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High-Pressure Gaseous Xenon TPC for 0- v Search in 136 Xe

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High-Pressure Gaseous Xenon TPC for 0- v  Search in 136 Xe. Azriel Goldschmidt, Tom Miller, David Nygren, Josh Renner, Derek Shuman, Helmuth Spieler, Jim Siegrist LBNL. Motivations. Xenon gas at high pressure offers excellent energy resolution - in principle - PowerPoint PPT Presentation
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TIPP 2011 1 High-Pressure Gaseous Xenon TPC for 0-v Search in 136 Xe Azriel Goldschmidt, Tom Miller, David Nygren, Josh Renner, Derek Shuman, Helmuth Spieler, Jim Siegrist LBNL
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Page 1: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 1

High-Pressure Gaseous Xenon TPCfor 0-v Search in 136Xe

Azriel Goldschmidt, Tom Miller, David Nygren, Josh Renner, Derek Shuman,

Helmuth Spieler, Jim SiegristLBNL

Page 2: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 2

Motivations• Xenon gas at high pressure offers excellent energy resolution - in principle

(within a factor 3 of best Ge diodes! )

• Electroluminescence provides linear gain with extremely low fluctuations - helps to preserve this high intrinsic energy resolution.

• HP Xe TPC can provide total energy and image of the particle tracks for topological discrimination of event type (Gotthard TPC: x30 rejection)

Page 3: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 3

Context

• R&D is focused on the NEXT Collaboration, now preparing for a 100 kg 136Xe TPC detector for Canfranc Underground Laboratory, Spain.

NEXT is funded by Spain at ~5M € for constructionSpain-Portugal-Colombia-France-Russia-US collaboration

• Applications may include -ray imaging for Homeland security/non-proliferation, medical physics/imaging

Page 4: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 4

Xenon: Strong dependence of energy resolution on density!

For <0.55 g/cm3, ionization energy resolution is “intrinsic”

Ionization signal onlyHere, the

fluctuations are normal

Large fluctuations

between light/charge

WIMPs: S2/S1

suffers!

Page 5: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 5

Intrinsic energy resolutionE/E = 2.35 (FW/Q)1/2

– F Fano factor: F = 0.15 (HPXe) (LXe: F ~20)– W Average energy per ion pair: W ~ 25 eV– Q Energy deposited, e.g. 662 keV from Cs137 -rays:

E/E = 0.56% FWHM (HPXe)

N = Q/W ~26,500 primary electronsN = (FN)1/2 ~63 electrons rms!

Page 6: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 6

Intrinsic energy resolutionE/E = 2.35 (FW/Q)1/2

– F Fano factor: F = 0.15 (HPXe) (LXe: F ~20)– W Average energy per ion pair: W ~ 25 eV– Q Energy deposited, e.g. 2457 keV from 136Xe --> 136Ba:

E/E = 0.28% FWHM (HPXe)

N = Q/W ~100,000 primary electronsN = (FN)1/2 ~124 electrons rms!

Page 7: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 7

Gain and noiseImpose a requirement:

(noise + fluctuations) N(noise + fluctuations) 124 e—

Simple charge detection can’t meet this goal

Need gain with very low noise/fluctuations!

Electroluminescence (EL) is the key

Page 8: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 8

Electro-Luminescence (EL) (aka: Gas Proportional Scintillation)

• Physics process generates ionization signal• Electrons drift in low electric field region• Electrons enter a high electric field region• Electrons gain energy, excite xenon: 8.32 eV• Xenon radiates VUV (175 nm, 7.5 eV)• Electron starts over, gaining energy again• Linear growth of signal with voltage• Photon generation up to ~1000/e, but no ionization• Sequential gain; no exponential growth fluctuations are very

small• NUV = JCP N1/2

• Optimal EL conditions: JCP = 0.01 (Poisson: JCP = 1)

Page 9: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 9

Gain and noiseF constraint due to fixed energy deposit =

0.15Let “G” represent noise/fluctuations in EL

gainUncorrelated fluctuations can add in

quadrature: n = ((F + G)N)1/2

EL: G = JCP/NUV + (1 + 2PMT)2/Npe

Npe = number of photo-electrons per electronG 1.5/Npe

Npe > 10 per electron for G ≤ FE/E = 0.9% FWHM 137Cs 662 keV

Page 10: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 10

Virtues of Electro-Luminescence in HPXe

• Linearity of gain versus pressure, HV• Immunity to microphonics• Tolerant of losses due to impurities• Absence of positive ion space charge• Absence of ageing, quenching of signal• Isotropic signal dispersion in space• Trigger, energy, and tracking functions are

accomplished with optical detectors

Page 11: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 11

TPC with Electroluminescence: Total Energy and Track Imaging

Readout Plane A

- position

Readout Plane B- energy

Electroluminescent Layer

Page 12: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 12

Pressure vessel design study at 15 bars for 100 kg NEXT

~120

cm

Page 13: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 13

Laboratorio Subterraneo de Canfranc

Waiting for NEXT...

Page 14: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 14

LBNL-TAMU TPC Prototype

Page 15: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 15

Field cages/Light cagePTFE with copper stripes

Electroluminescence region10 kV across a 3 mm gap

19 PMTs and PMT bases

Page 16: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 16

PMT Array: inside the pressure vesselQuartz window 2.54 cm diameter PMTs

Page 17: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 17

Inserting the TPC...

carefully!

Page 18: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 18

Page 19: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 19

A Diagonal Muon Track - “reconstructed”

~ 14 cm

Page 20: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 20

A typical 137Cs waveform (sum of 19 PMTs)~300,000 detected photoelectrons

10ns/sample

Primary Scintillation (S1)T0 of event

Electroluminescence (S2)Structure indicates topology due to Compton scatters

Drift Time:z-position (~0.01mm/sample)

Page 21: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 21

Charge vs Drift Timeelectron lifetime of 900 ms

~5% charge loss forlongest drift of 60 ms (8 cm)

Page 22: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 22

HPXe @ 10 Atm, 137Cs 662 keVDrift time correction applied

keV

Coun

ts

Page 23: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 23

HPXe @ 10 Atm, 137Cs 662 keV

1.8% FWHM

29-36 keV Xe x-rays escape

keV

Coun

ts

Drift Time and Position corrections applied

Page 24: High-Pressure Gaseous Xenon TPC for 0- v   Search in  136 Xe

TIPP 2011 24

Conclusions and Outlook• Successful operation of xenon EL TPC in 10-15 Bar range• We have achieved E/E = 1.8% FWHM @ 662 keV (10 Atm)

– If F = G, and if no other effects, we expect: E/E = 0.9% FWHM• We do not yet claim to understand this factor of 2, but...• We do expect that this gap will be substantially reduced

– Likely contributing factors:• localization - dependence of signal on radius • calibration of gain and QE of each PMT• dissociative attachment of electrons in EL region to water/oxygen• mesh flatness• PMT after-pulsing

• NEXT is starting to happen! 100 kg 136Xe awaits us!


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