Tran - DESY Theory workshop 2008
Tran - DESY Theory workshop 2008
Tran - DESY Theory workshop 2008
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The Antiproton Spectrum<br />
Theoretical calculations describe the measured antiproton spectrum<br />
quite well<br />
→ No need for new physics in the antiproton spectrum (?)<br />
p – flux (m -2 sr -1 sec -1 GeV -1 )<br />
10 -2<br />
2<br />
3<br />
4<br />
1<br />
5<br />
1<br />
2<br />
3<br />
4<br />
5<br />
10 -1 10 -1 1 10<br />
Cosmic Ray P – David <strong>Tran</strong> Indirect Signatures of Gravitino Dark Matter with Broken R-Parity<br />
BESS(95+97)<br />
BESS(93)<br />
IMAX<br />
CAPRICE<br />
Bottino<br />
Bergstrom<br />
Biebar<br />
Mitsui λ(R,β)<br />
Mitsui λ(R)<br />
10 -3<br />
Kinetic Energy (GeV)
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