Physics Colloquium
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"Modeling Eclipsing Binary Stars from Light Curves" |
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Abstract: |
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Spring 2004 Colloquia |
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January 27 |
Dr.
Jose Perez, Department of Physics, University of North Texas, Denton,
Texas |
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February 3 |
Dr.
Yuriy A. Kosevich, Instituto de Investigacion en Comunicacion Optica,
Universidad Autonoma de San Luis Potosi, San Luis Potosi, Mexico |
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February 10 |
Professor
Suresh C. Sharma,
Department of Physics, University of Texas at Arlington, Arlington, Texas |
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February 17 |
Dr. David L. Allara, Department of Chemistry and Materials Research Institute, Pennsylvania State University, University Park, Pennsylvania “Building Molecule-Based Electronic
Devices” |
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February 24 |
Dr.
John Prince, Department of Physics, University of North Texas, Denton,
Texas |
| March 2 |
Professor
Anzhong Wang,
Center for Astrophysics, Space Physics, & Engineering Research, Department
of Physics, Baylor University, Waco, Texas |
| March 5 |
Dr.
Jeffrey Bennett, Astrophysicist and Science Writer (1) Provide a Contextual Framework: It is much easier to learn new facts or concepts if they can be "binned" into a pre-existing mental framework that gives a broad context for the detailed study to be undertaken. (2) Create Conditions for Conceptual Change: Many people hold misconceptions about scientific ideas. Therefore we cannot teach them the correct ideas unless we first help them unlearn their prior misconceptions. (3) Make the
Material Relevant: It's human nature to be more interested in subjects
that seem relevant to our lives. Therefore we must show students the many
connections between science and their personal concerns. (4) Limit
Use of Jargon: The number of new terms in many introductory science books
is larger than the number of words taught in many first courses in foreign
language, which is a clear recipe for failure. We must find ways to replace
jargon with plain language. (5) Challenge
Your Students: Don't dumb your teaching down; by and large, students will
rise to meet your expectations, as long as you follow the other strategies
and practice good teaching. Bio: Dr. Jeffrey Bennett is
an astrophysicist (Ph.D, 1987 University of Colorado) who specializes
in math and science education. He has taught at every level from elementary
school through college, and is the author of leading college-level textbooks
in astronomy, mathematics, statistics, and the new science of astrobiology.
He served two years as a Visiting Senior Scientist at NASA headquarters,
where he developed education programs
for the Hubble Space Telescope and other astrophysics missions. He proposed
the idea for and helped develop the Voyage Scale Model Solar System, a
permanent, outdoor exhibit on the National Mall in Washington, DC. Learn
more about Dr. Bennett at http://www.jeffreybennett.com |
| March 9 |
Professor
Sam Matteson, Department of Physics, University of North Texas, Denton,
Texas |
| March 23 |
Dr.
Zhibing Hu, Department of Physics, University of North Texas, Denton,
Texas |
| March 30 |
Professor
R. F. O'Connell, Department of Physics and Astronomy, Louisiana State
University, Baton Rouge, Louisiana |
| April 6 |
Professor Wolfgang Schleich, Abteilung für Quantenphysik, Universität Ulm, Ulm, Germany "Interference,
Correlations and Entanglement in Higher Dimensions: Quantum Information" |
| April 13 | Professor
Mike Fanelli, Department of Physics, University of North Texas, Denton,
Texas "The Road to Mars" The Red Planet Mars has always drawn the attention and wonder of Earthlings. Since the early 1970s, our robotic emissaries have revealed Mars to be a complex, intriguing locale, neither the abode of life imagined early in the 20th century, nor the "dead" planet suggested by the first flyby spacecraft. Perhaps most significantly, orbiting spacecraft indicated the presence of large volumes of flowing water on the Martian surface sometime in its past. This discovery led to speculation of an early, warmer and wetter period in Martian history, in contrast to the cold, dry world of today. During such a warm era, life may have originated on Mars as it did on the early Earth. Starting in 1997, a small armada of robot explorers have reached Mars and radioed back tantalizing data suggesting that a substantial amount of water may still exist on Mars today, frozen under the soil. To untangle the mysteries of Mars' past, NASA and ESA have adopted a "follow the water" strategy. In this talk I will detail the rationale for this strategy and the exciting results which continue to unfold today. |
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April 16 |
Dr.
