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Note: This information is incomplete as not all information has been forwarded for inclusion in this page.
Click here for:Date: | Monday (usually) |
Time: | 4:00-5:00 PM |
Place: | NRC 108 |
Inquiries: | atr@osuunx.ucc.okstate.edu, krasins@master.ceat.okstate.edu |
Date: | Thursday |
Time: | 1:30-3:00 PM |
Place: | Classroom Building, Room 106, Studio D |
& Kaufman Hall, Room 341, OU | |
Inquiries: | shaown@vms.ucc.okstate.edu |
Date: | Thursday |
Time: | 4:00-5:00 PM |
Place: | PS 110 |
Inquiries: | atr@osuunx.ucc.okstate.edu |
Speaker: | Professor Thomas J. Weiler |
Department of Physics and Astronomy | |
Vanderbilt University | |
Date: | Thursday, January 22, 1998 |
Time: | 1:30 |
Place: | TELECOM 127 |
Title: | Puzzles in the Highest Energy Cosmic Ray Data, |
and Proposed Solutions |
Please note new time.
Speaker: | Professor Thomas J. Weiler |
Vanderbilt University | |
Date: | Thursday, January 22, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | Where are We in Understanding Particles and Interactions, |
and Where are We Going with New Experiments? |
The electroweak theory plus QCD works so well that it has been named the Standard Model. Nevertheless, its failure and its successor are expected to be unveiled in the next round of accelerator commissioning. We discuss how the Standard Model is tested with present accelerators, and what theory will replace it in the near future.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Professor Lisa Mantini |
Department of Mathematics | |
Oklahoma State University | |
Date: | Thursday, January 29, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | Maxwell's Theory, Twistor Theory, |
and Unitary Representations |
The twistor construction of solutions of Maxwell's equations and other massless field equations will be given. The symmetries of these solutions under the group SU(2,2) are illustrated. Generalizations of this method to constructions of unitary representations of the Lie groups SU(p,q) will be explained.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Dr. G.C. Cho |
Institut fuer Halbleitertechnik II | |
RWTH-Aachen, Germany | |
Date: | Monday, February 2, 1998 |
Time: | 3:30 PM |
Place: | NRC 106 |
Title: | Dynamics of THz-Plasmon-Phonon |
Oscillations in Semiconductors |
Femtosecond spectroscopy opens a way toward investigation of the interactions of light and matter occurring at a time scale shorter than the period of a lattice or collective charge carrier oscillation. Coherent plasmon and phonon oscillationscan be launched by impulsive optical excitation of charge carriers in semiconductors. By using pump-probe techniques these oscillations are monitored phase-sensitively in the time domain. In compound semiconductors, the THz-electric-field oscillations associated with coherent plasmons and phonons enable the study of the dynamical electro-optic process on an ultrashort time scale. In this talk, I will present the femtosecond-optical study of THz-plasmon-phonon oscillations in GaAs and CdTe.
Refreshments served at 3:15.
Speaker: | Dr. Min Xiao |
Department of Physics | |
University of Arkansas | |
Date: | Thursday, February 5, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | Electromagnetically Induced Transparency |
and Its Applications in Multi-Level Atomic Systems |
I will present the simple theory of electromagnetically induced transparency (EIT) in ideal three-level atomic systems and our experimental demonstrations of this EIT effect in three-level lambda-type and ladder type systems. Applications of this EIT effect in lasing without inversion and in enhancing efficiency of nonlinear optical processes (such as four-wave mixing) will be discussed.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Professor Min Xiao |
Department of Physics | |
University of Arkansas | |
Date: | Friday, February 6, 1998 |
Time: | 3:00 PM |
Place: | NRC 207 |
Title: | Enhancement of Nondegenerate Four-Wave Mixing Based on |
Electromagnetically Induced Transparency in Rubidium Atoms |
I will describe an experimental demonstration of enhancing the efficiency of nondegenerate four-wave mixing (NDFWM) based on electromagnetically induced transparency (EIT) in a lambda-type three-level system of rubidium atoms. Due to EIT effect, the linear absorption term is greatly reduced, while the nonlinear generation term chi(3) is resonantly enhanced, permitting us to observe a significant enhancement of the NDFWM signal in an optically dense medium. If time allows, I will also describe our recent experiment on coherent transient measurements in rubidium atoms by diode-laser frequency switching.
