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Abelian-Higgs Cosmic String Evolution with CUDA

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arxiv 1809.00995 v2 pith:CCBTNJXO submitted 2018-08-30 physics.comp-ph astro-ph.COgr-qchep-ph

classification physics.comp-phastro-ph.COgr-qchep-ph
keywords cosmicimplementationnetworksabelian-higgscodecosmologicalcurrentdiscuss
verification ladder T0 review T1 audit T2 compute T3 formal
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Topological defects form at cosmological phase transitions by the Kibble mechanism, with cosmic strings and superstrings having the most interesting phenomenology. A rigorous analysis of their astrophysical consequences is limited by the availability of accurate numerical simulations, and therefore by hardware resources and computation time. Improving the speed and efficiency of existing codes is therefore essential. All current cosmic string simulations were performed on Central Processing Units. In previous work we presented a General Purpose Graphics Processing Unit implementation of the evolution of cosmological domain wall networks. Here we continue this paradigm shift and discuss an analogous implementation for local Abelian-Higgs strings networks. We discuss the implementation algorithm (including the discretization used and how to calculate network averaged quantities) and then showcase its performance and current bottlenecks. We validate the code by directly comparing our results for the canonical scaling properties of the networks in the radiation and matter eras with those in the literature, finding very good agreement. We finally highlight possible directions for improving the scalability of the code.

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Cited by 1 Pith paper

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  1. Scaling solutions for current-carrying cosmic string networks. II. Biased solutions

    hep-ph 2025-06 conditional novelty 5.0 of 10

    By relaxing the unbiased-loss assumption in the CVOS model, the paper finds new asymptotic scaling solutions for current-carrying cosmic strings, some of which have no unbiased analog.

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