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The MIT
DEPARTMENT OF PHYSICS presents
The 3rd Annual Pappalardo
Fellowships in Physics Symposium

FRIDAY,
MAY 14, 2004
2:00 - 5:00
PM

MIT
Room
W20-307
Mezzanine Lounge, Stratton Student Center
Cambridge, MA
Mission
Statement
The mission of the MIT Pappalardo Fellowships in Physics is to
sustain a distinguished postdoctoral program for the Department
that identifies, recruits and supports the most talented and promising
young physicists at an early stage in their careers.
This initiative was made possible by the encouragement and generosity
of Mr.
A. Neil Pappalardo, EE '64, an MIT alumnus with a long history
of generosity to both the Institute and the Department of Physics.
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Schedule
of Speakers
| 2:00 pm |
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Introductory Remarks |
| 2:15 pm |
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"Getting A Picture of an Extra-Solar Planet"
I will discuss an exciting new approach to studying extra-solar
planetary systems using nulling interferometry. This technique
should make it possible to directly image a few of the closest
extra-solar planetary systems in the near future using comparatively
modest instrumentation. The challenges are in obtaining truly
exquisite levels of wavefront and optical path control.
|
| 2:30 pm |
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Question & Answer |
| 2:45 pm |
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"Prospecting for the First Stars in the Universe"
Sometime in the first billion years after the Big Bang, stars
began to "turn on." We have only a crude understanding
of how and when this happened, since the primordial stars
have not survived to the present day and so cannot be observed
directly. However, we do know that their construction must
have been a delicate physical process.
Using new observations with the Magellan and Keck telescopes,
we are combing through intergalactic space to study the by-products
of these early stars, much as a biologist might search the
fossil record for evidence of extinct species. I will describe
what these measurements have revealed about the history of
early star formation, and the impact that these first stars
and galaxies had on their surrounding environment.
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| 3:00 pm |
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Question & Answer |
| 3:15 pm |
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"Searching for Gravitational Waves in Coincidence with
Gamma-Ray Bursts"
Gamma-Ray Bursts (GRBs) are huge explosions at cosmological
distances. Though theories and models of their nature are
quite diverse, evidence is growing that GRBs may be associated
with certain types of supernovae. These explosions would also
be a source of gravitational waves, and gravitational-wave
detectors such as LIGO (Laser Interferometric Gravitational-wave
Observatory) are currently searching for weak signals in coincidence
with known GRBs detected by satellites. In this talk, I will
motivate this kind of externally-triggered search, and introduce
a multi-burst approach, in which the search is expanded to
include more potential triggers from the HETE-2 satellite.
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| 3:30 pm |
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Question & Answer |
| 3:45 pm |
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Intermission |
| 4:00 pm |
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"Wiring Up an Atom: Toward an Electrical Measurement
of a Single Nuclear Spin"
This talk will discuss initial steps in an experiment that
lives at the interface between electronic devices and quantum
measurements, in which we use a standard conductance measurement
to probe one of the most "quantum" of all natural
systems. By placing a single molecule between two metal electrodes,
and measuring the transport of electric current through the
molecule, we hope to demonstrate a direct electronic readout
of the spin of a single nucleus. Electronic detection of one
nuclear spin will be an exciting result by itself, with applications
in fields ranging from quantum information processing to biology.
But most importantly, this work may open the door to a new
class of experiments that combine the complexity and sensitivity
achievable in electronics circuits with the precision and
breadth of quantum effects visible in molecular physics.
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| 4:15 pm |
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Question & Answer
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| 4:30 pm |
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"Ultracold Atoms in Optical Lattices: Tunable
Quantum Many-Body Systems"
Following the discovery of Bose-Einstein condensation
in 1995, recent years have witnessed enormous progress in
the physics of quantum degenerate atomic gases. In particular,
it has become possible to create "artificial crystals"
of ultracold neutral atoms using optical lattices. I will
show that this allows for quantum simulations of complex solid-state
systems like high-temperature superconductors, which are hopelessly
beyond conventional computational means. Moreover, new quantum
phases and model systems can be engineered that are not accessible
in electronic solids at all. I will give an overview of these
exciting developments from a condensed matter point of view.
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| 5:00 pm |
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Finis |
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Speaker
Biosketches
Joshua Folk Joshua
received his B.S. in Physics with Honors from Stanford University
in 1995. He spent two years in the Peace Corps in Tanzania before
returning to graduate school, again at Stanford, in 1998, with Charles
Marcus as his advisor. He received his Ph.D. in March 2003, and
worked for five months as a postdoctoral researcher with Prof. Isaac
Chuang at MIT before his Pappalardo Fellowship began in September
of that year.
Walter Hofstetter
Prior to coming to MIT in the fall of 2003 as a Pappalardo Fellow
in Physics, Walter was a postdoctoral fellow at Harvard University
(2001-03). He obtained his Ph.D. in Physics from Augsburg University,
Germany, in 2000, and his Diploma from Ludwig-Maximilians-University
in Munich in 1997. Walter's main topics of research are quantum
effects in electronic nanostructures and strongly correlated systems.
More recently, he has become interested in the emerging field of
condensed matter phases in ultracold atoms.
Benjamin Lane
As a Pappalardo Fellow in Physics, Ben works at the MIT Center for
Space Research. Previously, he was a graduate student in the Caltech
Planetary Science department, working with Prof. Shri Kulkarni on
high angular resolution techniques in astronomy, including interferometry
and adaptive optics. Before graduate school Ben worked for Dr. Mark
Colavita at the Jet Propulsion Laboratory on interferometry. He
obtained an undergraduate degree in Astronomy from Caltech in 1997.
Katherine Rawlins
Katherine is originally from California. She earned her undergraduate
degree from Yale University in 1996, and her Ph.D. from the University
of Wisconsin-Madison in 2001 for work on the AMANDA experiment (the
Antarctic Muon and Neutrino Detector Array). Before becoming a Pappalardo
Fellow in 2003, Katherine was a winter-over scientist at Amundsen-Scott
South Pole Station, where the AMANDA experiment is located. Here
at MIT, she has moved from neutrino astrophysics to gravitational-wave
astrophysics, and is analyzing data with LIGO (Laser Interferometric
Gravitational-wave Observatory) and their burst sources working
group.
Robert Simcoe Rob
specializes in observational astrophysics, with particular interest
in the interplay between galaxies and intergalactic matter in the
early universe. He is also engaged in the development of optical
and infrared instrumentation for large ground-based telescopes (including
the Magellan Observatory in Chile, where MIT is a partner institution).
In 1997, Rob completed his undergraduate studies at Princeton University.
He obtained his Ph.D. in Astronomy from Caltech in 2003.
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