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WO2002082064A1 - Systeme de detection de defauts ameliore - Google Patents

Systeme de detection de defauts ameliore Download PDF

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Publication number
WO2002082064A1
WO2002082064A1 PCT/US2002/010783 US0210783W WO02082064A1 WO 2002082064 A1 WO2002082064 A1 WO 2002082064A1 US 0210783 W US0210783 W US 0210783W WO 02082064 A1 WO02082064 A1 WO 02082064A1
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WO
WIPO (PCT)
Prior art keywords
radiation
scattered
collected
channels
line
Prior art date
Legal status (The legal status is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the status listed.)
Ceased
Application number
PCT/US2002/010783
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English (en)
Inventor
Mehdi Vaez-Iravani
Jeffrey Alan Rzepiela
Carl Treadwell
Andrew Zeng
Robert Fiordalice
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KLA Corp
Original Assignee
KLA Tencor Corp
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Filing date
Publication date
Priority claimed from US09/828,269 external-priority patent/US6538730B2/en
Application filed by KLA Tencor Corp filed Critical KLA Tencor Corp
Priority to JP2002579784A priority Critical patent/JP2004524538A/ja
Publication of WO2002082064A1 publication Critical patent/WO2002082064A1/fr
Anticipated expiration legal-status Critical
Ceased legal-status Critical Current

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    • GPHYSICS
    • G01MEASURING; TESTING
    • G01NINVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
    • G01N21/00Investigating or analysing materials by the use of optical means, i.e. using sub-millimetre waves, infrared, visible or ultraviolet light
    • G01N21/17Systems in which incident light is modified in accordance with the properties of the material investigated
    • G01N21/47Scattering, i.e. diffuse reflection
    • GPHYSICS
    • G01MEASURING; TESTING
    • G01NINVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
    • G01N21/00Investigating or analysing materials by the use of optical means, i.e. using sub-millimetre waves, infrared, visible or ultraviolet light
    • G01N21/84Systems specially adapted for particular applications
    • G01N21/88Investigating the presence of flaws or contamination
    • G01N21/95Investigating the presence of flaws or contamination characterised by the material or shape of the object to be examined
    • G01N21/9501Semiconductor wafers
    • GPHYSICS
    • G01MEASURING; TESTING
    • G01NINVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
    • G01N21/00Investigating or analysing materials by the use of optical means, i.e. using sub-millimetre waves, infrared, visible or ultraviolet light
    • G01N21/84Systems specially adapted for particular applications
    • G01N21/88Investigating the presence of flaws or contamination
    • G01N21/8806Specially adapted optical and illumination features
    • G01N2021/8822Dark field detection
    • GPHYSICS
    • G01MEASURING; TESTING
    • G01NINVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
    • G01N21/00Investigating or analysing materials by the use of optical means, i.e. using sub-millimetre waves, infrared, visible or ultraviolet light
    • G01N21/17Systems in which incident light is modified in accordance with the properties of the material investigated
    • G01N21/21Polarisation-affecting properties

Definitions

  • This invention relates in general to defect detection, and, in particular, to an improved system for detecting anomalies on surfaces, such as particles and surface- originated defects such as crystal-originated particles (“COPs”), surface roughness and micro-scratches.
  • COPs crystal-originated particles
  • the SPl 181 TM detection system available from KLA-Tencor Corporation of San Jose, California, the Assignee of the present application, is particularly useful for detecting defects on unpattemed semiconductor wafers. While the SP1 TOI system provides unsurpassed defect sensitivity on bare wafers or unpattemed wafers, this is not the case when it is used for inspecting wafers with patterns thereon such as wafers with memory arrays. In this system, all of the radiation collected by a lens or ellipsoidal mirror is directed to a detector to provide a single output. '.' " Thus, since pattern on the wafer will generate Fourier and/or other strong scattering signals, when these signals are collected and sent to the detector, the single detector output becomes saturated and unable to provide information useful for detecting defects on the wafer.
  • inspection systems for detecting patterned wafers may be also used for inspecting unpattemed wafers, such systems are typically not optimized for such purposes.
  • Systems designed for the inspection of unpattemed or bare wafers may have difficulties handling the diffraction or other scattering caused by the patterned structures on patterned wafers, for reasons such as those explained above.
  • AITTM inspection system For the inspection of patterned wafers, entirely different inspection systems have been employed.
  • AITTM inspection system is available from the Assignee of the present application, KLA-Tencor Corporation of San Jose, California; such system is also described in a number of patents, including U.S. Patent No. 5,864,394.
  • spatial filters are employed to shield the detectors from the diffraction or scattering from the patterned structures on the wafer.
  • the design of such spatial filters can be based on prior knowledge of the patterned structures and can be quite complex.
  • this system utilized a die to die comparison process in order better to identify the presence of a defect.
  • CMP Chemical mechanical planarization
  • One important parameter for morritoring the quality of unpattemed or bare films on silicon wafers is the surface roughness.
