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The present application relates generally to systems and methods of inspecting semiconductor wafers, and more specifically to a semiconductor wafer inspection system and method capable of detecting and measuring wafer defects in which the scattering power of the defect exceeds the dynamic range of the system.
Systems and methods of inspecting semiconductor wafers are known for detecting and measuring defects occurring on a surface of a semiconductor wafer. For example, a conventional laser-based surface scanning inspection system is typically configured to detect localized light scatters on a semiconductor wafer surface. Such localized light scatters may be indicative of one or more defects in the wafer surface that may render an integrated circuit(s) (IC) fabricated on the wafer to be inoperative. In a typical mode of operation, the conventional surface scanning inspection system sweeps a laser light beam in a predetermined direction, while the wafer being inspected rotates under the swept beam at an angle of about 90° to the predetermined sweep direction. Next, the conventional surface scanning inspection system detects a light beam reflected from the wafer surface, and samples the detected signal in both the predetermined direction of the swept beam and in the direction of rotation to obtain a two-dimensional array of data. When the light beam sweeps over a defect in the wafer surface, the data obtained by the wafer inspection system generally corresponds to the beam shape of the laser spot power at the wafer surface. This is because such wafer surface defects are generally much smaller than the spot size of the laser beam. After the conventional surface scanning inspection system has detected a defect, the system may attempt to measure the size of the defect by determining the value of the maximum scattering power of the defect, and may also determine the location of the defect on the surface of the wafer.
One drawback of the above-described conventional laser-based surface scanning inspection system is that the maximum scattering power of a detected defect may exceed the dynamic range of the system. As a result, the electronics within the wafer inspection system may saturate, thereby causing at least some of the defect size measurements performed by the system to be at a power level at which the measurements become nonlinear due to the saturation effects.
One way of addressing the effects of saturation on defect size measurements made by the conventional laser-based surface scanning inspection system is to employ a data extrapolation technique. However, such data extrapolation techniques are often difficult to perform in conventional wafer inspection systems. Alternatively, the conventional surface scanning inspection system may perform a nonlinear least squares fit of the measurements to a given Gaussian shape, which may be characterized by a number of parameters including an estimated amplitude, an estimated inverse correlation matrix, and an estimated pulse center location. However, conventional algorithms for performing such nonlinear least squares fit techniques often require a significant amount of processing time. Further, relatively small changes in the data resulting from, e.g., noise or a non-ideal signal, may lead to significantly large changes in the estimated parameters.
It would therefore be desirable to have an improved system and method of inspecting semiconductor wafers that can measure the size and determine the location of a defect in a surface of a semiconductor wafer while avoiding the drawbacks of conventional wafer inspection systems and methods.
In accordance with the present invention, a system and method of inspecting semiconductor wafers is provided that is capable of measuring the size and determining the location of a wafer surface defect whether or not the scattering power associated with the defect exceeds the dynamic range of the system.
In one embodiment, the semiconductor wafer inspection system includes an optical module including a surface scanning mechanism and a light channel (LC) detector including LC optics. In the preferred embodiment, the surface scanning mechanism is an acousto-optic deflector (AOD), and the LC optics comprises a quadcell photodetector. The AOD is configured to emit at least one collimated beam of laser light toward a surface of a semiconductor wafer at an oblique angle of incidence θI, and the LC optics is configured to detect a light beam specularly reflected from the wafer surface at an angle of reflection θI.
In the presently disclosed embodiment, the height of a defect detected on a semiconductor wafer surface using the surface scanning laser beam is obtained by determining the height of a Gaussian shape representing data collected by the wafer inspection system. In one embodiment, the height of a geometric Gaussian shape in three dimensional space is determined by defining a plurality of cross-sectional areas of the Gaussian shape, each cross-sectional area corresponding to a respective intermediate height of the Gaussian shape, determining a respective value of each defined cross-sectional area of the Gaussian shape, determining a respective value of the natural logarithm of each intermediate height of the Gaussian shape, determining a natural logarithm of the height value corresponding to a zero cross-sectional area value based on the substantially linear relationship between the natural logarithm of the intermediate heights and the cross-sectional areas, and determining the inverse natural logarithm of the value determined in the third determining step to obtain the height of the Gaussian shape. The disclosed method further includes determining a slope corresponding to the substantially linear relationship between the natural logarithm of the intermediate heights and the cross-sectional areas to obtain a 1/e area of the Gaussian shape.
