Vortex Motion in Niobium Thin Films
Jesse Young, Prof. Joseph Amato, Colgate University
In the mixed state of a superconductor, magnetic flux penetrates the superconductor in quantized bundles called vortices. A vortex is a small cylindrical region where the metal returns to its normal conducting state. A current sent across a thin film will induce the vortices to move, inducing power loss and heating. Using an atomic force microscope, it is possible to create a periodic array of pinning sites to study vortex
The Effects of Mechanical Strain on Mesoscopic Bismuth Thin Films
Steven A. Waldauer, State University of New York at Buffalo
A prior research project at Michigan State University, involving thin bismuth films, found that the electrical resistance of the films seemed to vary with an applied mechanical strain. Furthermore, this effect seemed to increase as temperatures decreased. This current project, began as an REU program at Michigan State, intends to further explore this phenomenon in detail.
The current stages this project involves sample production and the continuing experimentation of samples at decreasing temperatures. Bismuth film samples are produced using a photolithography process on a glass substrate. Each bismuth pattern is a few microns wide and about 100 to 150 angstroms thick. Piezoelectric wafers provide mechanical strain. Samples are glued to the wafer using vacuum grease, and the entire sample is cooled in a cryostat. Commercial strain gages are used for calibration. Resistance measurements are collected electronically using standard four terminal measurements and data acquisition software.
Future experimentation
will provide more precise measurements of the effects of applied strain
on measured resistance as well as determine the temperature at which this
effect is maximized. It is expected that the conclusion of this project
will provide a better definition of this phenomenon as well as a possible
physical explanation.
Linewidth of Transitions in Mn12 Acetate
Joe Loomis, Prof. M. E. Parks, Colgate University
Mn12 Acetate is a ferromagnetic molecular cluster with a total spin S = 10 that exhibits quantum tunneling of its magnetic moment at low temperatures. Time domain terahertz spectroscopy is used to study the linewidth of the transition from m = 10 to m = 9 , which has an energy 300 GHz. The linewidth provides information about how the magnetic moment couples to its environment, which is important for understanding the tunneling process. I measured the linewidth to be surprisingly large (5 GHz). Possible explanations for this linewidth will be discussed.
Interface-Controlled and Diffusion-Limited Kinetics of Alloy Formation in Pb/Sn Thin Films
Anthony Clark, Prof. E. J. Cotts, Binghamton University
Thin film reactions regularly exhibit two distinct growth regimes, interface-controlled and diffusion-limited. It can be shown that after the growing alloy reaches a certain thickness, the interface-controlled kinetics will always change over to a diffusion-limited process. In this study, thermal analysis on the Pd/Sn system was performed using differential scanning calorimetry (DSC). The rate of one-dimensional intermetallic growth in our planar samples was calculated from heat flow data. In Pd/Sn (L) diffusion couples, we found that interface-controlled kinetics are sustained for an extended period of time. At longer times we observed the transition to diffusion-limited kinetics, at which point our data qualitatively agrees with previous studies. To our knowledge, this is the first time the interface-controlled growth mechanism has been so explicitly portrayed for the Pd/Sn system.
Pentacene Thin Film Field Effect Transistors
Katie Lotterhos, Binghamton University, Prof. Robert Dynes, University of California at San Diego
Research at UCSD is exploring pentacene as a possible substitute for
silicon in thin film field effect transistors (FET). With fabrication possible
at lower temperatures, pentacene FETS would be easier to mass produce and
cheaper than silicon. Several attempts were made to develop the pentacene
thin film layer. The three methods used were growing crystals by vapor
phase transport, growing films via vapor phase transport, and growing films
by thermal evaporation. We will discuss the methods used to fabricate a
pentacene FET, results, and pathways for further research.
