instruments
Review Electroluminescence and Electron Avalanching in Two-Phase Detectors
Alexey Buzulutskov 1,2
1 Budker Institute of Nuclear Physics, 630090 Novosibirsk, Russia; [email protected] 2 Novosibirsk State University, 630090 Novosibirsk, Russia
Received: 7 May 2020; Accepted: 10 June 2020; Published: 18 June 2020
Abstract: Electroluminescence and electron avalanching are the physical effects used in two-phase argon and xenon detectors for dark matter searches and neutrino detection, to amplify the primary ionization signal directly in cryogenic noble-gas media. We review the concepts of such light and charge signal amplification, including a combination thereof, both in the gas and in the liquid phase. Puzzling aspects of the physics of electroluminescence and electron avalanching in two-phase detectors are explained, and detection techniques based on these effects are described.
Keywords: two-phase detectors for dark matter search; liquid noble-gas detectors; proportional electroluminescence in noble gases; electron avalanching at cryogenic temperatures
1. Introduction The ultimate goal for liquid noble-gas detectors is the development of large-volume detectors of superior sensitivity for rare-event experiments. A typical deposited energy in such experiments might be rather low: of the order of 0.1 keV in coherent neutrino-nucleus scattering experiments, 1–100 keV in those of dark matter search and 100 keV in those of astrophysical and accelerator neutrino detection. ≥ Accordingly, the primary ionization and scintillation signals produced by a particle in noble-gas liquid have to be amplified in dense noble-gas media at cryogenic temperatures. The idea of two-phase detectors [1] is based on the requirement of amplification of such weak signals (see reviews [2,3]). In particular, the scattered particle produces in the liquid phase two types of signals: that of primary scintillation recorded promptly (S1 signal) and that of primary ionization recorded with delay (S2 signal). While for the readout of the S1 signal it is sufficient to use optical devices such as photomultiplier tubes (PMTs) and silicon photomultipliers (SiPMs) having their own electronic amplification, to record the S2 signal, one has to amplify it in the detection medium directly (in case of the low deposited energy). In two-phase detectors this is done in the following way: the primary ionization electrons, after drifting in the liquid phase, are emitted into the gas phase where their (S2) signal is amplified. In “classic” two-phase detectors, the way to amplify the S2 signal is provided by electroluminescence (secondary scintillation) produced by drifting electrons under high electric fields. The second possible way to amplify the S2 signal is that of electron avalanching (electron multiplication) at high electric fields. In the following, we refer to these two ways of amplification as those of light and charge signal amplification, respectively. This review is dedicated to the issue of S2 signal amplification. We review all known concepts of light and charge signal amplification (i.e., those based on electroluminescence and electron avalanching in cryogenic noble-gas media), including a combination thereof, both in the gas and in the liquid phase. We explain puzzling aspects of the physics of electroluminescence and electron avalanching in two-phase detectors and describe detection techniques based on these effects.
Instruments 2020, 4, 16; doi:10.3390/instruments4020016 www.mdpi.com/journal/instruments Instruments 2020, 4, 16 2 of 31 Instruments 2020, 4, x FOR PEER REVIEW 2 of 31 Instruments 2020, 4, x FOR PEER REVIEW 2 of 31 2. BasicMany Concepts methods of Signalfor light Amplification and charge insignal Two-Phase amplification Detectors in two-phase detectors have been proposed,Many andmethods some offor these light are and described charge signalin review amplifications [2–6]. Among in two-phase this variety, detectors two basic have concepts been proposed,can beMany distinguished, and methods some of forthat these light most are and other described charge concepts in signal review come amplification sfrom. [2–6]. Among in two-phase this variety, detectors two basic have concepts been canproposed, beThe distinguished, basic and concept some ofthat of these light most are signal other described amplificationconcepts in reviewscome is from.that [2– of6 ]. the Among “classic” this two-phase variety, two detector basic concepts(see [3]); canit is beprovidedThe distinguished, basic byconcept the effect that of light mostof proportional signal other amplification concepts electr comeoluminescence is that from. of the “classic”(EL): see two-phaseFigure 1. Here detector each (see drifting [3]); itelectron is providedThe of basic the by concept ionization the effect of light of(S2) proportionalsignal signal amplification emits electr lightoluminescence in is thatthe EL of thegap (EL): “classic” under see highFigure two-phase electric 1. Here detector field, each the (seedrifting light [3]); electronitintensity is provided of being the by ionizationroughly the effect proportional (S2) of proportional signal toemits the electroluminescence electriclight in field.the EL This gap concept (EL): under see splitshigh Figure electricinto1. Heretwo field, sub-concepts: each the drifting light intensityelectronwith indirect of being the and ionization roughly direct proportional (S2)optical signal readout. emits to the lightFor electric the in the former, ELfield. gap theThis under optical concept high readoutelectric splits intogoes field, two via the sub-concepts:a light wavelength intensity withbeingshifter indirect roughly (WLS). and proportional direct optical to the readout. electric field.For the This former, concept the splits optical into readout two sub-concepts: goes via a withwavelength indirect shifterand direct (WLS). optical readout. For the former, the optical readout goes via a wavelength shifter (WLS).
