6533b82cfe1ef96bd128f34f
RESEARCH PRODUCT
Magneto-elastic oscillations and the damping of crustal shear modes in magnetars
Nikolaos StergioulasJosé A. FontPablo Cerdá-duránMichael GablerEwald Müllersubject
Shear (sheet metal)PhysicsDipoleSpace and Planetary ScienceAstrophysics::High Energy Astrophysical PhenomenaAstronomy and AstrophysicsAstrophysicsResonant absorptionMagneto elasticMagnetohydrodynamicsMagnetarLower limitMagnetic fielddescription
In a realistic model of magneto-elastic oscillations in magnetars, we find that crustal shear oscillations, often invoked as an explanation of quasi-periodic oscillations (QPOs) seen after giant flares in soft gamma-ray repeaters (SGRs), are damped by resonant absorption on timescales of at most 0.2s, for a lower limit on the dipole magnetic field strength of 5 10 13 G. At higher magnetic field strengths (typical in magnetars) the damping timescale is even shorter, as anticipated by earlier toy-models. We have investigated a range of equations of state and masses and if magnetars are dominated by a dipole magnetic field, our findings exclude torsional shear oscillations of the crust from explaining the observed low-frequency QPOs. In contrast, we find that the Alfv´ en QPO model is a viable explanation of observed QPOs, if the dipole magnetic field strength exceeds a minimum strength of about several times 10 14 G to
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2010-11-25 | Monthly Notices of the Royal Astronomical Society: Letters |