30 November 2025 to 5 December 2025
Building 40
Australia/Sydney timezone
AIP Summer Meeting 2025 - University of Wollongong

Metastable Helium Atom Production by Positron Impact

4 Dec 2025, 13:55
15m
Hope Theatre (Building 40)

Hope Theatre

Building 40

University of Wollongong Northfields Avenue Wollongong NSW 2522
Contributed Oral Atomic and Molecular Physics Atomic and Molecular Physics

Speaker

Mr Liam Wymer (Research School of Physics, Australian National University)

Description

We have adapted one of the ANU positron beamlines, which use a Surko buffer gas trap and a strong magnetic field, to enable direct measurements of reaction products from atomic collision experiments. An effusive gas jet was added to the beamline, which allowed us to cross a helium beam with the high-resolution, pulsed positron beam. Long-lived (metastable) neutral excited helium atoms formed in the positron collisions were detected by a strategically positioned channel electron multiplier (CEM).

Helium has two long-lived metastable states (2$^3$S and 2$^1$S), though only the 2$^1$S state is directly accessible to positrons. Excitation of the 2$^3$S state requires a spin-flip from the ground state and since positrons do not have access to the exchange interaction like electrons, they instead require the spin-orbit interaction, which is both weaker for positrons than electrons and weak for helium in general (spin-orbit scales roughly with atomic number Z$^4$). Thus, we expect only 2$^1$S excitation.

In the experiment, a pulsed positron beam crosses a He beam and metastable atoms are detected with high efficiency (~ 90%) by a CEM. Time-of-flight techniques and electrostatic retardation are used to separate the relatively slow He atoms from faster reaction products (ions, positrons, electrons, positroniums). The 2$^1$S state has a lifetime of ~ 19 ms, which is far longer than the average flight time of the atoms from the collision volume to the detector (~ 40 $\mu$s).

Excitation of the He 2$^1$S state as a function of incident positron energy will be presented and compared with previous measurements using conventional gas-cell arrangements and with theory.

Authors

Joshua Machacek (Research School of Physics, Australian National University) Mr Liam Wymer (Research School of Physics, Australian National University) Sean Hodgman (The Australian National University) Mr Sharan Kumar (Research School of Physics, Australian National University) Stephen Buckman (Australian National University) Prof. Tim Gay (Dept of Physics and Astronomy, University of Nebraska)

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