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Spectral signatures of compact sources in the inverse Compton catastrophe limit
Author(s) -
Μαρία Πετροπούλου,
Tsvi Piran,
A. Mastichiadis
Publication year - 2015
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/stv1523
Subject(s) - physics , photon , compton scattering , electron , lorentz factor , inverse , compton wavelength , radiative transfer , computational physics , astrophysics , quantum mechanics , lorentz transformation , geometry , mathematics
The inverse Compton catastrophe is defined as a dramatic rise in the luminosity of inverse Compton scattered photons. It is described by a non-linear loop of radiative processes that sets in for high values of the electron compactness and is responsible for the efficient transfer of energy from electrons to photons, predominantly through inverse Compton scatterings. We search for the conditions th...

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