Alexander Ayriyan1, Ján Buša Jr.1,2, Hovik Grigorian1,3 and Gevorg Poghosyan4
1 Laboratory of Information Technologies, JINR
2 Institute of Experimental Physics, SAS, Slovakia
3 Department of Theoretical Physics, YSU, Armenia
4 Karlsruhe Institute of Technology, Germany
We have introduced parallel algorithm simulation of neutron star configurations for set of equation of state models. The performance of the parallel algorithm has been investigated for testing set of EoS models on two computational systems. It scales when using with MPI on modern CPUs and this investigation allowed us also to compare two different types of computational nodes.