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Machine learning and structure formation in modified gravity

Betts, Jonathan C; van de Bruck, Carsten; Arnold, Christian; Li, Baojiu

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Authors

Jonathan C Betts

Carsten van de Bruck

Christian Arnold



Abstract

In general relativity, approximations based on the spherical collapse model such as Press–Schechter theory and its extensions are able to predict the number of objects of a certain mass in a given volume. In this paper, we use a machine learning algorithm to test whether such approximations hold in screened modified gravity theories. To this end, we train random forest classifiers on data from N-body simulations to study the formation of structures in lambda cold dark matter (CDM) as well as screened modified gravity theories, in particular f(R) and nDGP gravity. The models are taught to distinguish structure membership in the final conditions from spherical aggregations of density field behaviour in the initial conditions. We examine the differences between machine learning models that have learned structure formation from each gravity, as well as the model that has learned from CDM. We also test the generalizability of the CDM model on data from f(R) and nDGP gravities of varying strengths, and therefore the generalizability of extended Press–Schechter spherical collapse to these types of modified gravity.

Citation

Betts, J. C., van de Bruck, C., Arnold, C., & Li, B. (2023). Machine learning and structure formation in modified gravity. Monthly Notices of the Royal Astronomical Society, 526(3), 4148–4156. https://doi.org/10.1093/mnras/stad2915

Journal Article Type Article
Acceptance Date Sep 20, 2023
Online Publication Date Sep 29, 2023
Publication Date 2023-12
Deposit Date Feb 1, 2024
Publicly Available Date Feb 1, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 526
Issue 3
Pages 4148–4156
DOI https://doi.org/10.1093/mnras/stad2915
Public URL https://durham-repository.worktribe.com/output/2189465

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