  • Surface roughness is typically measured by an instrument such as the HRP® instruments from KLA-Tencor Corporation, the Assignee of the present application, or by means of other instruments such as atomic force microscopes or other types of scanning probe microscopes such as scanning tunneling microscopes.
  • One disadvantage of such instruments is the slow speed of their operation. It is therefore desirable to provide an alternative system which may be used for giving a measure of surface roughness at a speed much faster than the above-described instruments.
  • One aspect of the invention is based on the observation that the collectors in the SPl 161 instruments preserve the azimuthal information of the scattered radiation by the surface inspected.
  • the collectors in the SPl 161 instruments preserve the azimuthal information of the scattered radiation by the surface inspected.
  • the collectors in the SPl 161 instruments preserve the azimuthal information of the scattered radiation by the surface inspected.
  • the surface inspection system of one aspect of this invention collects radiation scattered from the surface by means of a collector that collects scattered radiation substantially symmetrically about a line normal to the surface.
  • these channels will carry information related to scattered radiation at corresponding relative azimuthal positions of the scattered radiation.
  • the channels are separated from each other by separators to reduce cross-talk.
  • the collected scattered radiation carried by at least some of the channels may then be used for determining the presence and/or characteristics of anomalies in or on the surface.
  • the multiple views of the same event can significantly facilitate the process of real time defect classification (RTDC).
  • the system can then be used for inspecting both unpatterned and patterned wafers.
  • the SPl rai scheme is modified by diverting a portion of the collected radiation in the manner described above to different channels while preserving azimuthal information, a versatile tool results that can be optimized for the inspection of both unpattemed and patterned wafers. In this manner, semiconductor manufacturers no longer have to employ two different tools, each optimized for the detection of patterned or unpattemed wafers.
  • the signals containing pattern diffraction can be discarded and the remaining signals not containing pattern scatter may then be used for the detection and classification of anomalies in or on the surface of the wafer. While the above-described systems are particularly useful for the inspection of semiconductor wafers, they can also be used for he inspection of anomalies on other surfaces such as flat panel displays, magnetic heads, magnetic and optical storage media and other applications.
  • the radiation collected by a collector may be filtered by means of a spatial filter having an angular gap of an angle related to the angular separation of expected radiation components scattered by pattern on the surface.
  • the filtered radiation at some relative positions of the surface relative to the filter will contain information concerning defects of surfaces unmasked by pattern scattering that would interfere with the measurements.
  • the detector outputs can then be used for detecting the presence and/or characteristics of anomalies in or on the surface.
  • the SP1 TOI tool or the above-described systems may be used for distinguishing between particles and micro-scratches caused by CMP.
  • Scattered radiation along directions close to the normal direction is collected by a first detector and radiation scattered along directions away from the normal direction is collected by a second detector.
  • a ratio is then derived from the outputs of the two detectors to determine whether an anomaly on the surface is a micro-scratch or a particle.
  • the CMP micro-scratches tend to scatter radiation from an oblique incident beam in the forward direction while particles tend to scatter such radiation more evenly. Radiation scattered by the surface along forward scattering directions is collected separately from scattered radiation in other scattering directions. Two different signals are derived from the separately collected scattered radiation and compared for determining whether an anomaly on the surface is a micro-scratch or particle.
  • an S-polarized radiation beam and a P- polarized radiation beam are provided sequentially in oblique direction(s) to the surface during two different scans of the surface.
  • the radiation scattered by a defect during the first and second scans is collected to provide a pair of signals indicative of the scattered radiation of two different incident polarizations.
  • the pair of signals is then compared to a reference to determine whether an anomaly on the surface is a micro-scratch or particle.
  • a database correlating haze values with surface roughness of thin films is provided.
  • the haze value of the surface is then measured by a tool such as the SPl 131 or one of the above-described systems, and a roughness value of the surface may then be determined from the measured haze value and the database.
  • the database may be compiled by means of a tool such as the SPl or one of the above- described systems for measuring the haze values of representative thin films and another tool such as an HRP® profiler or other type of profilometer or a scanning probe microscope for measuring the surface roughness of such films.
  • Fig. 1 is a schematic diagram of the SPl 131 system useful for illustrating the invention.
  • Fig. 2 is a schematic diagram illustrating a convergent hollow cone of radiation to illustrate one aspect of the invention.
  • Fig. 3A is a schematic view of a possible arrangement of multiple fiber channels for carrying scattered radiation collected by the ellipsoidal collector of the system of Fig. 1 to illustrate one aspect of the invention.
  • Fig. 3B is a schematic view of an multi-anode photomultiplier tube (PMT) that can be used in conjunction with an arrangement of multiple fiber channels such as that shown in Fig. 3 A to illustrate one aspect of the invention.
  • PMT multi-anode photomultiplier tube
  • Fig. 4 is a schematic view of an arrangement of fiber channels/multiple detectors for carrying scattered radiation collected by the lens collector in the narrow channel of the system of Fig. 1 to illustrate an aspect of the invention.
  • Fig. 5 A is a cross-sectional view of a defect inspection system to illustrate the preferred embodiment of the invention.
