Upload
lehuong
View
217
Download
5
Embed Size (px)
Citation preview
Emission Microscopy analysis of hot cluster defects of imagers processed on SOI
G. Meynants, W. Diels, J. Bogaerts, W. Ogiers CMOSIS nv, Coveliersstraat 15, 2600 Antwerp, Belgium
[email protected] , +32 3 260 17 32 Introduction
On the IISW 2011, we reported on the successful development of 2 and 4 MPixel backside illuminated global shutter image sensors [1], manufactured with an SOI based backside thinning flow [1,2]. The SOI thinning flow was chosen because of the easier thickness control due to the strong selectivity of the thinning etch step to the buried oxide layer. More recently we have developed new SOI based image sensors intended for backside illumination. However, during frontside illuminated testing of devices processed on SOI substrates using 3 or 10 micron epitaxial layers, a large amount of hot pixel cluster defects were observed. An example dark image is shown in figure 1a. These devices were frontside illuminated control devices, processed with a standard CIS flow, but on SOI substrates. They were intended only to demonstrate the functionality of the design on SOI before the BSI processing steps would take place. In the devices reported in [1], these hot clusters were only present on certain areas of the wafer and with much lower occurrence.
EMMI analysis results
These cluster defects were analyzed using emission microscopy (EMMI). A microscope containing a near-‐infrared (NIR) sensitive CCD camera was used to observe electroluminescence on the hot pixel clusters during operation of the image sensor. The NIR image is overlaid on a visible image to allow locating the emission center on the chip. This experiment demonstrated an excellent correlation between the electroluminescence captured by the EMMI system and the hot cluster positions as seen in the images captured from the chip (see fig. 1).
More detailed microscope emission pictures showed the location of the electroluminescence centers inside the pixel, pointing to two n+/p-‐well junctions inside the pixel that operate at the highest potential inside the pixel. Figures 2 and 3 show a microscope view with the emission centers and the pixel layout side-‐by-‐side. Figure 2 shows emission at an n+ diffusion area connected to the drain of one of the in-‐pixel source followers. Figure 3 shows emission at the drain of the reset transistor. Increasing the supply voltage of the in-‐pixel source followers and the voltage on the drain level of the reset transistor increased the EMMI signal and also increased the size of the hot clusters in the image taken with the sensor. It is not clear if this is due to an increase in intensity or a shift to shorter wavelength, where the EMMI camera is more sensitive.
This electroluminescence explains the hot clusters in the dark images captured by the sensor. The clusters are caused by self-‐absorption of the emitted photons by the surrounding photodiodes. The dark image shown in fig. 1a shows that the clusters are several pixels wide. For many clusters, the center pixel is black again because of the very high radiation present close to the emission center. This causes an integration of charges during the readout of the FD reset level, reversing the pixel signal.
This photo-‐emission or electroluminence can only be explained by radiative recombination. The band-‐to-‐band radiative recombination rate is very low in silicon, because it is an indirect bandgap material and a phonon-‐assisted transition is normally required. However, the presence of localized crystallographic defect in the silicon, either a chemical impurity or a physical defect, can replace the role of the phonon and cause emission of photons at sub-‐bandgap energies. Besides this, hot carriers
can cause higher-‐energy photoemission, either through interband transitions, also called “avalanche emission”, or trough intraband transitions, also called “deceleration emission” [3,4]. Since the energy of the emitted photons is higher than the Si bandgap energy, we conclude that hot carriers are responsible for the effect that we observe. The presence of the defect at random locations in the pixel array points to crystallographic defects caused by impurities. When these are located close to the reverse biased n+/p junction, we expect that these assist to form avalanche emission centers.
