Pair Production and Radiation Effects in Clouds Illuminated by Gamma Ray Sources

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dc.creatorDermer, C. D.
dc.creatorBoettcher, M.
dc.creatorLiang, E. P.
dc.date2001-07-12
dc.date.accessioned2026-07-07T01:59:17Z
dc.date.available2026-07-07T01:59:17Z
dc.descriptionMany classes of gamma-ray sources, such as gamma-ray bursts, blazars, Seyfert galaxies, and galactic black hole sources are surrounded by large amounts of gas and dust. X-rays and gamma-rays that traverse this material will be attenuated by Compton scattering and photoelectric absorption. One signature of an intervening scattering cloud is radiation-hardening by electrons that have been scattered and heated by the incident radiation, as illustrated by a Monte Carlo calculation. Compton scattering provides backscattered photons that will attenuate subsequent gamma rays through γγpair-production processes. We calculate the pair efficiency for a cloud illuminated by gamma-ray burst radiation. An analytic calculation of the flux of X-rays and gamma rays Thomson scattered by an intervening cloud is presented. Illuminated clouds near GRBs will form relativistic plasmas containing large numbers of electron-positron pairs that can be detected within ~1-2 days of the explosion before expanding and dissipating. Localized regions of pair annihilation radiation in the Galaxy could reveal gamma-ray sources embedded in dense clouds, or sites of past GRB explosions.
dc.description4 pages, 3 figures, in 4th INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain
dc.identifierhttps://arxiv.org/abs/astro-ph/0107217
dc.identifierhttp://arxiv.org/abs/astro-ph/0107217
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3050
dc.subjectAstrophysics
dc.titlePair Production and Radiation Effects in Clouds Illuminated by Gamma Ray Sources
dc.typetext

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