An Efficient Optimization of Hll Method for the Second Generation of Intel Xeon Phi Processor


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详细

In this paper, a new approach to vectorization of algorithms of computational fluid dynamics to simulate the dynamics of astrophysical objects is presented. A co-design of a computational model, from the formulation of equations to software tools, is described. The code performance is analyzed. A speed of 245 gigaflops on Intel Xeon Phi 7250 accelerator and 302 gigaflops on Intel Xeon Phi 7290 accelerator is reached. The code developed is used to solve a problem of interaction of different astrophysical objects such as galaxies, gas clouds, stars clusters.

作者简介

I. Kulikov

Institute of Computational Mathematics and Mathematical Geophysics Siberian Branch

编辑信件的主要联系方式.
Email: kulikov@ssd.sscc.ru
俄罗斯联邦, Novosibirsk, 630090

I. Chernykh

Institute of Computational Mathematics and Mathematical Geophysics Siberian Branch

Email: kulikov@ssd.sscc.ru
俄罗斯联邦, Novosibirsk, 630090

B. Glinskiy

Institute of Computational Mathematics and Mathematical Geophysics Siberian Branch

Email: kulikov@ssd.sscc.ru
俄罗斯联邦, Novosibirsk, 630090

V. Protasov

Novsibirsk State Technical University

Email: kulikov@ssd.sscc.ru
俄罗斯联邦, Novosibirsk, 630073


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