LIQUID XENON-FILLED WIRE CHAMBERS. Presented by S. E. Derenzo Lawrence Berkeley Laboratory University of California Berkeley, California

Similar documents
Final report on DOE project number DE-FG07-99ID High Pressure Xenon Gamma-Ray Spectrometers for Field Use

GEM: A new concept for electron amplification in gas detectors

Generic Detector. Layers of Detector Systems around Collision Point

X-ray ionization yields and energy spectra in liquid argon

Proportional Counters

Particle Energy Loss in Matter

DETECTORS. I. Charged Particle Detectors

General Overview of Gas Filled Detectors

Quality Assurance. Purity control. Polycrystalline Ingots

Particle Energy Loss in Matter

electrons out of, or ionize, material in their paths as they pass. Such radiation is known as

X-ray ionization yields and energy spectra in liquid argon

R&D on Astroparticles Detectors. (Activity on CSN )

Radiation Detection. 15 th Annual OSC Readiness Training Program.

hν' Φ e - Gamma spectroscopy - Prelab questions 1. What characteristics distinguish x-rays from gamma rays? Is either more intrinsically dangerous?

Radionuclide Imaging MII Detection of Nuclear Emission

Alpha-particle Stopping Powers in Air and Argon

3. Gas Detectors General introduction

Gamma and X-Ray Detection

Ionization of liquid krypton by electrons, gamma rays and alpha particles

BWXT Y-12 Y-12. A BWXT/Bechtel Enterprise SMALL, PORTABLE, LIGHTWEIGHT DT NEUTRON GENERATOR FOR USE WITH NMIS

Ionization Detectors. Mostly Gaseous Detectors

Chapter 3 Gas Filled Detectors

Measurement of the transverse diffusion coefficient of charge in liquid xenon

Development of New MicroStrip Gas Chambers for X-ray Applications

LAAPD Performance Measurements in Liquid Xenon

Ionization Detectors

Seminar talks. Overall description of CLAS12 (Jefferson Lab) MAPS. Talks on Feb. 6 th, (Contact JR) (Contact TS)

PANDA-X A New Detector for Dark Matter Search. Karl Giboni Shanghai Jiao Tong University

Nuclear Physics Laboratory. Gamma spectroscopy with scintillation detectors. M. Makek Faculty of Science Department of Physics

Nuclear Physics and Astrophysics

PHOTOELECTRON COLLECTION EFFICIENCY AT HIGH PRESSURE FOR A GAMMA DETECTOR ENVISAGING MEDICAL IMAGING

Design optimisation of X-ray detectors for SSM

PHYS 3446 Lecture #12

Two-phase argon and xenon avalanche detectors based on Gas Electron Multipliers

Gamma Spectroscopy. References: Objectives:

Radiation Detection and Measurement

Radioactivity. Lecture 6 Detectors and Instrumentation

Advances in the Micro-Hole & Strip Plate gaseous detector

EEE4106Z Radiation Interactions & Detection

THE GEIGER-MULLER TUBE AND THE STATISTICS OF RADIOACTIVITY

Chem 481 Lecture Material 3/20/09

Siberian Branch of Russian Academy of Science. A. Buzulutskov, A. Bondar, L. Shekhtman, R. Snopkov, Yu. Tikhonov

arxiv:physics/ v1 3 Aug 2006

Factors Affecting Detector Performance Goals and Alternative Photo-detectors

mean free path stopping power absorption coefficient detected recoil rate detected 0νββ events

Contents. Charged Particles. Coulomb Interactions Elastic Scattering. Coulomb Interactions - Inelastic Scattering. Bremsstrahlung

Rn assay and distillation purification

Synchrotron Radiation a Tool for Precise Beam Energy Measurements at the ILC

Performance of a triple-gem detector for high-rate particle triggering

Performance of high pressure Xe/TMA in GEMs for neutron and X-ray detection

arxiv:physics/ v2 27 Mar 2001

Looking at Cosmic Muons to verify Einstein's Special Relativity

Dual Isotope Imaging with LaBr3:Ce Crystal and H8500 PSPMT

08 - Miscellaneous and historical detectors

GEM-based photon detector for RICH applications

Experimental Particle Physics

Experimental Particle Physics

Introduction. Principle of Operation

PoS(TIPP2014)033. Upgrade of MEG Liquid Xenon Calorimeter. Ryu SAWADA. ICEPP, the University of Tokyo

