Nuclear Instruments and Methods in Physics Research B 164±165 (2000) 891±896 www.elsevier.nl/locate/nimb Eects of under- and overlayers on particle and photon emission from solid argon induced by 2 MeV protons D.E. Grosjean a, R.A. Baragiola a a,* , W.L. Brown b Laboratory for Atomic and Surface Physics, Engineering Physics, University of Virginia, Thornton Hall, Charlottesville, VA 22901, USA b Bell Labs, Lucent Technologies, Murray Hill, NJ 07974, USA Abstract We studied electron emission, luminescence, and sputtering of thin condensed gas ®lms by 2 MeV protons. For thin Ar ®lms, an external electric ®eld causes nearly complete extraction of excited electrons, hindering hole recombination. This leads to a reduction in luminescence and sputtering. We have observed that overlayers of N2 annul the eects of external electric ®elds and also that they decrease ion-induced luminescence from the bulk of the Ar ®lms. In related experiments, 20 nm Krypton layers were grown between the metal substrate and the Ar ®lms. We found that these underlayers change the dependence of particle and photon emission on Ar ®lm thickness and dramatically increase electron emission. We discuss these new eects in terms of internal electric ®elds produced by unbalanced holes and of changed reactions of excitons and holes at the interfaces. Ó 2000 Elsevier Science B.V. All rights reserved. PACS: 79.20.)m; 34.50.Dy; 78.60.Hk; 71.35.)y Keywords: Electron emission; Luminescence; Sputtering; Rare gas solids; Excitons 1. Introduction Many of the unsolved fundamental questions in atomic collisions in solids are in the area of radiation eects in insulators induced by electronic excitations. Searching for answers to those questions is motivated not only by the need for fundamental insight but also because of the potential implications in other areas such as radiation biol- * Corresponding author. Tel.: +1-804-982-2907; fax: +1-804924-1353. E-mail address: [email protected] (R.A. Baragiola). ogy, astronomy, semiconductor processing, and nuclear energy production. A characteristic of the eects of electronic energy deposition in insulators is their strong dependence on the type of material. Relevant properties include the chemical composition, the transport of electrons, holes, and excitons through the material and interfaces, and their trapping at defects and at the surface. In view of this complexity we have chosen to study rare gas solids, the simplest insulators, with the aim of isolating the important basic phenomena. These materials have desirable properties, including being chemically inert, and having weak internal electric ®elds in their ground state, so they behave 0168-583X/00/$ - see front matter Ó 2000 Elsevier Science B.V. All rights reserved. PII: S 0 1 6 8 - 5 8 3 X ( 9 9 ) 0 1 1 1 3 - 1 892 D.E. Grosjean et al. / Nucl. Instr. and Meth. in Phys. Res. B 164±165 (2000) 891±896 like a dense gas. Electronic excitations in rare gas solids have been described in several reviews [1±7], and abundant information exists from gas-phase experiments [8,9] which can be used in the search for a microscopic understanding of processes in the solid. The basic events in electronic excitations by fast ions and their subsequent decay are the following. By multiple collisions, the projectiles produce a track of predominantly single ionizations and excitations. The 2 MeV protons used in our study have an electronic stopping cross-section of 6.5 ´ 10ÿ15 eV atom/cm2 , or 6.5 eV per atomic layer [10]. The energy is mainly deposited into electron± ion pairs and excited Ar (excitons). For a typical 75 nm Ar ®lm this translates into an average electronic energy loss of 1.2 keV, which results in 44 ionizations and 21 direct excitations [11]. Electrons and ions can migrate by diusion and under the in¯uence of internal electric ®elds from trapped charges, charges in the ionization track, image charges induced in the substrate, and by externally applied electric ®elds. The ions which