Research
Graduate
Left-Handed light refers to electromagnetic radiation propagating
in a medium that has simultaneous negative values for electric
permittivity and magnetic permeability. These materials, called
metamaterials, don't exist in nature and must be engineered.
Negative permittivity and permeability have remarkable consequences,
primarily because they lead to a negative refractive index.
Therefore, light undergoes "negative refraction"
in such material and bends the "wrong" way. Furthermore,
the Doppler Effect and Cerenkov Radiation are reversed. Current
research seeks to use transformation optics to fabricate an
invisibility cloak, a material that bends radiation of particular
frequencies in such a way that there is minimal absorption
and reflection. Another useful application is the development
of so-called "superlenses". These are lenses made
of metamaterials that are able to overcome the diffraction
limit and achieve sub-wavelength focusing.
Ultimately,
I am interested in the marriage between negative refraction and general relativity. Does gravitation distort spacetime in such a way that gives rise to negative refraction? Are these effects visible in our universe? Researchers have recently shown that regions of negative refraction exist near the equator of rotating black holes. Rotating black holes (or Kerr black holes) are characterized by a region where light and matter are dragged along with the rotating black hole (gravitational frame dragging) but are able to escape its gravitational pull. This region, outside the event horizon, is called the ergosphere, and it has been shown that negative phase propagation is possible for plane waves escaping from here. The effect is enhanced along the equator and is directly proportional to the angular momentum of the black hole.
For more information on this
exciting field of research, see Dr. John Pendry's website
from Imperial College in London.
My adviser,
Dr. Ronald Mallett (adviser lineage)
is a member of the PAN
Group (Particle, Astro, and Nuclear Physics) in the
physics department at UConn.
Undergraduate
As an undergraduate,
I gained applied research experience as a NASA Undergraduate
Space Grant Intern. This program employs students as interns
in research institutions across the country to tackle the
most innovative and important questions/problems plaguing
NASA today. For my project, I worked in conjunction with the
nationwide, Deep
Ecliptic Survey team to study the Kuiper Belt under
the supervision of Dr. David Trilling. The Kuiper Belt yields
tremendous insight into the evolution of our solar system
because it contains ancient, pristine comet-like bodies orbiting
the Sun beyond Neptune. Because of the otherwise isolated
location of the Kuiper Belt, these objects (KBOs) do not significantly
interact gravitationally with the massive terrestrial part
of the Solar System. Therefore, their orbits have been virtually
untainted in time.
I worked on the photometric calibration of the Kuiper Belt to increase precision and accuracy on KBO flux measurements, and subsequently, on the KBO size distribution. By studying the size distribution of the Kuiper Belt, we can develop a more refined accretion timescale of the Solar System. My work has been to write the priority protocol for photometric calibration as well as the original software used to reduce photometric data.
This research has provided me with a wide breadth of skills and practices including computer programming in three languages (C, IDL, PHP). You can find my personal IDL library here. I also have used the following telescopes:
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NOAOs Blanco 4-m telescope at Cerro Tololo Inter-American Observatory in La Serena, Chile
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NOAOs Mayall 4-m telescope at Kitt Peak National Observatory in Tucson, Arizona
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Steward Observatory's Kuiper 61" telescope at Mt. Bigelow in Tucson, Arizona (shown below)
Government
I also had the opportunity
to intern with the US Department of Energy in Washington DC.
I worked in the Nuclear Division's Office of Space and Defense
Power Systems. In particular, I worked on innovative energy
conversion devices for use in NASA spacecraft. An example
of such is the Radioisotope Thermoelectric Generator (RTG).
This system uses the heat released from the alpha decay and
spontaneous fission of Plutonium-238 to power the vehicle.
The Cassini satellite, which recently took fly-by pictures
of Saturn's largest moon: Titan, uses RTGs as a supplementary
power source.

http://en.wikipedia.org/wiki/Image:Cutdrawing_of_an_GPHS-RTG.jpg
I was also lucky enough to visit the Princeton Plasma Physics Laboratory as well as Argonne-West National Laboratory in Idaho Falls, Idaho.