CHARACTERISATION OF CORONA-CHARGED OXIDE-PASSIVATED SILICON Simeon C. Baker-Finch and Keith R. McIntosh Centre for Sustainable Energy Systems, The Australian National University, Canberra ACT 0200, AUSTRALIA Email: simeon.baker-finch@anu.edu.au ABSTRACT Corona charge is used in the photovoltaic industry to help distinguish surface and bulk recombination. In this study, the deposition of corona charge on Si-SiO2 structures was investigated. The magnitude and polarity of the charge is directly measured with a Kelvin probe, while its effect upon surface recombination is inferred from the measurement of transient photoconductance. Corona charge is deposited on 5 Ω cm n-type Si passivated with a 20 nm thick oxide at a constant rate of 4 µC cm-2 min-1 until charge saturation is observed. The charge density observed at the saturation point is consistent with the onset of oxide breakdown. The oxide breakdown field is 5.5 MV cm-1 for positive charge and 11.9 MV cm-1 for negative charge. Transient photoconductance measurements indicate that the surface recombination is affected by the corona charge in two ways: (i) the recombination decreases due to the repulsion of like-polarity carriers from the Si–SiO2 interface, and (ii) the recombination increases due to interface damage induced by the charge. These two effects were distinguished by removing the surface charge with isopropanol. These results are consistent with those presented by Jin et al. (2007). INTRODUCTION Corona charging is used in various fields of applied electrostatics (Dascalescu et al. 1999), as a tool for charging electrets (Sessler 1987), for xerography (Sessler 1987, Günther & Xia 1993), and as a method to maintain device cleanliness (Ohmi et al. 1994). In the field of photovoltaics research, with few exceptions, the use of corona charge has been limited to novel characterisation methods involving the use of the charge as a non-permanent, non-invasive means of surface passivation (Schöfthaler et al. 1994, Schröder 2002). A surface concentration of corona-deposited charges on an oxidised Si surface is used to influence the carrier concentrations and recombination velocity in the Si near the Si-SiO2 interface. The corona charging process is one that depends on the use of an inhomogeneous electric field in air to produce a discharge of ions that are deposited on the surface of a sample at atmospheric pressure (Sessler 1987). It involves the placement of the sample on a grounded metal table beneath a needle to which a potential of several kilovolts is applied. The resultant high electric field in the vicinity of the needle tip ionises surrounding air molecules (Schöfthaler et al. 1994, Glunz et al. 1999). Depending on the polarity of the voltage applied at the source, the predominant ionic species are CO3or H3O+ (Schröder 2002). The electric field forces the ionised air molecules along the electric field lines toward the sample (Schöfthaler et al. 1994, Schröder 2002). ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh Corona charging is generally considered to be a non-destructive method for passivation of Si surfaces. Recently, however, Stesmans and Afanas’ev (2004) and Jin et al. (2007) have concluded that damage in the form of defects at the Si-SiO2 interface is incurred during the process. In this work, accurate Kelvin probe techniques are used to characterise the magnitude and lateral uniformity of both positive and negative corona charge as deposited on a thermal oxide of Si. Photoconductivity decay (PCD) techniques are used to determine the influence of corona charging upon the passivation of the Si surface, which itself depends upon the density of interface defects possibly incurred during charging, as well as the extent to which the charge deposited on the oxide surface repels carriers of likepolarity in the Si away from the Si-SiO2 interface. ACCURATE KELVIN PROBE MEASUREMENT OF CHARGE DENSITY ON OXIDE SURFACE The modern Kelvin probe is a non-contact, non-destructive device that employs a vibrating capacitor technique to measure the ‘work function difference’ between a vibrating tip and a conducting sample (Baikie and Estrup 1998). The vibrating tip is a reference surface that forms the counter electrode of a parallel plate capacitor, whose other plate is the sample surface. As the tip vibrates, electrons flow back and forth in the external circuit as an electric field is induced between the capacitor plates. A voltage, termed the applied or backing potential, denoted Va, is applied to the probe head in order to compensate for this external electric field. Va is the negative of the contact potential, Vc. For accurate derivation of surface charge density Qs from Kelvin probe