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Introduction
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GAMMA-RAY EMISSION FROM THE
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GAMMA-RAY EMISSION FROM THE
Contents
Introduction
Gamma-Ray Emissivity of the Interstellar Medium
The Interstellar Matter
The Molecular Clouds
The Atomic Hydrogen
The Ionized Hydrogen
The Interstellar Radiation Field
The magnetic field
Cosmic Rays
Cosmic Electrons
Cosmic Protons
The physical processes producing gamma-ray emissivity
Proton-Proton collisions
Electron Bremsstrahlung
Inverse Compton
Modeling the Gamma-Ray Emission of the Galaxy
The EGRET observations and the EGRET diffuse emission model
Beyond the EGRET model
The AGILE diffuse gamma-ray emission model
Mapping the matter distribution in the Galaxy
Line broadening and anomalous velocities
The dynamical ambiguity
Rotation curve
Diffuse matter distribution
Interstellar Radiation Field
Cosmic Rays
Observing the Diffuse Emission
The gamma-ray sky
New vs old model
Model vs Observations
AGILE and the Diffuse -ray emission
A simulated AGILE observation
AGILE performances optimization
The AGILE instrument
On-board tracks reconstruction
Event reconstruction in pair production detectors
The ''Kalmaex Algorithm''
Simulation Results
Background rejection
On-ground tracks reconstruction
Spectral capabilities
Conclusions
Acknowledgments
Bibliography
About this document ...
Andrea Giuliani 2005-01-21