Saul Teukolsky

Saul A. Teukolsky (born August 2, 1947) is a theoretical astrophysicist and a professor of Physics and Astronomy at Caltech and Cornell University. His major research interests include general relativity, relativistic astrophysics, and computational astrophysics.

Saul A. Teukolsky
Teukolsky in 1975
Born (1947-08-02) August 2, 1947
Johannesburg
Alma materUniversity of the Witwatersrand
Caltech
Known forNumerical Recipes
Scientific career
FieldsAstrophysics
Numerical relativity
InstitutionsCornell
Caltech
Doctoral advisorKip Thorne

Biography

Teukolsky received a Bachelor of Science in Honors Physics and Honors Applied Mathematics from the University of the Witwatersrand, South Africa in 1970. He went on to be a graduate student under Kip Thorne at Caltech where he received his Ph.D. in 1973. He returned to Cornell as an Assistant Professor of Physics and Astronomy in 1974 after serving as the Richard Chace Tolman Research Fellow for one year at Caltech. He was promoted to Associate Professor in 1977 and Full Professor in 1983. In 1999 he was named the Hans A. Bethe professor of physics and astrophysics, a position which he still holds. In 2003 he was elected to the National Academy of Sciences.

Teukolsky is one of the pioneers of numerical relativity: the subject that deals with equations involving general relativity using supercomputers. He is a coauthor of the Numerical Recipes series of books on scientific computing.[1] Today his research group works on numerical relativity calculations to predict signals from the LIGO and LISA experiments.[2]

gollark: Spirit brightening everyone's day as always!
gollark: It does not imply what you're implying it implies.
gollark: Like "well if the equations work similarly in some contexts that obviously means they're the same thing and very related!"
gollark: I'm sure you're going to say something stupid now.
gollark: It is, apparently, "a set of formal analogies between the equations for electromagnetism and relativistic gravitation; specifically: between Maxwell's field equations and an approximation, valid under certain conditions, to the Einstein field equations for general relativity."

References
  1. Numerical Recipes
  2. LIGO
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