  • Fig. 5B is a cross-sectional view of an arrangement of separate optical channels used in the embodiment of Fig. 5 A.
  • Fig. 6 A is a cross-sectional view of a defect inspection system to illustrate an alternative embodiment of the invention.
  • Fig. 6B is a cross-sectional view of an arrangement of segmented optical channels used in the embodiment of Fig. 6 A.
  • Fig. 7 is a top view of a portion of a defect inspection system to illustrate another alternative embodiment of the invention.
  • Fig. 8A is a schematic view of a multi-element detector in the embodiment of Fig. 7.
  • Fig. 8B is a schematic view of two multi-element detectors for use in the embodiment of Fig. 7.
  • Fig. 9A is a partly cross-sectional and partly schematic view of a defect inspection system to illustrate yet another alternative embodiment of the invention.
  • Figs. 9B and 9C are schematic views of filter wheels useful in the embodiment of Fig. 9 A.
  • Fig. 10 is a schematic view of a two-dimensional diffraction components from a pattern on a surface to be inspected illustrating an aspect of the invention.
  • Fig. 11 is a schematic view of a defect inspection system to illustrate one more alternative embodiment of the invention.
  • Fig. 12 is a schematic view of an asymmetric mask for use in the different embodiments of this invention.
  • FIGs. 13 A and 13B are schematic views of two masks used with the different systems of this application to illustrate yet another aspect of the invention.
  • Fig. 14 is a graphical plot of the interference intensity of thin film surfaces when illuminated with radiation of three different polarizations to illustrate another aspect of the invention.
  • Fig. 15 is a graphical plot of haze and surface roughness to illustrate yet another aspect of the invention.
  • Fig. 16 is a block diagram illustrating a system measuring surface roughness and haze of representative films for compiling a database useful for the invention of Fig. 15.
  • Fig. 1 is a schematic view of the SP1 TOI system 10 available from KLA- Tencor Corporation of San Jose, California, the assignee of the present application. Aspects of the SP1 TBI system 10 are described in U.S. Patent Application Serial No. 08/770,491, filed December 20, 1996 and U.S. Patent No. 6,201,601, both of which are incorporated in their entireties by reference. To simplify the figure, some of the optical components of the system have been omitted, such as components directing the illumination beams to the wafer.
  • the wafer 20 inspected is illuminated by a normal incidence beam 22 and or an oblique incidence beam 24.
  • Wafer 20 is supported on a chuck 26 which is rotated by means of a motor 28 and translated in a direction by gear 30 so that beams 22 and/or 24 illuminates an area or spot 20a which is caused to move and trace a spiral path on the surface of wafer 20 to inspect the surface of the wafer.
  • Motor 28 and gear 30 are controlled by controller 32 in a manner known to those skilled in the art.
  • the beam(s) 22, 24 may be caused to move in a manner known to those skilled in the art to trace the spiral path or another type of scan path.
  • the area or spot 20a illuminated by either one or both beams on wafer 20 scatters radiation from the beam(s).
  • the radiation scattered by area 20a along directions close to a line 36 perpendicular to the surface of the wafer and passing through the area 20a is collected and focused by lens collector 38 and directed to a PMT 40. Since lens 38 collects the scattered radiation along directions close to the normal direction, such collection channel is referred to herein as the narrow channel and PMT 40 as the dark field narrow PMT.
  • one or more polarizers 42 may be placed in the path of the collected radiation in the narrow channel.
  • the outputs of detectors 40, 60 are supplied to a computer 62 for processing the signals and determining the presence of anomalies and their characteristics.
  • the SPlTM system is advantageous for unpattemed wafer inspection since the collection optics (lens 38 and mirror 52) is rotationally symmetric about the normal direction 36, so that the orientation of the system in Fig. 1 relative to the orientation of defects on the surface of wafer 20 is immaterial. In addition, the angular coverage of the scattering space by these collectors is well matched to those required to detect the anomalies of interest in unpattemed wafer inspection applications.
  • the SPlTM system 10 has another important characteristic in that both its lens collector 38 and the ellipsoidal mirror collector 52 preserve the azimuthal information contained in radiation scattered by defects on surface of wafer 20.
  • certain defects and/or pattern on the wafer may scatter radiation preferentially along certain azimuthal directions more than other azimuthal directions.
  • system 10 may be advantageously adapted and modified for the detection of defects on patterned wafers.
  • One aspect of the invention is based on the recognition that, by segmenting the radiation collected by the lens 38 and/or ellipsoidal mirror 52, radiation scattered in different azimuthal directions may be detected separately.
  • the detectors detecting radiation diffracted or scattered by pattern may become saturated, while other detectors not detecting such diffraction or scatter will yield useful signals for the detection and classification of defects on wafer 20.
  • the lens 38 and ellipsoidal mirror 52 preserve the azimuthal information of the scattered radiation, knowledge of the type of pattern or defects present on wafer 20 can be advantageously used to design and position multiple detectors to advantageously detect and classify the defects on the wafer. This is especially true in the case of regular patterns such as memory structures on wafer 20, as will be explained below, since radiation diffracted by such regular patterns also tend to be regular.
