RSI is a 6-week program for 75 bright high school juniors (50
from the US, 25 from abroad) held each summer at MIT. After an
initial week of classes, the students are paired with research
mentors who may be faculty, staff, postdocs, or graduate
students. Under the supervision of their mentor, they do
research projects similar to summer UROPs. Although the project
duration is limited, the students are extremely bright, highly
motivated, and well supported by RSI staff and tutors. You will
not have to teach them latex or matlab or how to write good
prose. At the end of the program the students write papers
describing their research and give 10-minute oral presentations.
The typical RSI student is comparable to the very best MIT
sophomore physics major. Some of them participate in the
International Physics (or other) Oympiad. Some of them place in
the top 10 of the Intel (formerly Westinghouse) Science Talent
Search, aka the US national science fair.
RSI was featured in an article in Business Week magazine.
I love RSI and look forward to participating each summer as a
mentor. I have been involved with the program since 1998 and
have supervised a number of students, as follows.
1998: Natalia Toro, An Independent
Analysis of Evidence for n_m <-->
n_t Oscillations in the
Super-Kamiokande Atmospheric Neutrino Data (First Place, 1999
Intel Science Talent Search)
Being a RSI mentor requires that you or a co-worker be present
during the 5 weeks of research activities. (A few days' absence
is permissible.) In 2012 the research program dates are
June 29 to July 31. Mentoring typically involves meeting with the
student one to two hours per weekday, except July 4. Unless they
need specialized equipment, the students are able to work fairly
independently.
More information about the program is available at the Center for Excellence
in Education, the organization that runs RSI, and at the
local MIT RSI site.
More information for mentors is available here.
1999: Christopher Cueva, Gravitational
Lensing from a Point Source Orbiting a Schwarzschild Black
Hole
2001: Vivek Venkatachalam, Analysis of
the Omega Diagram for Cosmic Microwave Background Anisotropy and
Type Ia Supernovae (Ninth Place, 2002 Intel Science Talent
Search)
and David Yoshida, The Formation of
Supermassive Black Holes from Pre-galactic Fragments
2002: Joshua Gottlieb, Modeling
Spiral Density Waves in Black Hole Accretion Disks
2003: Drew Reese, On the Effectiveness
of Dark Energy and General Relativity in Modeling the
Universe
2004: Marissa Cevallos, Distribution and Detectability of Dark Matter
in the Present Universe (Semifinalist, 2005 Intel Science
Talent Search)
2005: Peter Roussev, Shrinking the
Wavefunction (Semifinalist, 2006 Intel Science Talent Search)
2007: Samantha Powers, Hydrogen Recombination in
Natural Masing
2008: Marianna Mao (supervised by Phillip Zukin and Sarah Vigeland), Gravitational Radiation from
Encounters with Compact Binaries in Globular Clusters (Finalist, 2009
Intel Science Talent Search)
2009: Shannon Grammel (supervised by Paola Rebusco), Comparison of Simulated and Observational Catalogs of
Hypervelocity Stars in Various Milky Way Potentials
Last modified: Thursday, April 26, 2012
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