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N µ up (yr -1 ) Upward Muon Events with 10 5 10 4 10 3 10 2 10 1 10 0 10 -1 10 -2 " 3/2 -> l + l - # " 3/2 -> (Wl,Z#,$#) ! -> µ + µ % E th µ = 50GeV B (1) B (1) -> (qq,l + l - ,W + W - ,ZZ,##) !! -> µ + µ % ATM 1000 10000 m ! (GeV) can need for for DM in o DM tion TeV ther para nific muo con serv spac S uate In F
value ρ(R o )=0.3 GeV/cm 3 [44]. Using these definitions, we can write r = √ Ro 2 + l 2 − 2R o l cos θ and the upper limit for Event the l integral Rates √ in Dependence Eq. (A3) can on be θ max obtained as l max = R o cos θ + Rs 2 − Ro 2 sin 2 θ for a given θ. For the NFW profile, some values for 〈J 2 〉 Ω ∆Ω and 〈J 1 〉 Ω ∆Ω are summarized in Table VII. 0.1 ◦ 1 ◦ 5 ◦ 25 ◦ 50 ◦ 70 ◦ 90 ◦ 〈J 2 〉 Ω ∆Ω 0.14 1.35 5.94 19.68 27.75 31.73 33.42 〈J 1 〉 Ω ∆Ω 0.00027 0.018 0.30 3.69 8.79 12.24 14.90 TABLE VII: The values of J factors for NFW profile for θ max =0.1 ◦ , 1 ◦ , 5 ◦ , 25 ◦ , 50 ◦ , 70 ◦ , 90 ◦ . In Fig. 20 we show 〈J n 〉 Ω ∆Ω factors as a function of θ max for DM annihilation (n =2)andDMdecay(n =1) evaluated for a cone wedge between θ max − 1 ◦ and θ max
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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
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 56 and 57: Contained Muon Flux for Leptophilic
Page 58 and 59: Decaying DM
Page 60 and 61: 2σ Decaying DM
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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