A method and apparatus for using reflectometry for measuring properties of thin films or scattering structures on semiconductor work-pieces is disclosed. The techniques described herein include a method for using multiple relative reflectance measurements to overcome effects of contamination buildup. While the methods are particularly advantageous for vacuum ultraviolet (VUV) wavelengths, the methods are generally applicable to any wavelength range, and are advantageous in situations where stable reference samples are not available.
The techniques described herein relate to the field of optical metrology. Optical methods for control of thin film properties in semiconductor (and other) device manufacturing environments have become widely accepted. Particular advantages of using optical metrology include a high measurement throughput and the fact that optical measurements are typically nondestructive.
The most common optical metrology techniques are reflectometry and ellipsometry. Ellipsometry is generally regarded as consisting of a “richer” dataset, including a measurement of two quantities per wavelength/incident angle. On the other hand, reflectometers are more robust due to less complex hardware configuration, have faster measurements, and typically have a smaller footprint. Generally speaking, if both technologies are capable of solving a given metrology problem, the reflectometer is a more cost effective choice for a high-volume production environment.
Semiconductor device manufacturing is characterized by continually decreasing feature sizes. For example, in integrated circuit (IC) devices, the shrinking of the gate length has caused a corresponding decrease in the gate dielectric thickness to the order of 1 nm. Consequently, an important manufacturing issue is control of properties of ultra-thin films such as for example silicon oxynitrides or hafnium silicate films. Usually, control of film thickness is of primary importance, but control of film composition can be equally important, since both properties influence the final IC device performance.
This shrinking of device dimensions is where vacuum ultra-violet wavelength metrology comes in. It is well-known that a decrease in incident wavelength enhances sensitivity of the detected signal to minute changes in samples properties. An example is reflectance of ˜1-2 nm silicon dioxide films on silicon substrates.
Somewhat less known in the art is the ability to distinguish the effects of multiple parameters on the detected spectrum as the incident wavelength decreases below DUV regions. The ability to determine changes in film thickness and composition independently is enhanced in the VUV region, where many films exhibit very rich absorption spectra. Thus, using only DUV wavelengths, it may be possible to distinguish thickness or composition changes in an ultra-thin film, but not simultaneously. To do this with a reflectometer, one must move to VUV wavelengths, as illustrated in “Optical characterization of hafnium-based high-k dielectric films using vacuum ultraviolet reflectometry” (C. Rivas, XV International Conference on Vacuum Ultraviolet Radiation Physics, published 2007) for the case of HfxSi1-xO2, or in
Consequently, a VUV reflectometer has been disclosed in U.S. Pat. Nos. 7,026,626, 7,067,818, 7,126,131, and 7,271,394, the disclosures of which are expressly incorporated herein by reference in their entirety. This reflectometer has overcome the difficulties involved with VUV operation, and in particular incorporates an inert gas environment, as well as a real-time reference procedure to enhance stability.
A formidable obstacle to stable, reliable metrology at VUV wavelengths is a buildup of contaminants on optical surfaces during operation. This contaminant buildup is generally characteristic of all optical systems operating in the VUV region, and has also been observed in initial 157 nm lithographic systems, as seen in “Contamination rates of optical surface at 157 nm in the presence of hydrocarbon impurities”, (T. M. Bloomstein, V. Liverman, M. Rothschild, S. T. Palmacci, D. E. Hardy, and J. H. C. Sedlacek, Optical Microlithography XV, Proceedings of the SPIE, Vol. 4691, p. 709, published 2002) and “Contamination monitoring and control on ASML MS-VII 157 nm exposure tool”, (U. Okoroanyanwu, R. Gronheid, J. Coenen, J. Hermans, K. Ronse, Optical Microlithography XVII, Proceedings of the SPIE, Vol. 5377, p. 1695, published 2004), as well as space-based VUV experiments, such as “Optical Characterization of Molecular Contaminant Films”, (Photonics Tech Briefs, January 2007). For fab production environments, the contaminant is thought to involve a photodeposition process as VUV light interacts with siloxanes, hydrocarbons, and other compounds common in fab environments.
