Search for Dark Matter Captured in the Sun with ... - KICP Workshops
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Systematic uncerta<strong>in</strong>ties<br />
Prelim<strong>in</strong>ary evaluation of systematic uncerta<strong>in</strong>ties<br />
Source of uncerta<strong>in</strong>ty Estimated effect<br />
Neutr<strong>in</strong>o oscillations pend<strong>in</strong>g<br />
DOM sensetivity spread*<br />
pend<strong>in</strong>g<br />
Interaction cross-section 3.6 – 7.1 %<br />
Muon propagation <strong>in</strong> ice < 1 %<br />
Ice model*<br />
Absolute DOM efficiency*<br />
1 – 20 %<br />
14 – 51 %<br />
time/position callibration < 3 – 5 %<br />
Statistical error on signal < 2 %<br />
* Full analysis per<strong>for</strong>med <strong>with</strong> an alternative signal simulation,<br />
<strong>in</strong>clud<strong>in</strong>g maximum llh-analysis (change <strong>in</strong> acceptance + PSF)<br />
23/07/12 Matthias Dann<strong>in</strong>ger IDM 2012<br />
14
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