Particles and Fields
Feynman Diagrams in Quantum Electrodynamics
Fred Vonstein, Union College
The following independent study is an effort to understand Quantum Field Theory; the simplest of which is Quantum Electrodynamics (QED), which describes interactions between charged particles and photons. The focus of the project was to learn how to calculate Feynman Diagrams. As an exercise, Compton scattering is calculated from the Feynman Diagram method. The calculation required a background study in such topics as covariant formalism, second quantization, and S-Matrix expansion.
Solution of the "Degenerate Model" for Parafermi Particles of Order Two
Terry Tarnowsky, Prof. Charles Nelson, Binghamton University
Fundamental theories allow for the existence of types of particles other than fermions and bosons. However, there has been no experimental identification of any of these mystery particles.
Paraparticles are particles with a paraquantization order greater than 2 (p>2) which obey a generalized statistics. Normal Fermi-Dirac and Bose-Einstein statistics correspond to paraquantization order 1 (p=1). Our goal is to obtain a generalization of the normal BCS theory for the case of p=2 parafermions. As an initial step, we construct a generalization of the quasi-spin treatment of a model simpler than that used in the standard BCS theory. In particular, we have solved the "Degenerate Model" for p=2 parafermions.
An Investigation of Future CDF Measurements of W Helicity in the Decay of the Top Quark
Brock Tweedie, University of 91自拍论坛
The top quark will soon be coming under greater scrutiny at CDF with RUN II of the Fermilab Tevatron collider. I have performed an investigation that gauges CDF抯 improved ability to measure the helicity of W bosons produced in the top quark抯 immediate decay. This measurement provides a direct indication of the spin structure of the weak interaction in that decay. Using simulated CDF Run II data, I study the W helicity sensitivity of the top decay抯 kinematic observables. Optimization of the helicity measurement via appropriate choices of observables and data cut is also addressed.
Tests of the e94 Range Stack Upgrades
Adam Rogers, Binghamton University, Dr. James Frank, Brookhaven National Laboratory
The purpose of the e787/e949 AGS experiments at Brookhaven National Laboratory is to detect the rare decay of a positive kaon into a positive pion and a neutrino-anti-neutrino pair. The new e949 experiment is expected to increase the sensitivity by about one order of magnitude. To achieve this goal, the detector is being upgraded to achieve this new desired sensitivity. One of the modifications taking place is the improvement of the energy resolution of the experiment. To accomplish this, the amount of light detected by the range stack was going to be increased by the purchase of 96 new scintillators, which were all to be tested before installation into the AGS detector. The goal was to measure the photoelectron yields with respect to position for each of the counters. The intensity with respect to position was also determined from the testing and this led to the determination of the attenuation lengths from each of the 96 scintillators. These new results were then compared to those for an old scintillator module. It was found that on average, the intensity of the modules increased considerably compared to the older module, by a factor of about 1.5 times, and the attenuation lengths increased by a factor of 2.5. These results show that the new modules are much more capable of detecting the rare kaon decays than the old modules.
Spin Correlations in Top Production and Decay at e+e- Colliders
Andrew E. Blechman, Cosmin Macesanu, Prof. Lynne H. Orr, 91自拍论坛
The top quark, recently
discovered at Fermilab, decays before it can hadronize; this allows its
spin information to be passed directly to its daughter particles. We study
these spin correlations in top production and decay at electron-positron
colliders, looking specifically at dilepton events. Using Monte Carlo
techniques,
we calculate tree-level cross sections in terms of quantities that are
directly observable experimentally.
Astronomy
Cataclysmic Variables
Jessica Lavine, Union College
Cataclysmic Variable stars are binary star systems that vary in magnitude due to the transfer of gas of the red giant star on to its white dwarf counterpart. The research consisted of observing the Cataclysmic Variable DQ Herculis in order to determine its change in magnitude, and observing other major characteristics of this eclipsing binary system. I will talk about my observations as well as the further research I plan on doing. I will also illustrate important aspects of image processing for CV observational research.
