English

Abelian-Higgs cosmic string evolution with multiple GPUs

Computational Physics 2020-11-19 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology

Abstract

Topological defects form at cosmological phase transitions by the Kibble mechanism. Cosmic strings and superstrings can lead to particularly interesting astrophysical and cosmological consequences, but this study is is currently limited by the availability of accurate numerical simulations, which in turn is bottlenecked by hardware resources and computation time. Aiming to eliminate this bottleneck, in recent work we introduced and validated a GPU-accelerated evolution code for local Abelian-Higgs strings networks. While this leads to significant gains in speed, it is still limited by the physical memory available on a graphical accelerator. Here we report on a further step towards our main goal, by implementing and validating a multiple GPU extension of the earlier code, and further demonstrate its good scalability, both in terms of strong and weak scaling. A 819238192^3 production run, using 40964096 GPUs, runs in 33.233.2 minutes of wall clock time on the Piz Daint supercomputer.

Keywords

Cite

@article{arxiv.2005.14454,
  title  = {Abelian-Higgs cosmic string evolution with multiple GPUs},
  author = {J. R. C. C. C. Correia and C. J. A. P. Martins},
  journal= {arXiv preprint arXiv:2005.14454},
  year   = {2020}
}

Comments

v2: additional benchmarks and discussion; version in press at Astronomy and Computing

R2 v1 2026-06-23T15:54:18.946Z