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Atomic collapse is a novel electronic phenomenon that occurs when relativistic electrons move in the vicinity of highly charged Coulomb centers. It was first observed by the Crommie group through the manipulation of charged atoms on graphene field-effect transistor (FET) devices.1 The basic idea was predicted 75 years ago and addresses the fundamental quantum mechanical question of what happens when the positive charge in the nucleus of an atom (+Ze) gets extremely large.2 In non-relativistic quantum mechanics the binding energies of atomic levels simply get deeper (and the wavefunctions more localized) as Z increases, corresponding to semi-classical circular orbits of smaller and smaller radii. When relativity is taken into account, however, the picture changes dramatically due to the presence of the Dirac sea (i.e., the negative energy continuum). When the atomic binding energy gets large enough (Fig. 1a)the Coulomb potential of the nucleus is predicted to rip an electron from the Dirac sea and leave behind a hole (i.e., a positron) (Fig. 1b). The difficulty in observing this novel type of electron-positron pair production is that for it to occur the positive charge on the nucleus must surpass a “critical charge” Zc = 1/α = 137, where α is the fine structure constant α = e2/ħc = 1/137. Creating a “supercritical” nucleus with Z > 137, however, is extremely difficult since such heavy nuclei are unstable, and so this phenomenon has not yet been unambiguously observed in bare atoms or nuclei.