measurement, the contributions of charges located at the Si-SiO2 interface, in the oxide, as well as on the surface of the oxide toward a profile of electric potential must be considered (see Fig. 1). This is particularly relevant when attempting to harness the increasing accuracy of Kelvin probe technologies. Previous publications in the field of photovoltaics (eg. Glunz et al. 1999) have neglected the contributions of all charges other than Qs, so that Qs = Vc ε ox d ox ……………………………………………………….. (1) where dox is the thickness of the oxide and εox is the dielectric permittivity of the oxide. In this work, all contributors to the profile of electric potential, Ψ(x), shown in Fig. 1 are included in the analysis. That is, we define ⎛ d f / 2 ⎞⎞ ε ⎛ ⎟⎟ ⎟ …………………………... Qs = ox ⎜⎜Vc − φ ms − ΨSi − Q f ⎜⎜ ⎟ d ox ⎝ ε ⎝ ox ⎠ ⎠ (2) in dark conditions, and where ΨSi is the potential in the Si at the Si-SiO2 interface, Qf is a density of fixed charge in the oxide, located at a distance df/2 from the Si-SiO2 interface and φms is the metal-silicon work function difference defined by Sze (2002) as φ ms = φ m − χ + (Ec − E f ,Si ) …………………………………….… (3) [ ] where φm is the work function of the Kelvin probe metal tip, χ is the electron affinity of Si, Ec is the conduction band energy level far from the Si surface, and Ef, Si is the Si Fermi level. ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh φms can be determined from known values and semiconductor properties. In the following experimental work, φm is assumed to be 5.1 eV. Values available in the literature range between 4.83 and 5.45 eV (Sachtler et al. 1966, Rivière 1966). Also, the quantity of Qf and an approximation of df are often known (Aberle 1999). Depending on the processing conditions, the value of Qf is between 5×1010 and 2×1011 cm-2; usually, df ≤ 2 nm (Aberle 1999). Girisch et al. (1988) describe a means of numerical calculation of ΨSi assuming that the electron and hole quasi-Fermi levels are constant throughout the surface space charge region. Note that with changing Qs, ΨSi is non-constant. The solution of Equation 2 for known (measured) Vc requires the iteration of Qs and parallel calculation of ΨSi for each iteration. As the value of Qs approaches the solution, the potential on the Kelvin probe tip (Qcontact in Fig. 1) converges to zero. In the following experimental work, a satisfactory value of Qs is found when |Qcontact| is less than 1 × 1015 cm-2. The technique proposed here is required for accurate estimation of Qs for Vc > -0.3 V. At values of Vc between -0.3 V and 1 V (-0.1 < Qs < 0.03 μC cm-2), ΨSi varies nonlinearly, and its magnitude is non-negligible, so the simplified relationship is not valid. Furthermore, Qs is overestimated for Vc > 1 V (a constant offset of ~0.3 μC cm-2 between the two solutions is observed). Fig. 1: The energy bands, electric field and electric potential profile in Si, oxide, probe tip system during Kelvin probe measurement. The potential gradient across the air gap is flat when Va compensates for the external electric field generated by the combination of charges QSi, Qit, Qf and Qs. ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh MAGNITUDE AND UNIFORMITY OF CORONA CHARGE ON OXIDEPASSIVATED SILICON Sample Preparation and Procedure The samples were fabricated from 4-5 Ω cm n-type Si wafers. They underwent the following processing steps: TMAH etch for 20 minutes at 85 °C; RCA clean; dry oxidation for 40 minutes in O2 at 950 °C; 30 minute in-situ anneal in N2 at the same temperature (resultant oxide thickness of 15 - 25 nm); anneal in forming gas at 400 degrees for 30 minutes. Wafers were cleaved into quarters. The thin layer of SiO2 was removed from the rear surface of the silicon via HF fuming and ~80 nm of aluminium was evaporated onto the bare Si surface. Corona charging was carried out with a conventional setup. A voltage of ±10 kV was applied to the source needle. The sample was left in the chamber for a period of time ranging from zero seconds to five minutes - the oxide surface became charged with a layer of static charge. In order to measure the uniformity of this layer of deposited charge across the surface of the sample, five test points were chosen on the sample surface, each at a distance of 0 to 25 mm from the sample centroid. The sample centroid was aligned directly below the tip of the corona needle. After each interval, a Kelvin probe was used to make 100 consecutive measurements of Va (thus Vc), at five test points. The mean was taken for the remaining analysis. The value of surface charge density Qs was determined for each value of Vc according to the calculation process described above. Qit was calculated from the integral of states across