Extended HI Envelopes Around Low Surface Brightness Galaxies
Diane Chin, Binghamton University, Dr. Karen O扤eil, Arecibo Observatory
Using the Arecibo Gregorian telescope, we undertook to look for extended neutral hydrogen gas around four low surface brightness galaxies in the direction of the Pegasus Cluster ([OBC97] P06-4, [OBC97] P04-1, [OBC97] P06-1, & [OBC97] P02-3). Although uncertainties in the beam pattern made final analysis of the data difficult, three of the galaxies observed appear to have HI gas extending 2-5 times farther than the optical (d27) diameter of the galaxies. Additionally, all three cases show the HI distribution to be fairly lopsided.
Image Analysis for the Peculiar Virgo Cluster Galaxy NGC 4383
Holly Burnside, Union College
In the 1920s, Edwin Hubble started categorizing the galaxies he observed according to their morphology (appearance), which may be linked in some way to their evolutionary history. He placed galaxies into two main classes: spiral and elliptical. His classification is still widely recognized by astronomers today. There are, however, many galaxies that do not fit into Hubble's categories, particularly galaxies in crowded environments. NGC 4383, located in the Virgo Cluster, roughly 16 Mpc (50 million light years) away, is one of these galaxies. The morphology of this galaxy was studied using optical blue, green, red, and Ha-line emission images, which were obtained at the WIYN telescope in Arizona. Optical light traces the stellar distribution of the galaxy and Ha emission is a tracer of recent formation. A Hubble Space Telescope image was used to examine the central regions of the galaxy at high resolution. The galaxy has active star formation concentrated in several large star-forming regions in the central regions and irregularities in the stellar and dust distributions. The peculiarities in this galaxy are most likely due to a gravitational interaction with another galaxy, which has perturbed the stellar and gas distributions and triggered star formation.
Pole Solutions for Koronis Family Asteroids using Sidereal Photometric Astrometry
Marko Krco, Prof. S. Slivan, Colgate University
According to the
currently accepted theory, the Koronis Family asteroids were created through
a cataclysmic disruption of a single parent body. If true, we would expect
the asteroids to have "remembered" the pole axis and spin direction of
the parent body in much the same way as they have retained its orbital
characteristics. Previous attempts to find correlations between the pole
solutions of the member asteroids were inconclusive. Our goal is to develop
and implement a computational method described by Drummond (1988) to determine
the pole solutions for several Koronis Family asteroids. Correlating these
findings with those of previous methods should provide conclusive
results.
Optical Physics
Ultra-Short Pulsed Laser Diagnostics Using an S.H.G. F.R.O.G.
Eugene Torigoe, Binghamton University; Prof. Linn Van Woerkom, Ohio State University
With the development of pulsed laser systems that can create pulses on the order of femto-seconds there arises the problem of properly characterizing these pulses. Experimenters who use these systems rely on the fact that they know the widths of the pulses as well as the distribution of frequencies along the pulse known as the pulse抯 chirp. A method of properly characterizing laser pulses was developed in 1993 by Rick Trebino, known as Frequency Resolved Optical Gating (F.R.O.G.). A FROG system consists of an apparatus that creates an image of the pulse on time-frequency axes, and an iterative algorithm that extracts the width of the pulse and the frequency distribution along the pulse from that image.
A Second Harmonic Generation (S.H.G.) F.R.O.G. apparatus was built and tested. The S.H.G. F.R.O.G. geometry is a particular type of FROG geometry based on a non-linear optical effect that transforms temporal information of the pulse into spatial characteristics of a signal pulse. The S.H.G. F.R.O.G. was used to characterize the laser pulses from the two 120 fs, 800 nm pulsed laser systems in the Van Woerkom lab.
