Tran - DESY Theory workshop 2008
Tran - DESY Theory workshop 2008
Tran - DESY Theory workshop 2008
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
The Antiproton Spectrum<br />
The minimal case:<br />
Antiproton flux [GeV -1 m -2 s -1 sr -1 ]<br />
10 -1<br />
10 -2<br />
10 0 0.1 1 10<br />
Background<br />
BESS 95+97<br />
BESS 95<br />
IMAX 92<br />
CAPRICE 94<br />
CAPRICE 98<br />
Signal<br />
Total<br />
10 -3<br />
Φ = 500 MV<br />
[A. Ibarra, DT <strong>2008</strong>]<br />
T [GeV]<br />
Together with the background, the flux is a factor ∼ 2 too large<br />
Is that enough to rule out the model?<br />
David <strong>Tran</strong><br />
Indirect Signatures of Gravitino Dark Matter with Broken R-Parity
Change language