anorlunda said:
You can see some liquid drop videos of nucleus shape changes, but the thread says that such simulations are not supported by QM calculations.
You can
of course do QM calculations that show non-spherical nuclei. In fact, the very thread you just linked to has an example from me -- I linked to a Time Dependent Hartree Fock calculation of 40Ca + 238U! You can clearly see the deformed nature (cigar shaped, as V50 points out) of 238U and the spherical structure of 40Ca.
And yes, nuclei have a shell structure, but it's rather complicated, as you don't have a nice 1/r potential. The shell structure is very important though - just like the noble gasses in chemistry, you have equivalently well bound nuclei - "doubly magic nuclei" - like
48Ca and
208Pb - where both the neutrons and protons are in closed shells. In fact, it's only near these closed shells that you're guaranteed to get spherical nuclei! In fact, if you didn't have the shell model, we'd have no explanation why the superheavy isotopes can exist at all - it's the shell structure that gives you enough stability.
Now, on the other end of the scale, we can talk about clustering in very light nuclei. Rather than talking about shells, you can talk about, say,
7Li as if it were a somewhat loosely bound ##\alpha## and ##t## pair. (That is, a large part of the ground-state wavefunction has an ##\alpha## and ##t## structure).
9Be is thought of as ##\alpha + \alpha + n##. And so on - this is where halo nuclei can appear. For instance,
11Li can be thought of as a
9Li core + 2n halo. It has a cross section comparable to
208Pb! Tl;dr - nuclei are complicated, but interesting.
But of course, in all this, you can't "tag" individual protons and neutrons inside the nucleus, you're always talking about wavefunctions.