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low energies, but it does not change the large discrepancies between our upward muon rates compared with Eq. (27) at energies closer to E µ ∼ m χ . 10 ∫ dN / dE µ (GeV -1 yr -1 ) 2 1.5 1 0.5 0 m ! = 500 GeV (Earth, upward) (Sun, upward) (Earth, contained) (Sun, contained) !! -> "" 100 200 300 400 500 E µ (GeV) whe give TeV In from 2π s dom shap the trin mos from muo T mos the
Neutrino Flux from DM Annihilation in the Galactic Center Erkoca, Gelmini, Reno and Sarcevic, Phys. Rev. D81, 096007 (2010) Model independent DM signals: <strong>neutrino</strong>induced upward and contained muons and cascades (showers) For dark matter density, we use different DM density profiles (Navarro- Frenk-White, isothermal, etc) Predictions for IceCube and Km3Net
Page 1 and 2: attempt to fit the Pioneer anomaly
Page 3 and 4: Bergstrom, Rep. Prog. Phys. 63, 793
Page 5 and 6: Dark Matter -What do we know? Dark
Page 7 and 8: What is dark matter? The unknowns:
Page 9 and 10: Dark Matter Detection Direct Detect
Page 11 and 12: σ Recent CRESST-II data (4.7 ) CRE
Page 13 and 14: Indirect DM searches: Detection of
Page 15 and 16: PAMELA Positron Fraction
Page 17 and 18: If the observed anomalies are due t
Page 19 and 20: Neutrino flux from DM annihilation
Page 21 and 22: ● Dark Matter Capture Rate : C
Page 23 and 24: Neutrino Detection Neutrinos intera
Page 25 and 26: Contained and Upward Muon Flux ●
Page 27 and 28: Neutrinos from DM annihilations Neu
Page 30 and 31: than the value required for a therm
Page 32 and 33: ! Attenuation Attenuation of of th
Page 36 and 37: Neutrino Flux from Dark Matter Neut
Page 38 and 39: Dark Matter Density Profiles [87] w
Page 40 and 41: Detection: neutrinos interacting be
Page 42 and 43: Contained and Upward Muon Flux Cont
Page 44 and 45: Muon Flux
Page 46 and 47: Muon Rates
Page 48 and 49: Hadronic Shower Spectra without tra
Page 50 and 51: Probing the Nature of Dark Matter w
Page 52 and 53: E I: Branching fractions for the tw
Page 54 and 55: than the value required for a therm
Page 56 and 57: Contained Muon Flux for Leptophilic
Page 58 and 59: Decaying DM
Page 60 and 61: 2σ Decaying DM
Page 62 and 63: N µ up (yr -1 ) Upward Muon Events
Page 64 and 65: Shower Events
Page 66 and 67: Probing the Parameter Space muon ev
Page 68: DM Detection with NeutrinoTelescope
Page 71: Summary Neutrinos could be used to

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