Tran - DESY Theory workshop 2008

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The Gamma-Ray Spectrum Spectrum for heavier gravitino: E 2 dJ/dE [GeV cm -2 s -1 sr -1 ] 10 -7 10 -6 0.1 1 10 100 E [GeV] David <strong>Tran</strong> Indirect Signatures of Gravitino Dark Matter with Broken R-Parity
The Gamma-Ray Spectrum Spectrum for heavier gravitino: E 2 dJ/dE [GeV cm -2 s -1 sr -1 ] 10 -7 10 -6 0.1 1 10 100 [A. Ibarra, DT 2007] E [GeV] m 3/2 = 150 GeV, τ 3/2 = 1.3 × 10 26 s. David <strong>Tran</strong> Indirect Signatures of Gravitino Dark Matter with Broken R-Parity
Page 1 and 2: Indirect Signatures of Gravitino Da
Page 3 and 4: Outline Based on A. Ibarra and D. T
Page 5 and 6: Indirect Detection Even for graviti
Page 7 and 8: The Gamma-Ray Spectrum The diffuse
Page 9 and 10: The Gamma-Ray Spectrum Calculate de
Page 11 and 12: The Gamma-Ray Spectrum Spectrum for
Page 13 and 14: The Gamma-Ray Spectrum Heavier grav
Page 15: The Gamma-Ray Spectrum Fragmentatio
Page 23 and 24: Outline 1 Gravitino Dark Matter 2 G
Page 25 and 26: The Positron Fraction Propagation i
Page 27 and 28: The Positron Fraction Experiments u
Page 29 and 30: The Positron Fraction Using the EGR
Page 31 and 32: The Positron Fraction The coinciden
Page 33 and 34: The Antiproton Spectrum Theoretical
Page 35 and 36: The Antiproton Spectrum Primary top
Page 41 and 42: Overview of the Indirect Signatures

Tran - DESY Theory workshop 2008

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