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Tel: (212) 854-6834
1976 B.S., Michigan State University (Astrophysics)
1980 Ph.D., SUNY at Stony Brook (Physics)
1981 Postdoc, Neils Bohr Institute
1981 -- 1984 Bantrell Research Fellow, California Institute of Technology
1984 -- 1988 Assistant Professor, Department of Astronomy
1992 -- 1994 Co-Director, Columbia Astrophysics Laboratory
1992 -- 1994 Chairman, Department of Astronomy
1989 -- present Associate Professor, Department of Astronomy
Research Interests:
Stellar Physics: Supernova Explosions, Neutron
Stars, Nucleosynthesis,
The Physics of Interacting Binaries, Millisecond Pulsars
Cosmology: Phase Transitions, Nucleosynthesis
Dynamics: Globular Cluster, Stability of the
Solar System, Special
Purpose Computers
Mathematics: Application of Ito Calculus and
Stochastic Differential
Equations in Astrophysics
I am a theoretical physicist with broad interests in astrophysics. I have developed a model for the orbital period variations seen in the Black Widow Pulsar system PSR B1957+20 which explains the observations and provides an attractive picture for the evolution of the system from a low-mass X-ray binary to a solitary millisecond pulsar or a millisecond pulsar with a family of planets. The novel feature of the model is that the companion is powered by the dissipation of heat by tidal friction. Detailed models of the structure and evolution of tidally powered objects are under development. In my work on cosmology, I have described the consequences of a first order phase transition in quantum chromodynamics on the early evolution of the universe, and shows how this transition might be detectable through its effect on big bang nucleosynthesis. I have performed a Monte-Carlo analysis of the consequences of supernova explosions in binaries. My interest in Ito calculus and stochastic differential equations arose from my trying to explain patterns in the ratios of abundances of elements in metal-poor stars. I believe that these techniques will have many applications in astrophysics.
Selected Publications:
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