{"title":"STAResNet: a Network in Spacetime Algebra to solve Maxwell's PDEs","authors":"Alberto Pepe, Sven Buchholz, Joan Lasenby","doi":"arxiv-2408.13619","DOIUrl":null,"url":null,"abstract":"We introduce STAResNet, a ResNet architecture in Spacetime Algebra (STA) to\nsolve Maxwell's partial differential equations (PDEs). Recently, networks in\nGeometric Algebra (GA) have been demonstrated to be an asset for truly\ngeometric machine learning. In \\cite{brandstetter2022clifford}, GA networks\nhave been employed for the first time to solve partial differential equations\n(PDEs), demonstrating an increased accuracy over real-valued networks. In this\nwork we solve Maxwell's PDEs both in GA and STA employing the same ResNet\narchitecture and dataset, to discuss the impact that the choice of the right\nalgebra has on the accuracy of GA networks. Our study on STAResNet shows how\nthe correct geometric embedding in Clifford Networks gives a mean square error\n(MSE), between ground truth and estimated fields, up to 2.6 times lower than\nthan obtained with a standard Clifford ResNet with 6 times fewer trainable\nparameters. STAREsNet demonstrates consistently lower MSE and higher\ncorrelation regardless of scenario. The scenarios tested are: sampling period\nof the dataset; presence of obstacles with either seen or unseen\nconfigurations; the number of channels in the ResNet architecture; the number\nof rollout steps; whether the field is in 2D or 3D space. This demonstrates how\nchoosing the right algebra in Clifford networks is a crucial factor for more\ncompact, accurate, descriptive and better generalising pipelines.","PeriodicalId":501309,"journal":{"name":"arXiv - CS - Computational Engineering, Finance, and Science","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2024-08-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - CS - Computational Engineering, Finance, and Science","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2408.13619","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We introduce STAResNet, a ResNet architecture in Spacetime Algebra (STA) to
solve Maxwell's partial differential equations (PDEs). Recently, networks in
Geometric Algebra (GA) have been demonstrated to be an asset for truly
geometric machine learning. In \cite{brandstetter2022clifford}, GA networks
have been employed for the first time to solve partial differential equations
(PDEs), demonstrating an increased accuracy over real-valued networks. In this
work we solve Maxwell's PDEs both in GA and STA employing the same ResNet
architecture and dataset, to discuss the impact that the choice of the right
algebra has on the accuracy of GA networks. Our study on STAResNet shows how
the correct geometric embedding in Clifford Networks gives a mean square error
(MSE), between ground truth and estimated fields, up to 2.6 times lower than
than obtained with a standard Clifford ResNet with 6 times fewer trainable
parameters. STAREsNet demonstrates consistently lower MSE and higher
correlation regardless of scenario. The scenarios tested are: sampling period
of the dataset; presence of obstacles with either seen or unseen
configurations; the number of channels in the ResNet architecture; the number
of rollout steps; whether the field is in 2D or 3D space. This demonstrates how
choosing the right algebra in Clifford networks is a crucial factor for more
compact, accurate, descriptive and better generalising pipelines.