simple circuits.
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Lenore Horner,
lhorner@siue.edu
Active Learning, Saturday morning
Equipment needs: powerpoint
Make Your Own Helmholz Resonator.
Lenore Horner, SIUE,
Edwardsville, IL 62026.
Most
people have blown across the top of a bottle to produce a pitch and in
general taller bottles produce lower pitches. Introductory physics
classes inadvertently perpetuate this over simplification by teaching
about pitch in cylindrical wind instruments where longer instruments
produce lower pitches. I present a relatively cheap and simple in-class
activity where students can discover for themselves that the pitch of a
bottle is more complicated than that of a cylindrical instrument.
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Rebecca Lindell,
rlindel@siue.edu
Active Learning, Either day
Promoting Active Learning in the Introductory Astronomy Classroom.
Rebecca Lindell and Tom Foster,
Southern Illinois University Edwardsville,
Edwardsville, IL 62026.
At Southern Illinois University Edwardsville, we have restructured our introductory astronomy course to include hands-on inquiry-based in-class group activities. These activities utilize a modified learning cycle approach to cover specific astronomical concepts that traditionally resist conceptual change, such as phases of the moon and seasons, or that students have difficulty mastering, such as Hubble's law and the Hertzsprung-Russell diagram. Each group activity is designed to be completed during one 50-minute class period and utilize hands-on equipment whenever possible. In this workshop we will discuss the design and implementation of these group activities into our introductory astronomy course, as well as results of evaluation of the successfulness of these activities at promoting conceptual understanding and reasoning skills. |
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Teaching Methods
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Tom
Foster, tfoster@siue.edu
Teaching Methods, Either day
Comments: Funded by SIUE's Excellence in Undergraduate Education
program.
Simple design problems for
physical science. Tom Foster,
Susan Wiediger, Southern Illinois University
Edwardsville, Edwardsville, IL 62026.
Illinois
State Learning Goal 11a
is all about design, yet it is the inquiry standard (11b) which gets
all the attention! At SIUE we have created a physical science course
with a design project as the capstone experience for the students. The
students are elementary education majors who are generally science
phobic, so we have created rubrics and other support mechanisms to help
the students succeed. Because of this, we feel the projects should have
applicability for grades9-12, if not younger. There is still more work
to do, but we will give you an update of our progress.
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Noella D'Cruz, ndcruz@jjc.edu
Teaching Methods, Either day
Equipment needs: computer and projector for PowerPoint presentation
Group Work in the Introductory Astronomy Class.
Noella D'Cruz,
Joliet Junior College,
Joliet, IL 60431.
Research has
shown that one of the ways students learn is through social
interactions. This semester I have incorporated a substantial amount of
group work in my introductory astronomy class to enable my non-science
major students to learn the material more deeply through interactions
with each other. I will discuss group projects, group tests, and other
activities that my students are involved in.
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Demonstrations
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Lenore
Horner, lhorner@siue.edu
Demonstrations, Saturday morning
Equipment needs: powerpoint
Using the Wiimote to teach Mechanics.
Lenore Horner, SIUE,
Edwardsville, IL 62026.
The remote for Nintendo's Wii
gaming system has a built-in 3-axis accelerometer and some position
capability. I will illustrate the possibilities and pitfalls of using
the remote to teach elementary kinematics.
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Research
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Tom Carter,
carter@fnal.gov
Research, Either day
Equipment needs: None besides PowerPoint
Comments: Please feel free to move this talk to the category you feel
is appropriate. I'm not sure if this is counted as "research" or as
"teaching methods"
Initial Results of Using
a PER Based Text and Online Tutoring System at a Community College.
Tom Carter, College of DuPage,
Glen Elynn, IL 60137.
I
will compare indicators of student knowledge and performance from a
class using the newer PER based textbook by Knight and the associated
MasteringPhysics online tutoring system to a class using the more
standard text by Halliday, Resnik and Walker and a less complex online
tutoring system, TYCHO. Indicators of student performance will include
average normalized gain on the FCI, performance on a locally
produced standardized exam and fraction of students successfully
retained in the class.
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Rebecca
Lindell, rlindel@siue.edu
Research, Either day
The Evolving Nature of Terminal Physics Masters Programs.
Rebecca Lindell, Kimberly Shaw and Lenore Horner,
Southern Illinois University Edwardsville,
Edwardsville, IL 62026.
Like many terminal masters programs, SIUE faces a shortage of qualified graduate students and thus risks elimination during funding crises. To better understand this problem, we undertook a research study investigating why students pursue terminal masters degrees in physics. As part of this research we collected survey data from nearly half of the identified terminal master's programs in the US. In addition, we conducted site visits at three institutions to determine why they produced nearly twice the national average of
master's degrees in year. Results of this research will be presented.