Neutron Induced Nuclear Counter Effect in Hamamatsu Silicon APDs and PIN Diodes

arxiv:physics/ v1 [physics.ins-det] 14 Feb 2005

He-3 Neutron Detectors

Momentum Measurement in B Field. Part II. Relative Momentum Error. Contribution from Multiple Scattering

Part II. Momentum Measurement in B Field. Contribution from Multiple Scattering. Relative Momentum Error

Energy loss of alpha particles - Prelab questions

Low Energy Particles in Noble Liquids

GEM at CERN. Leszek Ropelewski CERN PH-DT2 DT2-ST & TOTEM

A gas-filled calorimeter for high intensity beam environments

Nuclear Lifetimes. = (Eq. 1) (Eq. 2)

Modern Status of High Pressure Xenon Gamma-ray Spectrometers and their Applications.

Experimental Particle Physics

Particle Detectors. Summer Student Lectures 2007 Werner Riegler, CERN, History of Instrumentation History of Particle Physics

Applied Nuclear Physics (Fall 2006) Lecture 21 (11/29/06) Detection of Nuclear Radiation: Pulse Height Spectra

Nuclear Physics Lab I: Geiger-Müller Counter and Nuclear Counting Statistics

Detecting low energy recoils with Micromegas

Dark Matter Detection and the XENON Experiment. 1 Abstract. 2 Introduction

Gamma-Ray Polarimetry in the Pair Production Regime

GEM-based gaseous Photomultipliers for UV and visible photon imaging. Dirk Mörmann Amos Breskin Rachel Chechik Marcin Balcerzyk Bhartendu Singh

arxiv:astro-ph/ v1 26 Sep 2003

High pressure xenon gas detector with segmented electroluminescence readout for 0nbb search

3 Gaseous Detectors. Detectors for Particle Physics Manfred Krammer Institute for High Energy Physics, Vienna, Austria

Detection of X-Rays. Solid state detectors Proportional counters Microcalorimeters Detector characteristics

Chapter Seven (Nuclear Detectors)

Distillation purification and radon assay of liquid xenon

Lecture 4. Detectors for Ionizing Particles

EE6701 HIGH VOLTAGE ENGINEERING UNIT II-DIELECTRIC BREAKDOWN PART A

Position Sensitive Germanium Detectors for the Advanced Compton Telescope

GLOSSARY OF BASIC RADIATION PROTECTION TERMINOLOGY

Two-phase and gaseous cryogenic avalanche detectors based on GEMs

ORTEC AN34 Experiment 10 Compton Scattering

Scintillation Detector

Introduction to Radiation Monitoring

2. A proton is traveling with velocity v, to the right, through a magnetic field pointing into the page as indicated in the figure below.

Signals in Particle Detectors (1/2?)

RITU and the GREAT Spectrometer

Breakdown limit studies in high-rate gaseous detectors

Waste Characterization

Introduction to Accelerator Physics Part 1

PHY492: Nuclear & Particle Physics. Lecture 25. Particle Detectors

Transcription:

