Gamma-Rays and Neutrinos from Accretion Processes onto Collapsed Objects: Application to 3C 273
Chapter
Abstract
In this work we want simply to review the metodology used by the authors in the past in order to develop the very important and difficult problem of the calculation of the energy production spectra of the γ-rays and neutrinos produced in the accretion processes onto collapsed objects. Because of the complexity of the problem we start in describing the physical processes in the case of spherical symmetric accretion.
The results of these calculations will be used to evaluate the upper limit to the number of the black holes in the Galaxy and to fit the γ-ray COS B experimental data of the quasar 3C 273 and to predict the neutrino fluxes from the directions of 3C 273 and the Galactic Center.
Keywords
Black Hole Galactic Center Neutrino Flux Production Spectrum Accretion Process
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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