SIMBAD references

2018ApJ...854...98W - Astrophys. J., 854, 98-98 (2018/February-3)

Resonant inverse Compton scattering spectra from highly magnetized neutron stars.

WADIASINGH Z., BARING M.G., GONTHIER P.L. and HARDING A.K.

Abstract (from CDS):

Hard, nonthermal, persistent pulsed X-ray emission extending between 10 and ∼150 keV has been observed in nearly 10 magnetars. For inner-magnetospheric models of such emission, resonant inverse Compton scattering of soft thermal photons by ultrarelativistic charges is the most efficient production mechanism. We present angle-dependent upscattering spectra and pulsed intensity maps for uncooled, relativistic electrons injected in inner regions of magnetar magnetospheres, calculated using collisional integrals over field loops. Our computations employ a new formulation of the QED Compton scattering cross section in strong magnetic fields that is physically correct for treating important spin-dependent effects in the cyclotron resonance, thereby producing correct photon spectra. The spectral cutoff energies are sensitive to the choices of observer viewing geometry, electron Lorentz factor, and scattering kinematics. We find that electrons with energies <=15 MeV will emit most of their radiation below 250 keV, consistent with inferred turnovers for magnetar hard X-ray tails. More energetic electrons still emit mostly below 1 MeV, except for viewing perspectives sampling field-line tangents. Pulse profiles may be singly or doubly peaked dependent on viewing geometry, emission locale, and observed energy band. Magnetic pair production and photon splitting will attenuate spectra to hard X-ray energies, suppressing signals in the Fermi-LAT band. The resonant Compton spectra are strongly polarized, suggesting that hard X-ray polarimetry instruments such as X-Calibur, or a future Compton telescope, can prove central to constraining model geometry and physics.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): pulsars: general - radiation mechanisms: nonthermal - scattering - stars: magnetars - stars: neutron - X-rays: general

Simbad objects: 15

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2018ApJ...854...98W and select 'bookmark this link' or equivalent in the popup menu


2021.03.07-19:32:37

© Université de Strasbourg/CNRS

    • Contact