Search for Dark Matter Captured in the Sun with ... - KICP Workshops

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Systematic uncertainties Preliminary evaluation of systematic uncertainties Source of uncertainty Estimated effect Neutrino oscillations pending DOM sensetivity spread* pending Interaction cross-section 3.6 – 7.1 % Muon propagation in ice < 1 % Ice model* Absolute DOM efficiency* 1 – 20 % 14 – 51 % time/position callibration < 3 – 5 % Statistical error on signal < 2 % * Full analysis performed with an alternative signal simulation, including maximum llh-analysis (change in acceptance + PSF) 23/07/12 Matthias Danninger IDM 2012 14
Unblinding results (muon flux limit) 23/07/12 Matthias Danninger IDM 2012 15
Page 1 and 2: Search for Dark Matter Captured in
Page 3 and 4: Solar Dark Matter Search with IceCu
Page 9 and 10: IceCube 86-strings ✗ 1.5 km ‐ 2
Page 11 and 12: IceCube-79 string analysis details
Page 13 and 14: Multivariate analysis step (BDT var
Page 15 and 16: Reconstructed zenith (final analysi
Page 17 and 18: The observed angle to the Sun is fi
Page 19 and 20: Unblinding results (expected sensit
Page 21: Unblinding results (observed result
Page 25 and 26: Unblinding results (SD-cross-sectio
Page 27 and 28: Additional slides 23/07/12 Matthias
Page 29 and 30: Reconstructed zenith & BDT output (
Page 31 and 32: Sensitivity extends to WIMP masses
Page 33 and 34: New SUSY analysis with IceCube What
Page 35 and 36: Global SUSY analysis with IceCube M

Search for Dark Matter Captured in the Sun with ... - KICP Workshops

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