In the preferred embodiment, the method of obtaining the height of a defect detected on a semiconductor wafer surface using the surface scanning laser beam includes plotting the determined cross-sectional area values as a function of the determined natural logarithm of the height values substantially in accordance with the equation
in which “P0” is a maximum scattering power associated with the detected defect, and “R” is a positive definite symmetric matrix describing a shape associated with the laser beam.
Other features, functions, and aspects of the invention will be evident from the Detailed Description of the Invention that follows.
The invention will be more fully understood with reference to the following Detailed Description of the Invention in conjunction with the drawings of which:
U.S. Provisional Patent Application No. 60/514,289 filed Oct. 24, 2003 entitled EXTENDED DEFECT SIZING is incorporated herein by reference.
A system and method of inspecting a semiconductor wafer is disclosed that is capable of measuring the size and determining the location of a defect on a surface of a semiconductor wafer. The presently disclosed wafer inspection system can perform such sizing and locating of wafer surface defects whether or not the scattering power associated with the defect exceeds the dynamic range of the system.
For example, the AOD 102 may include a solid state laser such as a 532 nm wavelength diode-pulsed solid state laser, or any other suitable type of laser. In the preferred embodiment, the AOD 102 emits the laser light beam 108 to produce a focused laser spot having a diameter of about 30 microns for scanning the wafer surface 107, in which the incident angle θi of the emitted light beam 108 is about 65 degrees. It should be understood that the laser light beam 108 may alternatively be emitted by the AOD 102 at any suitable angle of incidence to produce any suitable spot size on the wafer surface. The surface scanning inspection system 100 further includes a theta stage 103 upon which the wafer 106 is held during inspection. The theta stage 103 is configured to rotate and to translate the wafer 106 through a scan line 112 produced by the AOD 102, thereby generating a spiral pattern of light used to inspect the wafer surface 107. The theta stage 103 includes an encoder such as an optical encoder that provides counts indicative of the rotational position of the stage 103 relative to a predetermined reference point. It is noted that the structure and operation of the theta stage 103 are known to those skilled in this art and therefore need not be described in detail herein.
In the preferred mode of operation, the surface scanning inspection system 100 (see
In the presently disclosed embodiment, the corresponding location of each data sample on the wafer surface 107 is expressed as
xin,xs, yin,xs, (1)
in which the index “in” designates samples in the radial or “in scan” direction, and the index “xs” designates samples in the tangential or “cross scan” direction.
When the light beam 108 sweeps over a defect in the wafer surface 107, the data samples obtained by the surface scanning inspection system 100 generally correspond to the beam shape of the laser spot on the surface 107. This is because wafer surface defects are normally much smaller than the spot size of the laser beam 108. For example, the data samples may be represented by a geometric Gaussian shape that is non-isotropic due to the angle of incidence θi and the non-orthogonal sampling of the data.
The locations (xin,xs, yin,xs) of the data samples on the wafer surface 107 may be expressed as a column vector, i.e.,
Accordingly, the optical laser spot power at the wafer surface 107 may be expressed as
power({right arrow over (z)})=P0 exp(−({right arrow over (z)}−{right arrow over (z)}0)′R−1({right arrow over (z)}−{right arrow over (z)}0)), (3)
in which “P0” is the maximum scattering power of the defect, “{right arrow over (z)}0” denotes the location of the defect, and “R” is a positive definite symmetric matrix describing the beam shape.
For example, if a laser spot is a Gaussian with a density of density(x)=e−x
density(x, y)=e−x
Equation (4) above may be rewritten as
Accordingly, for this illustrative example,
In the event the sampled data comprises non-saturated data (i.e., the data sampling is linear), the surface scanning inspection system 100 may determine the value of P0 in equation (3) above by identifying the largest value in the collection of measured data points, which may be expressed as
power(xin,xs, yin,xs). (7)
However, this technique for determining the value of P0 generally does not yield useful results when the maximum scattering power of a detected defect exceeds the dynamic range of the surface scanning inspection system 100, i.e., when the sampled data comprises saturated data. As a result, at least some of the defect size measurements performed by the wafer inspection system may be at a power level at which the measurements become nonlinear due to the saturation effects.
