The GEM scintillation in He-CF 4, Ar-CF 4, Ar-TEA and Xe-TEA mixtures

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

CCD readout of GEM-based neutron detectors

Because light behaves like a wave, we can describe it in one of two ways by its wavelength or by its frequency.

Chapter 4 Scintillation Detectors

Reference literature. (See: CHEM 2470 notes, Module 8 Textbook 6th ed., Chapters )

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

Abstract... I. Acknowledgements... III. Table of Content... V. List of Tables... VIII. List of Figures... IX

Particle Energy Loss in Matter

Analytical Spectroscopy Review

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

Precise Measurement of the Absolute Yield of Fluorescence Photons in Atmospheric Gases

Neutron Detection. n interactions with matter n detection High/low energy n detectors

PERFORMANCE OF A ROOM TEMPERATURE GAS PROPORTIONAL SCINTILLATION COUNTER IN X-RAY ANALYSIS OF METALLIC ALLOYS EXCITED WITH ALPHA PARTICLES

Detecting high energy photons. Interactions of photons with matter Properties of detectors (with examples)

3 - Atomic Absorption Spectroscopy

Proportional Counters

Lecture 16 Light transmission and optical detectors

Light and Atoms. ASTR 1120 General Astronomy: Stars & Galaxies. ASTR 1120 General Astronomy: Stars & Galaxies !ATH REVIEW: #AST CLASS: "OMEWORK #1

Supplementary Materials

Visualization of Xe and Sn Atoms Generated from Laser-Produced Plasma for EUV Light Source

LAAPD Performance Measurements in Liquid Xenon

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

III. Energy Deposition in the Detector and Spectrum Formation

Particle Energy Loss in Matter

Plasma Radiation. Ø Free electrons Blackbody emission Bremsstrahlung

EE 5344 Introduction to MEMS CHAPTER 5 Radiation Sensors

Chem 155 Midterm Exam Page 1 of 10 Spring 2010 Terrill

Atomization. In Flame Emission

Taking fingerprints of stars, galaxies, and interstellar gas clouds

Chemistry 311: Instrumentation Analysis Topic 2: Atomic Spectroscopy. Chemistry 311: Instrumentation Analysis Topic 2: Atomic Spectroscopy

SIGN: A Pressurized Noble Gas Approach to WIMP Detection

Analysis of γ spectrum

Taking fingerprints of stars, galaxies, and interstellar gas clouds. Absorption and emission from atoms, ions, and molecules

ASTR-1010: Astronomy I Course Notes Section IV

Dedicated Arrays: MEDEA GDR studies (E γ = MeV) Highly excited CN E*~ MeV, 4 T 8 MeV

Quality Assurance. Purity control. Polycrystalline Ingots

Taking Fingerprints of Stars, Galaxies, and Other Stuff. The Bohr Atom. The Bohr Atom Model of Hydrogen atom. Bohr Atom. Bohr Atom

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

Oddities of light production in the noble elements. James Nikkel

Complete the following. Clearly mark your answers. YOU MUST SHOW YOUR WORK TO RECEIVE CREDIT.

Two-phase and gaseous cryogenic avalanche detectors based on GEMs

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

Factors Affecting Detector Performance Goals and Alternative Photo-detectors

IR Spectrography - Absorption. Raman Spectrography - Scattering. n 0 n M - Raman n 0 - Rayleigh

25 Instruments for Optical Spectrometry

Instrumental Analysis: Spectrophotometric Methods

Chemistry Instrumental Analysis Lecture 19 Chapter 12. Chem 4631

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

Prof. Jeff Kenney Class 5 June 1, 2018

An Investigation of Benzene Using Ultrafast Laser Spectroscopy. Ryan Barnett. The Ohio State University

high energy state for the electron in the atom low energy state for the electron in the atom

Richard Miles and Arthur Dogariu. Mechanical and Aerospace Engineering Princeton University, Princeton, NJ 08540, USA

