Research Proposal : Michael O ’ Boyle

نویسنده

  • Michael O’Boyle
چکیده

This project aims to develop a new framework which enables compilers to adapt with and exploit the exponential growth in hardware performance. This is achieved by systematically describing the program optimisation space and by developing new approaches to explore this space in a manner independent of application or underlying architecture. Furthermore, by transcending the distinction between compile-time and run-time and by integrating currently distinct areas of program comprehension and transformation, this project aims to develop a systematic optimisation approach suitable for a diverse range of requirements from cost critical hardwired embedded applications to super-computing grand challenge applications and just-in-time compilation of downloaded applications for reconfigurable FPGA based processors. Given this foundational work, this project aims to change the area of optimising compilation from one that is ad hoc and reactive to hardware evolution to one based on solid foundations that drives architectural change whereby the next generation of hardware is co-designed by compiler technology.

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منابع مشابه

Extrapolating gravitational-wave data from numerical simulations

Michael Boyle and Abdul H. Mroué Center for Radiophysics and Space Research, Cornell University, Ithaca, New York 14853, USA Theoretical Astrophysics, 350-17, California Institute of Technology, Pasadena, California 91125, USA Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 3H8, Canada (Received 19 May 2009; published 29 Decembe...

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Improved methods for simulating nearly extremal binary black holes

Mark A. Scheel, Matthew Giesler, 2 Daniel A. Hemberger, Geoffrey Lovelace, 1 Kevin Kuper, Michael Boyle, Béla Szilágyi, and Lawrence E. Kidder Theoretical Astrophysics 350-17, California Institute of Technology, Pasadena, CA 91125, USA Gravitational Wave Physics and Astronomy Center, California State University Fullerton, Fullerton, California 92834, USA Center for Radiophysics and Space Resear...

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Comparing Post-Newtonian and Numerical-Relativity Precession Dynamics

Serguei Ossokine, 2 Michael Boyle, Lawrence E. Kidder, Harald P. Pfeiffer, 4 Mark A. Scheel, and Béla Szilágyi Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario M5S 3H8, Canada Department of Astronomy and Astrophysics, 50 St. George Street, University of Toronto, Toronto, ON M5S 3H4, Canada Center for Radiophysics and Space Research, Cornell University, It...

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Modeling the source of GW150914 with targeted numerical-relativity simulations

Geoffrey Lovelace, Carlos O. Lousto, James Healy, Mark A. Scheel, Alyssa Garcia, Richard O’Shaughnessy, Michael Boyle, Manuela Campanelli, Daniel A. Hemberger, Lawrence E. Kidder, Harald P. Pfeiffer, Béla Szilágyi, 6 Saul A. Teukolsky, and Yosef Zlochower Gravitational Wave Physics and Astronomy Center, California State University Fullerton, Fullerton, California 92834, USA Center for Computati...

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Synthesis, characterization and using Fe3O4@SiO2@FeCl3 as a new nanocatalyst for aza-Michael reaction between amines and ethyl crotonate

In this article, recyclable Fe3O4@SiO2@FeCl3 was synthesized and entirely characterized by various techniques including XRD, FT-IR, SEM, EDX and VSM analysis. The catalytic ability of produced Fe3O4@SiO2@FeCl3 was studied in the aza-Michael reaction of diethyl amine and ethyl crotonate which lead to high yie...

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تاریخ انتشار 2007