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Véronique SANGLARD Université de Lyon, UCBL1 CNRS/IN2P3/IPNLyon [email protected] http://edelweiss.in2p3.fr QuickTime™ et un décompresseur TIFF (non comp sont requis pour visionner c Status of EDELWEISS-II Status of EDELWEISS-II

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Status of EDELWEISS-II. Outline. EDELWEISS experiment EDELWEISS-I limits EDELWEISS-II setup EDELWEISS-II preliminary results. *Expérience pour DEtecter Les WIMPs En SIte Souterrain (Underground experiment to detect WIMP). The EDELWEISS collaboration. CEA Saclay CSNSM Orsay - PowerPoint PPT Presentation

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Page 1: Status of EDELWEISS-II

Véronique SANGLARDUniversité de Lyon, UCBL1

CNRS/IN2P3/[email protected]

http://edelweiss.in2p3.fr

QuickTime™ et undécompresseur TIFF (non compressé)

sont requis pour visionner cette image.

Status of EDELWEISS-IIStatus of EDELWEISS-II

Page 2: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 2

OutlineOutline

EDELWEISS experiment

EDELWEISS-I limits

EDELWEISS-II setup

EDELWEISS-II preliminary results

Page 3: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 3

The EDELWEISS collaborationThe EDELWEISS collaboration CEA Saclay CSNSM Orsay IPN Lyon Institut Néel Grenoble FZ/ Universität Karlsruhe JINR Dubna

*Expérience pour DEtecter Les WIMPs En SIte Souterrain (Underground experiment to detect WIMP)

Page 4: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 4

EDELWEISS @ LSM EDELWEISS @ LSM (Laboratoire (Laboratoire

Souterrain de Modane)Souterrain de Modane)

Page 5: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 5

Heat and Ionization Ge detectorsHeat and Ionization Ge detectors

Simultaneous measurement of

Heat @ 17 mK with Ge/NTD sensor

Ionization @ few V/cm with Al electrodes

Different charge/heat ratio for nuclear recoils (WIMP, neutrons) and electron recoils (, )

EI/ER = 0.3 for nuclear recoils

EI/ER = 1 for electronic recoils

Event-by-event discrimination of electron recoils (main background) Neutrons 73Ge(n,n',) Gammas

IonizationguardIonizatio

ncenter

Fiducial volume(≈ 57%)

Heat

Thermometer(Ge NTD)

Reference electrode

Center electrodeGuard

Electrodes

Ge crystal

Center electrodeGuard ring

7 cmm=320g

Ionization threshold

Amorphous (Ge or Si) ~ 60 nm

Page 6: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 6

EDELWEISS-I EDELWEISS-I (V.S. et al., (V.S. et al., PRD PRD 7171, 122002 (2005)), 122002 (2005))

62 kg.d with 3 detectors Best sensitivity up to

2003, but Background

Neutrons : 1 n-n coincidence observed (2 singles expected by MC)

Surface electron recoils Miscollected charge

events at low energy Leak of events down to

the nuclear recoil band not visible in coincidence events

Rate compatible with 210Pb contamination ( rate ~ 5 / kg.d)

QuickTime™ et undécompresseur TIFF (non compressé)

sont requis pour visionner cette image.

Page 7: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 7

EDELWEISS-II setupEDELWEISS-II setup Cryogenic installation (~ 20 mK)

Reversed geometry cryostat Dilution refrigerator + pulse tube Room for up to 120 detectors

Shielding Clean room + deradonized air

(15 mB/m3) 20 cm Pb 50 cm PE Active veto (> 98% coverage)

Facilities Remotely controlled sources for

calibrations and regenerations Remote operations (cryogeny,

acquisition, …) Detector storage and repair

within the clean room 9 cool-downs since January 2006

Page 8: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 8

EDELWEISS-II setupEDELWEISS-II setup Cryogenic installation (~ 20 mK)

Reversed geometry cryostat Dilution refrigerator + pulse tube Room for up to 120 detectors

Shielding Clean room + deradonized air

(15 mB/m3) 20 cm Pb 50 cm PE Active veto (> 98% coverage)

Facilities Remotely controlled sources for

calibrations and regenerations Remote operations (cryogeny,

acquisition, …) Detector storage and repair

within the clean room 9 cool-downs since January 2006

QuickTime™ et undécompresseur TIFF (non compressé)

sont requis pour visionner cette image.

Page 9: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 9

EDELWEISS-II detectorsEDELWEISS-II detectors

“standard” Ge/NTD bolometers (320 g) as for EDELWEISS-I

Ge/NbSi bolometers (400 g)

“interdigit” Ge/NTD bolometers (200-400 g)

Page 10: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 10

Results from “standard” NTD Results from “standard” NTD detectorsdetectors

Commissioning background run (spring 2007) ~ 19 kg.d 8 lowest threshold detectors selected Only « pure center » events selected for better Ei resolution Reduction of factor 3 of and background

Recoil energy threshold (20-35 keV)

Ion

iza

tio

n/R

ec

oil

Ra

tio

Ion

iza

tio

n/R

ec

oil

Ra

tio

Page 11: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 11

Results from “standard” NTD Results from “standard” NTD detectorsdetectors

Ion

iza

tio

n/R

ec

oil

Ra

tio

Recoil energy threshold (20-35 keV)

Commissioning background run (spring 2007) ~ 19 kg.d 8 lowest threshold detectors selected Only « pure center » events selected for better Ei resolution Reduction of factor 3 of and background

Page 12: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 12

Results from “standard” NTD Results from “standard” NTD detectorsdetectors

Significant reduction of the background

Calibration with source (210Pb) to study the detector’s response to surface events

~ 100 kg.d of fiducial exposure accumulated after quality cuts (analysis still underway)

QuickTime™ et undécompresseur TIFF (non compressé)

sont requis pour visionner cette image.

