EGS: Lab Activities. Virtual Visitor Center at SLAC

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EGS Lab Activities (SLAC VVC) http://www2.slac.stanford.edu/vvc/egs/lab/lab.html of 2007-0-8 0: AM Virtual Visitor Center at SLAC EGS: Lab Activities Photons interact with material in many ways, but the three most dominant mechanisms for energies above a few kev are:. 2.. Photoelectric Effect The photon's energy is totally absorbed by the atom and an inner-shell electron is ejected. Immediately following this, an outer shell electron makes a transition to fill the gap in the inner shell and in the process emits photons (X-rays). Compton Scattering The photon scatters off an electron in an outer orbit of an atom and the energy of the incident photon is then shared between the outgoing electron and the scattered photon. Pair Production The photon "materializes" into an electron and its antiparticle, a positive electron (a positron ), while in the presence of the electromagnetic field of the nucleus. The above three mechanisms account for more than 99% of the interactions that take place between photons and matter. Which of the interactions is the most important at any given time depends on the energy of the photon and the medium in which it is traveling. However, these interactions are quantum in nature. This means that a specific interaction is never guaranteed, it is simply more (or less) probable than the others (depending on energy and material). The EGS program simulates this quantum nature by randomly selecting which interaction, if any, occurs with the correct (average) probabilities. In the following exercises, you will learn how to recognize these three basic interactions using the EGS computer code, which we have set up to allow you to create visual images of particle tracks in color. In particular, you will learn about: Interaction distances (the average distance to a collision). Which interaction type dominates. The random, but statistically determined, behavior of nature. Now, go to: Exercise : Interactions of 0. MeV photons in aluminum and lead Stanford Linear Accelerator Center, Menlo Park, CA Operated by Stanford University for the U.S. Dept. of Energy

EGS Lab Activity: Exercise, Interactions of 0. MeV photons in alu... http://www2.slac.stanford.edu/vvc/egs/lab/exercise.html of 2007-0-8 0:0 AM Virtual Visitor Center at SLAC EGS Lab Activity - Exercise Interactions of 0. MeV photons in aluminum and lead Figures through are provided for you so that you can predict how photons will interact with matter in an average sort of way. The EGS code will then allow you to visualize these events in a statistical sense, and you judge whether or not things look like what you predict. Click on the images below for a larger view. Figure - Al and Pb Figure 2 - Al Figure - Pb In this first exercise we will guide you through the use of the three figures by filling in some tables for you. However, you will run the EGS code. In Exercise 2, we will increase the energy of the photon to 0 MeV and let you do all the work! We have purposely chosen two types of materials for this study, one with a low atomic number (Al, Z=, r=2.70 g/cm ), and one with a high atomic number (Pb, Z=82, r=. g/cm ), so that you can predict beforehand and visualize afterwards how the choice of medium affects interactions. Using Figure, we have determined the average distance, l (cm), that a 0. MeV photon is expected to travel before interacting in either aluminum or lead, and we have put our numbers in the table below. Table Al Pb l (cm). 0.2 P int 0..0 What this tells us is that on average a 0. MeV photon will travel. cm in aluminum before experiencing an interaction, but it will travel about 0.2 cm for this to happen in lead. Let's now choose a thickness for the slabs of material, which we will soon have EGS throw photons at. From Table, a good guess might be to pick an aluminum thickness of 2 cm, because with a l of. cm, we can anticipate that some of the photons might pass right through the slab without interacting at all. On the other hand, the l for lead is 0.2 cm, suggesting just the opposite--most of the photons impinging upon the lead will probably interact with it. Fortunately, we have a simple formula for also determining the probability that a photon will interact as it passes through a slab of material: P int = e -t/l = probability to interact