the band gap, where all states (a density of 5×1010 cm-2 eV-1) were donor-like, and the energy-dependent capture cross sections of electrons and holes were those of Aberle et al. (1992). The resultant value of Qit was 2×10-8 C cm-2. Note that the calculation process is fairly insensitive to this charge. Qf was set at 5 × 1010 cm-2 and df at 2 nm. Results and Discussion Fig. 2 illustrates the measured values of Qs at each of five measurement points for a range of corona charging times and for both charge polarities. The mean, minimum and maximum of these five measurements is summarised as a function of time in Fig. 3. Fig. 2: Measured Qs values at various distances from the centroid. The sample was subject to corona charging at +10 kV (left) or -10 kV (right) potential for the period of time shown. Lines represent the parabolic least squares fit curve for each data set. ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh Fig. 3: Mean (solid line), maximum and minimum (dashed lines) Qs as a function of corona charging time for both positive and negative corona needle potentials. A quantitative summary of the observed uniformity of deposited surface charge is provided in Fig. 4. Percentage nonuniformity of surface charge (∆Qs) is defined as ⎛Q − Qs ,min ⎞ ⎟ ……………………………………… (4) ΔQs = 100⎜⎜ s ,max ⎟ Q s , max ⎠ ⎝ where Qs, max and Qs, min are the maximum and minimum charge densities, respectively, of the values of surface charge measured across the sample after each charging interval. Fig. 4: Charge nonuniformity, ∆Qs, for a range of corona charging intervals. Corona arrangements that do not feature a gate electrode (such as the one used in this work) are generally expected to deliver a current of ionised air particles with a bellshaped distribution (Sessler 1987). This work suggests that after one minute of ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh charging, uniformity improves so that no point within a two centre radius of the sample centroid is characterised by a surface charge that is more than 10% different from any other point within that radius. Regardless of charge polarity, a limit is observed on the maximum magnitude of surface charge that can be deposited using the corona discharge chamber (as shown in Fig. 3). For positive charge, this limit is around 1.9 µC cm-2, and is observed across the sample after 30-40 seconds charging time. In the negative case, the limit is around 4.1 µC cm-2, and is reached after 60 seconds charging time. After the limit is reached, no more surface charge can be deposited by corona charging. As a result, for longer charging time, the initially bell-shaped/parabolic distribution of charge becomes more uniform as the outside areas of the sample (where charge deposition rate is less) reach the charge limit, and ∆Qs decreases (see Fig. 4). The observed charge limit is attributed to oxide breakdown, which occurs at field strengths of between 5 and 15 MV cm-1 (O’Shea et al. 1995, Weinberg et al. 1976). At the observed limit of positive charging, the field appearing across a 20 nm thick oxide is approximately 5.5 MV cm-1. The equivalent field for the negative charge limit has a magnitude of approximately 11.9 MV cm-1. It is plausible that the oxide breakdown field differs depending on surface charge polarity. Note that a median oxide thickness of 20 nm was assumed in order to calculate Qs and to approximate the breakdown field strengths (the processing steps involved in the sample preparation may have led to a range of oxide thicknesses of between 15 and 25 nm). The mean rate of charge deposition is approximately 4 µC cm-2 min-1 during the prebreakdown linear phase for both positive and negative charging. Further investigation of the limitation on deposited charge for samples with a range of thicknesses is necessary to confirm that oxide breakdown is responsible for the prohibition of further charge deposition. CORONA-DEPOSITED SURFACE CHARGE AND EFFECTIVE CARRIER LIFETIME Sample Preparation and Procedure Samples were prepared as for the experimental work described above with the following difference: the rear oxide was not removed via HF fuming and the rear surface was not coated with Al. Two identical samples were subjected to an identical series of charge intervals under opposite corona needle potentials. After each charging interval, a measurement of effective lifetime, τeff, was achieved using the PCD technique (Kane and Swanson 1985). Finally, IPA solution was used to remove the surface charge from the samples (Ohmi et al. 1994), and PCD measurement was once again undertaken. The PCD or transient lifetime technique involves the measurement of the decay of lightgenerated electron-hole pairs as a function