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Contained Muon Flux for Leptophilic DM
Upward Muon Flux 1 d! / dE µ (GeV -1 km -2 yr -1 ) 10 4 10 3 10 2 10 1 10 0 10 -1 10 -2 " 3/2 -> l + l - #, m "3/2 = 400 GeV, $ = 2.3 x 10 26 sec " 3/2 -> (Wl,Z#,%#), m "3/2 = 400 GeV, $ = 2.3 x 10 26 sec & '> µ + µ ' , µ & = 2 TeV, $ = 2.9 x 10 26 sec B (1) B (1) ->(qq,l + l - ,W + W - ,ZZ,##) , m (1) B = 800 GeV , B = 200 && -> µ + µ ' , m & = 1 TeV, B = 400 ATM a f T t s F c a f 10 -3 10 -4 100 1000 E µ (GeV)
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attempt to fit the Pioneer anomaly
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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 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 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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