EGS Lab Activity: Exercise, Interactions of 0. MeV photons in alu... http://www2.slac.stanford.edu/vvc/egs/lab/exercise.html 2 of 2007-0-8 0:0 AM In this equation t (cm) is the thickness of the slab and l comes from Table. As you may have guessed, the second row in our table contains values for P int, obtained by using this formula (try it yourself). So what does it tell us? Well, we should expect that about % (P int = 0.) of the time the incident photons will interact within 2 cm of aluminum, which means that 7% of them will pass on through without doing anything. On the other hand, 2 cm of lead seems to be a "show stopper" (pun intended), for the prediction is that 00% (P int =.0) of the time they will interact. But remember, life in the atomic world is based on probabilities, and you can bet that if we throw enough photons at the lead slab, even one that is this thick, a few will occasionally get through. This is a statistical world that we live in and the best we can do is to make predictions about what will happen on average. EGS is designed to demonstrate this for us. Now, before moving on to the EGS "experiment" that we are going to ask you to perform, we need to gather a little more information. As we have been saying, nature not only randomly decides when a photon is going to interact with matter, it also chooses the type of interaction in a random way. The actual physics itself is based on part of the standard model known as quantum electrodynamics (QED), and with it we can make plots like those provided to you in Figure 2 and Figure. The curves in these figures provide us with a way of determining the relative probability e.g., a fraction that lies between 0 and that an interaction, once it occurs, will be one of the three basic mechanisms that we are studying. Again, remember that if there is a 0% chance that a particular interaction occurs, there is a 0% chance that something else could happen. Both cannot happen at the same time. Nature spins its random numbers, and the simulation does the same. So let s continue with our exercise by making use of the two new figures we have provided you. For the 0. MeV photon, we have determined the relative probability (contribution) for each of the three processes for both aluminum and lead, and we have entered this information into Table 2 shown below (note that we are talking about "relative" probabilities and their sum must add up to unity). Table 2 Photoelectric Compton Pair Production Al 0.00.0 0 Pb 0.78 0.22 0 Table told us that in a 2 cm slab of aluminum we can expect % of the photons to interact. Table 2 tells us to expect that 00% of the time interactions will be of the Compton variety (photon scatters off an orbital electron of an atom and the two particles share the incoming energy as they make their way through the rest of the material). Let s have the EGS code demonstrate this for us before we go any further. In the fields on the "EGS to Order" Simulation Tool (this link will open the tool in a new browser window) change the following parameters from their default settings. Parameter Value Particle Type Photon Incident Kinetic Energy. MeV of particles in beam 0 Incident particle vertical spread Uniform in Y axis = On

EGS Lab Activity: Exercise, Interactions of 0. MeV photons in alu... http://www2.slac.stanford.edu/vvc/egs/lab/exercise.html of 2007-0-8 0:0 AM Target Medium Target Length Target Radius Lead 2 cm cm Then you only need to click on the "generate" button and, voila, you get what you see. You can keep clicking the generate button and each time you get a different picture with the same average probabilities... just like nature does it. What about switching the slab from 2 cm of aluminum to 2 cm of lead? Well, just do it! Now, go to: Exercise 2: Interactions of 0 MeV photons in aluminum and lead Stanford Linear Accelerator Center, Menlo Park, CA Operated by Stanford University for the U.S. Dept. of Energy

00 kev/2-cm Al Results for 0 runs with 0 Photons Each Run Interact Penetrate 2 7 7 8 9 0 7 Total 7 Fraction 0.7 ± 0.0 0. ± 0.0 Prediction 0. 0.7 Stanford Linear Accelerator Center 7

EGS Lab Activity: Exercise 2, Interactions of 0 MeV photons in alu... http://www2.slac.stanford.edu/vvc/egs/lab/exercise2.html of 2007-0-8 0: AM Virtual Visitor Center at SLAC EGS Lab Activity - Exercise 2 Interactions of 0 MeV photons in aluminum and lead In this exercise we have simply increased the photon energy from 0. MeV to 0 MeV and we would like you to fill in all the blanks in a new set of tables that we have provided for you (below). Simply use Figures through, like we did in the previous exercise, to complete the tables. Table l (cm) P int Al Pb Table Photoelectric Compton Pair Production Al Pb When you have filled in the blanks, use the "EGS to Order" simulation tool to create the images and see if the images match your predictions. This time we recommend that you select an aluminum thickness of 20 cm and a lead thickness of cm. Why? For no special reason other than it will make the tracks in the EGS images a little easier to discern from one another (wait and you will see what we mean). Also, always choose the radius to be half of the thickness because this gives us a nice aspect ratio for the picture. And, make sure your tracks are "spread out" in the Y axis so you can distinguish them. Stanford Linear Accelerator Center, Menlo Park, CA Operated by Stanford University for the U.S. Dept. of Energy

0 MeV/20 cm Al Results for 0 runs with 0 Photons Each Run Penetrate Compton Pair Production 2 7 8 9 0 Total Fraction Prediction 2 2 0.2 ± 0.0 0.29 7 2 8 0 2 0. ± 0.08 0. ± 0.0 0. 0. Stanford Linear Accelerator Center 27

fig.gif (GIF Image, 0x pixels) http://www2.slac.stanford.edu/vvc/egs/lab/figures/fig.gif of 2007-0-8 0:2 AM

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fig.gif (GIF Image, 0x pixels) http://www2.slac.stanford.edu/vvc/egs/lab/figures/fig.gif of 2007-0-8 0: AM