do not reach the substrate will self-trap as Ar cluster ions [5] and later recombine with thermalized electrons into the excimer Ar2 . Directly formed excitons can diuse through the lattice and either be quenched at the substrate, trapped at the surface where they can lead to desorption, or self-trap into excimers in the bulk. Radiative decay of Ar2 to the repulsive part of the ground state potential leads to 9.8 eV luminescence and to energetic Ar atoms that can initiate a collision cascade that may result in sputtering (desorption). Our previous experiments demonstrated that the availability of electrons determines the amount of luminescence and the sputtering yield, because it aects the ability of the ions to recombine into excitons and excimers [12]. For low ionization densities, like those caused by 2 MeV protons, a thin ®lm can be depleted of free electrons by a suciently high, externally applied, electric ®eld. This essentially complete electron extraction is made possible by two factors. An electrostatic ®eld inside the ®lm, produced by trapped charges, prevents electrons from reaching the substrate and redirects them towards the surface where they can be extracted by the external electric ®eld if it is large enough [13]. There the electrons do not ®nd a surface potential barrier because Ar has a negative electron anity that allows even thermalized electrons to escape the solid. The importance of the negative electron anity is con®rmed by the observation that solid Kr and Xe, which have similar properties to Ar but positive surface barriers for electrons, yield much lower electron emission than Ar [13]. The sensitivity to the surface barrier suggests that the behavior of Ar can be changed drastically by modifying its surface with thin deposits of other materials. In this work we deposited thin layers of nitrogen with the idea of changing the surface barrier but kept the thickness low enough so that the attenuation of electrons in this layer is unimportant [14]. As we describe below, we observed that thin nitrogen overlayers cause a simultaneous reduction of electron yield and increase of luminescence, as well as the disappearance of the in¯uence of external electric ®elds. 2. Experiments The experiments were done in an ultrahighvacuum chamber attached to the 3.75 MV Van de Graa accelerator at Bell Laboratories, Lucent Technologies. Fig. 1 shows the setup schematical- Fig. 1. Experimental setup. D.E. Grosjean et al. / Nucl. Instr. and Meth. in Phys. Res. B 164±165 (2000) 891±896 ly; details have been published [3,11,15]. Condensed-gas ®lms are grown by vapor deposition of 99.9995% pure gas onto an Au substrate cooled to 8 K. The ®lms are grown at 100 nm/min and are expected to be polycrystalline [16]. Surrounding the target are heat shields cooled with LN2 ; the inner one acts also as an electrode (anode) to apply an electric ®eld to the target surface and collect electrons emitted from the target. The base pressure around the target is 1 ´ 10ÿ10 Torr. To ensure a clean substrate surface, a fresh gold ®lm is evaporated onto the substrate before growing a condensed gas ®lm. In the experiments, we measured sputtering, UV luminescence and electron emission during irradiation by 2 MeV protons. Excimer luminescence (9.8 eV) was detected by a vacuum ultraviolet spectrometer. Sputtering was measured with a quadrupole mass spectrometer calibrated against the decrease of ®lm thickness measured with Rutherford backscattering spectroscopy [17]. Electron emission was determined from target currents. The yields of electrons, sputtered Ar and luminescence photons are denoted by the symbols c, Y, and L, respectively. c and Y are expressed in number of particles ejected per projectile ion and L is the number of photons produced in the ®lm [11]. In the experiments where we study the eect of external electric ®elds, the anode voltage Va was scanned linearly from 0 up to +750 V and back down while recording luminescence, sputtering and electron emission simultaneously. During the measurements, the projectile ¯ux was kept low so that the total sputtering during a voltage scan was less than a monolayer. 