Measurements of liquid xenon s response to low-energy particle interactions

SCINTILLATION DETECTORS AND PM TUBES

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

Spectrophotometry. Dr. Shareef SHAIK ASST. PROFESSOR Pharmacology

Review: Properties of a wave

GEM: A new concept for electron amplification in gas detectors

Chapter V: Interactions of neutrons with matter

Introduction to the Diagnosis of Magnetically Confined Thermonuclear Plasma

Course Details. Analytical Techniques Based on Optical Spectroscopy. Course Details. Textbook. SCCH 211: Analytical Chemistry I

HIGH-PRESSURE HELIUM-3 SCINTILLATION POSITION-SENSITIVE DETECTOR OF THERMAL NEUTRONS

5.111 Lecture Summary #5 Friday, September 12, 2014

What is LIGHT? Reading Question

The TDCR method in LSC. P. Cassette Laboratoire National Henri Becquerel CEA/LNE, France

Laser Dissociation of Protonated PAHs

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

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

The Photon-Assisted Cascaded Electron Multiplier: a Concept for Potential Avalanche-Ion Blocking

SOLSPEC MEASUREMENT OF THE SOLAR ABSOLUTE SPECTRAL IRRADIANCE FROM 165 to 2900 nm ON BOARD THE INTERNATIONAL SPACE STATION

NEXT ELECTROLUMINESCENCE READOUT

ATOMS. Central field model (4 quantum numbers + Pauli exclusion) n = 1, 2, 3,... 0 l n 1 (0, 1, 2, 3 s, p, d, f) m l l, m s = ±1/2

05 - Scintillation detectors

EEE4106Z Radiation Interactions & Detection

Inelastic soft x-ray scattering, fluorescence and elastic radiation

CHM 424 EXAM 4 CRIB - COVER PAGE FALL

Key words: avalanche photodiode, soft X-ray detector, scintillation γ-ray detector, imaging device PACS: 07.85;95.55.A;85.60.D

1. What is the minimum energy required to excite a mercury atom initially in the ground state? ev ev ev

Radiation Detection for the Beta- Delayed Alpha and Gamma Decay of 20 Na. Ellen Simmons

Interaction of Ionizing Radiation with Matter

CHEM 1311A. E. Kent Barefield. Course web page.

Lecture 0. NC State University

2001 Spectrometers. Instrument Machinery. Movies from this presentation can be access at

ISPA-Tubes with YAP:Ce Active Windows for X and Gamma Ray Imaging.

Week 6: Ch. 8 Scintillation Counters

Photon Detector Performance and Radiator Scintillation in the HADES RICH

Analytical Technologies in Biotechnology Prof. Dr. Ashwani K Sharma Department of Biotechnology Indian Institute of Technology, Roorkee

GLOSSARY OF BASIC RADIATION PROTECTION TERMINOLOGY

The Dual-Phase Liquid Xenon Time Projection Chamber (TPC) of Münster

Detecting low energy recoils with Micromegas

Ionization Detectors

Review of Optical Properties of Materials

CHARGED PARTICLE INTERACTIONS

Scintillation Detectors

two slits and 5 slits

Scintillators General Characteristics

Study of infrared scintillations in gaseous and liquid argon Part I: methodology and time measurements

CCD OPERATION. The BBD was an analog delay line, made up of capacitors such that an analog signal was moving along one step at each clock cycle.

Properties of Light and Atomic Structure. Chapter 7. So Where are the Electrons? Electronic Structure of Atoms. The Wave Nature of Light!

A Triple-GEM Telescope for the TOTEM Experiment

Transcription:

The GEM scintillation in He-CF 4, Ar-CF 4, Ar-TEA and Xe-TEA mixtures M. M. Fraga, F. A. F. Fraga, S. T. G. Fetal, L. M. S. Margato, R. Ferreira Marques and A. J. P. L. Policarpo LIP- Coimbra, Dep. Física, Univ. Coimbra, 3004-516 Coimbra, Portugal

Motivation Experimental set-up Summary Emission spectra of Ar/CF 4 and He/CF 4. Excitation and de-excitation processes in CF 4 and CF 4 mixtures Emission spectra of Ar/TEA Total light yields Conclusions

The GEM - gas electron multiplier See http://gdd.web.cern.ch/gdd/ Magnitude of the electric field along the center of the GEM channel.

