Abstract
In this paper, we propose the last version of the numerical model for simulation of astrophysical objects dynamics, and a new realization of our AstroPhi code for Intel Xeon Phi based RSC PetaStream supercomputers. The co-design of a computational model for the description of astrophysical objects is described. The parallel implementation and scalability tests of the AstroPhi code are presented. We achieve a 73% weak scaling efficiency with using of 256x Intel Xeon Phi accelerators with 61440 threads.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
