The Coulomb de-excitation (Table 1), where the transition energy is shared between the colliding particles, is an important acceleration mechanism producing 'hot' (eV) exotic atoms (see Fig. 4a). The highly-energetic atoms were discovered experimentally in [52], and a multicomponent structure of the energy distribution was found in [46]. Recent experiments in liquid and gaseous hydrogen [47,48] found the shape of the kinetic energy distribution to be consistent with the Coulomb mechanism. The cascade calculations [29] show that the atoms with kinetic energy eV are not significantly decelerated between the Coulomb de-excitation and the nuclear reaction. For the atoms with eV the deceleration is important and the Coulomb peaks are expected to be smeared out.
The earlier calculations of the Coulomb transitions [16,17,18,19] were rather controversial. The latest calculations [20,21,22] seem to clarify the theoretical picture. This removes one of the uncertainties in the cascade calculation of the past where a Coulomb rate-tuning parameter was used to normalize the calculated high-energy component to the measurements in pionic hydrogen [29]. It is not excluded that the Coulomb de-excitation can be part of a multistep process. For instance, the formation of excited molecular states can be followed by a Coulomb-like decay [2,54,55].