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37. EFFECT OF RADIATION DAMAGE – SOFT ERRORS
37.1 Review/Background:
This lecture will focus on radiation-induced reliability issue, which is the fourth reliability mechanism other than NBTI, HCI, and TBBD. In the previous lecture, the importance of radiation related to a large of number of failures of memories as well as logic circuits is covered. Today, how radiation causes soft errors will be discussed. Soft errors refer to reversible errors, which is opposite to hard errors that result from punch- through and is permanent.
37.2 Source of radiation
The source of the radiation determines impact on the transistors. For example, those come from cosmos are very different than those from solar wind or packaging. Thus, the understanding of radiation sources is very important to understand the potential damage.
Figure. 37.1. Four different sources of radiation
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From Figure. 37.1, we have three different types of sources. They are comic ray, solar wind, and packaging process. When we hold our cell phones in classroom, then the source of disturbing our electronics will be comic ray, some of which have enough energy to penetrate to the ground level. Solar wind, which is the radiation from the sun, causes problems to satellites that are out of the atmosphere primarily. Packaging itself has radiative components, such as trace amount of Thorium, which emits alpha particle. A danger situation is the interaction between comic ray and packaging materials. For example, there are two types of p-type doping material Boron: Boron-10 and Boron-11. There is a small fraction of Boron-10 in the packing materials. When Boron 10 absorbs low-energy comic ray, it breaks up as Li(7) and alpha particle – each of which creates a huge number of electron-hole pairs.
Moreover, proton and α-particle are charged particles. According to Columbs law ,they will generate electron-hole pairs through electromagnetic interaction when they come through. Neutron, however, is not a charged particle. So it can penetrate a long distance without anything happening to it at most time. The longest distance it can go is 40 cm on average in Silicon based on Blackwall theory as discussed in the last lecture. So the likelihood of a neutron can hit a silicon atom in a 10-um device is very low. But when it happens, there will be a nuclear reaction between the neutron and silicon atom. The silicon atom will break apart and create three protons, a C-12, and a few α-particles. Therefore, once nuclear reaction happens, the device is guaranteed to fail.
In order to calculate the probability of failure due to particles from a certain source, we must know three things – the flux of particles from the source, and the efficiency of electron/hole pair generation due to each particle, and finally, the critical charge necessary to upset operation. Let us being with calculating the flux. We will derive the Bethe formula for the efficiency of charge generation in the next chapter.
Comic Ray : Let’s first talk about the cosmic ray. It consists of 92% proton, 6% α-particle (or 70% proton, 30% neutron). An important fact to know is that the cut-off of cosmic ray to reach the ground is 1 GeV. Any ray below this energy will be turned around by the earth’s magnetic field. As the plot shown in Figure. 37.2, the part we are primarily interested in is a small region on the top. The letters P, α, L, H and M stand for proton, α-particle, Lithium, Hydrogen, and Magnesium respectively. Interestingly, the
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scattering time for these particles is 300 million years in the space. The reason is that the density of them in cosmos is 1.7 × 10 g/cm . So we may find only single one particle in miles and miles.
Solar Wind . Next, we will take a look at solar wind. Unlike the earth, gas-like materials form the sun. So what actually happens is that the equator of the sun moves faster than the poles by around eight days. It results in tangled magnetic field that allows big holes, which is referred as the black sunspots. These are opening on the sun, through which the gas can escape. The energy density at surface is 1365 W/cm . But only a small portion of the solar wind can reach the earth and the other can deflected by the earth’s magnetic field. The process takes approximately 4 days.
Figure. 37.2. Energy vs. Flux intensity (comic ray)
One of the most interesting curves generated in the last century is shown in Figure. 37.3.
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Figure. 37.3. Radiation Flux Density vs. Altitude
The left side of the curve is the ground and the right side is the surface of atmosphere. The pressure measured by Hg presents the altitude. As shown, there is a peak of the flux near the surface of the atmosphere. The reason is that when the primary particles strike the atmosphere, it generates a creation number of electron-hole pairs with very high energy. Subsequently, a secondary generation that produces even much more pairs occurs due to these high-energy carriers. As the altitude goes down, recombination is dominant. It is the reason why the intensity decreases exponentially as approach the ground. A noteworthy fact is that a flying plane is near the height of the intensity peak, which explains why there is a guaranteed failure in one flight. Moreover, the source of the radiation damaging the satellites is solar wind due to similar reasons. We also can interpret the altitude dependency of radiation flux mathematically.