{ "id": "astro-ph/9704139", "version": "v1", "published": "1997-04-15T00:32:11.000Z", "updated": "1997-04-15T00:32:11.000Z", "title": "The Attenuation of Gamma-Ray Emission in Strongly-Magnetized Pulsars", "authors": [ "Matthew G. Baring", "Alice K. Harding", "Peter L. Gonthier" ], "comment": "4 pages, including 2 eps figures, with ESA style files, to appear in Proc. of the 2nd Integral Workshop, held in St. Malo, France, Sep. 1996", "categories": [ "astro-ph" ], "abstract": "Gamma-rays from pulsars can be efficiently attenuated in their magnetospheres via the mechanism of single-photon pair production and also the exotic QED process of photon splitting, which become prolific in fields approaching the quantum critical value of $B_{cr}=4.41\\times 10^{13}$ Gauss. Recently we have published results of our modelling of strongly-magnetized $\\gamma$-ray pulsars, which focused on the escape or attenuation of photons emitted near the pole at the neutron star surface in dipole fields, in a Schwarzschild metric. We found that pair production and splitting totally inhibit emission above around 10--30 MeV in PSR1509-58, whose surface field is inferred to be as high as $0.7B_{cr}$. Our model pulsar spectra are consistent with the EGRET upper limits for PSR1509-58 for a wide range of polar cap sizes. Here we review the principal predictions of our attenuation analysis, and identify how its powerful observational diagnostic capabilities relate to current and future gamma-ray experiments. Diagnostics include the energy of the gamma-ray turnover and the spectral polarization, which constrain the estimated polar cap size and field strength, and can determine the relative strength of splitting and pair creation.", "revisions": [ { "version": "v1", "updated": "1997-04-15T00:32:11.000Z" } ], "analyses": { "keywords": [ "gamma-ray emission", "strongly-magnetized pulsars", "attenuation", "polar cap size", "powerful observational diagnostic capabilities relate" ], "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable", "inspire": 461145 } } }