Superluminal Tunneling
Mark Kostuk, Union College
We present a numerical time-dependent solution to the Schrodinger equation for the evolution of a wavepacket incident on a potential barrier and examine the mechanism behind its superluminal propagation. Several groups have recently shown that photonic pulses tunneling through a potential barrier travel at speeds greater than the speed of light. A purely quantum phenomenon, tunneling has been studied since the 1930's in the form of stationary (time-independent) solutions, but these are insufficient for our current problem. In order to examine propagation speeds time-dependant solutions are required, however the difficulty of this situation makes analytical solutions impossible. We employ computer simulations and numerical approximations to the problem of tunneling in an effort to understand this bizarre behavior of nature. Superluminal travel violates causality; it allows for an effect to occur before its cause. Our simulations show that causality is not violated due to the probabilistic nature of quantum mechanics on information transmission.
Computation and Graphical Analysis of Infinite Planar X-Ray Wave Guides
Kevin Udwary, Siena College
X-rays propagation in an infinite planar dielectric wave-guide is useful for several reasons. First, the methods developed for an infinite planar wave-guide can be applied to more difficult cases, such as cylindrical wave-guides. Second, these methods can be applied to physical systems, such as x-ray "optical" fibers or quantum computing. The motion of x-rays through both metallic and a dielectric wave-guide were shown. The energy and allowed standing wave modes of the x-rays throughout the guide were examined and represented graphically using Mathematica. The limitations of the x-ray wave-guides were examined by viewing the effect on the x-ray wave-guide modes as the physical properties of the guide, such as the height, were changed.
Single-Photon Interference Experiments
Lauren Heilig, Colgate University
We present experiments
aimed at studying the wave-particle duality of light. A first set of
experiments
involve recording the interference of light at the single photon level
by passing an attenuated laser beam through a Mach-Zender interferometer.
Photon detection rates are measured as a function of the optical path length.
A second set of experiments underscores the particle nature of light using
parametric down-converted light.
General Physics
Thermal Conductivities of Various Textiles
Chris Carroll, Siena College
In order to obtain thermal data, a cylindrical tube was constructed to serve as a uniform heat source to the textile. By placing a power circuit down the center of the metallic tube, heat is generated and presented to the textile. Using a temperature-sensitive chip, the LM35 temperature sensor, a thermometer circuit was constructed to measure energy changes inside the apparatus. The power output of the circuit can then be used to calculate the conductivity.
Pressure Phenomena Through Various Textiles
Daniel Fisher, Siena College
The phenomenon of airflow through various textiles is a new and intriguing aspect of physics that can determine the efficiency of various articles of clothing or general textiles. A time constant for pressure leak-up can be observed by generating a vacuum inside a chamber at a known pressure, and attaching the textile to an orifice on the chamber. Upon the opening of a valve, the atmospheric pressure will then attempt to distribute itself by flowing to the lower pressure region through the textile. The time needed to leak up to atmospheric pressure inside the chamber can then be interpreted to generate a time constant. Using this time constant, it is possible to determine a relationship to some already known textile constants. Some practical applications from this research could be the determination of how well some types of clothing insulate the garment wearer, or their ability to handle a large pressure difference on each side of the textile across a known surface area.
Order and Packing in a Two-Dimensional Pile of Rods
Saul Lapidus, Prof. Scott Franklin, 91自拍论坛 Institute of Technology
In this talk, preliminary results on how anisometric granular materials pack, and how to quantify local and global order will be discussed. The experimental system under investigation is essentially a two-dimensional piles of rods. Granular materials pose a complex many-body problem for which much of statistical mechanics must be reworked. The general characteristics of ordinary (round) granular materials as well as rod-like (anisometric) particles will be discussed, as will future directions.
Simulating the Haystack: Modeling a 2-D Anisometric Granular Material
Kevin Stokely, Prof. Scott Franklin, 91自拍论坛 Institute of Technology
Granular piles are large collections of small, discrete particles. Because the particle size is macroscopic, thermodynamic effects do not affect the particles, and the pile often fails to settle into a minimum energy state. A simulation of the settling of long, thin, two-dimensional nails will be discussed, with a focus on the effects of the particle aspect ratio (length/width) on the final order and packing fraction of the piles. Previous research in the field, an overview of the simulation, and future modifications to the simulation will be presented.