of time. The technique used in this work is described by Kane and Swanson (1985) and involves the measurement of sheet photoconductivity over time by a contactless method. It employs the principle of inductive coupling - the time-varying sheet conductivity is transformed into an excess carrier density. Then, τeff is determined ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh τ eff (Δn ) = − Δn . ……………………………………………….. (5) dΔn / dt This effective lifetime represents the fundamental mode of carrier decay, and depends upon two separate components (Sproul 1994) 1 1 1 = + , ……………………………………………………. (6) τ eff τb τs where τb is the carrier lifetime in the bulk, and τs is the carrier lifetime near the surface. In this work, τb is assumed to remain constant, and variation of τeff is attributed to surface factors (ie. density of interface defects, carrier concentrations in the Si near the Si-SiO2 interface). During experiment, τeff is determined at ∆n = 1×1015 cm-2. Results and Discussion Positive and negative corona needle potentials proved to influence τeff differently, in accordance with Fig. 5. The lifetime improvement gained in the first stage of corona charging is lost more rapidly in the case of negative applied charge. Furthermore, once rinsed with IPA solution to remove all surface charge, a previously negatively-charged sample displays a significantly decreased τeff when compared to its initial charge-free value. A previously positively-charged sample does not experience such a large lifetime reduction. Jin et al. (2007) report a similar observation. Figure 5 indicates that for short enough charging intervals, lifetime improvement via field-effect passivation of the Si surfaces is achieved regardless of charge polarity. With an oxide thickness of 50 nm on 10-23 Ω cm p-type samples with a 400 Ω/□ surface-passivating phosphorus diffusion, Jin et al. (2007) did not observe improvement in τeff by negative charging until charging interval was increased to around 60 seconds. Given that the oxide used in this work is considerably thinner, and that there is no surface diffusion, it is reasonable that improvement in τeff is observed immediately (ie. for a charging time below 5 s). Indeed, small amounts of surface charge are likely to have a more pronounced impact on the samples used here. Fig. 5: τeff dependence upon corona charging time. ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh Certainly, after charging and charge removal with IPA solution, τeff is decreased when compared to initial (zero charging time) τeff values. Permanent damage at the Si-SiO2 interface (as observed by Jin et al. (2007)) is suspected. Further work will consider the impact of oxide breakdown (as observed during the charge characterisation process described above) upon the generation of interface defects during corona charging. SYNTHESIS OF KELVIN PROBE AND PCD RESULTS The results of Kelvin probe characterisation are synthesised with the photoconductivity decay measurements in Fig 6. The τeff measured by PCD after a certain period of corona charging is plotted against the Qs measured by the Kelvin probe after the same charging period. The relationship between Qs and τeff is compared to the ideal ‘U curve’ relationship between surface charge and τeff. The ideal curve was derived via numerical calculation of ΨSi (following the technique of Girisch et al. (1988) as described above) for varying Qs and with the constant input values for Qit, Qf and df defined in the experimental procedure for charge quantification. Fig. 6: Synthesis of PCD and Kelvin probe results for positive and negative corona charging as compared to the ideal relationship. Damage incurred at the interface during corona charging is thought to account for the degradation in carrier lifetime observed for larger values of Qs. Particularly once dielectric breakdown has been reached, interface damage leads to rapid lifetime decay. This is particularly noticeable for negative charging in Figure 6. Lifetime degradation may indeed be attributable to permanent damage at the Si-SiO2 interface incurred during oxide breakdown. ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh CONCLUSIONS For 5 Ω cm n-type samples with an oxide thickness of ~20 nm, a surface charge density of 2 µC cm-2 (equivalent to a breakdown field of 5.5 MV cm–1) or 4 µC cm-2 (equivalent to a breakdown field of 11.9 MV cm-1) is the highest surface voltage achieved by positive or negative corona charging, respectively. The magnitude and lateral uniformity of deposited charge was accurately determined using a Kelvin probe coupled with an appropriate calculation of the profile of the electric potential in the Si and oxide. Charge deposited in a single-needle corona discharge chamber is more uniform for charge intervals of increased length. PCD measurements indicate that surface recombination decreases when a small amount of corona charge is deposited onto the oxide surface. For longer charging intervals, the recombination increases due to interface damage induced during charging. Interface damage is more severe during negative charging. Processes occurring during the dielectric breakdown of SiO2 on oxide-passivated n-type silicon may be responsible for permanent damage occurring at the Si-SiO2 interface. ACKNOWLEDGEMENTS The authors would like to thank Mr Andrew Thomson, Ms Wendy Jellet and Ms Nina De Caritat for regular discussion and assistance in sample preparation. REFERENCES Aberle, A.G. (1999). Crystalline Silicon Solar Cells: Advanced Surface Passivation and Analysis. Centre for Photovoltaic Engineering, University of New South Wales. Baikie, I.D and Estrup, P.J. (1998) Low cost PC based scanning Kelvin probe. Review of Scientific Instruments, 69(11), 3902-3907. Dascalescu, L., Samuila, A., Rafiriou, D., Iuga, A and Morar, R. (1999). Multipleneedle corona electrodes for electrostatic processes application. IEEE Transactions on Industry Applications, 35(3), 543-548. Girisch, R.B, Mertens, R.P and De Keersmaecker, R.F. (1988). Determination of SiSiO2 interface recombination parameters using a gate-controlled point-junction diode under illumination. IEEE Transactions On Electronic Devices, 35(2), 203-222. Glunz, S., Biro, W. Rein, S. and Warta, W. (1999) Field-effect passivation of the SiO2Si interface. Journal of Applied Physics, 86(1), 683-691. Günther P. and Xia, Z. (1993). Transport of detrapped charges in thermally wet grown SiO2 electrets. Journal of Applied Physics, 74, 7269. Jin, H., Weber, K.J., Dang, N.C. and Jellet, W.E. (2007) Defect generation at the SiSiO2 interface following corona charging. Applied Physics Letters, 90, 262109. Kane, D. and Swanson, R. (1985). Measurement of the emitter saturation current by a contactless photoconductivity decay method. In Proceedings of the 18th IEEE Photovoltaic Specialists Conference, 578-583. Ohmi, T., Sudoh, S. and Mishima, H. (1994). Static charge removal with IPA solution. IEEE Transactions on Semiconductor Manufacturing, 7(4), 440-446. ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre Simeon C. Baker-Finch and Keith R. McIntosh O’Shea, S.J., Atta, R.M, Murrell, M.P. and Welland, M.E. (1995). Conducting atomic force microscopy study of silicon dioxide breakdown. Journal of Vacuum Science & Technology B: Microelectronics and Nanometer Structures, 13(5), 1945-1952. Rivière, J.C. (1966). The work function of gold. Applied Physics Letters, 8(7), 172. Sachtler, W.m Dorgelo, G. and Holscher, A. (1966). The work function of gold. Surface Science, 5, 221-229. Schöfthaler, M., Brendel, R., Langguth, G. and Werner, J. (1994). High-quality surface passivation by corona-charged oxides for semiconductor surface characterisation. In Proceedings of First WCPEC, Hawaii, 1509-1512. Schröder, D. K. (2002). Contactless surface charge semiconductor characterization. Materials Science and Engineering, B91-92, 196-210. Sessler, G. (1987). Introduction. Topics in Applied Physics Volume 33: Electrets. pp 110. Springer-Verlag. Sproul, A. (1994) Dimensionless solution of the equation describing the effect of surface recombination on carrier decay in semiconductors. Journal of Applied Physics, 76(5), 2851-2854. Stesmans, A. and Afanas’ev, V.V. (2004). Corona charging damage on thermal Si/SiO2 structures with nm-thick oxides revealed by electron spin resonance. Microelectronic Engineering, 72, 55-60. Sze, S. (2002). Semiconductor Devices: Physics and Technology (2nd ed). John Wiley and Sons, Inc. Warta, W., Biro, D. and Glunz, S.W. (1998). The effect of surface charges on the recombination at Si-SiO2 interfaces. In Proceedings of 2nd World Conference and Exhibition on Photovoltaic Solar Energy conversion, Vienna, 100-103. Weinberg, Z.A., Johnson, W.C. and Lampert, M.A. (1976) High-field transport in SiO2 on silicon induced by corona charging of the unmetallized surface. Journal of Applied Physics, 47(1), 248-255. BRIEF BIOGRAPHY OF PRESENTER Simeon is a final year student of Engineering and Arts at the Australian National University. He has just completed his honours thesis under the supervision of Dr Keith McIntosh at the Centre for Sustainable Energy Systems. This work involved the inclusion of corona charge for improved surface passivation of photovoltaic solar cells. ISES-AP - 3rd International Solar Energy Society Conference – Asia Pacific Region (ISES-AP-08) Incorporating the 46th ANZSES Conference 25-28 November 2008 Sydney Convention & Exhibition Centre