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Neutrinos from DM annihilations in the core of the Sun/Earth Neutrino flux depends on annihilation rate, distance to source (Earths core or Sun-Earth distance) and energy distribution of <strong>neutrino</strong>s, i.e. In equilibrium, annihila/on rate and capture rate related:
● Dark Matter Capture Rate : C ∼ ρ DM M σ χN p ρ DM =0.3 GeV cm −3 v DM ∼ 270 km s −1 v esc = 1156 km/s v esc = 13.2 km/s for the Sun for the Earth M is the mass of the Sun/Earth Capture rate in the Sun is about 10 9 times larger than capture rate in the Earth For the Sun, annihilation rate = C/2
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: Neutrino flux from DM annihilation
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 68: DM Detection with NeutrinoTelescope
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Summary Neutrinos could be used to
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