Applications (with CCD readout of the GEM scintillation) Alpha particle tracking: Triple GEM with Ar+40%CF 4 241 Am α particles E = 5.48 Mev Range in Ar = 3.42 cm (F. Fraga et al., IEEE Trans. Nuc. Sci. 49 (2002) 281) Thermal neutron detection: Proton and triton tracks in 3 He- 400 mbar CF 4 Triple GEM AmBe source with Polyethylene shielding (F. Fraga et al., NIM A 478 (2002) 357)

Applications X-ray imaging Car key ~5 cm radiography X-ray energy ~8keV Xe-10%CO 2 at 1bar absorption length ~3 mm

Objectives: measure the emission spectra of Ar- and He-CF 4 mixtures and identify the main emitting channels. quantify the total light yields; study other gas mixtures leading to a stable operation of the GEM detector and exhibiting large photon yields either in the visible and near infrared (NIR) or in the UV region.

Experimental set-up GEM Detection system Glass window X rays from: Fe-55 source (5.9 kev); X-ray generator Quartz window Front electrode -Vdrift Back electrode I (a.u.) 12 10 8 6 4 2 0 2 4 6 8 10 E (kev)

Detection systems Total light yields: 4 Planar-diffused silicon photodiode (UDT PIN-25DP) N ph / e I = ph Ω I.Q. e.t. 4π σ < 15% Q.E. 0.9 0.8 0.7 0.6 0.5 0.4 0.3 Photodiode 0.2 56 TUVP 0.1 0 200 300 400 500 600 700 800 900 λ (nm) 8 Photomultiplier (56 TUVP) (operating in the pulse mode) σ < 30% N ph / e = fcq Ω M..T.N 4π e

Emission spectra: 8 Monochromator (Applied Photophysics m. 7300, with a 1200 g/mm grating blazed at 500 nm) + photomultiplier (RCA C31034), cooled to -20ºC, operating in single photon counting mode. 8 Spectral sensitivity of the detection system is measured with:! Standard tungsten strip lamp (Osram WI 17/G) (λ >310 nm), previously calibrated against a black body (in Institute of Physics, Belgrade)! Deuterium lamp (200-370 nm);

Spectroradiometric calibration with the tungsten strip lamp s s Ω E M Osram WI 17/G NDF L 1 IF Calibration factor: S 1 I o R V N ( ) Q( ) 0 λ λ = S( λ)

Nº of photons entering the monochromator per second: S( λ ) = ε(t, λ). N c (T, λ). A. Ω E. λ. f ( λ) Ω E A ε( T, λ) N c (T,λ). λ» is the effective solid angle;» effective emitting area of the tungsten ribbon;» emissivity of tungsten;» nº of photons emitted per unit time, per unit area and per steroradian, by a blackbody at a temperature T, in the wavelength range between λ and λ+ λ

Charge Gains 1000 1000 Ar+3%TEA Ar+5%TEA Ar+5%CF4 Ar+10%CF4 100 100 Gain 10 1 Gain 10 1 Xe+4%TEA Xe+3%TEA He+40%Xe+3%TEA He+40%CF4 He+20%CF4 150 200 250 300 350 400 100 150 200 250 300 350 400 450 500 V GEM (V) V GEM (V) He Ar CF 4 Xe TEA I. P. (ev) 24,58 15,7 15,9 12,12 7,51 E exc (ev) 19,82 11,54 12,5 8,4 4,77

Emission spectrum of Ar+5%CF 4 mixture G = 40; λ = 4 nm (raw data) 1200 1000 800 CF 3 * (1E,2A 2 1A 1 ) Ar I 2p 3s lines I norm (a.u.) 600 400 OH - 200 0 200 300 400 500 600 700 800 900 λ (nm )

I norm (a.u.) 3 2 1 0 3 2 1 0 3 2 1 0 Ar + 5% CF 4 G=40 500 550 600 650 700 750 800 850 Ar + 10% CF 4 G=90 500 550 600 650 700 750 800 850 Ar + 67% CF 4 G=40 500 550 600 650 700 750 800 850 λ (nm) Visible and NIR emission spectra of Ar- CF 4 mixtures, normalized to the light intensity at 620 nm. Nph/e- 0,7 0,6 0,5 0,4 0,3 0,2 0,1 1 10 Gain 5% CF 4 10% CF 4 67% CF 4 Nº of photons emitted, between 400 and 1000 nm, per secondary electron, as a function of the effective gain, in Ar-CF 4 mixtures. (Measurements performed with the photodiode).

