High Energy Radiative Transfer Processes in the Superdense Degenerate Plasma

Details High Energy Radiative Transfer Processes in the Superdense Degenerate Plasma High Energy Radiative Transfer Processes in the Superdense Degenerate Plasma

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confs..41a&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 41-41"

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Scientific paper

The closed-form system for Kinetic equations has been obtained to describe the multiple interaction processes between high energy photons and particles, nuclei, as well as ions, taking into consideration the possible micro-processes which are typical for “n,p,e”, “A,n,e” and “A,e” phases of superdense degenerate plasma within the neutron stars and white dwarfs. Especially, the role of particle-antiparticle pairs' production and photo-ionization processes are discussed both in single- and multi-photon approaches. The considered system for Kinetic equations of the diffuse fields of photons and particles has been generalized to describe the neutrino-antineutrino beams' transfer problem, especially to estimate their expected flow based on the “secondary side-effects” observation - mainly due to photons, as well as other detectable particles.

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