TY - GEN
T1 - The Cactus computational collaboratory
T2 - 7th Symposium on the Frontiers of Massively Parallel Computation, Frontiers 1999
AU - Allen, Gabrielle
AU - Goodale, Tom
AU - Seidel, Edward
N1 - Publisher Copyright:
© 1999 IEEE.
PY - 1999
Y1 - 1999
N2 - We are developing a system for collaborative research and development for a distributed group of researchers at different institutions around the world. In a new paradigm for collaborative computational science, the computer code and supporting infrastructure itself becomes the collaborating instrument, just as an accelerator becomes the collaborating tool for large numbers of distributed researchers in particle physics, The design of this «Collaboratory» allows many users, with very different areas of expertise, to work coherently together on distributed computers around the world. Different supercomputers may be used separately, or for problems exceeding the capacity of any single system, multiple supercomputers may be networked together through high speed gigabit networks. Central to this Collaboratory is a new type of community simulation code, called «Cactus». The scientific driving force behind this project is the simulation of Einstein's equations for studying black holes, gravitational waves, and neutron stars, which has brought together researchers in very different fields from many groups around the world to make advances in the study of relativity and astrophysics. But the system is also being developed to provide scientists and engineers, without expert knowledge of parallel or distributed computing, mesh refinement, and so on, with a simple framework for solving any system of partial differential equations on many parallel computer systems, from traditional supercomputers to networks of workstations.
AB - We are developing a system for collaborative research and development for a distributed group of researchers at different institutions around the world. In a new paradigm for collaborative computational science, the computer code and supporting infrastructure itself becomes the collaborating instrument, just as an accelerator becomes the collaborating tool for large numbers of distributed researchers in particle physics, The design of this «Collaboratory» allows many users, with very different areas of expertise, to work coherently together on distributed computers around the world. Different supercomputers may be used separately, or for problems exceeding the capacity of any single system, multiple supercomputers may be networked together through high speed gigabit networks. Central to this Collaboratory is a new type of community simulation code, called «Cactus». The scientific driving force behind this project is the simulation of Einstein's equations for studying black holes, gravitational waves, and neutron stars, which has brought together researchers in very different fields from many groups around the world to make advances in the study of relativity and astrophysics. But the system is also being developed to provide scientists and engineers, without expert knowledge of parallel or distributed computing, mesh refinement, and so on, with a simple framework for solving any system of partial differential equations on many parallel computer systems, from traditional supercomputers to networks of workstations.
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U2 - 10.1109/FMPC.1999.750582
DO - 10.1109/FMPC.1999.750582
M3 - Conference contribution
AN - SCOPUS:85030656283
T3 - Proceedings - Frontiers 1999, 7th Symposium on the Frontiers of Massively Parallel Computation
SP - 36
EP - 41
BT - Proceedings - Frontiers 1999, 7th Symposium on the Frontiers of Massively Parallel Computation
PB - Institute of Electrical and Electronics Engineers Inc.
Y2 - 21 February 1999 through 25 February 1999
ER -