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Dark Matter distributionxyxzExpectedProfilev 2 ∝M/r=cons.andρ∝(M/r)/r 2ρ∝1/r 2for const.xzrotationcurveDivergent forr=0?NFW∝1/rIsotherm const.Halo profileObservedProfilexyRotation Curvexy2002,Newberg et al. Ibata et al,Crane et al. Yanny et al.diskRbulgeWim de Boer, Karlsruhe Seminar Oxford, May. 3, 2007 16zInner RingtotalDM1/r 2 haloOuter Ring1/r 2 profile and ringsdetermined from independentdirectionsNormalize to solar velocity of 220 km/s
N-body simulations show: Progenitor of 13 kpc ring= Canis Major Dwarf just below Galactic discWim de Boer, Karlsruhe Seminar Oxford, May. 3, 2007 17
Page 1 and 2: The dark connection between Canis M
Page 3 and 4: Thermal History of WIMPsThermal equ
Page 5 and 6: Example of DM annihilation (SUSY)χ
Page 7 and 8: EGRET on CGRO (Compton Gamma Ray Ob
Page 9 and 10: What about background shape?No SMNo
Page 11 and 12: Basic principle for indirect dark m
Page 13 and 14: Analysis of EGRET data in 6 sky dir
Page 15: Background scaling factors agree wi
Page 19 and 20: Excess of DM from Canis Major +tida
Page 21 and 22: Inner Ring coincides with ring of d
Page 23 and 24: Magnetic fields observed in spiral
Page 25 and 26: What about supersymmetry?Present da
Page 27 and 28: Expected SUSY mass spectra in mSUGR
Page 29 and 30: Direct Detection of WIMPsWIMPs elas
Page 31 and 32: DM annihilation in Sun and EarthSUN
Page 33: Summary on WIMP searchesIndirect de

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