One method for calibrating a VUV reflectometer system that takes into account contaminant buildup has been disclosed in U.S. patent application Ser. No. 10/930,339 filed on Aug. 31, 2004, Ser. No. 11/418,827 filed May 5, 2006 (now U.S. Pat. No. 7,282,703), Ser. No. 11/418,846 filed May 5, 2006, and Ser. No. 11/789,686, filed on Apr. 25, 2007, which are all expressly incorporated herein by reference in their entirety. This method involves using a reflectance ratio, which is independent of incident system intensity, to measure properties of contaminant layers on the calibration samples. The measured contaminant layer properties are used to calculate the reflectance spectra of the calibration samples, which enables the determination of the incident intensity from the intensity reflected from the calibration sample. Once the incident intensity is known, an absolute reflectance can be measured for any subsequent sample.
The techniques disclosed herein provide an alternate method (distinct from the above mentioned U.S. patent application Ser. Nos. 10/930,339, 11/418,827, 11/418,846, and 11/789,686) of measurement using reflectometry that bypasses system calibration and utilizes multiple reflectance ratios, independent of system intensity, to simultaneously measure the properties of an unknown sample and the contaminant buildup on reference surfaces. The method can provide better long-term measurement stability for some ultra-thin film measurements. In one embodiment the reflectometer utilizes vacuum ultraviolet (VUV) wavelength reflectometry.
In one embodiment a method of measuring properties of an unknown sample is provided. The method may comprise providing a reflectometer and at least one reference sample, wherein the at least one reference sample is unstable under conditions in which the reflectometer is operated, collecting a set of data from the unknown sample and at least one reference sample, and utilizing a combination of the unknown sample and reference sample data that is independent of incident intensity to determine a property of the unknown sample, without calibrating incident reflectometer intensity.
In another embodiment a system for measuring properties of an unknown sample is provided. The system may comprise at least one reference sample and a reflectometer, configured for collecting a set of data from the unknown sample and the at least one reference sample wherein the at least one reference sample is unstable under conditions in which the reflectometer is operated. The system may also comprise a computer operating a software routine configured to utilize a combination of the unknown sample and reference sample data that is independent of incident intensity to determine a property of the unknown sample, without calibrating incident reflectometer intensity.
In another embodiment a system for measuring properties of an unknown sample, may comprise at least one reference sample and a reflectometer configured for collecting a set of data from the unknown sample and the at least one reference sample wherein the at least one reference sample is unstable under conditions in which the reflectometer is operated. The system may further comprise a computer operating a software routine that selectably operates in at least one of a plurality of measurement modes, the plurality of measurement modes including at least a first measurement mode and a second measurement mode. The first measurement mode is configured to utilize a combination of the unknown sample and reference sample data that is independent of incident intensity to determine a property of the unknown sample, without calibrating incident reflectometer intensity. The second measurement mode is configured to utilize the reference sample data in a manner that is independent of incident intensity to determine one or more properties of one or more reference pieces, thereby determining the incident intensity of the reflectometer, after which reflectance of unknown samples may be determined.
In yet another embodiment, a method of measuring properties of an unknown sample, may comprising providing a reflectometer and at least one reference sample, wherein the at least one reference sample is unstable under conditions in which the reflectometer is operated and collecting a set of data from the unknown sample and at least one reference sample. The method further comprises selectably operating the system in at least one of a plurality of measurement modes, the plurality of measurement modes including at least a first measurement mode and a second measurement mode. The first measurement mode is configured to utilize a combination of the unknown sample and reference sample data that is independent of incident intensity to determine a property of the unknown sample, without calibrating incident reflectometer intensity. The second measurement mode is configured to utilize the reference sample data in a manner that is independent of incident intensity to determine one or more properties of one or more reference pieces, thereby determining the incident intensity of the reflectometer, after which reflectance of unknown samples may be determined.
As described below, other features and variations can be implemented, if desired, and a related method can be utilized, as well.