According to the present invention, a technique is provided for measuring the size and determining the location of a defect on a surface of a semiconductor wafer when the maximum scattering power of a detected defect exceeds the dynamic range of the surface scanning inspection system 100, i.e., the sampled data collected by the wafer inspection system comprises saturated data. It is noted that the disclosed technique may be employed in the voltage domain for sizing wafer defects.
The presently disclosed technique will be better understood by reference to the following analysis.
power({right arrow over (z)})>height, (8)
in which “power({right arrow over (z)})” is expressed as indicated in equation (3) above. Substituting this expression for power({right arrow over (z)}) in equation (8) yields
Equation (14) above shows that the area of a geometric Gaussian shape conceptually cut at a predetermined height (e.g., the area of the ellipse 402; see
π|R|1/2, (15)
in which “|R|1/2” is the square root of the determinant of the positive definite symmetric matrix describing the beam shape. It is noted that “π|R|1/2” is equal to the “1/e” area of the Gaussian shape. Accordingly, after plotting the area values as a function of the natural logarithm (ln) of the predetermined cut heights, and applying a least squares fit to the plot to form a linear plot, the intercept at which the area is zero is equal to the natural logarithm of the scattering power P0, and the slope of the linear plot is equal to the 1/e area of the Gaussian shape.
The presently disclosed technique for measuring the size and determining the location of a defect on a semiconductor wafer surface is illustrated by the following example.
y=−624x+440, (16)
in which the variable “y” represents the cross-sectional area of the Gaussian shape 502 and the variable “x” represents the natural logarithm of the predetermined cut height.
Accordingly, equation (16) above indicates that the cross-sectional area (y) is equal to zero when the natural logarithm of the cut height (x) equals about 0.705. The cut height at which the cross-sectional area equals zero may therefore be obtained by taking the inverse natural logarithm of 0.705, which is about 2.02. Because the cross-sectional area is equal to zero when the cut height equals the scattering power P0 of a wafer surface defect, as indicated in equation (14) above, P0 is equal to about 2.02. In this example, the actual height of the illustrative Gaussian shape 502 (i.e., the height that would be observed in the absence of saturation effects) is 2.0. Further, the slope of the linear plot 602, as expressed by equation (16) above, is equal to −624, which is the 1/e area of the Gaussian shape. In this example, the actual 1/e area of the Gaussian shape 502 (i.e., the 1/e area that would be observed in the absence of saturation effects) is 200π, or about 628. Based on these results, a correlation coefficient may be calculated as 0.9999. In general, if the correlation coefficient is much less than unity, then the linear least squares fit is considered to be poor. Because the correlation coefficient is equal to 0.9999 in this illustrative example, the linear least squares fit is consider to provide an accurate measure of the actual height of the Gaussian shape 502.
A method of operating the presently disclosed surface scanning inspection system to determine the amplitude (height) and the 1/e area of a Gaussian shape is illustrated with reference to
Having described the above illustrative embodiments, other alternative embodiments or variations may be made. For example, it was described that a linear least squares fit may be employed for fitting the cross-sectional areas to the natural logarithms of the predetermined cut heights. However, such linear least squares fitting was described for purposes of illustration, and other techniques may be employed, including a polynomial fit, a nonlinear least squares fit, or a noise weighted least squares fit technique.
It will be appreciated by those of ordinary skill in the art that further modifications to and variations of the above-described extended defect sizing technique may be made without departing from the inventive concepts disclosed herein. Accordingly, the invention should not be viewed as limited except as by the scope and spirit of the appended claims.
This application claims priority of U.S. Provisional Patent Application No. 60/514,289 filed Oct. 24, 2003 entitled EXTENDED DEFECT SIZING.
Number | Name | Date | Kind |
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5712701 | Clementi et al. | Jan 1998 | A |
20030058455 | Ebihara et al. | Mar 2003 | A1 |
Number | Date | Country | |
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20050114091 A1 | May 2005 | US |
Number | Date | Country | |
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60514289 | Oct 2003 | US |