The ATHENA Positron Accumulator           

   The positron is the anti-particle of the electron. As such is was the first anti-particle to be discovered, only a few years after Dirac's prediction of its existence in 1930 (the figure to the right shows a cloud chamber photo of Andersons first detection of a poistron from 1932. click on the image for a larger version and a desciption). It took many years before positron physics really took off. Only in the 1970's, with the invention of slow positron beams, did positrons become a precision tool in a vide variety of fields of physics and chemistry. First experimental evidence of positrons The ATHENA Positron Accumulator accumulates its positrons from a slow positron beamline that is a technological evolution of those early concepts of how to make a positron beam. Positrons are not a common occurrence in nature, just like any other form of antimatter. However, because electrons have a much lower restmass than e.g. protons, it is relatively easier to create positrons. Now as then there are two ways of generating positrons: By pair creation or from certain kinds of radioactive sources. Pair creation involves collisions with high enough energy that an electron-positron pair can be formed. If we use Einstein's famous formula:
We find that the electron rest mass is equal to 511 keV of energy. Since the restmass of the positron is identical, the collision will need to have a surplus of energy of at least 1022 keV for pair creation to take place.
   The other method for generating positrons is the one we use at the ATHENA Positron Accumulator because it is technically simpler. It only involves having a radioactive isotope of the right kind. Most people who have had physics in school know that in radioactive β decays what is really emitted is a high energy electron. This is more correctly called a β- decay since there is another kind as well. There are a few isotopes that decay by what is know as a β+ decay. This is similar to β- decays except that the particle emitted is not an electron but a high energy positron. The most commonly used isotope for making positron beams is  Na-22. This is convenient as it has a lifetime of 2.6 years, which is long enough that you don't need to get  a new radioactive source all the time, yet short enough that the specific activity is rather high.
   Unfortunately, regardless of whether one gets one's positrons from one or the other mechanism, they both yield positrons with a very wide variety of energies. In order to make a positron beam, a narrow energy spread is necessary, the narrower the better. This was a stumbling block that delayed the development of positron beams for so long. The solution turned out to be to stop the positrons in a solid. The trick is that once the positrons have stopped in the solid they will start a random walk diffusion around the solid. If the solid was made with the right thickness, there is a small chance that these slow positrons reach the surface of the solid before they annihilate. Once they reach the surface, a surprisingly wide variety of materials will kick them out. This is surprising because materials do not normally kick out electrons. After all there are electrons everywhere and they don't seem to leak out unless the material has been put under high voltage or something similar. So solids are generally very good at holding on to electrons but precisely because of this they are not very good at holding on to positrons; after all they have the opposite charge. Solids that do this trick are called positron moderators.
   The main technological development of positrons beams since the 1970s has consisted of finding materials that are ever more efficient at slowing down and emitting positrons. At present the best such solid is Neon.
Unfortunately neon is a gas at room temperature and only becomes a solid at very low temperatures. Therefore our radioactive source and its surroundings are kept at about 5-6 K or  -268 °C. We then let in neon gas and a layer of solid Neon grows on the cold surfaces. In this way about 3-4 ‰ of the positrons made in the radioactive source emerge and are captured in what we now can call a mono-energetic positron beam. This beam is guided to the main part of the Positron Accumulator by a magnetic field. Using a radioactive source with a source strength of 40 mCi we end up with a positron beam of about 5 million positrons per second.
   Since a positron beam originating from a radioactive source is by nature continious we can not use a method with opening and closing a gate electrode like we do for the antiproton pulses. Therefore we must use another method for capturing the positrons. Basically, to trap a particle it has to loose energy so it is no longer free to fly back out of the trap. This energy loss we achieve in the Positron Accumulator by having the positrons collide with gas molecules following a method first developed by the Surko research group at the University of California, San Diego.
Positron Accumulator





  Quicktime movie illustrating the transfer of positrons from the Positron Accumulator to the Mixing Trap
 
 
 

LVJ - Last  modified September 11, 2002