We present a numerical code, written in C, which can be used to simulate or to analyze the emission of Blazars over the entire electromagnetic spectrum. Our code can reproduce the following features: Synchrotron emission. (Inoue & Takahara 1996 ),(Rybicki & Lightman 1979) - Inverse Compton emission (Thomson & Klein-Nishina regime). (Band & Grindlay 1985),(Blumenthal & Gould 1970) - External Compton emission. - Accretion Disk variability using a Cellular Automata algorithm. - Temporal evolution of the emitting plasma energy distribution. - Flaring phenomena. - Light curves in the rest and in the Observer frame (taking account for time crossing effects) In the following pages, we present the results obtained by our code.
A Numerical Code to Study the Variability of Blazar Emission (Poster)
TOSTI, Gino;
2003
Abstract
We present a numerical code, written in C, which can be used to simulate or to analyze the emission of Blazars over the entire electromagnetic spectrum. Our code can reproduce the following features: Synchrotron emission. (Inoue & Takahara 1996 ),(Rybicki & Lightman 1979) - Inverse Compton emission (Thomson & Klein-Nishina regime). (Band & Grindlay 1985),(Blumenthal & Gould 1970) - External Compton emission. - Accretion Disk variability using a Cellular Automata algorithm. - Temporal evolution of the emitting plasma energy distribution. - Flaring phenomena. - Light curves in the rest and in the Observer frame (taking account for time crossing effects) In the following pages, we present the results obtained by our code.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
