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Millisecond Magnetars

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arxiv 2103.10878 v1 pith:KRD4WVW6 submitted 2021-03-19 astro-ph.HE

Millisecond Magnetars

Simone Dall'Osso , Luigi Stella This is my paper
classification astro-ph.HE
keywords magnetarsgammamillisecondbelievedburstsenergyfastgravitational
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Two classes of X-ray/$\gamma$-ray sources, the Soft Gamma Repeaters and the Anomalous X-ray Pulsars have been identified with isolated, slowly spinning magnetars, neutron stars whose emission draws energy from their extremely strong magnetic field ($\sim 10^{15}-10^{16}$ G). Magnetars are believed to form with millisecond spin period and to represent an important fraction of the whole population of young neutron stars. Newborn magnetars can convert very quickly their rotational energy into electromagnetic and/or gravitational waves, by virtue of their strong magnetic fields and fast spins. This chapter provides a brief summary of astrophysical problems and scenarios in which millisecond magnetars are believed to play a key role: these include Gamma Ray Bursts, Supernovae, Gravitational Wave events and Fast Radio Bursts.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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    astro-ph.HE 2026-07 conditional novelty 6.0

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  2. Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers

    astro-ph.HE 2026-07 conditional novelty 5.0

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  3. GFH-v2 Pipeline for Searches of Long-Transient Gravitational Waves from Newborn Magnetars

    astro-ph.IM 2025-12 unverdicted novelty 5.0

    GFH-v2 is an enhanced pipeline that improves sensitivity and computational performance for searching long-transient gravitational waves from newborn magnetars.