Speaker: | Professor John P. Ralston |
Department of Physics | |
University of Kansas | |
Date: | Thursday, February 12, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | The First Gauge Theory: A Story of Poverty and |
Riches, Intrigue and Deception, Brilliance and | |
Stupidity, and Untimely Tragic Death |
The history of wave optics and its influence on the emerging electromagnetic theory is a fascinating study of the early nineteenth century. Although it is commonly held that Maxwell first discovered the correct classical description of light, this is not the truth. More than 20 years before Maxwell, the equations of light were deduced using a Lagrangian variational method and symmetry principles by a physicist now almost entirely forgotten. What happened to the first gauge theory, how its author fared, and its influence on the later development of physics makes an intriguing story in the history of ideas. Reflection on the underlying fundamentals also reveals certain biases and misconceptions in modern teaching of physics.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Professor Satyanaray Nandi |
Department of Physics (OSU) | |
Date: | Wednesday, February 18, 1998 |
Time: | 3:30 PM |
Place: | PS 101 |
Title: | The Discovery of the Top Quark |
& Quarks by Computer |
"The Discovery of the Top Quark" by Tony M. Liss and Paul L. Tipton. "Quarks by Computer" by Donald H. Weingarten.
Finding the sixth quark involved the world's most energetic collisions and a cast of thousands. Yearlong computations have helped to confirm the fundamental theory behind quarks -- and, using its principles, even to identify a new particle.
Reading Materials may be picked up in the Help Session rooms PS 249 and PS 354.
Speaker: | Professor Thomas Palberg |
Scientific Workgroup -- Colloidal Physics | |
Johannes Gutenberg University | |
Date: | Thursday, February 19, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | Colloidal Dispersions |
Professor Thomas Palberg, who heads a large group of students and scientists at Johannes Gutenberg University, will speak about some of his refent work with colloidal suspensions which includes: growth kinetics of body centered cubic colloidal crystals, multiphase coexistence and non-linear rheology of colloidal suspensions in an optical model capillary viscometer, probing slow fluctuations in nonergodic systems, microscopic mechanisms of nonlinear rheology of crystalline colloidal suspensions, probing dynamics of dense suspensions with 3D cross correlation techniques, buckling instability in quasi 2D colloidal suspensions, and colloidal crystallization dynamics.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Dr. Amit Raychaudhuri |
Oklahoma State University and | |
University of Calcutta, Calcutta, India | |
Date: | Thursday, February 26, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | What is new in nu-physics |
The neutrino was postulated by Pauli in the 1930s to ensure energy conservation in beta decay. Though a lot of effort went into neutrino experiments, much about it remained unknown. How many kinds of neutrinos are there? Are neutrinos massless particles? We are only beginning to answer these basic questions now. Recent experiments on solar and atmospheric neutrinos seem to poind towards a curious phenomenon: 'neutrino oscillations' -- a simple quantum mechanical manifestation of a non-zero neutrino mass. These and related ideas will be the main theme of this talk.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Professor Joel Martin |
Department of Physics (OSU) | |
Date: | Wednesday, March 4, 1998 |
Time: | 3:30 PM |
Place: | PS 147 |
Title: | Color of Crystals |
The causes of color are diverse, but they all stem from the same root: It is the electrons in matter, through their varied responses to different wavelengths of light, that make the world a many-colored place.
Reading Materials may be picked up in the Help Session rooms PS 249 and PS 354.
Speaker: | Professor Kim Milton |
Department of Physics and Astronomy | |
University of Oklahoma | |
Date: | Thursday, March 5, 1998 |
Time: | 1:30 PM |
Place: | TELECOM 127 |
Title: | PT Symmetric Hamiltonians: |
Why Keep Hermiticity? |
Please note new location and time.
