41
          
        
        
          January 4–7, 2014
        
        
          
            Sundayafternoon
          
        
        
          Sunday, January 5
        
        
          12–1 p.m.
        
        
          Salon 4
        
        
          First Timers’
        
        
          Gathering
        
        
          Learn more about
        
        
          
            AAPT
          
        
        
          and the Winter Meeting
        
        
          Meet new friends and greet
        
        
          your old friends!
        
        
          tor to compare two related properties of the recombination process.
        
        
          In the first experiment, we use an isolated defect to measure effective
        
        
          diffusion lengths, i.e. the average distance traveled by a charge carrier
        
        
          before recombining. In the second experiment, we measure effective
        
        
          lifetimes, i.e. the average time it takes for a charge carrier to recom-
        
        
          bine. We use these measurements to connect the temporal and spatial
        
        
          distribution of electron-hole pair recombination. These complemen-
        
        
          tary properties can be used to further our understanding of charge
        
        
          carrier behavior in solar cell materials as a function of temperature
        
        
          and illumination.
        
        
          AA05:
        
        
          3-3:10 p.m.     Conquering Quantum Physics One
        
        
          Photon at a Time
        
        
          Contributed – Jamie L. Garrett, Southern Polytechnic State University,
        
        
          Powder Springs, GA 30127; 
        
        
        
          PhysicsQuest is a story-based activity book for middle school students
        
        
          created by the American Physical Society that introduces them to
        
        
          physics concepts through hands-on activities. Free kits are provided
        
        
          to teachers or parents who register on the PhysicsCentral website,
        
        
          as a way to engage middle school students at an age in which many
        
        
          students become disinterested in science. As the Society of Physics
        
        
          Students PhysicsQuest intern, I developed easy-to-do, inexpensive
        
        
          extension activities to complement the activities provided in the latest
        
        
          kit. The topic this year is Quantum Mechanics. Students will explore
        
        
          the photoelectric effect, spectroscopy, absorption spectra, and angular
        
        
          momentum and rotation. This talk will highlight several of the activi-
        
        
          ties created.
        
        
          AA06:
        
        
          3:10-3:20 p.m.    Modeling Mass-Radius
        
        
          Relationships of Planets Using Differential Equations
        
        
          Contributed – Kevin D. Thielen,* Eckerd College, St. Petersburg, FL
        
        
          33711; 
        
        
        
          Alexander K. Zielinski, Stephen P. Weppner, Eckerd College
        
        
          Models of mass-radius relationships for planets have been recently
        
        
          developed by making assumptions about the relationship between
        
        
          pressure and density in order to avoid having to work with more com-
        
        
          plex equations of state. In our model we construct a Non-linear Ho-
        
        
          mogeneous Ordinary Differential Equation, whose parameters can be
        
        
          readily obtained experimentally, and solve it numerically by making
        
        
          an observation about the relationship of density and compressibility
        
        
          as a function of pressure. We then compare our numerical results to
        
        
          models such as the Preliminary Earth Reference Model (PREM) and
        
        
          models of pressure density relationships of materials from low pres-
        
        
          sures up to pressures within the region of the Thomas Fermi Dirac
        
        
          theoretical EOS where electron degeneracy pressure becomes a factor.
        
        
          *Sponsored by Anne Cox
        
        
          AA07:
        
        
          3:20-3:30 p.m.     Evidence for Dark Matter in the
        
        
          Galactic Rotation Curve
        
        
          Contributed – Melvin Jason Ezell, Campbell University, P.O. Box 308,
        
        
          Buies Creek, NC 27506;
        
        
        
          Jacob K. Bartlett, Campbell University
        
        
          The mass of the dark matter halo, or “missing mass” interior to the
        
        
          Sun’s orbit was calculated by creating a galactic rotation curve for the
        
        
          Milky Way galaxy. This rotation curve was created by measuring the
        
        
          orbital velocity of interstellar hydrogen at different distances from the
        
        
          galactic core. A 4.6-meter radio telescope was used to collect data on
        
        
          the radio waves emitted by hydrogen at various galactic longitudes.
        
        
          Since hydrogen emits radio waves at a baseline frequency of
        
        
          1.42 GHz, the Doppler shifted wavelengths observed provided a
        
        
          means to calculate the orbital velocity of the galaxy’s matter. This
        
        
          rotation curve was then compared to the amount of visible mass in
        
        
          the galaxy and the missing mass was calculated. This research was
        
        
          converted to a laboratory exercise for undergraduate physics students
        
        
          at Campbell University which included a pre-assessment of content-
        
        
          specific knowledge and a post-assessment of learning outcomes.
        
        
          AA08:
        
        
          3:30-3:40 p.m.     Incorporating Data Visualization
        
        
          into ZENODO
        
        
          Contributed – Kevin Sanders, High Point University,  High Point, NC
        
        
          27262;
        
        
        
          ZENODO is a research hosting website made for all disciplines. It is
        
        
          built on the idea of all research shared, no matter the subject, no mat-
        
        
          ter the status of the researcher. ZENODO was developed alongside
        
        
          and on top of INVENIO, a digital library software suite, produced by
        
        
          the Digital Library Technology group at CERN. This talk will cover
        
        
          some of the technologies that came into play, as well as my role of
        
        
          beginning to incorporate data visualization into the website during
        
        
          my time spent at CERN through the University of Michigan REU.
        
        
          AA09:
        
        
          3:40-3:50 p.m.      A New Approach to Optics for Life
        
        
          Science Majors
        
        
          Contributed – Shauna Novobilsky, Mercyhurst University, Erie, PA
        
        
          16546l;
        
        
        
          Dyan Jones, Mercyhurst University
        
        
          Interactive learning strategies are frequently used in the teaching of
        
        
          introductory physics topics. Here we describe the development of a
        
        
          course for undergraduate students who are not majoring in the field
        
        
          of physics. By adapting the learning materials from a Studio Optics
        
        
          course and Optics for Biophysics course, we hope to create a course
        
        
          designed to bring interactive learning to the topic of optics. Adapt-
        
        
          ing the course to fit our curriculum will require a reduction in the
        
        
          amount of mathematics in the course, but the majority of the course
        
        
          requirements from the courses mentioned above will remain. This will
        
        
          create an environment that integrates lectures, lab, and simple prob-
        
        
          lem solving as well as a focus on a long-term project for the course.
        
        
          The hope is to create a course that is advantageous to non-physics
        
        
          majors who still have an interest in optics.