Nonaxisymmetric Precession of Magnetars and Fast Radio Bursts
نویسندگان
چکیده
The repeating FRBs 180916.J0158 and 121102 are visible during periodically-occuring windows in time. We consider the constraints on internal magnetic fields geometry if cyclical behavior observed for FRB~180916.J0158 FRB is due to precession of magnetars. In order frustrate vortex line pinning we argue that must be stronger than about $10^{16}$ Gauss, which large enough prevent superconductivity core destroy crustal lattice structure. conjecture field inside precessing magnetars has three components, (1) a dipole component with characteristic strength $\sim 10^{14}$ Gauss; (2) toroidal 10^{15}-10^{16}$ Gauss only occupies modest fraction stellar volume; (3) disordered 10^{16}$ Gauss. primarily responsible permitting precession, stops once this decays away, happens after 1000$ years. Conceivably, as damps bursting activity diminishes eventually ceases. model quadrupolar distortion star, its ordered components primarily, triaxial very likely prolate. address question whether or not spin frequency ought detectable precessing, by constructing specific bursts happen randomly time random directions distributed between cones relative single symmetry axis. Within context these models, find there geometries detecting unlikely.
منابع مشابه
On Associating Fast Radio Bursts with Afterglows
A radio source that faded over 6 days, with a redshift z ≈ 0.5 host, has been identified by Keane et al. (2016) as the transient afterglow to a Fast Radio Burst (FRB 150418). We report followup radio and optical observations of the afterglow candidate, and find a source that is consistent with an active galactic nucleus (AGN). If the afterglow-candidate is nonetheless a prototypical FRB aftergl...
متن کاملPhysical Constraints on Fast Radio Bursts
Fast Radio Bursts (FRBs) are isolated, ms radio pulses with dispersion measure (DM) of order 10 pc cm. Galactic candidates for the DM of high latitude bursts detected at GHz frequencies are easily dismissed. DM from bursts emitted in stellar coronas are limited by free-free absorption and those from HII regions are bounded by the nondetection of associated free-free emission at radio wavelength...
متن کاملRadio Emission from Magnetars
We discuss properties of the expected radio emission from Soft Gamma-ray Repeaters (SGRs) during their bursting activity in the framework of the model of Thompson, Lyutikov and Kulkarni (2002), in which the high energy emission is powered by the dissipation of super-strong magnetic fields in the magnetospheres through reconnection-type events. Drawing on analogies with Solar flares we predict t...
متن کاملMillisecond Proto-Magnetars & Gamma Ray Bursts
— In the seconds after core collapse and explosion, a thermal neutrinodriven wind emerges from the cooling, deleptonizing newly-born neutron star. If the neutron star has a large-scale magnetar-strength surface magnetic field and millisecond rotation period, then the wind is driven primarily by magneto-centrifugal slinging, and only secondarily by neutrino interactions. The strong magnetic fiel...
متن کاملThe Fluence and Distance Distributions of Fast Radio Bursts
Fast radio bursts (FRB) are millisecond-duration radio pulses with apparent extragalactic origins. All but two of the FRBs have been discovered using the Parkes dish, which employs multiple beams formed by an array of feed horns on its focal plane. In this paper, we show that (i) the preponderance of multiple-beam detections and (ii) the detection rates for varying dish diameters can be used to...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2022
ISSN: ['2041-8213', '2041-8205']
DOI: https://doi.org/10.3847/1538-4357/ac38a6