nuby said:
So if the conditions are right then could you say there is no limit on the mass/size of an atom?
If you exclude the concept of neutron stars as "giant nuclei",
there is a theoretical limit on the mass of an atom, but it is comparatively little known.
Let us assume the following : the EM coupling constant is exactly 1/137, and the nuclei are point-like (we remove those after, it is only for the sake of explanation). The coupling to the EM field does not only involve the coupling constant, but also the charge Z. At Z=137, the perturbative series can not converge anymore. Physically, the EM vacuum becomes unstable : an electron from a virtual pair is absorbed by the nucleus, and the positron flies away. This imposes a maximum Z. Together with the neutron drip line, which imposes a maximum N for each Z, this makes an absolute maximum A possible for an atom.
When you remove the simplifying conditions, you make model-dependent evaluations all pointing towards a maximum Z around 185. For one thing, this is very high compared to what we can do today, and much higher than the anticipated next island of stability. For another think, this instability is due to EM and not to the strong force, so technically, people would still call nuclei with very high Z (larger than this limit) unstable "bound states under QCD".
Note that the neutron star limit occurs much much much higher in A, and is somehow irrelevant here.
This mechanism is known as supercritical binding, was first discussed by the russian school following Pomeranchuk, and if you are interested in it (or want to know why it is interesting) you can read Gribov conception of quark confinement, which stems from the (possible) same phenomenon in QCD with light (physical) quarks.
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"Anomalous Positron Peaks from Supercritical Collision Systems", Phys. Rev. Lett. 54, 1761 - 1764 (1985)
Narrow positron peaks are observed in five supercritical collision systems with combined nuclear charge 180<~Zu<~188. The peaks do not originate from nuclear internal pair conversion and their production appears to occur in a narrow projectile-energy interval near the Coulomb barrier. The line shapes are consistent with emission by a source moving with the c.m. velocity. Particularly notable is an apparent independence of the peak energies on Zu. These observations are discussed in the context of the spontaneous decay of the QED vacuum and other new potential sources of line positron spectra.