  • Fig. 2 is a schematic view illustrating a convergent hollow cone of radiation which can be collected by lens 38 or mirror 52.
  • a spatial filter (not shown in Fig. 1) is employed to block the specular reflection of the normal incidence beam 22 from reaching detector 40, so that the radiation focused by lens 38 to PMT 40 has the shape of a convergent hollow cone illustrated in Fig. 2.
  • the ellipsoidal mirror 52 since the mirror is not a complete ellipse, it collects only radiation scattered at larger angles to the normal direction 36 without also collecting the radiation scattered at near normal directions, so that the radiation focused by mirror 52 towards detector 60 also has the shape of a convergent hollow cone as shown in Fig. 2.
  • Fig. 3A is a schematic view of a possible arrangement of multiple fiber channels receiving radiation in the convergent cone of radiation shown in Fig. 2, such as that collected by mirror 52, to illustrate the preferred embodiment of the invention.
  • the arrangement in Fig. 3A comprises two substantially concentric rings of optical fiber channels 72 that are used to carry the collected scattered radiation in the convergent hollow cone shown in Fig. 2.
  • Fourier components or other pattern scattering from the pattern on the wafer 20 may reach some of the fibers 72, thereby causing the detectors detecting the radiation from such channels to be saturated.
  • multiple fiber channels 72 effectively segments the collected scattered radiation into different sectors or segments so that only some of the fiber channels will receive a strong signal and can become saturated due to the Fourier or other pattern scatter leaving the remaining channels carrying information that can be analyzed for detecting anomalies.
  • various schemes may be employed to minimize the effects of the pattern scatter when the segmented approach of Fig. 3 A is used.
  • Fig. 3B is a schematic view of a multi-anode PMT. As shown in Fig. 3B, only the anodes 74 that are shaded are aligned with fibers 72, where anodes 76 are not aligned with any of the fibers 72.
  • FIG. 4 is a schematic view illustrating an arrangement 80 of fiber channels or multiple detectors 82 for the narrow channel.
  • fibers or detectors 82 may be aligned with the collected scattered radiation illustrated in Fig. 2 for the narrow channel collected by lens 38 for segmenting the radiation in a similar manner as that described above for the wide channel.
  • Fig. 5A is a partially cross-sectional view and partially schematic view of a defect inspection system to illustrate the preferred embodiment of the invention.
  • the two illumination beams 22 and 24, computer 62 and the mechanisms for moving the wafer are not shown in the figure.
  • Radiation scattered by spot 20a on wafer 20 and collected by lens 38 is reflected by mirror 102 to detector 40.
  • Stop 104 blocks the specular reflection of the normal incident beam 22 from detector 40 and results in a cone shape of the convergent beam in Fig. 2.
  • Beamsplitter 106 reflects and diverts a portion of the collected radiation from lens 38 to the arrangement 80 of optical fibers of Fig. 4.
  • the size of optical fibers 82 and the size of the hollow cone reflected by beamsplitter 106 are such that fibers 82 collect and convey most of the radiation in the hollow cone of radiation.
  • Each of the fibers 82 is then connected to a corresponding detector or a detecting unit in a multi-unit or multi-element detector.
  • beamsplitter 112 diverts a small portion of the radiation collected by ellipsoidal mirror 52 towards arrangement 70' of optical fiber channels 72, shown more clearly in Fig. 5B, where each channel 72 is connected to a separate detector or a separate detecting unit in a multi-element detector system (not shown).
  • beamsplitter 112 is such that it diverts radiation only within a narrow ring 114 to arrangement 70'.
  • Most of the radiation collected by mirror 52 is passed through beamsplitter 112 and focused to detector 60 to provide a single output as would be the case in normal SPlTM 1 operation.
  • the illumination beams 22, 24 and the mechanisms for moving the wafer have been omitted to simplify the figure.
  • system 100 retains substantially all of the features of system 10 of Fig. 1.
  • system 100 diverts a portion of the scattered radiation collected by each of lens 38 and mirror 52, and directs them towards fibers 82, 72 to convey the segmented radiation to a separate detectors or detecting units.
  • the system is compact and requires minimal additional space compared to the SPlTM system 10 of Fig. 1. In this manner, a single combined instrument may be optimized and used for both unpattemed and patterned wafer inspection, thereby eliminating the need for two separate instruments for the two types of wafer inspection.
  • an alternative defect inspection system 150 of Fig. 6A may be used.
  • the illumination beams 22, 24, computer 62 and the mechanisms for moving the wafer have been omitted to simplify the figure.
  • scattered radiation collected by lens 38 and by mirror 52 are reflected by mirror 112' towards an arrangement of optical fibers 152 which is shown more clearly in cross-section in Fig. 6B.
  • arrangement 152 includes a ring of fibers 82 conveying scattered radiation collected by lens 38 and a ring of fibers 72 conveying scattered radiation collected by mirror 52.
  • each of the fibers 72, 82 are connected to a separate detector or a detecting unit of a multi-unit detector.