Speaker: | Dr. Karen J. Meech |
Institute for Astronomy | |
University of Hawaii | |
Date: | Thursday, March 5, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | Comets -- Debris from the Primordial Solar System |
This talk will discuss how observations of distant comets are being used to infer conditions during the earliest era of our Solar System. The combination of new technology and large telescopes is enabling the observation and characterization of some of the solar system's smallest denizens. These observations are being combined with observations of extrasolar disks, detailed models of the early solar system and low temperature studies of laboratory ices to build up a consistent picture of the early era of our Solar System's history. Techniques for pushing comet observations to mag 30 to constrain activity, color and composition in the small body populations in the outer solar system will be discussed. A comparison of the fundamental information we can gain from observations of bright comets (using C/1995 O1 Hale-Bopp as an example) will be made with the observations of the distant comets, and unusual objects of intermediate distance.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Tim Wilson |
Department of Physics (OSU) | |
Date: | Wednesday, March 18, 1998 |
Time: | 3:30 PM |
Place: | PS 101 |
Title: | Material Science of Lasers |
Many solid-state materials can be made to lase, but only a few have proven to be commercially successful. Many years of effort were needed to develop blue light-emitting diodes and lasers, but devices based on indium gallium nitride are now set to revolutionize optoelectronics. The road to the realization of short-wavelength, wide-bandgap, II-VI semiconductor diode lasers was fraught with scientific challenges.
Reading Materials may be picked up in the Help Session rooms PS 249 and PS 354.
Speaker: | Professor Satya Nandi |
Department of Physics | |
Oklahoma State University | |
Date: | Thursday, March 19, 1998 |
Time: | 1:30 PM |
Place: | TELECOM 127 |
Title: | Gauge Mediated Supersymmetry Breaking |
Speaker: | Dr. Scott T. Acton |
School of Electrical & Computer Engineering, CEAT | |
Oklahoma State University | |
Date: | Friday, March 27, 1998 |
Time: | 3:30 PM |
Place: | NRC 108 |
Title: | Image Diffusion |
Image diffusion encompasses a broad class of adaptive image processing techniques based on partial differential equations. The image diffusion techniques are applicable to the image enhancement, feature extraction, scale-space generation, image segmentation and image restoration problems.
This talk explores the benefits and shortcomings of current anisotropic diffusion solutions and introduces recent innovations in the diffusion area. Specific advances in the theory include robust morphological diffusion coefficients, a diffusion technique that converges to locally monotonic root signals, extensions to multispectral imagery, multi-resolution (pyramidal) approaches, multigrid solutions and optimization techniques for ill-posed (nonconvex) image restoration problems. Applications to remote sensing, to video tracking and to automated inspection are presented. Other applications in the biomedical and telecommunications areas are discussed.
Coffee & cookies will be served prior to the seminar.
Speaker: | Professor Joel J. Martin |
Department of Physics, OSU | |
Date: | Thursday, April 2, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | Graduation's coming! What am I going to do now? |
(A report on the APS Career Development Meeting) |
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Steven Maier |
Department of Physics | |
Oklahoma State University | |
Date: | Thursday, April 9, 1998 |
Time: | 3:30 PM |
Place: | PS 101 |
Title: | Physics Education Resource Site |
The growing popularity and availability of the Internet to the general public has launched a seemingly infinite number of on-line "resources." It has been my goal to assess some of the more valuable web pages related to physics education and to index them on a single web page to be hosted by the OSU Physics Department's web page.
The Physics Education Resource Site is separated into two main categories: the student's main page and the educator's main page. Each of these pages are broken down into several sub categories (from "Science Forums" to "Pseudo-sciences"). The contents of these categories will be discussed and selected examples will be presented as they appear on the Internet.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 p.m. All students are welcome! Refreshments will be served.
Note different time and location.
Speaker: | Dr. William D. Phillips |
National Institute of Standards and Technology | |
Rice University | |
Date: | Thursday, April 9, 1998 |
Time: | 7:30 PM |
Place: | PS 141 |
Title: | Time, Einstein, and the Coldest Stuff in the Universe |
Atomic clocks are the most accurate timepieces ever made, and are essential for such features of modern life as synchronization of high speed communication and the operation of the Global Positioning System that guides aircraft, boats and backcountry hikers to their destinations. The limitations of atomic clocks come from the thermal motion of the atoms: hot atoms move fast and suffer from time shifts as predicted by Einstein's Theory of Relativity.
