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Explore the high-pressure gaseous xenon TPC technology for 0-v ββ search in 136Xe with excellent energy resolution and topological discrimination. This technology offers great potential for various applications in homeland security, medical physics, and more. Learn about the benefits of electro-luminescence in achieving optimal gain with minimal noise and fluctuations. Discover the virtues of electro-luminescence in HPXe, its application in TPCs for total energy and track imaging, and ongoing research and development efforts in this field. Stay informed on the latest advancements and future prospects in xenon TPC technology.
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High-Pressure Gaseous Xenon TPCfor 0-v Search in 136Xe Azriel Goldschmidt, Tom Miller, David Nygren, Josh Renner, Derek Shuman, Helmuth Spieler, Jim Siegrist LBNL TIPP 2011
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 energyand image of the particle tracks for topological discrimination of event type (Gotthard TPC: x30 rejection) TIPP 2011
Context R&D is focused on the NEXTCollaboration, now preparing for a 100 kg 136Xe TPC detector for Canfranc Underground Laboratory, Spain. NEXT is funded by Spain at ~5M € for construction Spain-Portugal-Colombia-France-Russia-US collaboration Applications may include -ray imaging for Homeland security/non-proliferation, medical physics/imaging TIPP 2011
Xenon: Strong dependence of energy resolution on density! Large fluctuations between light/charge WIMPs: S2/S1 suffers! Ionization signal only Here, the fluctuations are normal For <0.55 g/cm3, ionization energy resolution is “intrinsic” TIPP 2011
Intrinsic energy resolution E/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 electrons N =(FN)1/2~63 electrons rms! TIPP 2011
Intrinsic energy resolution E/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 electrons N =(FN)1/2~124 electrons rms! TIPP 2011
Gain and noise Impose 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 TIPP 2011
Electro-Luminescence (EL) (aka: GasProportional 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) TIPP 2011
Gain and noise F constraint due to fixed energy deposit = 0.15 Let “G” represent noise/fluctuations in EL gain Uncorrelated 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 electron G 1.5/Npe Npe > 10 per electron for G ≤ F E/E = 0.9% FWHM 137Cs 662 keV TIPP 2011 9
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 TIPP 2011
TPC with Electroluminescence: Total Energy and Track Imaging Readout Plane A - position Readout Plane B - energy Electroluminescent Layer TIPP 2011
Pressure vessel design study at 15 bars for 100 kg NEXT ~120 cm TIPP 2011
Laboratorio Subterraneo de Canfranc Waiting for NEXT... TIPP 2011
LBNL-TAMU TPC Prototype TIPP 2011
Field cages/Light cagePTFE with copper stripes 19 PMTs and PMT bases Electroluminescence region10 kV across a 3 mm gap TIPP 2011
PMT Array: inside the pressure vesselQuartz window 2.54 cm diameter PMTs TIPP 2011
Inserting the TPC... carefully! TIPP 2011
A Diagonal Muon Track - “reconstructed” ~ 14 cm TIPP 2011
A typical 137Cs waveform (sum of 19 PMTs)~300,000 detected photoelectrons Primary Scintillation (S1) T0 of event Electroluminescence (S2) Structure indicates topology due to Compton scatters Drift Time:z-position (~0.01mm/sample) TIPP 2011 10ns/sample
Charge vs Drift Timeelectron lifetime of 900 ms ~5% charge loss forlongest drift of 60 ms (8 cm) TIPP 2011
HPXe @ 10 Atm, 137Cs 662 keVDrift time correction applied Counts keV TIPP 2011
HPXe @ 10 Atm, 137Cs 662 keV Drift Time and Position corrections applied 1.8% FWHM Counts 29-36 keV Xe x-rays escape keV TIPP 2011
Conclusions and Outlook • Successful operation of xenon EL TPC in 10-15 Bar range • We have achievedE/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! TIPP 2011