3. Results and discussion Fig. 2 shows the eect of the anode voltage on the particle and light emission from a 75 nm thick Ar ®lms induced by 2 MeV ions. Electron emission saturates for Va > 200 V and a hysteresis is observed when scanning Va up and down [12,18]. This contrasts with the case of a bare Au substrate, where there is no hysteresis, and electron emission saturates at a few volts. The reason for the dierences is the production of long-lived, positively 893 Fig. 2. Electron yield c, luminescence L, and sputtering yield Y for 2 MeV H on a 75 nm Ar ®lm (*) and on 75 nm Ar ®lms covered with an overlayer of nitrogen 5 nm thick (open symbols) and 20 nm thick (closed symbols). The yields are given as a function of anode voltage. Some representative error bars pertaining to a given sample are shown. In addition there is a 10% sample-to-sample variation, so dierences in luminescence at high anode voltages for dierent N2 overlayer thicknesses are not signi®cant. For the case of a 20 nm N2 overlayer the sputtering of Ar atoms is undetectable above the background. charged traps in the insulator ®lm, which cause a positive surface potential that hinders electron collection at moderate Va [13]. Electron extraction means that holes are left behind that cannot be neutralized into excimers by recombination and therefore luminescence drops. As stated above, luminescence occurs in a transition from Ar2 to the repulsive part of the Ar2 ground state. This repulsion produces energetic Ar recoils that can initiate sputtering. Thus, the decrease of luminescence due to the removal of electrons leads to the observed decrease in sputtering. The fact that sputtering decreases less than luminescence when 894 D.E. Grosjean et al. / Nucl. Instr. and Meth. in Phys. Res. B 164±165 (2000) 891±896 electrons are extracted is evidence of pathways to sputtering that do not go through the excimer Ar2 . 3.1. Overlayers To test the role of the surface on particle emission and electric ®eld eects we deposited layers of other condensed gases on top of 75 nm Ar ®lms. A 10 nm layer of solid oxygen on top of the Ar ®lm was found to eliminate the electric ®eld eect on luminescence. Since oxygen is electronegative, and known to trap electrons, we did subsequent studies with nitrogen overlayers, seeking a simpler situation. Fig. 3 shows the eects of dierent thicknesses of nitrogen overlayers on 75 nm Ar ®lms. Even for the thinnest nitrogen coverage, 2 nm, the sputtering yield of Ar atoms is less than 15% of that for an uncoated argon ®lm, and is not shown in the ®gures. An external electric ®eld no longer aects the luminescence, but a 10 nm nitrogen overlayer reduces it to about 40% of its N2 -free level. As nitrogen coverage increases, the electron yield approaches the value c 1:5 of pure N2 determined for a 200 nm ®lm, as shown in Fig. 4. This value of c is much smaller than c 70 for an Ar ®lm of similar thickness [15]. Hysteresis is also present, signaling the formation of deeply trapped charges. Fig. 4. Electron yield for 2 MeV H incident on a 200 nm nitrogen ®lm deposited on Au, as a function of anode voltage. The observations shown in Fig. 3 indicate that a N2 overlayer prevents the extraction of electrons from an Ar ®lm and also indicate that the Ar/N2 interface quenches Ar excitons and/or holes, which are precursors to luminescence. On the other hand, we found that placing a 10 nm nitrogen layer under a 75 nm argon ®lm, increases the Ar2 luminescence to 1.2 times the value for the same Ar ®lm without this underlayer. The two experiments indicate that, although the N2 interface quenches holes or excitons, it does so less eectively than Au. 3.2. Kr underlayers Fig. 3. Dependence of Ar excimer luminescence and electron emission from 75 nm Ar ®lms on the thickness of nitrogen overlayers. The