neutrino

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DM Detection with NeutrinoTelescopes IceCUBE : 1 km 3 neutrino detector at South Pole ● detects Cherenkov radiation from the charged particles produced in neutrino interactions ● contained and upward muon events and showers ● contained muons from GC ● showers from GC with IceCUBE+DeepCore KM3Net : a future deep-sea neutrino telescope ● contained and upward muon events and showers ● upward muons from GC
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attempt to fit the Pioneer anomaly
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Bergstrom, Rep. Prog. Phys. 63, 793
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Dark Matter -What do we know? Dark
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What is dark matter? The unknowns:
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Dark Matter Detection Direct Detect
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σ Recent CRESST-II data (4.7 ) CRE
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Indirect DM searches: Detection of
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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 34 and 35: low energies, but it does not chang
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 70 and 71: profiles. We consider only smooth h
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neutrino

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