“…This transition to the final state can be realized in many ways, such as the sequential two-body decay via an intermediate resonance, the virtual sequential two-body decay via the correlated continuum of an intermediate nucleus, the direct decay into the three-particle continuum or its particular diproton (' 2 He') limit of two sequential two-body emissions. Different types of theoretical approaches exist which focus on the three-body decay width: the extended R-matrix theory [28,29], the real-energy continuum shell model (the so-called Shell Model Embedded in the Continuum (SMEC) [30,31,32,33,34]) describing sequential two-body emission, virtual sequential two-body emission and diproton emission via two sequential two-body emissions [33,34], the Gamow Shell Model (GSM) with no separation between two-and three-body decays from the multiparticle continuum [35], the three-body models with outgoing flux describing direct decay into the continuum [36], the three-body models combined with complex coordinate scaling [37], or the Faddeev equations combined with either outgoing flux or complex scaling [38].…”