Tran - DESY Theory workshop 2008
Tran - DESY Theory workshop 2008
Tran - DESY Theory workshop 2008
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The Gamma-Ray Spectrum<br />
Together with the assumed power law background, the angular<br />
dependence of the predicted spectrum is mild enough to be easily<br />
compatible with the EGRET results<br />
The predicted anisotropy and the presence of the line may be tested<br />
by GLAST<br />
The line may also be detectable by Cerenkov telescopes in galaxies<br />
such as M31<br />
David <strong>Tran</strong><br />
Indirect Signatures of Gravitino Dark Matter with Broken R-Parity
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