Figure 1. Basic concepts of light signal amplification in two-phase detectors, using proportional Figureelectroluminescence 1. BasicBasic concepts concepts (EL) ofin of lightthe light EL signal gap. amplification amplificationLeft: with indirect in two-phase optical readout detectors, via using wavelength proportional shifter electroluminescence(WLS), in two-phase (EL) (EL)Ar using in the excimer EL gap. emission Left: withwith in theindirect indirect vacuum optical optical ultraviolet readout readout (VUV) via wavelength at 128 nm. shifterRight: (WLS),with direct in two-phase optical readout, Ar using either excimer in two-phase emission Xe in usingthe vacuum excimer ultraviolet emission in(VUV) the VUV at 128 at nm.175 nm,Right: or within two-phase direct optical Ar using readout,readout, neutral eithereither bremsstrahlung inin two-phasetwo-phase Xe Xe(N using BrS)using emission excimer excimer emissionin emission the non-VUV in in the the VUV VUVrange at at 175(at 175 nm,200–1000 nm, or or in intwo-phasenm). two-phase Ar Ar using using neutral neutral bremsstrahlung bremsstrahlung (NBrS) (NBrS) emission emission in the in non-VUVthe non-VUV range range (at 200–1000 (at 200–1000 nm). nm). The basic concept of charge signal amplificationamplification in two-phase detectors is that of using a gas electronThe multipliermultiplierbasic concept (GEM)-like(GEM)-like of charge structure structure signal in amplificationin the the gas gas phase phase in that two-phasethat provides provides detectors electron electron avalanchingis avalanchingthat of using within within a gas the electronGEMthe GEM holes multiplier holes at cryogenic at cryogenic (GEM)-like temperatures: temperatures: structure see in Figureseethe Figure gas2 andphase 2 reviewand that review provides [4]. [4]. electron avalanching within the GEM holes at cryogenic temperatures: see Figure 2 and review [4].
Figure 2.2. BasicBasic concept of charge signal amplificationamplification in two-phase detectors, using gas electron Figuremultiplier 2. Basic (GEM)-like concept structures of charge [[4].4 ].signal amplification in two-phase detectors, using gas electron multiplier (GEM)-like structures [4].
Instruments 2020, 4, x FOR PEER REVIEW 3 of 31 Instruments 2020, 4, 16 3 of 31 In Sections 3–6, we describe in detail the physics and state-of-the-art of these basic concepts, as well as consider other (most developed) concepts of signal amplification in cryogenic noble-gas In Sections3–6, we describe in detail the physics and state-of-the-art of these basic concepts, as well media. as consider other (most developed) concepts of signal amplification in cryogenic noble-gas media.
3.3. LightLight SignalSignal Amplification Amplification in in the the Gas Gas Phase Phase of a of Two-Phase a Two-Phase Detector, Detector, Using Using Proportional Proportional ElectroluminescenceElectroluminescence
3.1.3.1. Three ELEL MechanismsMechanisms AccordingAccording toto modernmodern concepts,concepts, therethere areare threethree ELEL mechanismsmechanisms responsibleresponsible forfor proportionalproportional ELEL ∗ ∗ inin gaseousgaseous ArAr andand Xe:Xe: that of excimer ( 𝐴𝑟Ar 2∗ or Xe𝑋𝑒2∗ )) emissionemission inin thethe VUVVUV (“ordinary”(“ordinary” EL),EL), thatthat ofof emissionemission duedue toto atomicatomic transitionstransitions inin thethe nearnear infraredinfrared (NIR),(NIR), andand thatthat ofof neutralneutral bremsstrahlungbremsstrahlung (NBrS)(NBrS) emissionemission inin thethe UV,UV, visiblevisible andand NIRNIR range.range. TheThe energyenergy levellevel diagrams,diagrams, appropriateappropriate reactionsreactions andand theirtheir constants,constants, relevant to the former two mechanisms,mechanisms, are presented in Figure 33 andand TableTable1 .1. PhotonPhoton emissionemission spectraspectra forfor all all three three mechanisms mechanisms and and their their absolute absolute EL EL yields yields are are shown shown in in Figures Figures4 and4 and5 respectively 5 respectively for Arfor [Ar7]. [7] For. For other other noble noble gases gases the emissionthe emission spectra spectra and ELand yields EL yields look alikelook [alike4,5]. For[4,5]. Ar, For the Ar, EL the mechanisms EL mechanisms are described are described below below in detail. in detail.