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Student Research Symposium
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Jacob
Brown, JE-Brown2@wiu.edu
Student Research Symposium, Either day
Equipment needs: Powerpoint file
The Mass-Radius Relationship of Neutron Stars.
Jacob Brown, Western Illinois
University, Macomb, IL 61455.
I
will start off by explaining the different principles that are
important to finding the mass-radius relationship. This will include
the Pauli principle for compact stars vs. gravity, the
Tolman-Oppenheimer-Volkov equation, and the many different equations of
state. Next I will go into the project that I have been working on to
create a flexible program that will allow us to take different
equations of state and compare them to find the ultimate equation of
state. The final part of my presentation is to go into the goals for
the future that I want to attempt to do in getting this program up and
running.
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Daniel Rolando, dvrolando2@eiu.edu
Student Research Symposium, Saturday morning
Equipment needs: Yes, I will use a PowerPoint file. A computer that
runs MATLAB is desired. I will need the computer-projector system.
Comments: I prefer the time for my presentation to be at 10 am or after.
Application of
Molecular Dynamics to the Simulation and Visualization of the Motions
of Gas Atoms. Daniel Rolando,
Jie Zou, Eastern Illinois University, Charleston, IL 61920.
This
project applies a computational method, Molecular Dynamics, to the
study and simulation of the microscopic interactions and the resulting
motions of gas atoms. The current study is carried out for a simulation
cell of fifty Argon atoms based on the approach in Ref. [1]. Future
study will be performed for other materials, such as silicon. The force
between atoms is modeled by the Lennard-Jones pair potential. The
atomic positions and velocities are computed as functions of time by
numerically integrating Newton's Equations of Motion based on the
finite-difference method. A computer program is written in MATLAB to
implement the numerical algorithm. The obtained atomic trajectories are
presented in both still images and animations. The animations will help
students visualize the motions in a many-particle system. Equilibration
and equilibrium properties, such as the velocity distribution, are also
studied. [1] N. Giordano and H. Nakanishi, Computational Physics
(Addison-Wesley, 2006), 2nd ed.
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Gabriel Caceres,
gabriel-caceres@augustana.edu
Student Research Symposium, Friday afternoon
Equipment needs: Using PowerPoint presentation
CDMS Veto
Stability Study and Calibration. Gabriel
Caceres, Augustana College, Rock Island, IL 61201.
Most
experiments searching for dark matter particles have been led deep
underground to minimize the background produced by cosmic rays. The
Cryogenic Dark Matter Search (CDMS) lies 1/2 mile
underground in the Soudan Mine in Minnesota. Even though the muon rate
is
lowered by a factor of 10^5, the rate is still high enough to
produce background signals. To solve this problem, scintillator panels
have
been placed around the detector to veto cosmic induced events. This
work
studies the behavior over time of the scintillator veto panels. By
analyzing
and tracking the response to a LED pulser system, the stability was
determined to be within 3%. The absolute energy scale of the spectrum
was
then calibrated using radioactive sources, as well as the muon
distribution.
Knowing the absolute energy scale and where the veto trigger threshold
lies
provides useful information for calculating the amount of background
that
can be rejected.
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Ryan Lodes,
rdlodes@ilstu.edu
Student Research Symposium, Friday afternoon
Equipment needs: powerpoint, Projector, computer
Modeling Correlated Gene Distributions Within a Strand of DNA.
Ryan Lodes, Illinois State
University, Normal, IL 61761.
We
model a set of DNA strands consisting of one hundred or more genes, and
the genes code for one of twenty traits. In our model, traits one
through ten have meaning, and eleven through twenty represent junk DNA.
In order to be viable, a strand must have at least three genes for each
of traits one through ten. Each DNA strand, which represents and
individual of a population, is allowed to reproduce based on its
calculated fitness. During reproduction, it may mutate and exchange a
segment of its strand with another strand. After each reproduction
cycle, the strand fitness is calculated. We report on the distribution
of correlated genes within a DNA strand as the population evolves.
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Kara Lovelace and Michael
Stachyra, swdaniels@eiu.edu
Student Research Symposium, Friday afternoon
Equipment needs: Powerpoint
Angular Dependence of the Efficiency of Polarizers. Kara
Lovelace, Michael Stachyra and Dr. Steve Daniels,
Eastern Illinois University, Charleston, IL 61920.
The
angular dependence on the efficiency of crossed polarizers was
measured. Polarized light with axis perpendicular to the transmission
axis of a polarizer was incident on that polarizer. Transmitted light
was measured with lock in amplification. The efficiency of the
polarizer was measured as a function of incidence angle for the light.
Data will be presented indicating that the polarizer transmits less
than 1 part in 10,000 of the incident light it but this efficiency can
change by a factor of 4 over an angular incidence range of about
10°.
