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Phillip Colella

Phillip Colella
Phillip Colella.jpg
Colella in 1980
Nationality Flag of the United States.svg American
Alma mater University of California, Berkeley
Known for High-resolution schemes
Adaptive mesh refinement
Awards Member National Academy of Sciences (2004)
SIAM/ACM prize (2003)
Sidney Fernbach Award (1998)
Scientific career
Fields Applied Mathematics
Institutions Lawrence Livermore National Laboratory
Lawrence Berkeley National Laboratory
University of California, Berkeley
Thesis An Analysis of the Effect of Operator Splitting and of the Sampling Procedure on the Accuracy of Glimm's Method (1979)
Doctoral advisor Alexandre Chorin

Phillip Colella is an American applied mathematician and the Head of the Applied Numerical Algorithms Group at the Lawrence Berkeley National Laboratory. He has also worked at Lawrence Livermore National Laboratory. He is known for his fundamental contributions in the development of mathematical methods and numerical tools used to solve partial differential equations, including high-resolution and adaptive mesh refinement schemes. Colella is a member of the US National Academy of Sciences.

Colella received his bachelor's degree in 1974, Master's degree in 1976, and Ph.D. in 1979 degree from the University of California, Berkeley, all in applied mathematics. He received the Ph.D. degree under the supervision of Alexandre Chorin. He began his research career at Lawrence Berkeley National Laboratory, University of California, California. His primary area of research involves the development of High-resolution schemes and adaptive mesh refinement methods for the solution of partial differential equations. He has also applied computational methods in a variety of scientific and engineering fields, including low-speed incompressible flows, shock wave theory, combustion, magnetohydrodynamics, and astrophysical flows. Colella has also been the leader of a project in NASA's Computational Technologies for Earth and Space Sciences, called "Block-Structured Adaptive Mesh Refinement Methods for Multiphase Microgravity Flows and Star Formation".


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