Daniel K. Marble, Department of Mathematics, Physics, & Engineering,
Tarleton State University, Stephenville, Texas |
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April 20 |
Dr.
Dan Bruton, Department of Physics and Astronomy, Stephen F. Austin State
University, Nacogdoches, Texas "Modeling Eclipsing Binary Stars from Light Curves" Eclipsing binary stars are just one several types of variable stars. These stars appear as a single point of light to an observer, but based on its brightness variation and spectroscopic observations we can say for certain that the single point of light is actually two stars in close orbit around one another. The variations in light intensity from eclipsing binary stars is caused by one star passing in front of the other relative to an observer. A brightness versus time plot for a variable star is know as light curve. From these plots we can determine the relative masses and radii of the two stars as well as a few of the orbital parameters. http://www.physics.sfasu.edu/astro/binstar.html |
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Fall 2003 Colloquia |
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| September 16 |
Dr.
Sam Matteson, Department of Physics, University of North Texas, Denton,
Texas |
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September 23 |
Dr.
Roland Allen, Department of Physics, Texas A&M University, College
Station, Texas |
| September 30 |
Professor Arkadii Krokhin, Department of Physics, University of North Texas, Denton, Texas “Speed of Light and Sound in Photonic and Phononic Crystals” New periodic heterostructures
– photonic crystals – are expected to produce new media for information
technology by replacing traditional electronic devices by integrated photonic
circuits. In this talk I’ll consider fundamental optical properties of
photonic crystals in the low-frequency region. The question of interest
is: What is the speed of light in photonic crystals? Answering this question
we can understand what are the similarities and distinctions between optics
of natural crystals and artificial photonic crystals. Similar question
arises for phononic crystal – periodic elastic composites. I will consider
the problem of speed of sound in mixtures. I will explain why in water
with a speed of sound 1% that of air the speed of sound drops by two orders
of magnitude. |
| October 7 |
Dr.
Linda Reichl, Center
for Statistical Mechanics and Complex Systems, University of Texas, Austin,
Texas |
| October 14 |
Dr.
Wolfgang Schleich, University of Ulm, Ulm, Germany |
| October 21 |
Dr.
Bruce J. West, Senior Research Scientist, Mathematics Division, Army Research
Office, Research Triangle Park, North Carolina |
| October 23 |
Texas
Section APS/AAPT/SPS Meeting, Texas Tech University, Lubbock, Texas |
| October 28 |
Professor
Arup Neogi, Department of Physics, University of North Texas, Denton,
Texas The optical properties
of semiconductor nanostructures, including quantum wells, quantum dots,
and self-assembled organic-inorganic material systems, significant for
designing optoelectronic and photonic applications will be discussed.
We are studying the fundamental properties of these materials systems
using various optical diagnostic techniques based on ultrafast lasers.
The nano-photonic material research program and the existing experimental
facilities being developed at the Department of Physics at UNT will be
presented. |
| November 4 |
Dr.
Mini Das,
Physics Department, Indian Institute of Technology, Delhi, India Fiber gratings are emerging
as a key element in the field of optical communication and optical fiber
sensing. Fiber gratings are essentially formed by inducing periodic
refractive index change in the core of the optical fiber. This periodic
perturbation leads to coupling of optical power between the fiber modes,
resulting in interesting spectral properties that could be controlled
by changing the grating properties. The talk would cover a brief introduction
to fiber gratings and their mode coupling properties followed by classification
of gratings. Some important applications of these in dispersion compensation
and sensing would be discussed. Experimental results on the demonstration
of the first fiber based polariser would be elaborated (Experiments conducted
at the fiber optics division of Bell Laboratories, NJ, USA). Brief discussion
on the recent research advances in this field including an inverse scattering
technique that is used to design gratings with desired spectral response
would conclude the talk. |
| November 11 |
Dr.
