Speaker
Description
Using low-energy antiprotons, the antiProton Unstable Matter Annihilation (PUMA) experiment [1] aims to probe the isospin composition in the density tail of radioactive nuclei. For this purpose, the isotopes of interest are trapped with antiprotons in a dedicated Penning trap. By measuring the charge of the reaction products of the antiproton-nucleon annihilation, the experiment will provide the neutron-to-proton annihilation ratio as a new observable for nuclear structure theory. The experiment allows to investigate neutron skin formation of neutron-rich nuclei as well as halo nuclei. In a first measurement campaign before CERN’s long shutdown 3 (LS3), the PUMA collaboration plans to demonstrate this technique using hydrogen and helium isotopes. Furthermore, e.g.
This talk focuses on the future prospects of PUMA beyond LS3 and further. A currently planned future update is the implementation of a laser-ablation ion source, which enables the investigation of a broader range of stable nuclei. This modification will allow to study for example the proton-closed shell isotopic chains of
A possible future path of PUMA includes the study of hypernuclei. The extent to which the formation of antiproton atoms leads to the production of hypernuclei has been investigated in simulations [2]. Only using
[1] PUMA Collaboration, PUMA, antiProton unstable matter annihilation. Eur. Phys. J. A 58, 88 (2022)
[2] Schmidt, A., Gaitanos, T., Obertelli, A. et al. Production of hypernuclei from antiproton capture within a relativistic transport model. Eur. Phys. J. A 60, 55 (2024)