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Dark Matter Signals in Neutrino Telescopes Neutrinos are highly stable, neutral particles. Detection of neutrinos depend on their interactions, i.e cross section. IceCube Annihilation of dark matter particles could produce neutrinos, directly or via decay of Standard Model particles Neutrinos interacting with the matter,i.e nucleons, produce muons which leave charged tracks in the neutrino detector
Neutrino flux from DM annihilation in the core of the Sun/Earth, produced directly or from particles that decay into neutrinos (taus, Ws, bs) Erkoca, Reno and Sarcevic, PRD 80, 043514 (2009) Model-independent results for neutrino signal from DM annihilation in the Galactic Center Erkoca, Gelimini, Reno and Sarcevic, PRD 81, 096007 (2010) Signals for dark matter when DM is gravitino, Kaluza-Klein particle or leptophilic DM. Erkoca, Reno and Sarcevic, PRD 82, 113006 (2010)
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: If the observed anomalies are due t
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 68:
DM Detection with NeutrinoTelescope
Page 71:
Summary Neutrinos could be used to
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