LIQUID XENON-FILLED WIRE CHAMBERS Presented by S. E. Derenzo Lawrence Berkeley Laboratory University of California Berkeley, California Abstract We describe several types of small liquid xenon-filled chambers, each optimized for a particular property such as a real time spatial resolution of ±15 ~, resolution of ±10-7 sec, or a pulse height of 10-12 coulomb. a time Larger chambers combining all these properties will be of great value at NAL energies, and we describe some of the techniques necessary for their construction. Introduction In 1968, Luis Alvarez suggested that a filmless particle detector with!10 ~ space resolution could be developed by using a liquified noble gas as the detection medium. 1 He reasoned that a thousand-fold increase in density (when compared with gas-filled wire chambers) would simultaneously permit a decrease in detector thickness and an increase in ion statistics. Other resolution-limiting factors such as electron diffusion and a-rays would also be significantly reduced. Operation at one atmosphere pressure would allow the technique to be used over large areas and readout would be simplified if the initial ionization could be amplified in the liquid. Single Wire Chambers We have been operating liquid xenon-filled single-wire proportional chambers for two years.]') Figure 1 shows our single-wire chamber design, and Fig. 2 shows the pulse height of the 279-keV photopeak as a function of operating voltage for 2.9-, 3.5-, and 5.0-~ anode wires. ~he chamber counts well and the pulse-height curves are reproducible to ±lo% every time the chamber is filled. As mentioned in Ref. 2, the single-wire chamber produces two classes of avalanche pulses. The first type are proportional in size to the initial ionization and rise in ~2 x 10-7 sec (see Fig. 3(a)]. The second ~Geiger~ type are larger (~2 x 10-12 C), uniform in size, and rise more rapidly [see Fig. 3(b)]. The rise time shown in Fig. 3(b) is limited by the rise time of our charge amplifier. When the ~Geiger~ pulses are observed directly on an oscilloscope. the true rise time of ~lo-8 sec may be seen (see Fig. 4). Using the two collinear gamma rays from a 22Na source, we measured the time resolution of a single-wire liquid xenon chamber to be ~lo-7 sec. During this test electronegative impurities restricted the effective diameter of the chamber to approximately 1 mm. For details see Ref. 5. For decades the gas filling in wire chambers has included quenching agents to suppress sparking and to increase the size of the pulses. We have found that 2000 ppm ethylene (C 2 H 4 ) in liquid xenon also permits higher operating voltage and larger pulses. This comparison is shown in Fig. 5. Work supported by the United States Atomic Energy Commission. -388

Multi-Wire proportional Chambers We have designed and built a liquid xenon multi-wire proportional chamber specifically for detecting gamma rays in nuclear medicine. (For gamma rays in the 0.15 to 10-MeV range this approach provides an unprecedented combination of detection efficiency, spatial resolution, and potential for up-scaling.) 4 This chamber is shown in Fig. 6 and consists of 24 3.5-~ wires spot-welded to kovar pins sealed with glass to holes in the ceramic base. The wires are spaced 2.8 mm apart, and the wire plane is centered between two cathode planes spaced 15 mm apart. gross detection efficiency for 280-keV gamma rays is 65%. The At an operating potential of -4500 V the liquid gain is 10, and under these conditions the spatial resolution was measured to be 3 rom FWHM, demonstrating that the wires amplify independently without the addition of a quenching agent. For the development of a chamber possessing high spatial resolution for charged particles, however, it is very important to demonstrate amplification by arrays of much more closely spaced wires. To this end we ran three arrays of five wires 3.5 ~ in diameter with spacings of 150, 300, and 1000 ~ between opposing cathodes spaced 5 mm apart in a small test chamber. With a looo-~ spacing, gain sets in at 3800 V, reaching 10 at 5000 V. A further increase in voltage at the 1000-~ spacing and observation of gain at the 150- and 300-~ of sparks between the flat cathode and the wires of the anode. spacings was prevented by the occurrence Very recently we have learned that these sparks are initiated by field emission from the cathode. We will continue studies with closely spaced anodes (50 to 300 ~ apart) using specially polished cathodes and the addition of ethylene to suppress sparking and provide larger gain. In previous papers we have reported on schemes for producing closely spaced narrow conducting strips on an insulating substrate. Heidenhain Corporation can produce sub-micron chrome lines on glass or Mylar. 6 In addition, we have made Nory17 pressings with sharp ridges 50 ~ apart and then vacuum deposited metal at a grazing angle to produce conductive strips several ~ wide at the top of the ridges (see Fig. 7). Recently we have devised a method of attaching fine wire to a substrate in such a way that 98% of the wire does not touch the substrate. A Noryl pressing is made, producing sharp ridges 100 ~ wide, 100 ~ high, and 1 rom apart. Then 5-~ wire is wound around the ridges at right angles. The assembly is placed in a magnetic field while a current is passed through the wire. This serves to heat the wire and press it into the edge of the ridge. The result is shown in Fig. B. Multi-Wire Ionization Chambers Electron avalanche in the liquid is essential in reducing the complexity and cost of the readout. It is quite possible, however, using present technology, to build a liquid xenon multi-wire ionization chamber having no liquid gain with a space resolution of ±lo ~ and a time resolution of ±20 nsec. Unfortunately the readout requires that a low-noise charge-sensitive amplifier be attached to each wire, increasing the cost by approximately $20 per wire, and severely limiting its applications in physics experiments. Figure 9 shows the excellent spatial resolu 2 tion that we have measured for the ionization mode.,b -389