Emission spectra of He-CF 4 mixtures CF 4 +*, CF 3 +* I norm (nm) 500 400 300 200 He + 20% CF 4 He + 40% CF 4 Raw data I norm (a.u.) 800 600 400 CF 3 * 100 200 0 200 300 400 500 600 700 800 λ (nm) He+20% CF 4 : G = 335 He+40% CF 4 : G = 175 λ = 4 nm 0 200 300 400 500 600 700 800 900 λ (nm) Emission spectrum of He+40%CF 4, corrected for 2 nd order diffraction effects and the quantum efficiency of the detection system.

He-CF 4 mixtures 1200 600 I n (a.u.) 1000 800 600 400 200 0 0 20 40 60 80 100 % CF 4 He/CF Ar/CF 4 Ar/CF He/CF 44 Light intensity, normalized to the current, measured for λ = 620 nm, as a function of CF 4 concentration. Light intensity/electron current (a.u.) 500 400 300 200 100 20%CF4 40%CF4 85%CF4 0 400 500 600 700 800 wavelength (nm) Visible emission spectra of He-CF 4 mixtures, measured with a glass color glass filter (λ cutt-off =435 nm).

CF 4 Process Threshold (ev) Direct vibrational excitation ν 4 0.078 ν 3 0.159 Energy loss (ev) 0.078 0.159 Indirect vibrational excitation 4.0 0.4 Electron attachment 4.3 4.3 Electronic excitation (dissociation into neutral fragments) 12.5 (10) 12.5 (10) Dissociative ionization 15.9 15.9 All electronic excited states of CF 4 and CF 4 + (τ < 10 µs) seem to dissociate or predissociate.

Dissociation into neutral fragments in CF 4 e - + CF 4 CF 3 + F + e - Energy threshold: 10-12.5 ev (?) Dissociation energy: D(CF 3 F) = 5.25 ev Electronic excited states of CF 3* : 1E (7.95 ev), 2A 2 (7.68 ev), 2A 1 (8.40 ev). Observed electronic transitions: CF * 3 (1E,2A 2 1A 1 (repulsive state)) visible 620 nm CF * 3 (2A 1 1A 2 (ground state)) UV 265 nm

Total cross section for dissociation of CF 4 into neutrals Christophorou and Olthoff, J. Phys. Chem. Ref. Data, vol. 28, nº 4, 1999, 967.

100 40 80 30 Pm (%) 60 40 20 Vib-CF4 neutral diss. ion exc1 - He exc2 - He Pm (%) 20 10 0 25 50 75 100 125 150 E (kv/cm) Mean power lost in collisions in a He+40%CF 4 mixture. Penning ionization is not considered. Calculations based on the numerical solution of Boltzmann equation for a uniform electric field configuration. The code used was developed by the group of P. Ségur, CPAT, Toulouse, France 0 25 50 75 100 125 150 E (kv/cm) Mean power lost in collisions in a Ar+40%CF 4 mixture.

1000 1000 100 α exc (cm -1 ) 100 10 Ar+10%CF4 Ar+40%CF4 He+20%CF4 He+40%CF4 100% CF4 α exc (cm -1 ) 10 1 0,1 Ar+10%CF4 Ar+40%CF4 0 25 50 75 100 E (kv/cm) 0 25 50 75 100 E (kv/cm) Number of collisions per cm leading to dissociation of CF 4 into neutral fragments, as a function of the electric field. Number of collisions per cm leading to excitation of Ar* (2p+high lying forbidden) levels, as a function of the electric field.