projectiles are 2 MeV H . Luminescence is measured without applying an external electric ®eld. To test the role of the substrate in hole neutralization and the dependencies of the yields on the electric ®eld, we used a 20 nm Kr underlayer between the Ar and the Au substrate. The lower panel of Fig. 5 shows the Ar-thickness dependence of particle and photon emission for ®lms grown on Kr underlayers, and compares it with that of Ar ®lms grown directly on Au. In general, all the yields are seen to increase with ®lm thickness but luminescence is suppressed for very thin ®lms. The reason for this behavior is the radiationless conversion of holes and excitons into ground state Ar at the Au surface [3]. Holes can reach the substrate by diusion and at short distances to the substrate, D.E. Grosjean et al. / Nucl. Instr. and Meth. in Phys. Res. B 164±165 (2000) 891±896 Fig. 5. Dependence of the yields cS , L0 and Y 0 and the fractions cS =m on Ar ®lm thickness, for 2 MeV H . The superscripts S, 0 indicate measurements taken at saturation and zero anode voltage, respectively. The lines without symbols are for Ar ®lms grown on a bare substrate and the lines linking symbols correspond to Ar ®lms grown on a 20 nm Kr layer on top of Au. (- - - -) Electron emission, (Ð) luminescence, ( ) sputtering. their motion to the Au surface is enhanced by drift due to the strong image electric ®eld [19]. If the holes reach the interface before the ionized electrons can cool down suciently to allow recombination, they can neutralize by an Auger process [3,20,21]. Excitons can also reach the interface by diusion, where they can be quenched by resonance ionization followed by Auger neutralization, or by Auger deexcitation [20]. The increase of luminescence and sputtering when Ar is grown on a Kr overlayer can be attributed to the less ecient quenching of Ar excitons and holes at the Ar/Kr interface, similar to what we observed for the Ar± N2 interface. The reason is that Auger quenching processes are blocked in wide band-gap materials like Kr and N2 . In addition to the luminescence quenching, it is clear in the lower panel of Fig. 5 that sputtering, 895 luminescence, and electron emission were all higher for the Ar/Kr/Au case than for Ar/Au. We propose that this dierence is also related to the dierence in neutralization/deexcitation processes at the Ar/underlayer interface. In the Ar/Au case for no applied anode voltage, there is a ``dark zone'' extending about 35 nm from the interface in which holes tend to be neutralized at the substrate due to the image force attraction. By adding the intervening underlayer of Kr, this region is no longer such a sink for Ar holes. The most dramatic dierence this creates is the enhancement of the thin-®lm sputtering yield. For very thin ®lms (<50 nm), the dark zone is a large portion of the entire ®lm, removing most of the holes and excitons that can cause sputtering. The intervening Kr layer removes part of that dark zone from the Ar, and provides a slight re¯ecting surface for diusing excitons. Note that as the Ar ®lm thickness increases, it appears that the sputtering yield may approach the thick-®lm yield for Ar/Au, which would be expected for this surface process. A similar argument is used for the enhanced luminescence yield for thin ®lms; in that case, also, the yields look as if they may be similar for thicker ®lms. The electron yield for the Kr underlayer is enhanced by the additional electrons created in the Kr layer by the projectile and by the Ar excitons, described below. In the top panel of Fig. 5 we show ratios cS =m as a function of thickness, for 2 MeV H bombardment. Here the superscripts 0 and S indicate that measurements were made with zero or saturation anode voltage, respectively. The ratio cS =m gives the fraction of the total number of electron±hole pairs produced in the ®lm, m, that can be extracted. To obtain m, we divide the energy loss in the ®lm, calculated with known electronic stopping