Contrary to intuition, we can cool things by shining laser light on them. With laser cooling, we cool gases to less than one millionth of a degree above Absolute Zero. The slowly moving atoms in ruch a gas allow us to make even more accurate clocks, perhaps so good that they would lose or gain only a few billionths of a second a year. Laser cooling has also made possible the recent observation of a long-standing prediction of Einstein: Bose-Einstein condensation, hailed a one of the most important scientific developments in recent years.
This talk will be accessible to those whose last formal science education was in high school, but will discuss some of the most recent and exciting developments in physics.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Dr. Derek Sears |
Department of Chemistry | |
University of Arkansas, Fayetteville, AR | |
Date: | Friday, April 10, 1998 |
Time: | 2:00 PM |
Place: | PS 147 |
Title: | Sows Ears to Silk Purses: The True Story |
of Martian Meteorite Alan Hills 84001 |
The announcement of evidence for relic life in a Martian meteorite was met by universal skepticism by the scientific community in the summer of 1996. However, before the community could formally respond, the attention given the discovery by the media, the administrator for NASA and the President of the U.S., meant that NASA and NSF established funding programs to support this area of research and the establishment of a new Center for Astrobiology at the Ames Research Center in California. This episode provides an interesting comparison to the supposed discovery of cold fusion a few years ago, and provides many insights into the way Science, Politics and Human Affairs interact.
Reading Materials may be picked up in the Help Session rooms PS 249 and PS 354.
Speaker: | Dr. William D. Phillips |
National Institute of Standards and Technology | |
Date: | Friday, April 10, 1998 |
Time: | 3:30 PM |
Place: | PS 141 |
Title: | Optical Lattices: Atomic Physics |
Meets Solid State |
The interference patterns created by intersecting laser beams produces a periodic variation of intensity and polarization that can both cool atoms and trap them at regularly spaced lattice positions. Such optical lattices have many features in common with solid crystals, but with lattice spacings a thousand times larger. The quantum motion of the atoms in these optical lattice potentials can be studied by spectroscopy, Bragg scattering, and coherent redistribution of radiation.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 p.m. All students are welcome! Refreshments will be served.
Speaker: | Dr. Keith R. Dienes |
CERN, Geneva, Switzerland & | |
Institute of Advanced Studies, Princeton, NJ | |
Date: | Monday, April 20, 1998 |
Time: | 4:00 PM |
Place: | PS 110 |
Title: | String Theory and String Phenomenology: |
Where We Are and Where We're Heading |
String phenomenology is the interplay between the Planck-scale physics of string theory and the observable "low-energy" phenomena of modern particle physics. As such, it provides the means by which the ideas of string theory can have an impact at presently accessible energy scales. In this talk, I will provide a non-technical survey of the basic ideas of string theory, and I will highlight the role that string phenomenology plays in guiding present and future theoretical developments. I will also give examples of how string phenomenology suggests new and unconventional approaches for tackling some presently unsolved puzzles.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Please note that this talk is on a Monday.
Speaker: | Dr. Keith R. Dienes |
CERN, Geneva, Switzerland & | |
Institute of Advanced Studies, Princeton, NJ | |
Date: | Tuesday, April 14, 1998 |
Time: | 1:30 PM |
Place: | TELECOM 127 |
Title: | String Theory and Path to Unification: |
A Review of Recent Developments |
Please note that this talk is on a Tuesday.
Speaker: | Dr. Stephen P. Martin |
Institute for Particle Physics | |
University of California, Santa Cruz | |
Date: | Thursday, April 16, 1998 |
Time: | 1:30 PM |
Place: | TELECOM 127 |
Title: | Dynamical Supersymmetry Breaking |
in the Presence of an Anomalous U(1) Symmetry |
Please note location and time.
