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The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf of the LZ Collaboration DPF FNAL, July 31 2017

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Page 1: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

The LUX-Zeplin Dark Matter Search: detector design and

sensitivity Maria Elena Monzani on behalf of the LZ

Collaboration

DPF FNAL, July 31 2017

Page 2: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

LZ = LUX + ZEPLIN

LZ collaboration: •! 38 institutions (USA, UK, Portugal, Russia, South Korea) •! 250+ scientists, engineers, and technicians

LZ collaboration meeting, SURF, July 19 2017 2 MEM-DPF17

Page 3: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

!"#$

!%$&$'()*+,-./$01'$2#3454-678$

$

9:;$4<=$6>$?@A0B@1@6<C>6$

9:;$DE?@A0B@1($

Moore’s Law of Direct Detection

!#:;$DE?@A0B@1($

#3454-+7$

3 MEM-DPF17

Page 4: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

Noble Liquid TPCs for WIMP Detection

•! WIMP-induced nuclear recoils: ~ few keV energy –! S1, S2 ! event energy –! S2 image ! xy coordinate –! S1-S2 timing ! z coord. –! S2/S1 (Xe) ! recoil type –! S1 PSD (Ar) ! recoil type

•! No long-lived isotopes (Xe) •! Self-shielding •! Recoil discrimination

F+$

F'$

3$G:H?$

4 MEM-DPF17

Page 5: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

4,850 ft (Davis

Cavern)

Rn-reduced cleanroom

South Dakota folklore...

LZ at SURF

Page 6: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

LZ Detector Overview

Cathode high voltage feedthrough

Outer detector

PMTs

7 tonne active volume liquid Xe TPC. 10 tonnes total

Liquid Xe HX

Existing water tank

Gadolinium-loaded liquid scintillator veto

Instrumentation conduits

6 MEM-DPF17

Page 7: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

The Xenon TPC Detector

253 PMTs"

241 PMTs"

131 Skin PMTs"

7 MEM-DPF17

Page 8: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

–! 0.61 m thick Gd-loaded scintillator –! instrumented Xenon “skin” –! we can tag neutrons and gammas

In-situ monitoring of residual backgrounds

ROI + S.S. + Vetoes

LZ as a Discovery Instrument

8

Fiducial Mass: 5.6 T (Nominal)

ROI + Single Scatter

MEM-DPF17

Page 9: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

Screening + Simulations: the background table

9

Expected counts in 1,000 live days in an indicative 5.6-tonne fiducial mass in [1.5-6.5] keVee (ER) and [6-30] keV (NR):

•! ER/NR rejection is crucial to the success of the experiment •! PLR analysis: very powerful at rejecting residual ER counts

See

Am

y C

ottle

’s ta

lk

Page 10: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

High Statistics Calibrations in LUX

LUX 2015: 1.1 keVnr cutoff

LUX 2014: 3 keVnr cutoff

Charge Yield

Light Yield

Efficiency

arXiv:1512.03506

Electron Recoil (ER) (Tritiated methane)

Nuclear Recoil (NR) (DD neutron gun)

10

Page 11: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

WIMP Signal Region in LZ

40 GeV WIMP 1"

2"

PDF known with great precision

(x5)

(x500)

arXiv:1703.0914 11

Page 12: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

1,000 days of simulated LZ (5.6 T)

neutrinos ! = 6 x 10-48 cm2

12 arXiv:1703.0914

Page 13: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

LZ Projected Sensitivity: Spin Independent

13 arXiv:1703.0914

Page 14: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

THE SLAC TEST PLATFORM

Page 15: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

SLAC Noble Liquid Test Platform

GRID PROTOTYPING AND TESTING

Page 16: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

PHASE I TEST DETECTOR

Page 17: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

FULL-SCALE GRID LOOM AT SLAC

Page 18: The LUX-Zeplin Dark Matter Search: detector design and sensitivity · 2019. 9. 30. · The LUX-Zeplin Dark Matter Search: detector design and sensitivity Maria Elena Monzani on behalf

Summary and Outlook

•! LZ achieved CD-3 milestone on 02/09/17: –! 2016: LUX removed from Davis campus –! July 2017: surface assembly preparation –! July 2018: underground installation –! 2020: begin LZ commissioning

•! Long lead-time procurements underway •! Quality assurance and testing for hardware

underway; material screening program busy •! LZ benefits from excellent LUX calibrations

and understanding of backgrounds

•! LZ science run to start in 2021: –! 1000 live days, 5.6 tons fiducial mass –! Spin-Indep. sensitivity: 2.3#10-48 cm2

–! Start probing the neutrino floor 18