SIMBAD references

1995A&A...301..456C - Astronomy and Astrophysics, volume 301, 456-462 (1995/9-2)

Magnetic inverse Compton scattering above polar caps.

CHANG H.-K.

Abstract (from CDS):

Following Kundt & Schaaf (1993), it is shown that under certain conditions, inverse Compton scattering is the dominant mechanism for braking escaping charges above polar caps rather than the usually invoked curvature radiation. These conditions are: (i) the polar-cap temperature is that indicated by X-rays from PSRs and (ii) either γ<mec2/kT=103.5T6.5–1 or γ<107(σ/σT)0.25a80.5T6.50.5, where γ is the Lorentz factor of escaping charges, T polar-cap temperature, a curvature radius of magnetic fieldlines, σ cross section of magnetic inverse Compton scattering, and σT Thomson cross section. The cyclotron resonance of magnetic inverse Compton scattering sets an upper bound on the energy of those escaping charges if the strength of the parallel electric field E satisfies the condition E≲103.9GB13T6.52, with B being magnetic field strength.

Abstract Copyright:

Journal keyword(s): radiation mechanisms: non thermal - pulsars: general - X-rays: stars

Simbad objects: 3

goto View the references in ADS

To bookmark this query, right click on this link: simbad:1995A&A...301..456C and select 'bookmark this link' or equivalent in the popup menu