  • optically fransmissive cores of optical fibers that are located adjacent to each other in each of the two arrangements 70, 70', 80 are separated from each other by the claddings that envelope the cores so that crosstalk between adjacent cores is reduced.
  • optical channels other than fibers may be used and are within the scope of this invention. Where such channels do not include separators such as the cladding in the case of optical fibers, other optical separators may be employed to reduce crosstalk.
  • the scattering pattern due to a micro-scratch gives the highest concentration of energy and greatest detection uniformity when illuminated normally and captured in the near normal or narrow channel collected by lens 38.
  • the unique signature of the scratch in the form of an elongated pattern in the far-field allows for a simple method of classification. Therefore, if the eight or more fibers 82 arrange in a ring format is placed in the path of the hollow cone of light focused by lens 38 towards fibers 82 as diverted by beamsplitter 106, where the outputs of these fibers are directed onto a multi-channel detector or an array of individual detectors, by simple process of comparing the signals obtained through any two diagonally opposed fibers relative to the signals in the remaining fibers, the presence of the micro-scratch is obtained.
  • micro-scratches When illuminated obliquely, micro-scratches result in scattering patterns which can be distinguished from those due to particles, by using the multiple detection channels that were described above in conjunction with pattern inspection, viz. multiple fiber units 70 and 70'.
  • multiple detection channels that were described above in conjunction with pattern inspection, viz. multiple fiber units 70 and 70'.
  • the Fourier components from the memory array will spin as the wafer is rotated. These components will thus rotate and be at different azimuthal angles about the normal direction 36 of Figs. 1, 5A and 6A. This means that these Fourier components will be conveyed by different fibers 72, 82 as the wafer is rotated. Since the array of memory cells may have different dimensions in the X and Y directions of the wafer, as the wafer rotates, the number of detectors that are saturated by the Fourier components will change. This can be provided for by knowing the X and Y dimensions of the memory cells so that the number of Fourier diffraction components can be estimated.
  • a learn cycle is performed where the maximum number of Fourier components that need to be eliminated is determined by noting the maximum number of detectors with very strong, or saturated, outputs. During the subsequent measurement, this number of detector outputs may then be eliminated, where the outputs eliminated are the ones that are saturated or the ones that have the largest values.
  • cross-talk may be reduced by also eliminating the components adjacent to the detectors having the highest outputs.
  • the wafer in one position gives three Fourier components, and in another two, the three direct components together with two components adjacent to each would be eliminated for a total of nine detector outputs that are eliminated. This leaves seven useable detector outputs. This number will be maintained regardless of the exact orientation of the wafer. This allows the user to maintain the sizing option for the particles.
  • the fibers 72 and 82 are arranged rotationally symmetrically around a direction, such as axes 74 and 84 shown in Figs. 3A, 4, 5B and 6B.
  • the radiation scattering directions are partitioned into identical angular segments and radiation scattered within each segment is collected by a corresponding fiber.
  • beamsplitter or mirror 102, 112, 112' reflects or diverts a portion of the radiation collected by lens 38 or mirror 52
  • the azimuthal positions of the collected scattered radiation is preserved when the reflected or diverted radiation is directed to the fibers 72, 82.
  • axes 74, 84 correspond to the normal direction 36
  • the azimuthal positions of the collected scattered radiation about the axes 74, 84 corresponding to their azimuthal positions about the normal direction 36 are preserved.
  • the sum of the two signals from any two diametrically opposed fibers may be compared with the output signals of the remaining detectors to ascertain the presence of a micro-scratch.
  • the presence of Fourier or other scatter components will cause the detector to saturate so that the system will not be able to provide useful information concerning anomalies in the illuminated spot. For this reason, applicants propose segmenting the collected scattered radiation into different segments.
  • the segmentation is preferably fine enough that at least some of the detector signals contain no significant pattern scatter.
  • the segmentation is preferable for the segmentation to be such that each detector receives scattered radiation collected within an angular aperture of no more than ⁇ .
  • FIG. 7 is a top view of a rotationally symmetric collector such as an ellipsoidal or paraboloidal mirror 200 with two apertures 202, 204, where the two apertures are preferably centered at +90 and -90 azimuthal positions relative to the oblique beam 24 illustrated in Fig. 1 and 7.
  • a multi-element detector or detector array 206, 208 is placed in each of the two apertures, where the detector or array may be a multi-anode PMT or multi-PIN diode array.
  • Fig. 8A is a schematic side view of a portion of the detector or detector array 206, 208 of Fig. 7 along arrow 8A. As shown in Fig.
  • each of the detecting units 206a, 208a has a substantially rectangular shape, with width w.
  • the units 206a, 208a are arranged substantially with their elongated sides parallel to the normal direction 36.
  • each of the detecting units 206a, 208a collects scattered radiation within a small angular sector subtended by the widths of the elongated elements 206a, 208a towards the center axis 36 where the angle of such sector subtended is no more than ⁇ , so that at least some of the detectors would provide useful signals for detecting and characterizing anomalies on the sample surface without being masked by pattern scatter.