It is noted that the appended drawings illustrate only exemplary embodiments of the techniques disclosed herein and are, therefore, not to be considered limiting of its scope, for the techniques disclosed herein may admit to other equally effective embodiments.
The techniques described herein provide a method and apparatus for reflectometry for measuring properties of thin films or scattering structures on semiconductor work-pieces. In one embodiment vacuum ultraviolet (VUV) wavelength (or lower) reflectometry may be utilized.
Reflectance or ellipsometric data from ultra-thin gate dielectrics are often modeled using an effective medium approximation (EMA), as shown in “The accurate determination of optical properties by ellipsometry”, (D. Aspnes, Handbook of Optical Constants of Solids Volume I, ed. D. Palik, Academic Press, San Diego, published 1998) that combines two or more constituent components using a single volumetric fraction parameter. Such an approximation is strictly valid when the film dimensions are much smaller than the incident wavelength. Additionally, most EMA approximations make further assumptions about the geometric arrangements of the component materials. For example, the Bruggeman EMA model assumes that the material is a composite mixture of distinct regions, with each region having its own well-defined set of optical properties.
Even if this assumption is not strictly met, for ultra-thin silicon oxynitrides or hafnium silicates, treatment with the Bruggeman EMA model adequately describes the reflectance or ellipsometric data. Additionally, the volume fraction correlates well with the dominant changes in composition, such as percent nitrogen in a silicon oxynitride film. Consequently, for the purposes of this disclosure silicon oxynitride films will be treated as a Bruggeman EMA mixture of SiOx and SixNy components, while hafnium silicate films are modeled as Bruggeman EMA mixtures of HfOx and SiOx components. It is understood that any suitable model could be used in place of the EMA model, and that many film systems could be similarly treated, not limited to silicon oxynitrides and hafnium silicates. Additionally, the methods discussed herein are not limited to just thin film structures, but can also include scattering structures. In particular, the unknown sample could include 1-D or 2-D grating structures, which could be modeled using rigorous diffraction algorithms such as the rigorous coupled wave method.
So described, a model of a silicon oxynitride film consists of the film thickness and EMA mixing fraction of oxide (SiOx) and nitride (SixNy) components. The oxide and nitride components themselves are described by their optical properties, index of refraction n and extinction coefficient k, as functions of wavelength. Given the film's thickness and EMA fraction, the reflectance can be calculated at any wavelength using standard thin film Fresnel equations, as described in “Spectroscopic Ellipsometry and Reflectometry—A User's Guide”, (H. Tompkins and W. McGahan, John Wiley & Sons Press, New York, published 1999). A metrology measurement is usually performed on an unknown sample by measuring the reflectance of the sample and performing, for example, a Levenberg-Marquardt optimization, as shown in “Numerical Recipes in C (2nd Edition)”, (W. H. Press, S. A. Teukolsky, W. T. Vetterling, and B. P. Flanery, Cambridge University Press, Cambridge 1992), with the film thickness and EMA fraction treated as optimization parameters.
A production reflectometer typically does not directly measure the incident intensity (as provided from the source or the actual incident intensity on the measured sample), which is required to measure reflectance of an unknown sample, but instead will determine the incident intensity from the reflected intensity of a known calibration sample. The incident intensity can change over time due to variations in source intensity, environment (temperature and humidity), drift in optical alignment, and the like. A known calibration sample, often a silicon wafer with its native oxide, is first measured, and its reflectance assumed to be known. The incident intensity is determined by dividing the intensity reflected from the calibration sample by its assumed reflectance. The reflectance for an unknown sample is then determined by measuring the intensity reflected from the sample and dividing by the incident intensity.
Obviously, such a calibration method depends on the stability of the calibration sample. In VUV regions, stability is not guaranteed, since small differences in native oxide thicknesses are magnified in that region. In addition, the previously mentioned contamination that occurs confounds the stability of the calibration sample, since the photodeposition occurs every time the calibration sample is measured.
