Dr. Frank Timmes, professor in the School of Earth
and Space Exploration at Arizona State University and one of four
principal investigators for JINA-CEE, has been awarded a Simons Fellowship
in Theoretical Physics for Fall 2015 and Spring 2016. The Fellowship
provides funding to allow a faculty member to extend an institutionally-approved
sabbatical to a full academic year with the intent of providing strong
intellectual stimulation and leading to increased creativity and productivity
in research. Simons Fellows are chosen based on research accomplishment
in the five years prior to application and the potential scientific
impact of the fellowship.
Timmes, whose research foci are the progenitor evolution, explosion
and nucleosynthesis of supernovae and cosmic chemical evolution, plans
to use his academic year sabbatical to advance his JINA-CEE research
activities. "I am very excited about the opportunity provided by the
Simons Fellowship. It will give me the time and flexibility to pursue
collaborations with colleagues as research projects unfold", said
Timmes, who plans to visit the Kavli Institute for Theoretical Physics
at UC Santa Barbara, as well as experts in nuclear astrophysics at
Michigan State University and the University of Notre Dame. "I feel
fortunate because very few organizations fund sabbatical research
in Theoretical Physics", Timmes said of the award. "I am grateful
to the Simons Foundation for their support of our field".
The Simons Foundation is a private foundation based in New
York City, incorporated in 1994 by Jim and Marilyn Simons. Its mission
is to advance the frontiers of research in mathematics and the basic
sciences by sponsoring a range of programs that aim to promote a deeper
understanding of our world. The Simons Foundation Mathematics and
Physical Sciences division, established in 2010, supports research
in mathematics, theoretical physics and theoretical computer science
and provides funding for individuals, institutions and science infrastructure,
including the Simons Fellows.
Simons Fellows Awardees: Theoretical Physics
Related
Research
Evolution of carbon burning pulses in an 8 solar mass super-AGB
star in a space-time diagram. Nuclear burning develops at about
0.1 solar masses and propagates toward the center of the star
by a steady-state flame followed by a series of fuel starved
pulses. The color bar gives the magnitude of the nuclear energy
generate rate and light blue indicates convective regions.
Image credit: Rob Farmer, Carl Fields, Frank Timmes
http://sese.asu.edu/person/frank-timmes
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JINA-CEE,
March 2015