Impurities such as Cu, Fe, W, Cr, Ni commonly are present during wafer manufacturing. They introduce energy levels around mid bandgap [4]. In a standard bulk wafer, these impurities would diffuse into a gettering layer at the bottom of the wafer, where the impurities are trapped. In this case however, the SOI layer forms a barrier for the diffusion of some of these impurities, like Fe or Ni. Instead, these impurities diffuse as interstitials to certain areas in the pixel until they are trapped. For example, Fe can form iron-‐boron pairs (Fe-‐B) [6] or iron-‐phosphorus pairs [7]. It seems that at least some of these impurities get trapped near the n+/p junctions in this pixel that are connected to the pixel power supply or reset drain supply. When a strong electric field is present in this area, radiative recombination occurs.
These observations, and the fact that our first global shutter developments presented in IISW2011 did not show these cluster defects, pointed to solutions for this issue. Meanwhile our foundry partner in this project, TowerJazz has proposed a fix for the issue, and we have successfully demonstrated that this fix solved this issue on one of our BSI products. Fig. 5 shows a dark image taken on a backside thinned imager after this fix, with a 500 ms exposure at 50ºC.
Conclusion
Emission microscopy has demonstrated that radiative recombination at high voltage n+/p junctions was a cause of hot cluster defects in imagers processed on SOI substrates. Some impurities present in the silicon layer assist to form avalanche emission centers. This is probably the first time that light emission from junctions inside a pixel of an image sensor has been reported as one of the origins of hot pixel clusters. But the use of an array of avalanche electroluminescent diodes in silicon was already proposed in 1965 to form a monolithic display [8].
Acknowledgement
We thank Ingrid De Wolf of IMEC for making available the EMMI setup and assistance with the EMMI measurements.
References
[1] G. Meynants, et al, “Backside illuminated global shutter CMOS image sensors”, proc. IISW, Hokkaido, June 2011, p. 305-‐308 [2] B. Pain, “Backside Illumination Technology for SOI-‐CMOS Image Sensors”, IISW 2009 symposium on BSI, Bergen, June 2009 [3] H. Ivey, “Electroluminescence and Semiconductor Lasers”, IEEE Journal of Quantum Electronics, Vol. QE-‐2, No. 11, Nov. 1966, p. 713 -‐ 726 [4] S. M. Sze, “Physics of Semiconductor Devices”, 1981, J. Wiley & Sons. [5] J. Furihata, et al, “Heavy-‐Metal (Fe/Ni/Cu) Behavior in Ultrathin Bondes SOI Wafers Evaluated Using Radioactive Isotope Tracers”, Jpn. J. Appl. Phys, Vol. 39 (2000), pp 2251-‐2255. [6] D. Schroder, “Carrier Lifetimes In Silicon”, IEEE Trans. El. Dev., Vol. 44, No. 1, Jan. 1997 [7] T. Mchedlidze, et al, “An iron-‐phosphorous pair in silicon”, J. Phys.: Condens. Matter 16 (2004), L79-‐L84 [8] R.H. Dyck, “Avalanche luminescence in silicon and its utilization in monolithic light source array”, 1965 Proc. ISSCC, p. 64
a) b) fig. 1: a) dark image as captured by the image sensor, showing hot pixel clusters
b) image captured by the EMMI system (NIR image, blue, as overlay on visible image)
a) b) Fig. 2: a) image of EMMI system (NIR=red overlay);
b) layout and first junction in the pixel where the electroluminescence is originated (large yellow plate is a top metal layer)
Crop from a dark image
NIR overlay over visible
a) b) fig. 3: a) image of EMMI system (NIR channel =red overlay);
b) layout and junction where the electroluminescence is originated.
Fig. 4 : impurity caught inside the epitaxial layer Fig. 5: dark image captured by BSI diffusing and trapped at one of the in-‐pixel junctions. imager at 50ºC (500 ms exposure) after fix for hot clusters.
p-
p+n
TX
n+
p++
impurity (e.g. metal contaminant)
epitaxial layer (3 - 10 µm)
bulk wafer± 725 µm
(removed during backside thinning)
BOX (145 nm)
n+