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APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration
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APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

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Page 1: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

WIMP Search WithDEAP-1 @ SNOLAB

Chris JillingsSNOLAB Staff Scientist

For the DEAP-1 Collaboration

Page 2: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Dark matter Experimentwith Argon and

Pulse-shape discrimination

1. Direct WIMP dark-matter detection2. The detector3. Backgrounds and pulse-shape discrimination (PSD)4. Run plan for SNOLAB

DEAP-1 is a 7 kg liquid-argon detector with sensitivity to WIMP dark matter of 10-44 cm2.

It will demonstrate pulse-shape discriminationbetween electromagnetic events and nuclear recoils

at the level of 1 event in 108.

Page 3: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

-CDM with ~25% CDMequiv to 5 H atom per m3

Large-scale structure

Gravitational lensing

CMB

The Dark Matter Problem

Page 4: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Direct Detection

40Ar

40Ar

Use WIMP-nuclear elastic scattering:

Liquid argon scintillates in the far UV. Use wavelengthshifter (TPB) to convert to blue light.

LAr light yield ~ 40 photons/keV electron energy

Boulay and Himehttp://arxiv.org/astro-ph/0411358

Page 5: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

DEAP-1Quartzwindow

7 kg LAr

5” PMTETL 9390Bin polypro

8” long acrylicLight guide

Reflectivecoating &TPB

TPB

Page 6: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

The Detector

Page 7: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Backgrounds

• 39 Ar

• Other betas and gammas

• External neutrons

• (,n) in detector materials

• Surface contamination

Page 8: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

39Ar• N 39Ar = Activity x (Area ROI) x (1 year) x (7kg) • Activity (WARP astro-ph/0603131)

= 0.87 0.02 0.08Bq/kg • ROI (10 to 50 keV) ~ 0.2

• ~ 3 x 107 events• Goal = 0.2 events background• Requires leakage of

electrons to <10-8 PSD

Advertisements: DEAP-1: Bei Cai E14-00007 CLEAN: Hugh Lippincott E14-00009

0 keV 600 keV

0 60 keV20

Xe

Ar

Page 9: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Surface Backgrounds

• Radon in air during handling

• Daughter 218Po plates

• Subsequent decays embed nucleus in surface

• Pass through 210Pb (22 year half life)

• 210Po alpha decays• Recoil nucleus enters LAr

Acrylic222Rn

218Po

218Po

210Po

206Pb

Page 10: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Surface Backgrounds

• Remove surface of all acrylic parts.• Coat surfaces.• Store in sealed (and purged) container.• Build detector with minimum exposure

to air.

• Using gaseous-argon test cell– Expose acrylic to elevated Radon levels

(spike)– Verify previous measurements

Page 11: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Gamma and Neutron Flux

FluxMuonsNeutrons (Thermal)Neutrons (Fast) Radon (Surface)Radon (UGLab) 3.3± 0.4 pCi/L

NoriteK 1.20%238U 1.2 ppm232Th 3.2ppm

<0.27/m_/day4144.9±49.8±105.3 n/m_/day~4000 n/m_/day0.15± 0.12 pCi/L

Data from SNOLAB Users Handbookhttp://www.snolab.ca/

Page 12: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

(,n) and External Neutrons

• Monte-Carlo Studies:– Use measured SNOLAB neutron rates– Use (,n) from material assays

• Target 1 neutron per year– Replace Al dark box with SS– Fill dark box with polypropylene

• Monte Carlo results indicate target will be met.

Page 13: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

SNOLAB

Located at CVRD INCO’s nickel mine near Sudbury, Ontario

Shower,Lunch roomOffices,Meeting roomSNO

cavity

Waterplant

Car wash

Cube Hall

Cryopit

Ladder labs

Page 14: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Deep for DEAP

Mei and Hime: astro-ph/0512125

Flat-overburden sites

Page 15: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Lab SpaceExcavation Clean Rm Laboratory

Area Volume Area Volume Area Volume

Existing

Existing+ Phase I

Existing

+ Phase I &I I

20,049 f t 2 582,993 f t 3 12,196 f t 2 470,360 f t 3 8,095 f t 2 412,390 f t 3

1,863 m2 16,511 m3 1,133 m2 13,321 m3 752 m2 11,679 m3

65,340 f t 2 1,367,488 f t 3 41,955 f t 2 1,049,393 f t 3 26,117 f t 2 837,604 f t 3

6,072 m2 38,728 m3 3,899 m2 29,719 m3 2,427 m2 23,721 m3

77,636 f t 2 1,647,134 f t 3 53,180 f t 2 1,314,973 f t 3 32,877 f t 2 1,043,579 f t 3

7,215 m2 46,648 m 3 4,942 m2 37,241 m3 3,055 m2 29,555 m3

Laboratory and support spaces will be operated as Class 2000 clean rooms. 10 HEPA filtered air changes per hour.

Infrastructure includes: 2MW electrical service, 1 MW chiller capacity, emergency generator, Ultra Pure Water facility, Low background counting facility, high bandwidth network access, chemistry facilities, underground machine shop, light gauge rail line for material transport.

Page 16: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Installation at SNOLABSNOLAB approved siting DEAP-1 in SNO control room.

CurrentSurface Data at Queen’s

Summer 2007Install at site

Run Plan18 months physics data+ calibrations+ background runs

Page 17: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Page 18: APS April meeting Jacksonville, 2007 WIMP Search With DEAP-1 @ SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.

APS April meetingJacksonville, 2007

Gas and Liquid Flow