One way to deal with this problem has already been discussed with reference to the calibration techniques disclosed in the U.S. patent applications disclosed above. A measurement of reflectance for a thick (˜1000 Å) silicon dioxide on silicon substrate sample relative to a thin oxide sample (typically native silicon dioxide on silicon substrate) is independent of incident intensity, and can be used along with a regression technique to determine both the native oxide thickness as well as contaminant thickness on the thin oxide sample. The result of this analysis is used to calculate the reflectance of the native oxide calibration sample, Rc, which is used in combination with the intensity reflected from the calibration sample, Ic, to determine the incident intensity via I0=Ic/Rc. The reflectance of an unknown sample, Rs, can then be determined from its reflected intensity, Is, by Rs=Is/I0.
Disclosed herein is an alternate method for measuring thin film properties that uses reflectance ratios to bypass the system calibration completely. As used herein, the term “calibration” refers to the determination of incident intensity, I0. The method disclosed herein can lead to better long-term performance for some thin film systems, one example being thickness and concentration in ultra-thin silicon oxynitride.
One embodiment of the technique involves measuring the reflected intensity of three samples:
Sample 1—native oxide/Si reference piece,
Sample 2—˜1000 Å SiO2/Si reference piece,
Sample 3—the unknown sample (for example an oxynitride sample).
The unknown sample will normally consist of a standard silicon substrate of 150 mm, 200 mm, 300 mm, or 450 mm diameter with a deposited film stack. As shown in
The unknown sample is loaded into the system 301, and reflected intensities, I1, I2, and I3, are measured for Sample 1, Sample 2, and Sample 3 (for example Sample 1 being pad 1303 and Sample 2 being Pad 2304), respectively. Two ratios are formed:
I2/I1=R2/R1, and
I2/I3=R2/R3. Eq. 1
The equalities are true as long as I0 has not changed significantly during the measurement of the reflected intensities. I0 is usually stable for at least several minutes, meaning that several locations on Sample 3 could be measured and use the same I1 and I2 in the ratios. I1 and I2 need only be measured with whatever frequency a standard system calibration would normally be performed. An additional embodiment might incorporate the current method and the calibration methods disclosed in U.S. patent application Ser. Nos. 10/930,339, 11/418,827, 11/418,846, and 11/789,686 simultaneously, which are expressly incorporated herein by reference in their entirety. The same pads 303, 304 can be used for calibration of I0 or used as described in the current disclosure, depending on the particular measurement being done. Other ratio combinations can obviously be used as well. As described in more detail herein, the techniques provided herein are particularly advantageous in that the reference pieces need not be stable under the conditions that the reflectometer operates. Thus, reference pieces that, for example, are not stable in the VUV regime may still be utilized. For example, even though the contaminate build-up which may affect a VUV measurement may occur on the reference piece, rendering the reference piece unstable in VUV conditions, the reference piece is still suitable for the techniques described herein.
Thus, during operation instability of the reference sample may relate to the surface of the reference sample changing over time, such as for example, but not limited to contaminant buildup, airborne molecular contaminant removal, growth of films, other time dependent changes, etc. In addition, instability of the reference sample may also relate to inherent non-uniformities of the reference sample (across a given sample or from sample to sample), that may result, for example, from the sample production techniques. For example, bare thicknesses, native oxides, interface properties, surface roughness conditions, etc. may all initially vary across a sample and from sample to sample. Thus these may not change over time, however, from sample to sample or across a sample these conditions may be considered unstable. Thus, as used herein, instability may refer to both time dependent and non-time dependent variations.
The reason for framing the problem in terms of reflectance ratios instead of intensity ratios is that reflectance can be calculated in a straight-forward manner using standard thin film algorithms, as described in “Spectroscopic Ellipsometry and Reflectometry—A User's Guide”, (H. Tompkins and W. McGahan, John Wiley & Sons Press, New York, published 1999), along with values for the optical properties and thicknesses of the various films. For instance, if the SiO2 and Si optical properties are known and SiO2 thicknesses provided, the reflectances R1 and R2 can be calculated. Going further, if a measured R2/R1 is available, standard regression techniques can be used to optimize the thicknesses for the SiO2 layers, giving a measurement for both thicknesses, as long as the parameters are sufficiently decoupled. In principle, the optical properties of the SiO2 and Si layers could be determined as well, normally using parameterized dispersion models such as the Tauc-Lorentz model, as shown in “Parameterization of the optical functions of amorphous materials in the interband region”, (G. E. Jellison and F. A. Modine, Appl. Phys. Lett., Vol. 69 (1996), p. 371).
