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

Low-field magnetars have dipolar magnetic fields of 10<sup>12</sup>-10<sup>13</sup> G, 10-100 times weaker than the values of magnetic-field strength <i>B</i> ≈ 10<sup>14</sup>-10<sup>15</sup> G used to define classical magnetars, yet they produce similar X-ray bursts and outbursts. Using direct numerical simulations of magnetothermal evolution starting from a dynamo-generated magnetic field, we show that the low-field magnetars can be produced as a result of a Tayler-Spruit dynamo inside a proto-neutron star. We find that these simulations naturally explain key characteristics of low-field magnetars: weak (≲10<sup>13</sup> G) dipolar magnetic fields, strong small-scale fields and magnetically induced crustal failures producing X-ray bursts. These findings suggest that the formation channel of low-<i>B</i> magnetars is distinct from that for classical magnetars, reflecting potential differences in proto-neutron-star dynamos.

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Publication Details

Journal
Nature Astronomy
Published
2025-02-04
DOI
https://doi.org/10.1038/s41550-025-02477-y
Citations
6
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
6.93

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article

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

Jérôme Guilet, Toby S. Wood, Paul Barrère, R Raynaud et al.
6 citations
Nature Astronomy
Pulsars and Gravitational Waves Research
6.93
article

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

Jérôme Guilet, Toby S. Wood, Paul Barrère, R Raynaud, Andrei P. Igoshev, Rainer Hollerbach
article en
6 citations

Abstract

Low-field magnetars have dipolar magnetic fields of 10<sup>12</sup>-10<sup>13</sup> G, 10-100 times weaker than the values of magnetic-field strength <i>B</i> ≈ 10<sup>14</sup>-10<sup>15</sup> G used to define classical magnetars, yet they produce similar X-ray bursts and outbursts. Using direct numerical simulations of magnetothermal evolution starting from a dynamo-generated magnetic field, we show that the low-field magnetars can be produced as a result of a Tayler-Spruit dynamo inside a proto-neutron star. We find that these simulations naturally explain key characteristics of low-field magnetars: weak (≲10<sup>13</sup> G) dipolar magnetic fields, strong small-scale fields and magnetically induced crustal failures producing X-ray bursts. These findings suggest that the formation channel of low-<i>B</i> magnetars is distinct from that for classical magnetars, reflecting potential differences in proto-neutron-star dynamos.

Nature AstronomyVol. 9(4)
University of Geneva (CH), Centre National de la Recherche Scientifique (FR), University of Leeds (GB), Université Paris Cité (FR), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), Astrophysique, Instrumentation et Modélisation (FR), CEA Paris-Saclay (FR), Newcastle University (GB)
University of Leicester, Centre National d’Etudes Spatiales, Centre National de la Recherche Scientifique, Science and Technology Facilities Council, Division of Mathematical Sciences
Openalex Percentile: Top 4%
Pulsars and Gravitational Waves Research
6.93
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