publication . Preprint . 2015

Performance Analysis of an Astrophysical Simulation Code on the Intel Xeon Phi Architecture

Noormofidi, Vahid; Atlas, Susan R.; Duan, Huaiyu;
Open Access English
  • Published: 07 Oct 2015
We have developed the astrophysical simulation code XFLAT to study neutrino oscillations in supernovae. XFLAT is designed to utilize multiple levels of parallelism through MPI, OpenMP, and SIMD instructions (vectorization). It can run on both CPU and Xeon Phi co-processors based on the Intel Many Integrated Core Architecture (MIC). We analyze the performance of XFLAT on configurations with CPU only, Xeon Phi only and both CPU and Xeon Phi. We also investigate the impact of I/O and the multi-node performance of XFLAT on the Xeon Phi-equipped Stampede supercomputer at the Texas Advanced Computing Center (TACC).
arXiv: Computer Science::PerformanceComputer Science::Hardware ArchitectureComputer Science::Mathematical SoftwareComputer Science::Distributed, Parallel, and Cluster ComputingComputer Science::Operating Systems
ACM Computing Classification System: ComputerSystemsOrganization_PROCESSORARCHITECTURESSoftware_PROGRAMMINGTECHNIQUES
free text keywords: Computer Science - Distributed, Parallel, and Cluster Computing, Computer Science - Computational Engineering, Finance, and Science, D.1.3, I.6.8, D.2.8
Funded by
NSF| MRI: Acquisition of a GPU-Accelerated Parallel Supercomputer for Computational Science and Engineering Research at the University of New Mexico
  • Funder: National Science Foundation (NSF)
  • Project Code: 1040530
  • Funding stream: Directorate for Computer & Information Science & Engineering | Division of Advanced Cyberinfrastructure
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[1] S. Woosley and T. Janka. The physics of core-collapse supernovae. Nat. Phys., 1:147, 2005.

[2] K. A. Olive et al. Review of particle physics. Chin. Phys., C38:090001, 2014.

[3] H. Duan, G. M. Fuller, and Y.-Z. Qian. Collective neutrino oscillations. Ann. Rev. Nucl. Part. Sci., 60:569, 2010.

[4] H. Duan, G. M. Fuller, J. Carlson, and Y.-Z. Qian. Simulation of coherent nonlinear neutrino avor transformation in the supernova environment: Correlated neutrino trajectories. Phys. Rev. D, 74(10):105014, 2006.

[5] A. Mirizzi. Multi-azimuthal-angle e ects in self-induced supernova neutrino avor conversions without axial symmetry. Phys. Rev. D, 88(7):073004, 2013. [OpenAIRE]

[6] H. Duan, G. M. Fuller, and J. Carlson. Simulating nonlinear neutrino avor evolution. Comput. Sci. Disc., 1 (1):015007, 2008.

[7] J. Je ers and J. Reinders. Intel Xeon Phi coprocessor high-performance programming. Morgan Kaufmann, San Diego, 2013.

[8] Stampede User Guide, 2015 (accessed March 26, 2015). URL stampede.

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