In one embodiment, the techniques disclosed herein may be utilized in combination with the techniques disclosed in U.S. patent application Ser. Nos. 10/930,339, 11/418,827, 11/418,846, and 11/789,686. For example, a measurement software routine may be selectable between differing modes, a first mode being the techniques described herein and a second mode being the techniques described in the above mentioned U.S. patent applications. Thus, the system may selectably operate (automatically or based on user input) in at least one of a plurality of measurement modes, the plurality of measurement modes including at least a first measurement mode and a second measurement mode. The first measurement mode may be configured to utilize a combination of the unknown sample and reference sample data that is independent of incident intensity to determine a property of the unknown sample, without calibrating incident reflectometer intensity as described herein in more detail. The second measurement mode may be configured to utilize the reference sample data in a manner that is independent of incident intensity to determine one or more properties of one or more reference pieces, thereby determining the incident intensity of the reflectometer, after which reflectance of unknown samples may be determined such as described in the above referenced U.S. patent application Ser. Nos. 10/930,339, 11/418,827, 11/418,846, and 11/789,686.
The current method disclosed herein involves a regression analysis of both ratios in Equation 1 simultaneously. Basically, the parameters in the modeled ratios are optimized until both calculated ratios R2/R1 and R2/R3 agree with their corresponding measured ratios. One way to do the optimization is to use a version of the Levenberg-Marquardt routine generalized to multiple sample analysis. In such cases, the nonlinear chi-square merit function could be written as:
where the σi and σj are estimates of the standard error for each measured data point. The notation on the summation limits, N21 and N23, illustrates that the data range for the two datasets does not have to be the same.
The results of the optimization procedure are the measured parameters for all three samples. The reference pads 303, 304 will ordinarily undergo contaminant buildup due to extended use in the system, and so a contaminant layer will be included in the reflectance models for the reference pieces. Thus the result of the analysis include the thicknesses of both oxide (native and ˜1000 Å) thicknesses, thickness of contaminant in both reference pieces, and all of the same regression parameters for the unknown sample that would have been varied during a standard optical measurement, such as film thicknesses and optical properties (via the EMA fraction in the ultra-thin SiON case). The redundancy provided by having sample 2 involved in both datasets helps constrain the problem and yield better results for the unknown sample.
A series of simulations will follow to illustrate the usefulness of the method in the case of ultra-thin silicon oxynitride (SiON) gate films, which serve the role of Sample 3. For the purposes of this description, the optical properties n and k of the silicon native oxide, silicon dioxide (SiO2), silicon (Si), Silicon Nitride (Si3N4), and contaminant are regarded as known. The optical values were taken from a variety of literature sources or determined through other measurements. In particular, the contaminant optical properties could be determined using a controlled experiment similar to the methods disclosed in U.S. patent application Ser. No. 11/789,686, which is expressly incorporated herein by reference in its entirety. The SiON films are treated as Bruggeman EMA films composed of SiO2 and Si3N4. Aside from the optical properties, a full description of the ultra-thin oxynitride film is considered to be a specification of its thickness and EMA volume fraction. The volume fraction can be correlated to nitrogen content in the films, which is an important process control parameter along with the film thickness. In the present example, treatment of explicit interface layers and surface and interface roughness are ignored, but such effects could also be included in the models, if desired.
