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- W3124192939 abstract "Recent calculations of the hydromagnetic deformation of a stratified, non-barotropic neutron star are generalized to describe objects with superconducting interiors, whose magnetic permeability mu is much smaller than the vacuum value mu_0. It is found that the star remains oblate if the poloidal magnetic field energy is gtrsim 40% of total magnetic field energy, that the toroidal field is confined to a torus which shrinks as mu decreases, and that the deformation is much larger (by a factor sim mu_0/mu) than in a non-superconducting object. The results are applied to the latest direct and indirect upper limits on gravitational-wave emission from Laser Interferometer Gravitational Wave Observatory (LIGO) and radio pulse timing (spin-down) observations of 81 millisecond pulsars, to show how one can use these observations to infer the internal field strength. It is found that the indirect spin-down limits already imply astrophysically interesting constraints on the poloidal-toroidal field ratio and diamagnetic shielding factor (by which accretion reduces the observable external magnetic field, e.g. by burial). These constraints will improve following gravitational-wave detections, with implications for accretion-driven magnetic field evolution in recycled pulsars and the hydromagnetic stability of these objects' interiors." @default.
- W3124192939 created "2021-02-01" @default.
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- W3124192939 date "2012-02-01" @default.
- W3124192939 modified "2023-10-04" @default.
- W3124192939 title "Updated gravitational-wave upper limits on the internal magnetic field strength of recycled pulsars" @default.
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- W3124192939 doi "https://doi.org/10.1111/j.1365-2966.2011.20350.x" @default.
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