inria-00431637, version 1
Cosmological Simulations on a Grid of Computers
N° RR-7093 (2009)
Abstract: The work presented in this paper aims at restricting the input parameter values of the semi-analytical model used in Galics and MoMaF, so as to derive which parameters influence the most the results, e.g., star forma- tion, feedback and halo recycling efficiencies, etc. Our approach is to proceed empirically: we run lots of simulations and derive the correct ranges of values. The computation time needed is so large, that we need to run on a grid of com- puters. Hence, we model Galics and MoMaF execution time and output files size, and run the simulation using a grid middleware: Diet. All the complexity of accessing resources, scheduling simulations and managing data is harnessed by Diet and hidden behind a web portal accessible to the users.
- a – Ecole Normale Supérieure de Lyon - ENS Lyon
- b – INRIA
- 1:
- Université de Lyon – CNRS : UMR5668 – INRIA – École Normale Supérieure - Lyon – Université Claude Bernard - Lyon I
- 2:
- CNRS : UMR5668 – INRIA – École Normale Supérieure - Lyon – Université Claude Bernard - Lyon I – Laboratoire d'informatique du Parallélisme
- 3:
- CNRS : UMR5822 – IN2P3 – Université Claude Bernard - Lyon I
- 4:
- CNRS : UMR5574 – INSU – Université Claude Bernard - Lyon I – École Normale Supérieure - Lyon
- Collaboration : Grid'5000
- Domain : Computer Science/Distributed, Parallel, and Cluster Computing
- Keywords : Cosmology – N-body simulations – Parallel computing – Local uni- verse – Middleware – Grid-RPC
- Internal note : RR-7093
- inria-00431637, version 1
- http://hal.inria.fr/inria-00431637
- oai:hal.inria.fr:inria-00431637
- From:
- Submitted on: Thursday, 12 November 2009 16:32:05
- Updated on: Monday, 23 April 2012 16:24:19







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