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A connection between proto-neutron star Tayler-Spruit dynamos and low-field magnetars

Lookup NU author(s): Dr Andrei IgoshevORCiD, Dr Toby WoodORCiD

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This work is licensed under a Creative Commons Attribution 4.0 International License (CC BY 4.0).

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Author(s): Igoshev A, Barrère P, Raynaud R, Guilet J, Wood T, Hollerbach R

Publication type: Article

Publication status: Published

Journal: Nature Astronomy

Year: 2025

Volume: 9

Pages: 541–551

Print publication date: 01/04/2025

Online publication date: 04/02/2025

Acceptance date: 19/12/2024

Date deposited: 09/01/2025

ISSN (electronic): 2397-3366

Publisher: Nature

URL: https://doi.org/10.1038/s41550-025-02477-y

DOI: 10.1038/s41550-025-02477-y

Data Access Statement: We make data behind all main figures publicly available in Zenodo repository: 10.5281/zenodo.14335239 [62]. 8. For the proto-NS simulation, we used the MagIC code (commit 2266201a5),which is open source at https://github.com/magic-sph/magic. The magnetar spin-down was calculated with the GRB code (commit 84788793),also publicly available at https://github.com/rraynaud/GRBs. We used Magpies code publicly available at https://github.com/ignotur/magpies commit a1fde77. PARODY code is only available upon request same as its original version.

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