Positron beams, then and now

There have been positron beams in use at UCL since the early 1970’s since the first efficient positron moderator was discovered there by Paul Coleman, Karl Canter and co-workers [http://iopscience.iop.org/0022-3700/5/8/007]. The photograph below was taken in 1996, and shows a positron beam used in Dr David Cassidy’s PhD thesis (Positronium formation at surfaces and studies towards the production of cold antihydrogen, supervisor Mike Charlton, 1999). This beam, which is no longer operational, used a tungsten mesh grid as a moderator and produced around 1000 positrons/second. One can see a large diffusion pump at the lower end, and the black magnet coils used to guide the beam.
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Things have changed quite a lot since those days. The current setup in our lab (shown below) at the moment uses a rare gas solid moderator (neon) and produces more than 5 million positrons/second. There are four main sections to this beamline, (1) the shielded Na source and moderator that produces positrons, (2) the positron buffer gas trap that provides the pulsed beam (5 ns wide pulses with 500,000 positrons each), (3) the Ps spectroscopy chamber where our Ps producing silica target is placed and (4) the laser table, where our Nd:YAG pumps our Sirah pulsed dye laser and our Radiant pulsed dye laser. Together all these components are used to produce Rydberg positronium in a two step photon process. There are no more diffusion pumps to be found!

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Welcome to the new blog of the UCL Positronium Spectroscopy Group!

Based in the Physics Department at UCL, we are building a new experiment to create a pulsed source of positronium atoms. These are exotic atoms, made half of matter (an electron) and half of anti-matter (a positron).

Once we have made these atoms we will drive them to highly excited Rydberg states with pulsed lasers, and then manipulate them with electric fields, eventually making a slow beam for a precise gravity measurement, addressing the question of how anti-matter interacts with gravity.

We are just starting out on this project, and along the way there will be many experiments to perform, and many questions to answer: how can we make an intense source of positrons? How can we cool the positrons? What is the most efficient way of making positronium, and then exciting them to Rydberg states? How does anti-matter interact with gravity?

Over the coming months and years we will answer these questions, and many more! So come back to our blog and see how we’re getting on…