Speaker: | Dr. C. Robert O'Dell |
Andrew Hays Buchanan Professor of Astrophysics | |
Department of Space Physics and Astronomy | |
Rice University | |
Date: | Thursday, April 16, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | Using the Hubble Space Telescope to Explore |
the Star Forming Regions in the Orion Nebula |
The Orion Nebula is not only the dominant object in the early evening sky, but also the closest region of formation of massive stars. Such clusters are thought to be the prototypes of star formation in general. This talk will report on the results of using the Hubble Space Telescope to explore the Orion Nebula. This study has discovered that circumstellar disks seem to be the rule, rather than the exception. Although such disks were inferred to exist near other young stars, this is the first direct detection. Since such disks are the building blocks necessary for planet formation, these observations argue that planets may be the rule rather than the exception.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Dr. Stephen P. Martin |
Institute for Particle Physics | |
University of California, Santa Cruz | |
Date: | Friday, April 17, 1998 |
Time: | 4:00 PM |
Place: | PS 110 |
Title: | Signals of Supersymmetry Breaking |
Supersymmetry is a proposed extension of the Standard Model of high energy physics which predicts a plethora of new fundamental particles. If supersymmetry is correct, then many or all of these particles should be discovered within the next decade. Most of the outstanding questions about supersymmetry, both theoretical and phenomenological, revolve about the central issue of how it is spontaneously broken. In this talk, I will describe the motivations for supersymmetry, compare the two leading candidate ideas for describing supersymmetry breaking, and contrast their experimental consequences.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Please note that this talk is on a Friday.
Speaker: | Dr. K.S. Babu |
Institute of Advanced Studies, Princeton, NJ | |
Date: | Monday, April 20, 1998 |
Time: | 4:00 PM |
Place: | PS 110 |
Title: | Challenges and Prospects in |
Grand Unified Model Building |
The concept of grand unification, in which the strong, the weak and the electromagnetic interactions are unified into one, will be introduced. After describing its triumphs in explaining various observed phenomena, I will discuss the challenges that are faced by any realistic grand unified model. A new approach that overcomes these challenges will be presented. It has important ramifications for several fundamental problems such as fermion mass generation, neutrino oscillations and proton decay. I will conclude by outlining tests of this idea at ongoing and forthcoming experiments.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Please note that this talk is on a Monday.
Speaker: | Dr. K.S. Babu |
Institute of Advanced Studies, Princeton, NJ | |
Date: | Tuesday, April 21, 1998 |
Time: | 1:30 PM |
Place: | TELECOM 127 |
Title: | Linking Neutrino Masses and |
Proton Decay in Unified Theories |
Please note that this talk is on a Tuesday.
Speaker: | Dr. Joel Berendzen |
Physics Division, Los Alamos National Laboratory | |
Date: | Thursday, April 23, 1998 |
Time: | 4:00 PM |
Place: | PS 101 |
Title: | Around the World and Up One River: |
A Physicist Looks at Structural Biology |
There is excitement in structural biology today that echoes what geographers must have felt in the time of Magellan. New coastlines, in the form of novel protein structures from NMR and X-ray crystallography, appear almost weekly in the leading journals. Although to date we have seen perhaps only 10% of the 'globe' of all protein structural types, motifs have emerged that suggest the structures of a comparatively small number (~5000) of carefully-selected proteins might be used to predict the structures of the remainder to moderate (2.5A) resolution. A large-scale project along these lines is being organized right now. We discuss how physics and physicists can contribute to this effort. We end with a trip up one tributary, the family of heme proteins, to take a look at how a simple protein, myoglobin, works.
The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 p.m. All students are welcome! Refreshments will be served.
Speaker: | Dr. Wouter D. Hoff |
Date: | Wednesday, May 6, 1998 |
Time: | 3:45 PM |
Place: | PS 147 |
Title: | Towards Protein Physics Using Photoreceptors |
Dramatic advances in biochemistry have explained many aspects of the functioning of living organisms in terms of the remarkable properties of proteins. The next step is to understand the functioning of proteins in physical terms. Two major questions are: How do proteins spontaneously fold into highly specific structures upon their synthesis? And how do proteins perform their functions? In this talk these questions will be approached using photoreceptor proteins. In addition to being of importance in their own right as biological light sensors, these proteins provide unique opportunities to examine the basic principles of protein function and folding.
After the talk, let us decide whether we should continue through the summer, and, who will be the next speaker.
Last Updated: 14 April, 1998.
This page was prepared by Helen Au-Yang and Jacques H.H. Perk.
jhhp@jperk.phy.okstate.edu