  • the detector units 206a, 208a will provide useful signal components for detecting anomalies.
  • the above-described process of either estimating or determining through a quick leam cycle may be applied to the two detector or detector arrays 206, 208 for ascertaining the maximum number of pattern scatter components that need to be eliminated, so that the remaining detector signals can then be used for detecting anomalies.
  • the size of the semiconductor circuits is continually being reduced. Thus, when the cell size is reduced, this correspondingly reduces the number of Fourier or other scatter components. For larger cell sizes, if the width w of the detecting units of detectors or detector arrays 206, 208 are not reduced, each of the detecting units in the two detectors or detector arrays 206, 208 will become saturated so that again no useful signal results. This can be remedied by the scheme illustrated in Fig. 8B.
  • the detectors or detector arrays 206, 208 are labeled from the same side to the other; Dl, D2... D2n, D2n+1....
  • the odd numbered detecting units Dl, D3, D5... D2n+1... of multi-unit detector or detector array 206 are masked by a spatial filter 216.
  • detector or array 208 are masked by a spatial filter 218 as shown in Fig. 8B. In this manner, as relative rotation motion is caused between the sample surface and detectors or arrays 206, 208, the detecting units that are not covered would still provide useful signals.
  • Fig. 9A is a cross-sectional view of collector 52 of Fig. 1 modified to include the type of apertures or detector or detector arrays illustrated in Figs. 7, 8A and 8B.
  • the two apertures 202, 204 are, preferably, of a size such that each aperture comprises an azimuthal gap of about 10°-40° on each side centered on +90° azimuth.
  • the apertures are located only towards the bottom portion of the collector so that only scattered radiation along directions close to the surface are detected by the detectors or detector arrays 206, 208.
  • Two lenses 222, 224 with the appropriate F numbers are used for collecting and focusing the scattered radiation from the illuminated spot 20a to their respective detector or detector array 206, 208.
  • the two detector or detector arrays may be placed at the back focal planes of the two lenses 222, 224.
  • the masks 216, 218 may be placed between the illuminated spot 20a and the detectors or detector arrays 206, 208 by means of filter wheels 226, 228 rotated by actuators 232, 234 in a manner known to those skilled in the art so that the connections between these two actuators and the wheels are not shown and a detailed description of their operation is not necessary herein.
  • filter wheels 226, 228 rotated by actuators 232, 234 in a manner known to those skilled in the art so that the connections between these two actuators and the wheels are not shown and a detailed description of their operation is not necessary herein.
  • Only the mask portions 216, 218 of the two filter wheels 226, 228 are illustrated in Fig. 9A.
  • the features illustrated in Figs. 9 A, 9B and 9C may be combined with the systems 100, 150 of Figs. 5 A and 6A to further increase their versatility.
  • the outputs of detectors or detector arrays 206, 208 can obviously be added to the output of detector 60 at least partially to restore the sensitivity of the system when inspecting unpattemed wafers.
  • the feature of Figs. 9A-9C may be advantageously used as well. Since film roughness scatters P-polarized light more efficiently than S-polarized light, in such circumstances, it will be desirable to supply an oblique illumination beam 24 which is S-polarized, and collect only the S-polarized scatter from illuminated spot 20a.
  • the semi-circular S- polarizer may restrict the elevational collection angles of the aperture to within a range of about 55 to 70° from the normal direction 36. This is helpful since the amount of scatter caused by film roughness increases with the elevation angles to the wafer surface.
  • Fig. 9C illustrates an alternative filter wheel that may be used for the inspection of bare or unpattemed wafers. If the directions of the expected pattern scatter surface are known, spatial filters may be designed to block such scattering, thereby detecting only the scatter by anomalies on the surface.
  • Fig. 10 is a schematic view illustrating the two-dimensional Fourier components of an array structure when illuminated with normal incidence radiation. As the sample rotates, all of the spots at the intersections of the X-Y lines will rotate, thereby generating circles.
  • the cell size of a regular memory array on the wafer is such that its X and Y dimensions are not larger than about 3.5 microns, for example, this means that for 488 nanometers wavelength radiation used in the illumination beams 22, 24, the first Fourier component is at about 8° to the normal direction 36. Therefore, if a spatial filter is employed, blocking all collected radiation in the narrow channel that is at 8° or more to the normal direction 36 will leave an annular gap of 2 or 3° ranging from the rim of the central obscuration (i.e. 5 or 6°) to the rim of the variable aperture at about 8°. Under these conditions, as the wafer spins, no Fourier components can possibly get through the annual gap and scatter from the array is suppressed. In one embodiment, the spatial filter used leaves an annular gap between about 5 to 9° from the normal direction 36.
  • a spatial filter is designed for the narrow channel; it will be understood that similar spatial filters may be designed for the wide channel as well. Such and other variations are within the scope of the invention.
  • the collection aperture of at least some of the detectors are preferably no larger than the angular separation between the expected pattern scatter.