Global Warming's Effect on the Sea Level
Jeff Reardon, Siena College
Global Warming is
becoming a threatening problem in today's world. Though its effects may
be decades away they must be realized. The change in sea level alone will
be a serious condition. Sea water expands differently in the different
regions of the ocean. These regions are the arctic, subtropical, and tropical
regions. Each region has a different equation on how the temperature acts
at certain depths. The expansion of sea water at these depths is effected
by pressure and salinity. The average depth of the ocean varies along with
the volume for each region. All of these factors determine how the sea
level will change due to a rise in surface temperature. The results of
this will be discussed using graphs and data tables.
Biophysics
Optical Anisotrophy of Interacting Chromophores in Protein Complexes: Exploration of a Stochastic Theory*
Laura A. Allaire,** Prof. R. S. Knox, 91自拍论坛, Jennifer Dawson,*** Kent State University
Excitation transfer among light-harvesting chromophores is of critical importance to photosynthesis. The fundamental mechanism for this transfer is well known to be the interaction between Coulomb-induced transition dipole moments, but the complexity of the environment of the chromophores makes numerous approximations necessary when comparing predicted with measured results. Over the past several years both the knowledge of protein structures and the accuracy of fast optical measurements have increased to a stage at which some of these approximations may be assessed. A theory of optical anisotropy under development by Gülen and Knox [1] is intended to combine various aspects of existing stochastic theories (e. g., [2,3]) in order to address this issue. We report here preliminary calculations based on this theory for comparison with anisotropy data on C-phycocyanins [4] and peridinin-chlorophyll-protein complexes [5].
* Supported in part by USDA NRICGO grant 95-37306-2014 and NSF REU grant PHY 99-87413.
** Present address: Institute of Optics, 91自拍论坛, 91自拍论坛, NY 14627-0186
*** Present address: Department of Physics, Kent State University, Kent, OH 44242-0001
#R. S. Knox and D. Gülen, Photochem. Photobiol. 57, 40-43 (1993); D. Güle and R. S. Knox, in preparation.
2. H. Haken and P. Reineker, Z. Physik 249, 253-268 (1972)
3. R. Wertheimer and R. Silbey, Chem. Phys. Lett. 75, 243-248 (1980)
4. M. Debreczeny et al., J. Phys. Chem. 99, 8412-8419 and 8420-8431 (1995)
5. F. J. Kleima et al., Biophys. J. 78, 344-353 (2000)
Quantum Computation
Scott Oppenheimer, Binghamton University, Marjorie Quant, United States Air Force - Rome, NY Research Center
Using quantum probabilities for computation leads to novel and unexpected algorithms Shor抯 factoring algorithm and Grover抯 search algorithm are two such algorithms that are faster than their conventional peers. Using the additive nature of quantum probabilities, non-deterministic algorithms can solve exponential problems in polynomial time. The current state of the art in quantum computers (ion trap, and NMR) will also be discussed.
Probability Backflow of the Klein-Gordon Particle
John McVeigh, Prof. Shimon Malin, Colgate University
Quantum mechanics is a powerful theory of nature that sometimes produces counterintuitive results. For two superposed plane waves of certain characteristics, it can be shown that there are values of time and space that yield negative probability current. The goal of my research is to investigate the occurrences of negative probability current for the Klein-Gordon particle.
