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TCU Box 298840
Fort Worth, TX 76129
Phone: (817) 257-7375
Fax: (817) 257-7742
Email:physics@tcu.edu
This page maintained
by Kaoru Yoshida
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Fall 2002 Seminar Information
Friday September 13 at 2.00 p.m.
Tucker Technology Center, TTC 139
(Professional Development Center)
Dissertation:
Sal Portillo
Department of Physics and Astronomy
TCU
Absolute doubly differential bremsstrahlung
cross sections from rare gas atoms
Refreshments and the Dissertation Oral Examination will follow
Sponsor: Dr. Quarles
Cecil and Ida Green Honors
Chair in Physics, 2002
Thursday September 26
3:00 p.m.
Tucker Technology Center, TTC 139
(Professional Development Center)

Dr.
Pat Richard
Cortelyou-Rust Distinguished Professor
Director, J R Macdonald
Laboratory
Physics Department, KSU
Multiply Excited States of Ions
and Atoms
Coffee will be served after the talk
For further information and directions to the campus
call Department at 817-257-7375
Sponsor: Dr. Quarles
Monday October 7 at 3.00 p.m.
Tucker Technology Center, TTC 139
(Professional Development Center)
Dissertation:
Darron Robbins
Department of Physics and Astronomy
TCU
Spectroscopic and Theoretical Studies of
Novel Germanium-Carbon and Mixed Germanium-Silicon-Carbon Clusters
Refershments served at 2:45 p.m. in TTC 139
Dissertation Oral Examination will follow
Sponsor: Drs. Graham and Rittby
Thursday October 24 at 7.00 p.m.
Tucker Technology Center, TTC 139
(Professional Development Center)
Refreshments will follow
Dr.
David Ceperley
Department of Physics
University of Illinois at Urbana-Champaign
Atom Scale Simulations: From Classical
to Quantum
Sponsor: Dr. Miller
Friday October 25 at 3.00 p.m.
Tucker Technology Center, TTC 139
(Professional Development Center)
Refreshments will follow
Dr.
David Ceperley
Department of Physics
University of Illinois at Urbana-Champaign
Path Integrals and High Pressure Hydrogen
Sponsor: Dr. Miller
Friday November 8 at 1.00 p.m.
SWR 357
Refreshments will follow
Pre-Dissertation:
Greg Sherman
Department of Physics and Astronomy
TCU
Interferometric Probing of Microscale Materials
Sponsor: Dr. Bradley
Tuesday November 12 at 3.00 p.m.
Tucker Technology Center, TTC 139
(Professional Development Center)
Refreshments will follow
Dr.
Gleb Gribakin
Department of Applied Mathematics
and Theoretical Physics
Queens Unviersity Belfast
How do vibrations enhance positron-molecule
annihilation by a factor of 1000?
Sponsor: Dr. Quarles/TCU-RF
Friday December
6 at 3.00 p.m. in TTC 139
Refreshments will follow
Dr. Manfred Cuntz
Department of Physics
University of Texas at Arlington
Orbital Stability and Habitability of Terrestrial
Planets in the 47 UMa System
Abstract: I will discuss whether Earth-type
habitable planets can in principle exist in the 47 UMa planetary system.
The system of 47 UMa consists of two Jupiter-type planets outside
the stellar habitable zone, and thus resembles our own Solar System
most closely compared to all exosolar planetary systems discovered
to date. The definition of habitability follows the concept previously
introduced by Franck et al. (2000a,b) [Tellus 52B, 94; J. Geophys.
Res. 105, E1, 1651], which assumes the long-term possibility of photosynthetic
biomass production under geodynamic conditions. Based on this concept,
it is argued that Earth-type habitable planets around 47 UMa are in
principle possible! The likelihood of those planets critically depends
on the assumed parameters of the planetary surface models. The likelihood
also depends on the assumed stellar luminosity/age, considering that
these parameters dictate the extent of the stellar habitable zone.
Clearly, habitable planets are impossible outside of 1.25 AU, as those
planets would be orbitally unstable due to the gravitational influence
of the two giant planets.
Sponsor: Dr. Marcum
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