Dissociative ionization of CF 4 PES Dipole Ionization Zhang et al, Chem. Phys. 137 1989, 391 Fragmentation (%) (e,e+ion) Ion Products 3µ s < τc ~ < 10µ s A) CF +* 4 dissociates before emitting: D(CF 3 -F) = 5.25 ev IP (CF 3 ) = 9.25 ev CF +* 3 CF 3+ + hν (UV) B) CF 4 +* emits before dissociating CF + * 4 (C ~ ) CF CF CF + 4 + * 4 + * 4 (X ~ ) + hν(~ 160 nm) (A ~ ) + hν(~ 240 nm) (B ~ ) + hν(~ 290 nm)

CF 4 + Excitation and de-excitation mechanisms CF 4 * CF 4 dissociation Ar + X Ar** products IR X Ar* (2p) products CF 4 (ν ) CF 3 + F NIR Ar* (3s) X products Ar X = Ar, CF 4, H 2 O,... CF 4 Ar

Excitation and de-excitation mechanisms CF He + 4 products (CF 4+ ) * He** CF 4 He* products dissociation CF 4 * CF 4 + CF 4 X X = He, H 2 O,... CF 3 + F CF 4 (ν ) CF 4 He

Ar-TEA (mm) 100 P v = 30 torr 10 T = 293 k 1 0,1 120 140 160 180 200 220 240 260 280 light intensity/current (a.u.) 120 100 80 60 40 20 0 Ar + 3% TEA λ (nm) 240 260 280 300 320 340 360 380 λ (nm) Absorption length versus wavelength Emission spectrum ( λ = 4 nm)

Excitation and de-excitation mechanisms Ar** X products Ar + X = TEA, Ar, H 2 O,... Ar* (2p) X products TEA * Ar* (3s) X products Ar TEA + Ar Ar 2 * UV VUV TEA Ar

Total light yields (PMT) 1,0 0,8 0,6 Nph/e- 0,4 0,2 0,0 0 100 200 300 400 500 600 700 800 Gain ΤΕΑ mixtures: σ syst < 25% ; He/CF 4-0.1-0.3 ph/e -

0,16 0,12 He+CF 4 0,08 0,04 0,00 10 100 1000 Q.E. 1 0,1 0,01 0,001 Gain (a) 200 300 400 500 600 700 800 900 λ (nm) Quantum efficiency of the photodiode and PMT. Nph/e- Nph/e- 1,0 0,9 0,8 0,7 0,6 0,5 0,4 0,3 0,2 0,1 0,0 Ar+10%CF 4 (b) 1 10 Gain photodiode PMT + filter Photodiode 56 TUVP Nº of photons (λ > 400 nm) emitted per secondary electron as a function of the effective gain in (a) He+20%CF 4 and He+40% CF 4 ; (b) Ar+10%CF 4

Pulse height spectra from 5.9 kev X-rays 50 G A =50 R = 41% 40 G A =80 R = 58% 10 8 G A =320 R = 46% Nº counts/s 40 30 20 30 20 6 4 10 10 2 0 0 0 40 80 120 160 channel # Ar+3%TEA V GEM = 290 V G eff = 640 (R = 53% for G= 460) 0 20 40 60 80 100 120 Channel # Xe+3%TEA V GEM = 320 V G eff = 370 0 0 40 80 120 160 Channel # He+40%CF 4 V GEM = 460 V G eff = 320

Conclusions Ar-CF 4 mixtures emit mainly in the visible (CF 3* ) and in the NIR (Ar I 2p-3s atomic lines, which can be detected even for high CF 4 concentrations). He-CF 4 emit both in the UV and visible (CF 3* ) Visible emissions are more important in Ar/CF 4 than in He/CF 4. The GEM detector has been operated with Ar- and Xe-TEA mixtures but, for TEA concentrations above 5%, large leakage currents arise and the detector becomes unstable. No visible or NIR light was detected in Ar-TEA mixtures Light emitted in the gas (single GEM) was detected with a PMT operating in the pulse mode. The energy resolution is limited by statistics associated with charge multiplication process.