FigureFigure 3.3. EnergyEnergy levels levels of of the the lower lower excited excited and and ionized ionized states states relevant relevant to tothe the ternary ternary mixture mixture of Ar of Ardoped doped with with Xe Xeand and N N2 in2 in the the two-phase two-phase mode mode [7]. [7]. These These are are shown shown for for gaseous Ar, gaseousgaseous NN22,, gaseousgaseous Xe,Xe, liquidliquid ArAr andand XeXe inin liquid Ar. The solid arrows indicate the radiative transitions observedobserved inin experimentsexperiments andand relevantrelevant toto thethe presentpresent reviewreview (i.e.,(i.e., whenwhen thethe excitationexcitation isis inducedinduced byby ionizationionization oror electroluminescence).electroluminescence). The numbers next to each arrow show the photonphoton emissionemission bandband ofof thethe transition,transition, defineddefined byby majormajor emissionemission lineslines oror byby fullfull widthwidth ofofthe the emission emission continuum.continuum. TheThe dasheddashed arrowsarrows indicateindicate the the most most probable probable non-radiative non-radiative transitions transitions induced induced by atomicby atomic collisions collisions for Ar,for XeAr, and Xe
Nand2 species N2 species and theirand their pair combinationspair combinations in the in gas the and gas liquidand liquid phase. phase.
ProportionalProportional ELEL isis characterizedcharacterized byby aa reducedreduced ELEL yieldyield ((YY/N/N),), whichwhich byby definitiondefinition isis thethe numbernumber ofof photonsphotons producedproduced perper driftingdrifting electronelectron perper atomicatomic densitydensity andand perper unitunit driftdrift path.path. ItIt isis typicallytypically plottedplotted as a a function function of of the the reduced reduced electric electric field field (E/N (E),/N the), the latter latter being being expressed expressed in Townsends: in Townsends: 1 Td 17 2 1 1= Td10−=17 V10 cm− 2V atom cm −1atom, corresponding− , corresponding to 0.87 tokV/cm 0.87 kVin /gaseouscm in gaseous Ar at 1.00 Ar atatm 1.00 and atm 87.3 and K. 87.3 K.
Table 1. Basic reactions of excited species relevant to the performance in the two-phase mode, namely in Ar in the gas and liquid phase, doped with Xe (1000 ppm in the liquid and 40 ppb in the gas phase) and N2 (50 ppm in the liquid and 135 ppm in the gas phase), their rate (k) or time (τ) constants reported
Instruments 2020, 4, 16 4 of 31
Table 1. Basic reactions of excited species relevant to the performance in the two-phase mode, namely Instrumentsin Ar in 2020 the, 4 gas, x FOR and PEER liquid REVIEW phase, doped with Xe (1000 ppm in the liquid and 40 ppb in the gas phase)4 of 31
and N2 (50 ppm in the liquid and 135 ppm in the gas phase), their rate (k) or time (τ) constants reported in the literature and their time constants reduced to given atomic densities at 87 K (τTP), in particular in the literature and their time constants reduced to given atomic densities at 87 K (τTP), in particular 19 −3 22 −3 forfor Ar Ar to to that that of of 8.63 8.63 × 1019 cmcm and3 and 2.11 2.11 × 10 10 cm22 cm in the3 in gas the and gas liquid and liquid phase, phase, respectively respectively [7]. The [ 7]. × − × − Thereferences references presented presented in th ine thetable table are those are those of [7]. of [7].