  • a spatial filter may be constructed where all of the collected radiation in the narrow or wide channel is blocked except for a small angular aperture where the angle of the angular aperture is not larger than the angular separation between pattern scatter.
  • the wafer map will be a series of data-valid, and saturated sectors. If the scan is repeated a second time where the center position of the angular aperture is shifted relative to its position during the first scan by the minimum angular separation of the patterned scatter, one would again obtain a similar map comprising data- valid and saturated sectors as before. However, in those areas that were saturated during the first scan, one now has valid data. Therefore, by combining the two data sets using the logical OR operation, a full wafer map of valid data can be achieved.
  • asymmetric mask 250 illustrated in Fig. 11.
  • the two sector shaped apertures 252, 254 are offset from a diametrically opposite position by an angle which is equal to the expected minimum angular separation of pattern scatter.
  • the detectors 40 and 60 will then provide a full wafer map when the wafer is scanned.
  • Fig. 12 is a schematic view of a defect detection system illustrating another alternative embodiment of the invention.
  • the scattered radiation collected by collector 52 when illuminated by beams (not shown), such as beams 22, 24 of Fig. 1, the scattered radiation collected by collector 52 (omitted from Fig. 12 to simplify the figure) are focused to a triangular-shaped device 262 having two mirrors 262a, 262b on opposite sides of the device.
  • the illumination beams have also been omitted for simplicity.
  • the scattered radiation are, therefore, reflected into two opposite hemispheres by device 262.
  • Mirror 262a reflects half of the scattered radiation towards PMTl and mirror 262b reflects the other half of scattered radiation towards PMT2 and asymmetric mask 250 may be employed between mirror 262a and PMTl and between mirror 262b and PMT2. In this manner, the two PMTs will provide two wafer maps useful for anomaly detection and classification.
  • One aspect of this invention covers two algorithms for classifying CMP defects.
  • the first method is based on the spatial distribution of the light scattered by defects.
  • Theoretical simulation and experimental results indicate that the light scattered by CMP micro-scratches is primarily in the direction of specular reflection while light scattered by particles (especially, small particles) has a different spatial distribution.
  • defect classification can be achieved by measuring the distribution of the scattered light. It can be implemented by using two or more detectors placed at proper positions around the scatterers. Or, using one detector with two or more spatial filters/masks. Three different ways of implementing this algorithm are set forth below.
  • the second algorithm is based on a dual-polarization method. This method compares the scattering signal from a defect using incident S and P polarized beams. Theoretical simulation indicates that the scattering intensity is proportional to the local interference intensity seen by the defects. This interference intensity is different for S and P polarized light and has a dependence on the height above the wafer surface. Thus, the interference intensity seen by a particle (an above-surface defect) is very different from that seen by a micro-scratch (at or below the wafer surface). Defect classification can be achieved by comparing the scattering signal strength using both S and P polarized incident light or radiation.
  • DWN dark field channels
  • DNN the channel carrying scattered radiation collected by the lens collector originating from a normal illumination beam
  • DWO the channel carrying scattered radiation collected by the ellipsoidal mirror originating from an oblique illumination beam
  • DNO the channel carrying scattered radiation collected by the lens collector originating from an oblique illumination beam.
  • the dual-channel method uses two dark-field channels, for example the DWO and the DNO channels. The principle of this method is based on the fact that particles and micro-scratches have different spatial scattering patterns.
  • a micro-scratch preferentially scatters light in certain directions, resulting in the signal captured in one channel being significantly larger than that in the other channel.
  • the oblique channels DWO and DNO are used, micro-scratches are preferentially captured in the DWO channel or the signal in DWO channel is significantly larger than that in DNO channel.
  • the size ratio of a defect is less than certain fraction number (example: 0.8), it is classified as a micro-scratch. If a defect is only captured in DWO channel but not in DNO channel, it is classified as a CMP micro-scratch. If a defect is only captured in DNO channel but not in DWO channel, it is classified as a particle.
  • the implementation in normal channels is similar to that in oblique channels.
  • the difference is that the light scattered from a CMP micro-scratch is preferentially towards narrow channel (DNN) in normal incidence instead of wide (DWN) channel.
  • DNN narrow channel
  • DWN wide
  • the defect classification is achieved by calculating the size ratio of a defect captured in both DNN and DWN channels. If the size ratio for a defect is close to one, it is classified as a particle. However, if the size ratio of a defect is larger than certain number (example: 1.6), it is classified as a micro-scratch.
  • the third method of implementing algorithm #1 uses two masks.
  • One of the masks (#1) is designed to capture preferentially the scatter from CMP micro- scratches; this mask is illustrated in Fig. 13 A, where the shaded region indicates the area where radiation is blocked, and the non-shaded region indicates the area where radiation fransmittance is allowed.
  • the other one (#2) is designed to block the light scattered by CMP micro-scratches; this mask is illustrated in Fig. 13B, where the shaded region indicates the area where radiation is blocked, and the non-shaded region indicates the area where radiation fransmittance is allowed.
  • the calibration curves of both mask configurations are needed.
  • the defect classification is achieved by calculating the size ratio of a defect captured in both mask configurations.
