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Green's matrix for Compton reflection of polarized radiation from cold matter

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dc.contributor.author Poutanen, J
dc.contributor.author Nagendra, K. N
dc.contributor.author Svensson, R
dc.date.accessioned 2008-07-21T11:33:36Z
dc.date.available 2008-07-21T11:33:36Z
dc.date.issued 1996-12
dc.identifier.citation Monthly Notices of the Royal Astronomical Society, Vol. 283, No. 3, pp. 892 - 904 en
dc.identifier.issn 0035-8711
dc.identifier.uri http://hdl.handle.net/2248/2775
dc.description.abstract The Compton-reflected spectrum from cold matter for incident X-rays and gamma-rays with arbitrary angular, spectral and polarization properties can be determined by a simple folding of Green's matrix with the incident spectrum. We calculate Green's matrix by numerically solving the polarized radiative transfer equation for an optically thick planar slab of neutral matter using a method based on discrete space theory. We account for both angular and polarization properties of the fully relativistic Compton scattering cross-section as well as photoelectric absorption and the generation of a fluorescent Fe line. We describe through simple models the basic characteristics of polarized spectra produced by Rayleigh and Compton scattering. The emphasis is on exact computations of Compton-reflected spectra. For the first time, the Fe line equivalent width can be calculated self-consistently for an arbitrary angular distribution of the incident spectrum using Green's matrix formalism. en
dc.format.extent 2027138 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Royal Astronomical Society en
dc.relation.uri http://adsabs.harvard.edu/abs/1996MNRAS.283..892P en
dc.subject Polarization en
dc.subject Radiative transfer en
dc.subject Scattering en
dc.subject Galaxies:seyfert en
dc.subject Gamma rays :theory en
dc.subject X-rays:general en
dc.title Green's matrix for Compton reflection of polarized radiation from cold matter en
dc.type Article en


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