3.2. Electroluminescence due to Excimer Emission 3.2. Electroluminescence Due to Excimer Emission In ordinary (excimer) EL, the electrons accelerated by the electric field excite the atoms, which in turnIn ordinary produce (excimer)the excimers EL, (excited the electrons molecules) accelerated in three-body by the electriccollisions. field The excite excimers the atoms, are produced which in ∗ ∗ turnin either produce a singlet the excimers 𝐴𝑟 (∑ (excited) or a triplet molecules) 𝐴𝑟 (∑ in ) three-body state. These collisions. states decay The with excimers photon areemission produced in the VUV, peaked at 128 nm for Ar and 175 nm for Xe (see Figures 3 and 4 and reactions (1) and (2) in Table 1):
Instruments 2020, 4, 16 5 of 31
1P + 3P + in either a singlet Ar2∗ u or a triplet Ar2∗ u state. These states decay with photon emission in theInstruments VUV, peaked2020, 4, x atFOR 128 PEER nm REVIEW for Ar and 175 nm for Xe (see Figures3 and4 and reactions (1) and (2)5 of in 31 TableInstruments1): 2020, 4, x FOR PEER REVIEW 5 of 31 e− + Ar e− + Ar∗ (1) 𝑒 + 𝐴𝑟→𝑒→ + 𝐴𝑟∗ (1) 𝑒 + 𝐴𝑟→𝑒 + 𝐴𝑟∗ (1) Ar∗∗+ 2Ar Ar2∗∗+ Ar (2) 𝐴𝑟 +2𝐴𝑟→→ 𝐴𝑟 + 𝐴𝑟 (2) 𝐴𝑟∗ +2𝐴𝑟→𝐴𝑟∗ + 𝐴𝑟 (2) + Ar𝐴𝑟2∗∗ →22Ar𝐴𝑟+ℎ𝜈hν (3) ∗ → (3) 𝐴𝑟 →2𝐴𝑟+ℎ𝜈 (3)
FigureFigureFigure 4.4. 4. Photon Photon emission emission spectraspectra in gaseousgaseousseous Ar Ar due due to to ordinary ordinary scintillations scintillationsscintillations in inthe thethe VUV VUVVUV measured measuredmeasured in [8], NBrS EL at 8.3 Td theoretically calculated in [9] and avalanche scintillations in the near infrared inin [[8],8], NBrSNBrS ELEL atat 8.3 Td theoretically calculatedcalculated inin [[9]9] and avalanche scintillationsscintillations inin the near infrared (NIR) measured in [10,11]. Also shown are the photon detection efficiency (PDE) of SiPM (MPPC (NIR)(NIR) measuredmeasured inin [[10,11].10,11]. Also shown are thethe photonphoton detectiondetection eefficiencyfficiency (PDE)(PDE) ofof SiPMSiPM (MPPC(MPPC 13360-6050PE (Hamamatsu)) at overvoltage of 5.6 V and the transmittance of the acrylic plate (1.5 mm 13360-6050PE13360-6050PE (Hamamatsu))(Hamamatsu)) atat overvoltageovervoltage ofof 5.65.6 VV andand thethe transmittancetransmittance ofof thethe acrylicacrylic plateplate (1.5(1.5 mmmm thick) [12]. thick)thick) [[12].12].
FigureFigure 5. 5.Summary Summary of of experimentalexperimental data on reduced reduced electroluminescence electroluminescence (EL) (EL) yield yield in ingaseous gaseous Ar Arfor for allall known known (EL) (EL) mechanisms: mechanisms: forfor NBrS EL below 1000 1000 nm nm,, measured measured in in [9,13] [9,13 at] at8787 K; K;for for ordinary ordinary EL EL Figure 5. Summary of experimental data on reduced electroluminescence (EL) yield in gaseous Ar for inin the the VUV, VUV, due due to to excimer excimer emission emission goinggoing viavia ArAr*(3p(3p554s4s1)1 )excited excited states, states, measured measured in [9,13] in [9,13 at] 87 at K 87 K all known (EL) mechanisms: for NBrS EL below 1000 nm, measured in [9,13]* at 875 K;1 for ordinary EL andand in in [14 [14]] at at 293 293 K; K; for for EL EL in in the the NIR NIR duedue toto atomicatomic transitionstransitions going going via via Ar Ar(3p*(3p4p54p) 1excited) excited states states in the VUV, due to excimer emission going via Ar*(3p54s1) excited states, measured in [9,13] at 87 K measuredmeasured in in [15 [15]] at at 163 163 K. K. and in [14] at 293 K; for EL in the NIR due to atomic transitions going via Ar*(3p54p1) excited states measuredThe singlet in [15] and at triplet 163 K. excimer states are responsible respectively for the fast and slow emission components observed in proportional EL. Their time constants are of 4.2 ns and 3.1 μs respectively: The singlet and triplet excimer states are responsible respectively for the fast and slow emission components observed in proportional EL. Their time constants are of 4.2 ns and 3.1 μs respectively:
Instruments 2020, 4, 16 6 of 31
Instruments 2020, 4, x FOR PEER REVIEW 6 of 31 The singlet and triplet excimer states are responsible respectively for the fast and slow emission seecomponentsInstruments Table 1 and2020 observed, references4, x FORin PEER proportional therein. REVIEW Ordinary EL. Their EL timehas a constants threshold are in ofthe 4.2 electric ns and field, 3.1 µ ofs respectively: about 4 6Td of 31(see see FigureTable1 5),and defined references by the therein. energy Ordinary threshold EL of has11.5 a5 thresholdeV of Ar atom in the excita electriction field,in Equation of about (1). 4 Td (see see Table 1 and references therein. Ordinary EL has a threshold in the electric field, of about 4 Td (see FigureOrdinary5), defined proportional by the energy EL threshold has two ofcharacteri 11.55 eVstic of Ar properties: atom excitation a threshold in Equation and (1).linear field Figure 5), defined by the energy threshold of 11.55 eV of Ar atom excitation in Equation (1). dependenceOrdinary (far proportional enough from EL has the two threshold). characteristic For properties:Xe, this can a threshold be seen andfrom linear Figure field 6 dependencepresenting Ordinary proportional EL has two characteristic properties: a threshold and linear field compilation(far enough fromof the the experimental threshold). data For Xe,on EL this yield can by be seen2007: fromthe results Figure of6 presentingthe different compilation groups are ofclose, the experimentaldependence data (far onenough EL yield from by the 2007: threshold). the results For of Xe, the this different can be groups seen arefrom close, Figure with 6 thepresenting exception withcompilation the exception of the of experimental early works. data on EL yield by 2007: the results of the different groups are close, of early works. withThe the absolute exception photon of early yields works. of ordinary (excimer) EL were theoretically calculated for Ne, Ar, Kr The absolute photon yields of ordinary (excimer) EL were theoretically calculated for Ne, Ar, and Xe Thein [16] absolute using photon Monte yieldsCarlo ofsimulation ordinary (excimerin microscopic) EL were approach: theoretically see Figure calculated 7. One for canNe, seeAr, Krfrom Kr and Xe in [16] using Monte Carlo simulation in microscopic approach: see Figure7. One can theand figure Xe in that [16] well using above Monte the Carlo EL threshold, simulation the in microscopic theoretical predictionsapproach: see are Figure in rather 7. One good can agreementsee from see from the figure that well above the EL threshold, the theoretical predictions are in rather good withthe thefigure yields that wellmeasured above thein experiment EL threshold, at the room theoretical temperature, predictions for Arare inand rather Xe. goodExtrapolating agreement the agreement with the yields measured in experiment at room temperature, for Ar and Xe. Extrapolating theoreticalwith the ELyields yield, measured the EL threshold in experiment was determined at room temperature, as 1.5, 4.1, 2.6for andAr and2.9 Td Xe. for Extrapolating Ne, Ar, Kr and the Xe respectivelythetheoretical theoretical [16].EL EL yield, yield, the the EL EL threshold threshold was was determined determined as 1.5, as 4.1, 1.5, 2.6 4.1, and 2.6 2.9 and Td 2.9 for Td Ne, for Ar, Ne, Kr Ar, and Kr Xe and Xerespectively respectively [16]. [16 ].
FigureFigure 6.6. 6.ReducedReduced Reduced ELEL EL yields yields yields for for for ordinary ordinaryordinary (excimer) (excimer)(excimer) EL inEL Xe inin measured XeXe measuredmeasured by di byff byerent different different groups, groups, groups, as a function as asa a functionoffunction the reduced of ofthe the electricreduced reduced field electric electric [17]. field field The [17]. references[17]. ThThee referencesreferences in the figure inin thethe are figure figure those are are of those [those17]. of of [17]. [17].