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Thomas
Traynor, ttraynor@iwu.edu
Student Research Symposium, Saturday morning
Investigation
into Factors Affecting the Operating Deflection Shapes of a Mandolin.
Thomas Traynor,
Illinois Wesleyan,
Bloomington Il, IL 61701.
Like any vibrating object the front and back plate of a mandolin will
have mode shapes and operating deflection shapes when vibrated. The goal
of this project was to test whether or not shaking the front plate, a
common practice by luthiers during construction, changes the operating
deflection shapes that occur during the vibration of the front plate.
Some luthiers claim that shaking the front plate during construction
will actually break down some of the cellular structure in the wood
causing the instrument to have a better sound, like a well played
mandolin. Using speckle pattern interferometry, the front plate of a
mandolin was characterized during construction before and after it had
been shaken. This data will also be compared to the analysis of the
front and back plate of a student mandolin.
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Ryan
Tockstein, rtockst@siue.edu
Student Research Symposium, Either day
Equipment needs: Will be using PowerPoint file
Effect Of Area Ratio Changes On Exit Pressure In A C-D Rocket
Nozzle. Ryan Tockstein,
Southern Illinois University Edwardsville, Edwardsville, IL 62026-1654.
The
research presented involves the pressure changes in a chemical rocket
engine nozzle. Specifically, the research explains how changing the
area ratio of a rocket nozzle affects the pressure of the exhaust gas
at the exit of the nozzle. Equations involving the pressure, area
ratio, and mach number were analyzed to show the relationship of the
area ratio and exit pressure. Results of this project will be presented.
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James Kristoff and Ryan Linton,
jskrist@ilstu.edu
Student Research Symposium, Either day
Equipment needs: Computer, Projector
Comments: We will be using a powerpoint File.
Turning Heat into Electricity: Making Better Thermoelectrics.
James Kristoff and Ryan Linton,
Illinois State University,
Normal, IL 61761.
For
nearly two hundred years we've known about
materials that could be used to convert heat into electricity. However,
these thermoelectrics have been somewhat inefficient. The new field of
nanoscience has re-opened the search for higher efficiency to enable
the recovery of waste heat from factories and automobiles and to enable
new high efficiency refrigerators. Our focus is on the study the
properties of silicon and germanium when they are combined in atomic
layers at the nano-scale. We have constructed a special deposition
system to make these new materials and plan to measure their properties
as a function of layer composition and thickness.
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Sebastian Grobe, grobe@ilstu.edu
Student Research Symposium, Saturday morning
Equipment needs: We will bring our own laptop, will need a projector for our Mac.
Comments: Please schedule Sebastian for talk #6 within the 7 ILP talks.
Limitations of Decomposition Based Imaging.
Sebastian Grobe,
University High School and ILP, Illinois State University,
Normal, IL 61790.
We examine
theoretically and experimentally an imaging scheme that uses the
scattered light intensity profile to reconstruct the locations of
absorbers embedded in a turbid medium. This method is based on an a
priori knowledge of the scattered light patterns associated with a
single absorber that is located at various positions inside the medium.
We discuss the range of validity of this method, its sensitivity with
regard to noise and propose an algorithm to improve its accuracy.
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Sawyer Campbell, grobe@ilstu.edu
Student Research Symposium, Saturday morning
Equipment needs: We will bring our own laptop, will need a projector for our Mac.
Comments: Please schedule Sawyer for talk #7 within the 7 ILP talks.
Calibration of Webcams for Imaging.
Sawyer Campbell,
Intense Laser Physics Theory Unit, Illinois State University,
Normal, IL 61790.
We
generalize a previously proposed imaging scheme to situations for which
the set of hidden objects embedded in the highly scattering medium can
take arbitrary shapes. We compare the accuracy of images obtained from
optical detection fibers with those from a CCD camera. The latter
approach is more efficient and can be applied to non-contact
geometries, but it requires an a priori linearization of the obtained
digitized images. We discuss some details of this calibration for the
camera and establish its potential as a new tool for decomposition
based imaging.
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Nic Chott, grobe@ilstu.edu
Student Research Symposium, Saturday morning
Equipment needs: We will bring our own laptop, will need a projector for our Mac.
Comments: Please schedule Nic for talk #2 within the 7 ILP talks.
Classical Phase Space Approach to Pair-Creation.
Nic Chott,
Intense Laser Physics Theory Unit, Illinois State University,
Normal, IL 61790.
We explore
the mutual coherence properties of electrons that are created by a
sub-critical time-dependent force field. We compare the spatial
evolution of the quantum field theoretical density with that of a
relativistic classical mechanical ensemble. We find that portions of
the electron cloud that were created sufficiently far from each other
are not able to show interference patterns as they pass each other. The
corresponding classical phase space density reveals interesting spiral
shaped gaps, which have their manifestation in the corresponding
quantum field theoretical data.
