Tran - DESY Theory workshop 2008

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Outline 1 Gravitino Dark Matter 2 Gamma Rays 3 Positrons 4 Antiprotons 5 Antideuterons 6 Conclusions David <strong>Tran</strong> Indirect Signatures of Gravitino Dark Matter with Broken R-Parity
The Antiproton Spectrum Theoretical calculations describe the measured antiproton spectrum quite well → No need for new physics in the antiproton spectrum (?) p – flux (m -2 sr -1 sec -1 GeV -1 ) 10 -2 2 3 4 1 5 1 2 3 4 5 10 -1 10 -1 1 10 Cosmic Ray P – David <strong>Tran</strong> Indirect Signatures of Gravitino Dark Matter with Broken R-Parity BESS(95+97) BESS(93) IMAX CAPRICE Bottino Bergstrom Biebar Mitsui λ(R,β) Mitsui λ(R) 10 -3 Kinetic Energy (GeV)
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 and 16: 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: The Positron Fraction The coinciden
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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