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Soft Gamma Repeaters and Anomalous X-ray Pulsars: Magnetar Candidates

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arxiv astro-ph/0406133 v3 pith:YSFFFBR5 submitted 2004-06-04 astro-ph

classification astro-ph
keywords anomalousgammamagnetarpulsarsrepeaterssoftx-rayarticle
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This article is a review of Soft Gamma Repeaters and Anomalous X-ray Pulsars. It contains a brief historical record of the emergence of these classes of neutron stars, a thorough overview of the observational data, a succinct summary of the magnetar model, and suggested directions for future research in this field.

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 24 citations worldwide. Full citation record

  1. Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with QED Vacuum Resonance

    astro-ph.HE 2026-03 unverdicted novelty 6.0 of 10

    Strong resonant Compton scattering controlled by magnetic twist and plasma drift can wash out vacuum-resonance 90° PA swings in magnetar soft X-rays and, at high drift, add an extra swing.

  2. Magnetic Moment of Octet Baryons in Isospin Asymmetric Magnetized Strange Matter

    hep-ph 2026-06 unverdicted novelty 4.0 of 10

    Combined CQMF and χCQM models show that Dirac sea effects cause scalar condensates to increase with magnetic field strength, leading to monotonic growth in effective masses of octet baryons in magnetized strange matter.

  3. Exploring GRBs and supernovae connection: does a superluminous hypernova population exist?

    astro-ph.HE 2025-04 unverdicted novelty 2.0 of 10

    A review of gamma-ray burst supernova associations finds that a superluminous hypernova population is not established; only GRB 111209A/SN 2011kl supports the link, and even that event has alternative explanations.

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