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David Wischhusen, grobe@ilstu.edu
Student Research Symposium, Saturday morning
Equipment needs: We will bring our own laptop, will need a projector for our Mac.
Comments: Please schedule David for talk #1 within the 7 ILP talks.
Role of External Forces in Pair-Creation.
David Wischhusen, Q. Su, R. Grobe,
Intense Laser Physics Theory Unit, Illinois State University,
Normal, IL 61790.
Relativistic quantum electrodynamics describes the complicated quantum
field theoretical nature of electrons and positions during the
interesting process of their creations. Theoretical studies to date
about these interactions are limited by our ability to obtain and
analyze the solutions for the complicated systems. The newly developed
computational quantum field theory has opened the field to answering
many fundamental questions. Many famous mysteries such as the Klein
paradox and the Zitterbewegung have been revisited and could be
resolved. The validity of some models, on the other hand, has been
questioned concerning important issues regarding locality and causality
during these processes. I am proposing a set of computer simulations to
investigate the effects due to a scalar potential versus a vector
potential to model an external force. This work will help us to
understand the fundamental nature of locality and causality.
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Matthew Norton, grobe@ilstu.edu
Student Research Symposium, Saturday morning
Equipment needs: We will bring our own laptop, will need a projector that talks with our Mac.
Comments: Please schedule Matthew Norton for talke #3 within the 7 ILP talks.
Monte Carlo Simulations to Optimize Portfolios.
Matthew Norton, Q. Su, R. Grobe, E.A. Norton,
Intense Laser Physics Theory Unit, Illinois State University,
Normal, IL 61790.
The counter
intuitive reduction of the variance for a combination anti- and
uncorrelated random signals is not only of interest in statistical
physics but of essential importance in understanding the multi-stock
portfolios in the financial world. The balancing (minimization of the
variance) of portfolios has been intensely studied by Markowitz,
Michaud and Ibbitson. I will use random number based Monte-Carlo
numerical simulations to study the stability of the weights that
characterize a particular portfolio. I will study the sensitivity of
the optimization with regard to a small variation in the parameters
that define the random signals. I will also examine the question
whether the optimization operation and the time averaging commute. This
question is non-trivial as the optimization can be a nonlinear process
for which is it difficult to get a good intuition.
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Tim Garvin, grobe@ilstu.edu
Student Research Symposium, Saturday morning
Equipment needs: We will bring our own laptop, will need a projector for our Mac.
Comments: Please schedule Tim for talk #4 within the 7 ILP talks.
Laser Beam Widening Mechanisms in Turbid Media.
Tim Garvin,
Intense Laser Physics Theory Unit, Illinois State University,
Normal, IL 61790.
We examine
theoretically and experimentally the transverse intensity profile of a
laser beam as it traverses through a turbid medium. By increasing the
concentrations of milk in an aqueous solution we examine the transition
from the weakly scattering to the diffusive regime. The experimental
data of the transverse beam profiles are inferred in a non-contact
geometry from photos of the exit surface of the medium for various
scattering strengths. The intensity distributions are compared with
theoretical data are obtained from Monte Carlo simulations.
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Isaac Goodin, grobe@ilstu.edu
Student Research Symposium, Saturday morning
Equipment needs: We will bring our own laptop, will need a projector for our Mac.
Comments: Please schedule Isaac for talk #5 within the 7 ILP talks.
Using Shadows in Imaging in Highly Scattering Systems.
Isaac Goodin, Intense Laser Physics Theory
Unit, Illinois State University, Normal, IL 61790. We suggest that the
concept of the point-spread function traditionally used to predict the
blurred image pattern of various light sources embedded inside turbid
media can be generalized under certain conditions to predict also the
presence and location of spatially localized absorbing inhomogeneities
based on shadow point spread functions associated with each localized
absorber in the medium. The combined image obtained from several
absorbers can then be decomposed approximately into the arithmetic sums
of these individual shadow point spread functions with suitable weights
that can be obtained from multiple regression analysis. This technique
permits the reconstruction of the location of absorbers.
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Other
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Jeff Chamberlain,
jchamber@ic.edu
Other, Either day
Economy Robot using the SX Chip: The Programmable Acceleration
Car.
Jeff Chamberlain, Illinois College,
Jacksonville, IL 62650. This project modified a radio-controlled car by
replacing the motor control circuitry with a simple circuit using the
SX microcontroller. Programs in BASIC control the motor allowing a wide
variety of motion. LED indicators and pushbutton switches were added to
the car's body to create a self-contained variable acceleration car.
Potential experiments in basic mechanics and in robotics will be
discussed.
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Newly
Registered Presentations and Updates (added descriptions)
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