HISTORY OF AMBER
AMBER has a long history. It was originated by Paul Weiner, who worked in the Kollman group in the late 1970s, and the second release, mainly the work of group member U.C. Singh, incorporated the first versions of the free-energy approaches (in the gibbs module). George Seibel put the code on a more general and maintainable basis, and more recent additions were made by Kollman group members Jim Caldwell and Bill Ross.
AMBER is currently developed as an active collaboration among Kollman and his group (which numbers from 15 to 20, including students, postdoctoral researchers, and visitors), Case and research programmer Mike Crowley at TSRI, Tom Cheatham at NIH, Ken Merz at Penn State, David Ferguson at the University of Minnesota, Tom Darden at the National Institute for Environmental Health Sciences (NIEHS), Carlos Simmerling at SUNY Stony Brook, and Dave Pearlman at Vertex Pharmaceuticals in Boston.
"Even though I am working in the pharmaceutical industry," said Pearlman, "I am still working with and on AMBER. The collaborative effort is a tribute to the openness of Peter Kollman and David Case and their groups." Various modifications made by users get incorporated, Pearlman notes, first as independent modules, and then, as usage warrants, in the main package for public distribution. For example, Tom Darden of NIEHS developed the Particle Mesh Ewald (PME) solvers for the SANDER module of the code, important for dealing with long-range interactions.
Pearlman worked on the calculation of free-energy derivatives and is now working on a module to analyze statistical error in ensemble calculations on the fly, which should help in the intercomparison of free energy calculations. "I'm also working on the idea of using a 'free-energy grid' around the target molecule to help drive the direction of modification of an ongoing calculation towards tighter binding or similar outcomes," Pearlman said. "AMBER is not just a code package; it's an environment in which to think and do chemistry."
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