We present gamma-ray flux predictions as expected from neutralino annihilation in the Milky Way, in the Large Magellanic Cloud and in the Andromeda Galaxy in the frame of an effective minimal supersymmetric model and for different dark matter density profiles. We then compare our predictions with the data from the Galactic Center taken from EGRET, CANGAROO-II and HESS.
TeV gamma-rays from neutralino annihilation in the Milky Way and in extragalactic objects
FORNENGO, Nicolao;
2005-01-01
Abstract
We present gamma-ray flux predictions as expected from neutralino annihilation in the Milky Way, in the Large Magellanic Cloud and in the Andromeda Galaxy in the frame of an effective minimal supersymmetric model and for different dark matter density profiles. We then compare our predictions with the data from the Galactic Center taken from EGRET, CANGAROO-II and HESS.
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