Searching for Dark Matter with the EDELWEISS Experiments
Searching for Dark Matter with the EDELWEISS Experiments
Searching for Dark Matter with the EDELWEISS Experiments
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ection [cm 2 ] (normalised Cross−section to nucleon) [cm 2 ] (normalise<br />
40<br />
42<br />
44<br />
46<br />
48<br />
10<br />
Maximum Likelihood Analysis <strong>for</strong> Low Mass<br />
−42<br />
http://dmtools.brown.edu/<br />
Spin Independent σA [cm -2 ]<br />
120712090201<br />
10 −44<br />
10 −40<br />
10-40 10 −46<br />
10 −42<br />
10-42 XENON1T (proj.)<br />
Preliminary<br />
10 −44<br />
10<br />
120712090201 −48<br />
TU Dresden. G. Adam Cox 6 December 2012<br />
Preliminary<br />
XENON1T (proj.)<br />
EURECA (proj.)<br />
10 50<br />
10 100 1000<br />
| | | | | | | |<br />
• Preliminary<br />
EDW-II PLB 702,5 (2011) 329<br />
DAMA/LIBRA http://dmtools.brown.edu/<br />
EPJ C56 (2008)<br />
CoGeNT PRL 106 (2011)<br />
• In principle, CRESST should II 2σ arXiv:1109.0702 obtain better<br />
limits CRESST by using II entire 1σ arXiv:1109.0702 parameter<br />
space (should be relatively trivial<br />
CDMS Science 327, 1619 (2010)<br />
to add ionization energy)<br />
+ Low E, PRL 106 (2011)<br />
• Need XENON100 to have an arXiv:1207.5988 accurate<br />
gamma background model<br />
EURECA (proj.)<br />
+ PRD 86, 051701(R) (2012)<br />
EDW-III proj. 24kg(fid) 6 months<br />
EDW & CDMS comb. PRD 84 (2011)<br />
XENON100 PRL 107 (2011)<br />
Buchmüller et al, 2011<br />
Bertone et al, 2011<br />
• Improved analysis to come<br />
beginning of 2013<br />
WIMP Mass [GeV/c 2 10 100 1000<br />
WIMP Mass [GeV/c<br />
]<br />
2 10 50<br />
WIMP Mass [GeV/c] 2 ]<br />
38<br />
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