Figure 7. Measured reduced EL yield for ordinary (excimer) EL at room temperature for Ar and Xe Figure(data 7. points), MeasuredMeasured as a reducedfunction reduced ELof EL th yield yielde reduced for for ordinary electric (excimer)field, (excimer) compared EL EL at at toroom Monte temperature Carlo simulation for for Ar and data Xe (data(curves), points), for as asNe, a Ar,function Kr and of Xe th the (frome reduced [16], with electric permission field, field, compared from Elsevier). to Monte Carlo simulation data (curves), for Ne, Ar, Kr and XeXe (from(from [[1616],], withwith permissionpermission fromfrom Elsevier).Elsevier). Far enough from the threshold, the EL yield can be parametrized by a linear function, indicating theFar proportionality enough from of the the threshold, EL yield to the the EL electric yield canfield: be parametrized by a linear function, indicating the proportionality of the EL yield to the electric field:
Instruments 2020, 4, 16 7 of 31
Far enough from the threshold, the EL yield can be parametrized by a linear function, indicating the proportionality of the EL yield to the electric field:
h 17 1 2 1i Y/N 10− photon electron− cm atom− = a E/N b (4) · − 17 2 1 where reduced electric field E/N is given in Td (10− V cm atom− ). This equation is universally valid for all temperatures and gas densities. Parameter “b” defines the electric field threshold for proportional EL, while parameter “a” describes the light amplification factor, namely the number of photons emitted by drifting electron per applied voltage across the EL gap. For Ar, Kr and Xe this parameter was measured to be 81 [14], 120 [18] and 140 [17] photon/kV respectively. The parametrization of the experimental data by linear field dependence was presented in [14] and [17] for Ar and Xe respectively:
Y/N = 0.081 E/N 0.190, for Ar; (5) · − Y/N = 0.140 E/N 0.474, for Xe. · − However, near the EL threshold this parametrization gives overestimated EL yield values, due to contribution of neutral bremsstrahlung electroluminescence (see Section 3.3). In this case the experimental data relevant to ordinary EL should be used directly. In particular, in two-phase Ar at 87 K and 1.0 atm, the number of photons in the VUV emitted by drifting electron per 1 cm, deduced from experimental data of Figure5, is 345 and 43 at electric field of 8 and 4.6 Td respectively, the latter corresponding to the nominal operation field of the DarkSide experiment.
3.3. Electroluminescence Due Neutral Bremsstrahlung Effect In addition to the ordinary EL mechanism, there is a concurrent EL mechanism, based on bremsstrahlung of drifting electrons scattered on neutral atoms, so-called neutral bremsstrahlung (NBrS) [9,13,19]: e− + Ar e− + Ar + hν (6) → The development of the mechanism is described in detail in [9]. The NBrS differential cross section is proportional to elastic cross section (σel(E)) of electron-atom scattering [9]: !1/2 dσ 8 re 1 E hν = − [(E hν) σ (E) + E σ (E hν)] (7) dν 3 c hν E − · el · el −
2 2 Here re = e /mec is the classical electron radius, c = νλ is the speed of light, E is the initial electron energy. For electron-atom scattering cross sections in Ar, see Figure8. Consequently, the NBrS EL yield is predicted to be maximal for electron energies of the order of 10 eV where the elastic cross section has a maximum, thus corresponding to the electric fields of 4–5 Td. This is confirmed in Figure9 showing the absolute yield of NBrS EL theoretically calculated in [9], in comparison with that of ordinary EL. NBrS EL has a continuous emission spectrum, extending from the UV (200 nm) to the visible and NIR range (1000 nm) and even to the radio frequency range [20]: see Figure4. From Figures4 and9 one can see that NBrS EL, albeit being significantly weaker than ordinary EL above the Ar excitation threshold, has no threshold in electric field, in contrast to ordinary EL, and thus dominates below the threshold. Accordingly, the NBrS effect can explain two remarkable properties of proportional EL observed in experiment [9,13,19]: that of the photon emission below the Ar excitation threshold and that of the substantial contribution of the non-VUV spectral component above the threshold. Instruments 2020, 4, 16 8 of 31 InstrumentsInstruments 20202020,, 44,, xx FORFOR PEERPEER REVIEWREVIEW 88 ofof 3131
Figure 8. Electron scattering cross sections in Ar: elastic (𝜎 ), momentum-transfer (𝜎 ), excitation Figure 8. Electron scattering cross sections in Ar: elastic ( 𝜎σ el), momentum-transfer (σ𝜎 trans ),), excitationexcitation (𝜎 ) and ionization (𝜎 ) (from [9], with permission from Elsevier). ((σ𝜎exc ) and ionization (σ𝜎ion