  • the size ratio of mask#l and mask#2 is close to one, it is classified as a particle. However, if the size ratio of a defect is larger than certain number (example: 1.15), it is classified as a micro-scratch.. If a defect is only captured in mask#l configuration but not in mask#2 configuration, it is classified as a CMP micro-scratch. If a defect is only captured in mask#2 configuration but not in mask#l configuration, it is classified as a particle.
  • Algorithm #1 can also be implemented with a multi-anode PMT.
  • the advantage of this method is that it can be done in one scan. It is essentially the same as using two masks, but only one scan is needed for data collection.
  • Algorithm #2 utilizes two incident polarizations, S and P. Two scans are needed for this method. One is for S-polarization; the other is for P-polarization. The PSL calibration curves for both S- and P- polarizations are used.
  • the defect classification is achieved by calculating the size ratio of a defect captured in both P and S scans. If the size ratio of P and S scans is close to one, it is classified as a particle. However, if the size ratio of a defect is other than one (example: ⁇ 0.65 or >1.85 depending on film thickness), it is classified as a micro-scratch.
  • the interference intensity for the two polarizations will vary with film thickness.
  • the changes in interference intensity of the two polarizations are out of phase; when the P polarization interference intensity is at a maximum, the S polarization interference intensity will be at a minimum and vice versa.
  • the size ratio for CMP defects will either be greater or less than 1.0 depending upon the thickness of the dielectric film.
  • a defect is captured only in one polarization but not the other, it is classified as a CMP micro-scratch or particle depending on the film thickness. This method has been successfully demonstrated using oxide CMP wafers.
  • the SPlTM instrument is calibrated using PSL spheres so that the size ratio of the detected intensities during the P and S scans is normalized to 1 for particles. Thus, the particles present would give rise to ratios at or around 1.
  • a second set of intensity ratios clusters at a value greater than 1, indicating a set of defects that scatter more in response to P-polarized illumination than S-polarized illumination.
  • CMP defects such as micro-scratches; this would be true even where scattered intensities are detected only during the P scan and not during S scan since in that instance the ratio is infinite and therefore greater than 1.
  • a third group of ratios are at zero or close to zero values. These are deemed to indicate particles, for the reasons explained below.
  • haze measured from the films varies with surface roughness of the films if there is little film thickness variation.
  • Most dielectric films CVD deposited for integrated circuit applications are quite uniform. Hence, haze measurements may provide a quick alternative to the measurement of film roughness.
  • a database may be constructed by measuring surface roughness of representative films 302 of different thicknesses using the KLA-Tencor High Resolution Profiler, or AFM type tool 304, and measuring haze values of these same films using the SPlTM system 10, or one of the combined systems (e.g.
  • any other tool that can be used to measure haze in order to build a database using computer 310 of the correlation between haze and surface roughness for films of different thicknesses. Measurement of like films of various thicknesses may be preferable since surface roughness increases with film thickness.
  • a database may then be constructed such as the graphical plot shown in Fig. 15. Then if it is desirable to determine the surface roughness of an unknown film, its roughness may be determined by measuring the haze of the film using an instrument such as system 10 of Fig. 1 or the combined instruments described above. The haze measurement is then used to select a corresponding roughness value from the database for a film of known thickness, such as from the graph shown in Fig. 15. This will save the end user in the fabrication facility up to an hour for each film since it takes only about one minute to measure the haze value and correlate the haze measurement with the RMS roughness calibration curve of Fig. 15.

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Abstract

Selon la présente invention, les rayonnements diffusés par la surface d'un échantillon (20a) sont recueillis par un collecteur (38,52) qui collecte les rayonnements de façon sensiblement symétrique autour d'une ligne perpendiculaire à la surface (20a). Les rayonnements recueillis sont dirigés vers des canaux à des angles d'azimut différents de façon que les informations liées aux positions d'azimut respectives des rayonnements diffusés recueillis autour de la ligne sont préservées. Les rayonnements recueillis sont convertis en signaux respectifs représentatifs des rayonnements diffusés à des angles d'azimut différents autour de la ligne. On détermine la présence et/ou l'absence de caractéristiques d'anomalies à partir des signaux. Dans un autre mode de réalisation, les rayonnements recueillis par le collecteur (38,52) peuvent être filtrés au moyen d'un filtre spatial comprenant un espace annulaire d'un angle lié à l'angle de séparation de la diffusion des motifs attendue. On peut comparer les signaux obtenus à partir des canaux de collecte étroits et larges afin de distinguer les microrayures des particules. On peut recueillir des rayonnements diffusés vers l'avant à partir d'autres rayonnements et les comparer afin de distinguer les microrayures des particules. On mesure l'intensité de la diffusion lorsque la surface est illuminée séquentiellement par des rayonnements à polarisation S et P, et on procède à une comparaison afin de distinguer les microrayures des particules.
PCT/US2002/010783 2001-04-06 2002-04-03 Systeme de detection de defauts ameliore Ceased WO2002082064A1 (fr)

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