Page 13: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 13

Results from Ge/NbSi detectorsResults from Ge/NbSi detectors

200

150

100

50

0

806040200

x10-3

200

150

100

50

0

806040200

x10-3

Transient

Thermal

Heat signal of thermometer NbSiA :Surface event Bulk event

Thermometer Thermometer NbSiNbSi BB

Thermometer Thermometer NbSi NbSi AA Thermometer Thermometer NbSi NbSi AA

Thermometer Thermometer NbSiNbSi BB

Time (ms)

200

150

100

50

0

806040200

x10-3

200

150

100

50

0

806040200

x10-3

Transient

Thermal

Heat signal of thermometer NbSiA :Surface event Bulk event

Thermometer Thermometer NbSiNbSi BB

Thermometer Thermometer NbSi NbSi AA Thermometer Thermometer NbSi NbSi AA

Thermometer Thermometer NbSiNbSi BB

200

150

100

50

0

806040200

x10-3

200

150

100

50

0

806040200

x10-3

Transient

Thermal

Heat signal of thermometer NbSiA :Surface event Bulk event

Thermometer Thermometer NbSiNbSi BB

Thermometer Thermometer NbSi NbSi AA Thermometer Thermometer NbSi NbSi AA

Thermometer Thermometer NbSiNbSi BB

Time (ms)

Developed @ CSNSM since 2003 Goal : active identification of

surface events using athermal phonon measurement with NbSi thin film thermometers

Each signal = thermal + athermal component

For surface events, athermal higher in corresponding thermometer

Thermal signals proportional to the deposited energy

Discrimination parameter = asymetry of athermal part of signals from the two surfaces

Surface rejection ok, some problems in 2007 with film contacts / leak currents

Resolutions hasn’t reached Ge/NTD performances

Page 14: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 14

Results from Ge/NbSi detectorsResults from Ge/NbSi detectors Developed @ CSNSM since 2003 Goal : active identification of

surface events using athermal phonon measurement with NbSi thin film thermometers

Each signal = thermal + athermal component

For surface events, athermal higher in corresponding thermometer

Thermal signals proportional to the deposited energy

Discrimination parameter = asymetry of athermal part of signals from the two surfaces

Surface rejection ok, some problems in 2007 with film contacts / leak currents

Resolutions hasn’t reached Ge/NTD performancesData taken with 1 NbSi detector

May & June 2007 ~ 1,5 kg.d fiducial

Page 15: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 15

Results from Ge/Interdigit Results from Ge/Interdigit detectordetector

Radial coordinate (cm)

Z (cm) guard electrode G : + 1V

guard electrode H : - 1V

A electrodes : + 2V B electrodes + 1V

C electrodes : - 2VD electrodes : - 1V

Electrons trajectoriesholestrajectories

A & CBulk event

A , B & CEvent in

low-field area

A & BNear surface

event

Keep the standard phonon detector Modify the E field near surfaces with interleaved

electrodes (6 ionization channels) Use B and D signals as vetos against surface

events From preliminary sea-level measurements

Surface event rejection > 95 % Fiducial volume ~ 50 %

Page 16: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 16

Results from Ge/Interdigit Results from Ge/Interdigit detectordetector

Few kg.d of background runs @ LSM with a 200g detector Performance as expected

(resolutions, threshold, …)

Currently 3 new 400g detectors Precise measurement of

rejection

A promising detector with a simple design

calibration

Neutron calibration

EDELWEISS-IIID-201

EDELWEISS-IIID-201

Page 17: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 17

Results from Ge/Interdigit Results from Ge/Interdigit detectordetector

Few kg.d of background runs @ LSM with a 200g detector Performance as expected

(resolutions, threshold, …)

Currently 3 new 400g detectors Precise measurement of

rejection

A promising detector with a simple designER threshold < 20 keV

No event below Q=0.5

EDELWEISS-IIID-201 (4 kg.d)

Page 18: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 18

Current run (May 2008 - …) Current run (May 2008 - …) Instrumented detectors:

23 “standard” Ge/NTD bolometers

5 “NbSi” bolometers 4 “Interdigit” bolometers

~ 10 kg of GeQuickTime™ et un

décompresseur TIFF (non compressé)sont requis pour visionner cette image.

Page 19: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 19

ConclusionConclusion “standard” Ge/NTD detectors

Improved background understanding : significant reduction of , and backgrounds

100 kg.d recorded and in analysis Ge/NbSi detectors

Surface rejection ok Resolution improvements needed

Ge/Interdigit detectors December 2008 : 9 additional detectors July 2009 : 120 kg.d fiducial exposure with

threshold < 20 keV Up to 35x320g Ge crystals available for

reconfiguration as Ge/Interdigit

Page 20: Status of EDELWEISS-II

SANGLARD V., « Dark Energy and Dark Matter », Lyon, 2008 July 10th 20

EDELWEISS prospectsEDELWEISS prospects 1st Goal :

4x10-8 pb in 2010 Acquire physics data

with 32 Ge/ID

2nd Goal : Few 10-9 pb in 2012 ~ 70 detectors Ge/ID

EURECA (see H. Kraus’s talk next session)