Comparisons of
If Sample 2 did not change, the reflectance of Sample 3 could be extracted directly from the ratios in
An example of a simultaneous multiple ratio fit of a SiON film is shown in
In some embodiments, the underlying oxide and possibly even interface regions of the reference pieces can be pre-characterized using a ratio measurement or other means, and those parameters fixed to the pre-characterized values during normal measurements. After such pre-characterization, only the contaminant layer on the reference pieces and properties of the unknown sample would be treated as unknowns in multiple ratio measurements. A further generalization might treat multiple contaminant layers, due to different types of photodeposited contaminants, or to distinguish the effects of photocontaminants from airborne molecular contaminants, which are known to absorb on wafer surfaces in normal fab environments.
An experiment demonstrating the effectiveness of the disclosed method consisted of 5 SiON samples, each measured at 5 measurement sites/wafer per day for 10 days. The measurement sites were slightly changed locally on the SiON samples each day to prevent photocontaminant buildup on the SiON samples themselves from affecting the results. The results for standard deviation of the 10 day measurements for each site are a metric of the stability for the SiON measurement. Photocontamination was allowed to occur on the two reference pieces. These conditions simulate the way the SiON process would be monitored in a fab production environment—i.e. each SiON sample would only be measured once, while the reference pieces would likely be used for many measurements, and consequently undergo the photocontamination process.
Each of the 250 measurements consists of 3 reflected intensities—one each from the two reference pads and one from the SiON measurement site. The data was first analyzed by calibrating I0 using a dual pad calibration procedure with the two reference pads (similar to methods discussed in patent application Ser. Nos. 11/418,827, 11/418,846, and 11/789,686), and the thickness and percent nitrogen (via the EMA fraction) were analyzed using an EMA model and standard reflectance analysis. The 10-day standard deviation was computed for thickness and percent nitrogen for each site of each sample. The data was then recomputed using the multiple ratio analysis method described in this disclosure. The same optical models were used for reference and SiON materials for the recomputed data. The current method resulted in an average improvement in the 10-day standard deviation of approximately 37% for thickness and 26% for nitrogen percent.
In practice, similar stability enhancements can also be achieved through further optimization of the contaminant properties, or even alternate choices in calibration materials. The significance of this study lies in the fact that a stability enhancement was achieved using the disclosed method with the same reference pads, without further optimization of the reference or SiON material descriptions.
It is noted that the SiON description used for the analysis, in particular the oxide and nitride component optical properties, was generated using standard reflectance measurements by calibrating I0. The good fit in
As previously mentioned, one particularly attractive feature of the current method is that it may be combined with a multiple pad calibration procedure using the same or even additional reference pads on a single measurement platform. The multiple ratio method used may depend on the particular film measurement being done. In other words, whether or not to calibrate I0 and generate reflectance or to use a multiple ratio calculation instead, or even which multiple ratio method to use, could be recipe dependent.
It is noted that the current method has been illustrated using a specific example, and one will recognize that many variations on the current procedure are possible, while still remaining within the scope of this disclosure. Additionally, the method described herein has been described for use with VUV reflectometer measurements, for which it is particularly advantageous, but the concept is valid for reflectance measurements carried out at any wavelength. The method described herein has also described a moving stage and sample holder, and can obviously be conceived to include automation via robotic wafer handling, fab interface software, and any number of other common modifications of optical metrology equipment for manufacturing environments.
Further modifications and alternative embodiments of the techniques disclosed herein will be apparent to those skilled in the art in view of this description. It will be recognized, therefore, that the techniques disclosed herein are not limited by these example arrangements. Accordingly, this description is to be construed as illustrative only and is for the purpose of teaching those skilled in the art the manner of carrying out the techniques disclosed herein. It is to be understood that the forms of the techniques disclosed herein shown and described are to be taken as the presently preferred embodiments. Various changes may be made in the implementations and architectures. For example, equivalent elements may be substituted for those illustrated and described herein, and certain features of the techniques disclosed herein may be utilized independently of the use of other features, all as would be apparent to one skilled in the art after having the benefit of this description of the techniques disclosed herein.
This application is a continuation of U.S. patent application Ser. No. 12/072,878 filed on Feb. 28, 2008 now abandoned.
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