Jacek Kowalski, Department
of Physics, University
of North Texas, Denton,
Texas Real-world networks such as
power grids, World-Wide Web, the Internet, biological and social networks
exhibit interesting scaling properties that cannot be explained in the
framework of "classical" random graph theory. Strong clustering
is another feature of such real-life networks. Analysis of their robustness
is a challenging problem of obvious importance. A review of several popular
approaches to the description of such systems will be discussed and some
open problems given. |
| November 18 |
Dr. Manfred A. Cuntz, Department of Physics, University of Texas at Arlington, Arlington, Texas “Stars,
Planets and Stellar Activity Enhancements”
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| November 25 |
Dr.
Gerald B. Cleaver, Center for
Astrophysics, Space Physics & Engineering Research, Department
of Physics, Baylor University, The enhancement of superstring theory to M-theory has profound implications for cosmology. I review the most significant aspects of the M-theory cosmological picture resulting from the combined effects of (1) M-theory’s (10+1)-dimensional spacetime (compared to string theory’s (9+1)-dimensional spacetime), (2) M-theory’s realization that strings have a width determined by the size of the additional spatial direction (transforming strings into membranes), and (3) the M-theory prediction of spatial surfaces called D-branes. The role of membranes and D-branes in the pre-Big Bang and inflationary eras are discussed. M-theory revisions of the original Brandenberger-Vafa string inflation model are briefly summarized. I also discuss the Randall-Sundrum model and its extensions, which offer a D-brane explanation for the apparent weakness of gravity in our 3+1 large dimensions.
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| Spring 2003 Colloquia | |
| January 24 |
Professor
Arkady Krokhin, Instituto do Fisica, Universidad Autonoma de Puebla, Puebla,
Mexico |
| January 28 |
Professor
Paolo Grigolini, Department of Physics, University of North Texas, Denton,
Texas |
| February 4 |
Professor
Donald Kobe, Department of Physics, University of North Texas, Denton,
Texas |
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February 11 |
Dr.
Victor V. Kozlov, Abteilung
fuer Quantenphysik, Universitaet Ulm, Germany Fundamental
and applied aspects of nonlinear propagation of solitons and solitary
waves in optical fibers are overviewed in context of their information
capacity, with main emphasis on the transition from classical concepts
towards quantum dynamics. Classical solitons are known as self-organizing
themselves into stable spatially and temporally localized objects, and
as such are considered as robust carriers of classical information. The
talk will address the question of whether quantum solitons can serve equally
well for carrying quantum information. The discussion will include: How
to entangle two or more initially uncorrelated solitons, how to entangle
(actually, intra-entangle) a soliton with itself, and how to design a
quantum-optical network - quantum Internet. |
| March 4 |
Professor
Sam Matteson, Department of Physics, University of North Texas, Denton,
Texas |
| March 11 |
Professor
Constantino Tsallis, Brazilian
Center for Research in Physics, Rio
de Janeiro, Brazil |
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March 25 |
Professor
Jianzhong Wu, Dept. of Chemical and Environment Engineering, University
of California, Riverside |
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April 1 |
Dr.
Richard Stallcup, Research Physicist, Zyvex Corporation, Richardson, Texas |
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April 15 |
Jack
G. Hehn, Director of Education, American Institute of Physics, College
Park, Maryland The
American Institute of Physics (AIP) in collaboration with its ten Member
Societies undertakes a number of programs to strengthen physics departments
and their programs. AIP staff members visit University campuses
and meet with members of the Society of Physics Students (SPS), groups
of faculty and administrators, and local employers to learn more about
current concerns. I will talk about two specific AIP programs as
examples. (1) The National Task Force on Undergraduate Physics has published
a report “Strategic Programs for Innovation in Undergraduate Physics”
giving examples of Physics Departments that have shown success in increasing
physics majors and student participation. (2) The Physics Teacher Education
Coalition is a program designed to increase the role of Physics Departments
in the science preparation of future teachers in grades K-12. An
outcome of this program is to form a coalition of colleges and universities
to take a leadership role in preparing future teachers. |