crosssection [10], by W 27 eV, the mean energy spent per pair in Ar [1]. For Ar on Au, cS =m 1 and consistent with previous results for thin ®lms under condition of weak ionization density [12,13]. As stated above, ecient electron extraction results from the negative electron anity of Ar and the internal electric ®eld produced by trapped charges, which pushes electrons to the surface and away from the substrate. The Kr underlayer causes a substantial increase of cS =m, which is larger by a 896 D.E. Grosjean et al. / Nucl. Instr. and Meth. in Phys. Res. B 164±165 (2000) 891±896 factor of 1.4 than in the case of Ar on Au, even when the electron±hole pairs created in the Kr layer are included in m. A likely mechanism for the enhanced electron yield is the ionization of the Kr layer by Ar excitons diusing to the interface. The process is near resonant since the Ar excitation energy (12.1 eV) is very close to the ionization energy (band gap) of Kr, 11.9 eV [1]. An eect of this type has been observed in the case of Kr impurities in an Ar matrix, which are eciently ionized by diusing Ar excitons [22]. The values of LS /L0 and YS /Y0 and their thickness dependencies are similar to those for the clean Au substrate, and consistent with the variation of electron extraction. 4. Conclusions The use of N2 overlayers and Kr underlayers have allowed us to test models of the dynamics of holes and electrons in thin Ar ®lms produced in dilute ionizations. Overlayers as thin as 5 nm of oxygen or nitrogen greatly reduced the electron yield, and prevented the applied ®eld from reducing luminescence. This was taken as con®rmation that electron removal is needed to produce the excess charges that set up an internal electric ®eld responsible for complete charge separation. Electron emission from Ar is dramatically increased by Kr underlayers because Ar excitons are converted into electron±hole pairs at the Ar/Kr interface. Acknowledgements This work was supported by NSF, Division of Materials Research. References [1] N. Schwentner, E.E. Koch, J. Jortner, Electronic Excitations in Condensed Rare Gases, Springer, Berlin, 1985. [2] G. Zimmerer, in: U.M. Grassano, N. Terzi (Eds.), ExcitedState Spectroscopy in Solids, North-Holland, Amsterdam, 1987, p. 37. [3] C.T. Reimann, W.L. Brown, R.E. Johnson, Phys. Rev. B 37 (1988) 1455. [4] I.Ya. Fugol, Adv. Phys. 37 (1988) 1. [5] E. Hudel, E. Steinacker, P. Feulner, Phys. Rev. B 44 (1991) 8972. [6] R.E. Johnson, J. Schou, Dansk. Vid. Sels. Mat. Fys. Med. 43 (1993) 403. [7] G. Zimmerer, Nucl. Instr. and Meth. B 91 (1994) 601. [8] G.S. Hurst, C.E. Klots, Adv. Rad. Chem. 5 (1972) 1. [9] E. Elson, M. Rokni, J. Phys. D 29 (1996) 716. [10] H.H. Andersen, J.F. Ziegler, Hydrogen Stopping Powers and Ranges in all Elements, Pergamon Press, New York, 1977. [11] D.E. Grosjean, R.A. Baragiola, R.A. Vidal, W.L. Brown, Phys. Rev. B 56 (1997) 6975. [12] D.E. Grosjean, R.A. Baragiola, W.L. Brown, Phys. Rev. Lett. 74 (1995) 1474. [13] R.A. Baragiola, M. Shi, R.A. Vidal, C.A. Dukes, Phys. Rev. B 58 (1998) 13212. [14] J. Schou, in: R.A. Baragiola (Ed.), Ionization of Solids by Heavy Particles, Plenum Press, New York, 1992, p. 351. [15] D.E. Grosjean, Ph.D. Thesis, University of Virginia, 1996. [16] A. Kouchi, T. Kuroda, Jpn. J. Appl. Phys. 29 (1990) L807. [17] C.T. Reimann, Ph.D. dissertation, University of Virginia, 1986. [18] D.E. Grosjean, R.A. Baragiola, in: R.A. Baragiola (Ed.), Ionization of Solids by Heavy Particles, Plenum Press, New York, 1992, p. 381. [19] D.E. Grosjean, R.A. Baragiola, W.L. Brown, Nucl. Instr. and Meth. B 157 (1999) 116. [20] E.E. Koch, B. Raz, V. Saile, N. Schwentner, M. Skibowski, W. Steinmann, Jpn. J. Appl. Phys. (Suppl. e Pt. 2) (1974) 775. [21] R.A. Baragiola, in: J.W. Rabalais (Ed.), Low Energy IonSurface Interactions, Wiley, New York, 1994, Chapter 4. [22] Z. Ophir, B. Raz, J. Jortner, V. Saile, N. Schwentner, E.-E. Koch, M. Skibowski, W. Steinmann, J. Chem. Phys. 62 (1975) 650.
© Copyright 2026 Paperzz