neutrino

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!"##$%$"&'()*+'%,"-#.'/,)&0+')%' 1)(*,2%'3+#"/$*4')..%' !"##$%$"&'()*+'%,"-#.'/,)&0+')%' /"&%*(-/*$3+#45.+%*(-/*$3+#4'6$*,'*,+' 1)(*,2%'3+#"/$*4')..%' Earth’s velocity adds RICCARDO CERULLI RICCARDO CERULLI 7-&2%' /"&%*(-/*$3+#45.+%*(-/*$3+#4'6$*,'*,+' )&&-)#'8".-#)*$"& constructively/destructively 7-&2%' )&&-)#'8".-#)*$"& 2-6 2-6 keV 2-6 keV to the Sun’s DAMA/LIBRA DAMA/LIBRA ! ! 250 250 250 kg kg kg (0.87 (0.87 ton"yr) 9(-:$+(;'?@ABC -> annual modulation ton"yr) 9(-:$+(;'?@ABC DE'F)('?? DE'F)('?? NOP'FG77'DHHAC
Indirect DM searches: Detection of the products of DM annihilation (or decay) in the Galactic Center, Sun, Earth, DM halo, etc. producing electrons, positrons, gammarays (PAMELA, ATIC, FERMI/LAT, HESS, Veritas …) and <strong>neutrino</strong>s (IceCube, KM3Net…)
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: σ Recent CRESST-II data (4.7 ) CRE
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 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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neutrino

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