Energy States and Error Bounding for an Initial Gaussian Wavefunction in the 1-D Infinite Square Well
David Etlinger, Prof. Joseph Eberly, 91自拍论坛
The 1-D infinite square well (i.e., a potential that completely bounds a wavefunction to a finite interval of the real line) is a simplistic model of particle motion that nevertheless remains useful in both theory and practice. However, simplification often introduces errors that must be bounded if a model is to have any validity. Gaussian wavefunctions are often used to describe particles in traps, but the infinite extent of such functions is in conflict with the square well model, and leads to error. Given a Gaussian with an initial momentum in a square well, we have calculated an explicit expression for the expected energy states of the particle. We have then carefully bounded the errors introduced through approximations, and shown under what parameters the model is valid. ./2001/index.html 000755 000766 000024 00000002621 07477214367 014302 0 ustar 00munson staff 000000 000000
INTRODUCTION
Welcome to the twentieth annual 91自拍论坛 Symposium for Physics Students. This series of symposia was instituted to provide an opportunity for undergraduates to present an account of their own personal research at a meeting whose format was chosen to closely resemble those of professional scientific societies. Your audience will include both students and faculty members, and will provide you with the opportunity to address a knowledgeable and appreciative assembly of fellow researchers.
Scientific research
is an extraordinary activity. To quote Albert Einstein: "The most incomprehensible
thing about the universe is that it is comprehensible." I certainly hope
that many of you will decide to pursue careers which involve you intimately
in mankind抯 great intellectual adventure � to comprehend nature.
Arie Bodek, Chair
Department of Physics
and Astronomy
./2001/program_2001.html 000755 000766 000024 00000033273 07510101126 015263 0 ustar 00munson staff 000000 000000
University of 91自拍论坛
Department Physics and Astronomy
91自拍论坛,
New York 14627-0171
91自拍论坛 symposium for physics students
April
21, 2001
Program
8:30-9:00
Lobby
and Room 271, Registration and Coffee
9:00-9:15
Room
106, Welcome: Prof. Paul Tipton, Chair, RSPS XX
9:15-10:30
Room
109 Condensed Matter
Session
Chair: Prof. Joshua Diamond, Siena College
9:15
Vortex Motion in
Niobium Thin Films
Jesse Young, Prof.
Joseph Amato, Colgate University
9:30
The Effects of
Mechanical Strain on Mesoscopic Bismuth Thin Films
Steven A. Waldauer,
State University of New York at Buffalo
9:45
Linewidth of Transitions
in MN12 Acetate
10:00
Interface-Controlled
and Diffusion-Limited Kinetics of Alloy Formation in Pb/Sn Thin Films
Anthony Clark,
Prof. E. J. Cotts, Binghamton University
10:15
Pentacene Thin
Film Field Effect Transistors
Katie Lotterhos,
Binghamton University, Prof. Robert Dynes, University of California at
San Diego
9:15-10:30
Room
106 Particles and Fields
Session
Chair: Prof. Robert Pompi, Binghamton University
9:15
Feynman Diagrams
in Quantum Electrodynamics
Fred Vonstein,
Union College
9:30
Solution of the
"Degenerate Model" for Parafermi Particles of Order Two
Terry Tarnowsky,
Prof. Charles Nelson, Binghamton University
9:45
An Investigation
of Future CDF Measurements of W Helicity in the Decay of the Top Quark
Brock Tweedie,
91自拍论坛
10:00
Test of the e94
Range Stack Upgrade
Adam Rogers, Binghamton
University, Dr. James Frank, Brookhaven National Laboratory
10:15
Spin Correlations
in Top Production and Decay at e+e- Colliders
Andrew Blechman,
Cosmin Macesanu, Prof. Lynn H. Orr, 91自拍论坛
10:30-11:00
Break,
Room 271
11:00-12:00
Room
106 Astronomy
Session
Chair: Prof. Rebecca Surman, Union College
11:00
Cataclysmic Variables
Jessica Lavine,
Union College
11:15
Extended HI Envelopes
Around Low Surface Brightness Galaxies
Diane Chin, Binghamton
University, Dr. Karen O扤eil, Arecibo Observatory
11:30
Image Analysis
for the Peculiar Virgo Cluster Galaxy NGC 4383
Holly Burnside,
Union College
11:45
Pole Solutions
for Koronis Family Asteroids Using Sidereal Photometric Astrometry
Marko Krco, Prof.
