Abstract. Charge symmetry breaking in the A = 4 hypernuclear system is reviewed. The data on binding energies of the mirror nuclei and hypernuclei are examined. At the Mainz Microtron MAMI the high-resolution spectroscopy of decay-pions in strangeness electro-production is used to extract the Λ hyperon ground state binding energy in 4 Λ H. This binding energy is used together with the 4 Λ He ground state binding energy from nuclear emulsion experiments and with energy levels of the 1 + excited state for both hypernuclei from γ-ray spectroscopy to address the charge symmetry breaking in the strong interaction. The binding energy difference of the ground states in the mirror pair is reduced from its long accepted value ΔB 4
Charge symmetry and charge independence breakingThe nuclear interactions have a small charge-dependent component breaking the near symmetry between protons and neutrons in their interactions and their contributions to nuclear properties. However, the concept of charge symmetry is quite useful in describing many facets of nuclear physics, e.g. the observation of nearly identical levels and spin-parity assignments of excited nuclear states in mirror nuclei. The fundamental cause of the charge dependence of nuclear forces, i.e. charge-symmetry breaking (CSB) and charge-independence breaking (CIB), is due to the differences in the up and down quark masses and due to electromagnetic effects.A very important consequence of CSB is the fact that neutrons are heavier than protons (by only approximately ΔM/M ∼ 0.1 %) despite the larger electrostatic repulsion of the quarks inside the proton that would make the proton heavier. The decay of free neutrons (allowed by their larger mass) during the primordial nucleosynthesis left a large fraction of protons unbound, now existing mainly in the stars and providing a slow-burning fuel for the universe. The very reverse, protons being heavier than neutrons, would be a disaster for life as we know it.