Top-Down Models and UHECRs - rencontres de blois

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Status of topological defect models – necklaces: 1e+27 E 3 J(E)/m −2 s −1 eV 2 1e+26 1e+25 1e+24 1e+23 ν p γ p+γ 1e+22 1e+18 1e+19 1e+20 1e+21 1e+22 E/eV ⇒ shape of spectrum allows only sub-dominant contribution • UHE photon fraction reduced Rencontres de Blois 2008 Michael Kachelrieß Top-Down Models
Cosmic necklaces: [Blanco-Pillado, Olum ’07 ] Rencontres de Blois 2008 Michael Kachelrieß Top-Down Models
Page 1 and 2: Top-Down Models and UHECRs Michael
Page 3 and 4: Bottom-up versus top-down models Bo
Page 5 and 6: The standard candidate: WIMP inflat
Page 7 and 8: Status of neutralino DM after LEPII
Page 9 and 10: Indirect detection claims: Signal f
Page 11 and 12: Indirect detection claims: Signal f
Page 13 and 14: Reminder: GZK puzzle as motivation
Page 15 and 16: Reminder: GZK puzzle as motivation
Page 17 and 18: Modification factor: AGASA excess 1
Page 19 and 20: GZK suppression - dependence on n s
Page 21 and 22: Top-Down Models UHECR primaries are
Page 23 and 24: Gravitational creation of superheav
Page 25 and 26: Gravitational creation of superheav
Page 27 and 28: Properties of superheavy matter: wa
Page 29 and 30: Properties of superheavy matter: wa
Page 31 and 32: Detection of superheavy matter: ind
Page 33 and 34: Lifetime: stable: annihilation give
Page 35 and 36: Fragmentation of heavy particles co
Page 37 and 38: Fragmentation of heavy particles ˜
Page 39 and 40: Signatures of SHDM decays flat spec
Page 41 and 42: Signatures of SHDM decays flat spec
Page 43 and 44: Topological defect models + “gene
Page 45 and 46: Topological defect models + “gene
Page 47: Status of topological defect models
Page 51 and 52: Elmag. cascades and EGRET limit: EG
Page 53 and 54: Sensitivity of neutrino detectors N

Top-Down Models and UHECRs - rencontres de blois

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