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- W2496887802 abstract "Abstract It is argued that bumps in the timing histories Ω( t ) of the anomalous X-ray pulsars (AXPs) IE 1048.1-5937 and IE 2259+586 are the signature of a magnetar undergoing radiative precession, wherein the hydromagnetic deformation of the neutron star couples to an oscillating component of the vacuum-dipole radiation torque to produce an anharmonic wobble with period τ pr ∼ 10 yr. An analysis of Euler’s equations of motion for a biaxial magnet reproduces the amplitude and recurrence time of the bumps for IE 1048.1-5937 and IE 2259+586, predicts Ω( t ) for the next 20 years for both objects, and predicts a testable statistical relation between d Ω/ dt and τ pr for the AXP population overall. Radiative precession of soft gamma-ray repeaters is also discussed, together with implications for the internal (e.g. viscosity) and magnetospheric (e.g. e + e − pair currents) properties of magnetars." @default.
- W2496887802 created "2016-08-23" @default.
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- W2496887802 date "2000-01-01" @default.
- W2496887802 modified "2023-09-25" @default.
- W2496887802 title "Bumpy Spin-Down of Anomalous X-Ray Pulsars: The Link with Magnetars" @default.
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- W2496887802 doi "https://doi.org/10.1017/s0252921100060991" @default.
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