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Low Energy WIMP Search Results from CDMS Pheno 2011 Lauren Hsu Fermilab for the CDMS Collaboration Slide material contributed by David Moore 1
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Low Energy WIMP Search Results from CDMS

Feb 15, 2016

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Low Energy WIMP Search Results from CDMS. Lauren Hsu Fermilab for the CDMS Collaboration Slide material contributed by David Moore . Low Mass WIMPs. Lowering the CDMS Threshold. Lowering analysis threshold below 10 keV yields sensitivity to low mass WIMPs in region of contention. - PowerPoint PPT Presentation
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Page 1: Low Energy WIMP Search Results from CDMS

Pheno 2011 1

Low Energy WIMP Search Results from

CDMSLauren Hsu

Fermilabfor

the CDMS CollaborationSlide material contributed by David Moore

Page 2: Low Energy WIMP Search Results from CDMS

Pheno 2011 2

Low Mass WIMPs

Page 3: Low Energy WIMP Search Results from CDMS

Pheno 2011 3

Lowering the CDMS Threshold• Lowering analysis threshold below 10 keV yields sensitivity to low

mass WIMPs in region of contention.• The cost = sacrifice some background rejection due to worsening

timing resolution. Accept > 1 event background.

Page 4: Low Energy WIMP Search Results from CDMS

Pheno 2011 4

Low Threshold Dataset

Page 5: Low Energy WIMP Search Results from CDMS

Pheno 2011 5

Energy Calibration

Page 6: Low Energy WIMP Search Results from CDMS

Pheno 2011 6

Candidate Events

Page 7: Low Energy WIMP Search Results from CDMS

Pheno 2011 7

90% C.L. Limits

Page 8: Low Energy WIMP Search Results from CDMS

Pheno 2011 8

Background Composition

Page 9: Low Energy WIMP Search Results from CDMS

Pheno 2011 9

Comparison to CoGeNT Data

Page 10: Low Energy WIMP Search Results from CDMS

Pheno 2011 10

Naive Energy Rescaling

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Summary• Presented analysis of CDMSII data with threshold

lowered from 10 to 2 keV• Backgrounds present in this analysis have been

characterized. No excess events over expected background were observed

• Despite no background subtraction, observed rate of events is incompatible with interpretation of CoGeNT and DAMA data as evidence for spin-independent elastic scattering of WIMPs

• Compatibility between CDMS and CoGeNT data requires majority of CoGeNT excess to be due to background and unexpectedly small CDMS background

Ahmed et al., PRL 106 131302 (2011), arXiv: 1011.2482

Page 12: Low Energy WIMP Search Results from CDMS

Pheno 2011 12

Shallow Site Comparison

Page 13: Low Energy WIMP Search Results from CDMS

Pheno 2011 13

Zero Charge Events

Page 14: Low Energy WIMP Search Results from CDMS

Pheno 2011 14

Background Composition

Page 15: Low Energy WIMP Search Results from CDMS

Pheno 2011 15

Candidate Events

Page 16: Low Energy WIMP Search Results from CDMS

Pheno 2011 16

Rate by Detector

Page 17: Low Energy WIMP Search Results from CDMS

Pheno 2011 17

CDMSLITE

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Pheno 2011 18

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