S. Slivan, Colgate University
11:00-12:-00
Room
109 Optical Physics
Session
Chair: Prof. Enrique Galvez, Colgate University
11:00
Ultra-Short Pulsed
Laser Diagnostics Using an S.H.G.F.R.O.G.
Eugene Torigoe,
Binghamton University, Prof. Linn Van Woerkom, Ohio State University
11:15
Superluminal Tunneling
Mark Kostuk, Union
College
11:30
Computation and
Graphical Analysis of Infinite Planar X-Ray Wave Guides
Kevin Udwary, Siena
College
11:45
Single-Photon Interference
Experiments
Lauren Heilig,
Colgate University
12:00-1:00
Lunch,
Meliora Building
1:15-2:30
Room
106 General Physics
Session
Chair: Prof. Scott Franklin, 91自拍论坛 Institute of Technology
1:15
Thermal Conductivities
of Various Textiles
Chris Carroll,
Siena College
1:30
Pressure Phenomena
Through Various Textiles
Daniel Fisher,
Siena College
1:45
Order and Packing
in a Two-Dimensional Pile of Rods
Saul Lapidus, Prof.
S. Franklin, 91自拍论坛 Institute of Technology
2:00
Simulating the
Haystack: Modeling a 2-D Anisometric Granular Material
Kevin Stokely,
Prof. S. Franklin, 91自拍论坛 Institute of Technology
2:15
Global Warming抯
Effect on the Sea Level
Jeff Reardon, Siena
College
1:15-1:30
Room
109 Biophysics
Session
Chair: Prof. John Andersen, 91自拍论坛 Institute of Technology
1:15
Optical Anisotropy
of Interacting Chromophores in Protein Complexes: Exploration of a Stochastic
Theory
Laura A. Allaire,
Jennifer Dawson, Prof. R. S. Knox, 91自拍论坛
1:30-2:15
Room
109 Quantum Mechanical Systems
Session
Chair: Prof. John Andersen, 91自拍论坛 Institute of Technology
1:30
Quantum Computation
Scott Oppenheimer,
Binghamton University, Marjorie Quant, United States Air Force � Rome,
NY Research Center
1:45
Probability Backflow
of the Klein-Gordon Particle
John McVeigh, Prof.
Simon Malin, Colgate University
2:00
Energy State and
Error Bounding for an Initial Gaussian Wavefunction in the 1-D Infinite
Square Well
David Etlinger,
Prof. Joseph Eberly, 91自拍论坛
Optional Tours
2:35
Cars should
leave for Laboratory for Laser Energetics
or
2:35
Research Labs
in Bausch and Lomb Building
Name Time Location
Allaire, Laura
1:15
Room 109
Blechman, Andrew
10:15
Room 106
Burnside, Holly
11:30
Room 106
Carroll, Chris
1:15
Room 106
Chin, Diane
11:15
Room 106
Clark, Anthony
10:00
Room 109
Etlinger, David
2:00
Room 109
Fisher, Daniel
1:30
Room 106
Heilig, Lauren
11:45
Room 109
Kostuk, Mark
11:15
Room 109
Krco, Marko
11:45
Room 106
Lapidus, Saul
1:45
Room 106
Lavine, Jessica
11:00
Room 106
Loomis, Joe
9:45
Room 109
Lotterhos, Katie
10:15
Room 109
McVeigh, John
1:45
Room 109
Oppenheimer, Scott
1:30
Room 109
Reardon, Jeff
2:15
Room 106
Rogers, Adam
10:00
Room 106
Stokely, Kevin
2:00
Room 106
Tarnowsky, Tery
9:30
Room 106
Torigoe, Eugene
11:00
Room 109
Tweedie, Brock
9:45
Room 106
Udwary, Kevin
11:30
Room 109
Vonstein, Fred
9:15
Room 106
Waldauer, Steven
9:30
Room 109
Young, Jesse
9:15
Room 109