Gamma-Ray Detection The density and atomic number of liquid xenon make it attractive for the absorption and detection of gamma rays. In order to study the energy resolution obtainable, we built an ionization chamber with a Frisch grid. experimental setup are shown in Fig. 10. rays obtained thus far is 10.5% FWHM The chamber and The best resolution for 279-keV gamma (shown in" Fig. 11), comparable to NaI(Tl). The amount of liquid xenon required for the absorption of a multi-gev electromagnetic shower is quite expensive ($3/cc) but there is hope for the future. For every megawatt-year generated by nuclear power reactors, 57 grams of Xe are produced. only important contamination is 10.76-yr 8SKr, which can be reduced to levels of 10 pci per STP liter Xe by distillation followed by a series of dilutions (with atmospheric Kr) and redistillations. C. A. Rohrmann 9 estimates that by 1980 the annual recovery of xenon will exceed 10 tons per year at a cost of 2S per liquid cc. Summary We have developed several versions of liquid xenon-filled chambers, each optimized for a particular property such as unexcelled real time spatial resolution (±ls ~), good energy resolution (±5% for 279-keV gamma rays), good pulse height 12 (10- coulomb for minimum ionizing particles passing through 0.7 rom liquid Xe), or 7 good time resolution (±10- sec for a I-mm-thick chamber). We are working on the technology to allow us to combine several such properties in chambers covering useful areas. Acknowledgments We are indebted to Joe Savignano, Tony Vuletich, and Buck Buckingham for essential contributions to all phases of this work. This work was supported in part by the U.S. Atomic Energy Commission and in part by NASA. Boiling point Appendix - Selected Properties of Liquid Xenon -l08.l00c (1 atm) Freezing point -111. BOC (1 atm) Density STP gas/boiling-liquid volume ratio 3.057 g/cc SlB.9 (1 atm) 1 x 105 em/sec at 60 V/cm e- dri~t veloeitylo 2 x los em/sec at 500 V/cm [ 3 x 10 5 em/sec from 3 to 60 kv/cm The Ion pairs per 100 ~ Energy loss per 100 ~ Radiation length Collision length Present cost 2000 (minimum ionization) 43 kev (minimum ionization) 25 mrn 450 mm $3/cc References ll. W. Alvarez, Lawrence Radiation Laboratory, Group A Physics Note No. 672, 196B, unpublished. -390

2R. A. Muller, S. E. Derenzo, G. smadja, D. B. Smith, R. G. Smits, H. Zaklad, and L. W. Alvarez, Phys. Rev. Letters 27, 532 (1971). 3Recently workers at Oubna have reported on some excellent new work using a singlewire proportional chamber filled with high-pressure gases and solidified noble gases: A. F. Pisarev, v. G. Pisarev, and G. S. Revenko, Dubna Reports JINR Pl3-6450 and JINR - Pl3-6449 (1972). 4H Zak1ad, S. E. Derenzo, R. A. Muller, G. Smadja, R. G. Smits, and L. W. Trans. IEEE NS-19, 206 (1972). 5s. E. Derenz~ B. Smith, R. G. Smits, H. Zaklad, L. W. Alvarez, and R. A. MUller, Lawrence Radiation Laboratory Report UCRL-20118 and NAL Summer Study Report 55-181 (1970). 6Heidenhain Corporation, 8225 Traunreut, West Germany. Alvarez, 7Naryl is a class of thermoplastic resins manufactured by General Electric, Noryl Avenue, Selkirk, New York 12158. BThe collimated alpha source used in Ref. 2 is described in Lawrence Radiation Laboratory Report UCRL-20BS7 (1971). 9c. A. Rohrmann, Isotopes and Radiation Technology!, 3, 253 (1971). lol. Miller, S. Howe, and W. Spear, Phys. Rev. ~, 871 (1968). -391

