- Regular teas most Tuesday and Thursday afternoons: 3:00--3:30 PM,
Youngchild 88
September, 1997
- Tu 23 Sep 3:00 PM Y-90: First tea of the year
- Th 25 Sep 11:10 PM Chapel: Matriculation Convocation; Speaker
Richard Warch.
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- Tu 30 Sep 11:10 PM Chapel: Convocation; Speaker
Tony Kushner.
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October, 1997
- Th 02 Oct 11:10 AM Y-90: Important meeting of junior and senior
majors; sophomores also invited.
- Mo 06 Oct: Deadline for abstracts to Argonne Symposium
- Mo 13 Oct: Department picnic -- Sage Basement -- 6:30
Preparation; 7:00 Meal. Sign up on list on door to Y-88. Charge will
not exceed $2.00
- Sa 18 Oct: Admission Office Prospective Student Open House
- Sa 25 Oct 10:00 of 10:30 AM to noon (probably): Parent's Weekend
Reception and Open House
- MoTu 27-28 Oct: Visit from Washington University dual degree
program cancelled.
- Fr 31 Oct: Admission Office Prospective Student Open House
November, 1997
- FrSa 7-8 Nov: Argonne Symposium
- Sa 8 Nov: Admission Office Prospective Student Open House
- Mo 10 Nov 4:15 PM Youngchild 161: Science Hall Colloquium:
``From Window Glass to
Polyester: the Materials Science of Everyday Objects''
Dr. Robin
Selinger, Department of Physics, Catholic University, Washington DC
Dr. Selinger is a condensed matter theorist and does computer modeling.
- Tu 11 Nov 11:10 AM Youngchild 90: First Physics Colloquium:
``How Things Bend: Dislocations in Crystals''
Dr. Robin Selinger
- Th 19 Nov 3:30 PM Tea 4:00 PM Second Physics Colloquium:
``Theoretical and Computational Modeling of Nonsequential
Ionization'', Scot Shaw, LU, '98
- Tu 25 Nov 3:30 PM Tea 4:00 PM Talk Y-90: Third Physics Colloquium:
``Saturated Absorption Laser Spectroscopy'', Mark Nornberg, LU, '98
``3D Visualization in Reciprocal Space of Smectic Liquid Crystal Phase
Transitions'', James Truitt, LU, '98
December, 1997
- 13 Dec: Graduate Record Examination
January, 1998
- FrSaSu 9-11 Jan: Departmental retreat at Bjorklunden
- Th 29 Jan 4:15 PM Y-161: Science Hall Colloquium
``The Acoustics of Drums''
Dr.~Thomas Rossing,
Professor of Physics at Northern Illinois University, former
President of the American Association of Physics Teachers, expert in
musical acoustics and the physics of music, author of the text used in
Physics of Music.
When struck by a drumstick or beater, a drumhead vibrates in a
complicated manner and radiates sound. In order to understand the
vibrations, it is useful to describe them in terms of normal modes,
which describe the motion of the drumhead(s), the shell, and the
enclosed air. Vibrational modes and sound radiation from a variety of
drums will be described in this talk.
- Fr 30 Jan 3:00 PM Y-161: Fourth Physics Colloquium
``The Physics of Bells'', Dr.~Thomas Rossing
Bells have been a part of nearly every culture in history. In this
talk, we will compare church bells, carillon bells, temple bells,
handbells and ancient Chinese two-tone bells. The talk will include
videotapes of a wide variety of bells.
February, 1998
- Tu 17 Feb 4:00 PM Y-90: Fifth Physics Colloquium:
``Dynamo and Chaotic Magnetic Field in a Laboratory Plasma''
Stewart C. Prager, Professor of Physics, University of
Wisconsin-Madison
Place a hot, million degree plasma in a donut-shaped vacuum chamber
and what happens? Two things of particular interest. First, magnetic
field is generated spontaneously. Current flows in the plasma
``resistor'' with no applied voltage. This laboratory ``dynamo effect''
is similar to the natural dynamos found in the Earth, sun, and other
stars. Second, the plasma, if unheated, cools down in one-thousandth of
a second. These two macroscopic effects arise from tiny fluctuations,
or waves, in the plasma which cause the magnetic field lines to wander
chaotically in space. These effects are observed in the MST plasma
physics experiment at the University of Wisconsin.
Our understanding of dynamo and energy transport has advanced to the
point that we are beginning to control them. We can reduce the magnetic
turbulence and the resultant plasma cooling, a result with impact on the
quest for a fusion energy source.
- Sa 21 Feb: Scholarship weekend
- Th 26 Feb 11:10 PM Chapel: Convocation; Speaker
Richard Rodriguez.
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- FrSaSu 27 Feb-1 Mar: Laser/Chaos Workshop
March, 1998
April, 1998
- We 8 Apr 4:15 PM Y-161: Physics/Chemistry Colloguium:
Let There Be Light: Genesis of Sodium Nightglow and Long
Meteor Trails,
Dr. Dudley Herschbach, Baird Professor of Science, Department of
Chemistry, Harvard University; Nobel Laureate in Chemistry, 1986
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Professor Herschbach will discuss recent progress in solving the
50-year old problem of identifying the origin of sodium
nightglow. He has found new support for the proposition that
sodium nightglow is generated by sodium atoms, ablated from meteors,
undergoing reactions with ozone and oxygen. He and his research
students are perhaps best known for their development of an experimental
technique that employs colliding atomic and molecular beams so as to
observe microscopically the temporal evolution of chemical reactions.
At Harvard, Prof. Heschbach's introductory course is referred to as ``Chem
Zen''.
- Th 9 Apr 11:10 PM Chapel: Convocation; The Impossible Takes
a Little Longer
Dudley Herschbach.
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Professor Herschbach will offer personal observations on teaching and
learning, learning and teaching, and the architectural character of
frontier science.
- ThFrSa 23-25 Apr: NCUR Conference
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- Th 23 Apr 1:30-3:00 PM: Wisconsin Science Teacher Convention
- Th 30 Apr, FrSa 1-2 May: Visit by Research Corporation
consultants
May, 1998
- Mo 11 May 4:15 PM Y-161: Phi Beta Kappa Lecture/Science Hall
Colloquium
``Symmetry - From Kaleidoscopes to Theories of Everything and Nothing''
Dr. HowardGeorgi, Phi-Beta-Kappa visiting
lecturer. Professor of Physics, Harvard University. Major contributor
to current grand unification theories in elementary particle physics.
- Tu 12 May 11:10 AM Y-90: Physics Colloquium
``The Logic of the LHC: How do we know where to look unless we really
know what we are looking for?''
Dr. Howard Georgi
The Higgs boson is a hypothetical particle which may or may not
exist. The Large Hadron Collider (LHC) in Geneva (to which I hope the
US High Energy Physics program will make a major contribution) is
not simply a machine to look for a particle that may not exist.
Instead, the LHC is needed because we know that there is new
physics involving the W and Z bosons that should begin to show up at the
LHC. What makes it exciting is that we do not know what the
new physics is. I will attempt to explain, in a very elementary way,
accessible to graduate students and advanced undergraduates, how we can
know where to look for this new physics, even though we don't know what
it is. The answer has to do with symmetry and the scattering of
Goldstone bosons. I will illustrate the crucial physics pictorially
with computer animations.
- Th 21 May 11:10 PM Chapel: Honors Day Convocation; Speaker
Richard Holbrooke.
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June, 1998
- Su 14 Jun: Commencement