To vacuum and gas supply t (a) BNC (signal out) Guard ring Glass insulation Cathode High voltage feed - through Fine wire anode Guard ring ~ 1 11 ---1 Fig. 1. Liquid xenon single-wire proportional chamber. Glass feedthrough -392

1000... anode dio..2.9p. 400f- 3.5p.../.. S.Op.......... 279 KeV Photop.ak 100...a " E 0.. :i 0 40.. (,)!! I 0........ N (h 41-...... : ~.. :::I Q. 10 l-.. ~...'.. ri',... ~-.4 - I I 0 I 2 3 4 Volta ge (KV) Fig. 2. Pulse height VB voltage in liquid xenon single-wire proportional chamber with 8-mm-diam cathode and 2.9-, 3.5-, and 5.0-~-diam anodes. Signal is 279-keV photopeak from 203 Hg source. -393

Charge Tektronlcs 545 amplifier scope I 0.02volts /,r ~ /.!.I - 1' A ~IOOnsec m 0.5/ / ~ 1~1/ 'I LJ - --Ie)OnfeC!I m B Fig. 3. Pulses from chamber of Fig. 1 seen on a charge amplifier with a gain of 0.4 V/pC. Az proportional pulse. B: "Geiger" pulse. -394~

Tecktronlcs 545 scope Chamber I~r I v~lts "",... I t-"""" 1- I-U ~Or sec A O.OO~ volts ~ ~ f - 1-1 - B I-IOOnsec Fig. 4. "Geiger"-type pulses from chamber of Fig. I seen directly on an oscilloscope. A: I-megohm load. B: 12S-ohm load. -395

No quencher added 4000... 2000 ppm C.H.. added Liquid Xe 279 KeV Photopeak... 1000 5.0~ anode 8mm cathode 400 ~ E ~ 100 :::J 0 0.. 40 '0 at 10.~ (J) at 4 U) :::J Q.. o 2 3 4 5 6 Voltaoe (KV) Fig. 5. Pulse height VB voltage in single-wire chamber for 5-~ anode in pure liquid xenon and in liquid xenon containing- 2000 ppm C H 4, 2-396

Fig. 6. Gamma-ray chamber 15 rom thick, containing 24 3.5-p-diam wires and 24 cathode strips. A: shows ceramic chamber wall and support for anode wires and cathode strips. -397

Fig. 6. Gamma-ray chamber 15 mm thick, containing 24 3.5-~-diam wires and 24 cathode strips. B: shows assembled chamber. -398

Fig. 7. Array of conducting strips produced by vacuum depositing metal at a grazing angle onto a series of Noryl ridges 40 ~ wide and 100 ~ apart. Fig. B. Array of 5-~ wires banded to Noryl ridges 1 mm apart. Current is passed through the wire in a magnetic field to heat the wire and press it into the ridges. -399

600 Chamber gop =0.7 mm 400 5300 0 u 200 100 0-75 -50-25 0 25 50 75 Source position (microns) Fig. 9. Image of a 38-~ wide collimated alpha sou~ce detected by a O.7-mm-thick liquid xenon ionization chamber. (See Refs. 2 and 6 for details.) 500 Wire spacing =50IJlT rms = 15IJ UI +0-400

SIQnal out Frisch Grid Cathode Hv Grid Hv- Fig. 10. Liquid ~enon ionization chamber with Frisch grid and collimated gamma source. -40t

.. '" c "I. -. ::s. o U 279 kev \"~ r---t---+---t-...irl-------f--f-------"-j-------f-- I. r----t---+---t-----tl':~_t--r-~_t--.~r_._--~.-----.. I :. 100 200 Pulse height (channels), Fig. 11. Pulse-height spectrum for 279-keV gamma rays seen in setup of Fig. 10. FWHM is 10.5%, comparable to NaI(Tl}. -402