sokrates said:
What is the basis to say that the wavefunction of a multi-electron system is the product of individual wavefunctions of the electrons that form the system?
It follows from the antisymmetry requirement/Pauli exclusion principle for fermions. It's follows fairly easily that the simplest way to satisfy that requirement is to describe the wave function in the term of a Slater determinant.
In other words, how does theory ensure that the multi-electron wavefunction is seperable into variables r1 and r2?
It's not. It's the assumption that the wave function can be described using a single determinant of one-electron functions which is the essence of the Hartree-Fock approximation.
Even in Hartree form (where things like exchange interaction and exclusion principle is not readily captured)
That would be a Hartree product. (which doesn't satisfy antisymmetry) Since the Hartree-Fock method uses a Slater determinant, so it'd actually be:
\Psi(r1,r2) = \phi_1(r_1)\phi_2(r_2) - \phi_1(r_2)\phi_2(r_1)
(where the coordinate r is assumed to include spin)
Hartree-Fock
does get exchange right. (Within the constraint of a single-determinant description). It's implicit in the derivation. It's the correlation energy that's completely neglected.
I learned from Wikipedia that this is really an ansatz in the HF theory. But is there any convincing reason that the well-versed quantum camp could deliver here?
Well, as stated above, it's an easy way to satisfy the antisymmetry requirement. Second, it's a fairly decent approximation, given the relative simplicity of it.
The biggest problem is getting the kinetic energy of the electrons. That's the single biggest energy term. Due to correlated motion, that's a many-body problem, and quite difficult to solve. So how would you, for instnace, calculate the motion of the planets around the sun? You'd probably go with first describing them as moving independently of each other and then include their effect on each other as an averaged effect. That's essentially what Hartree-Fock does. IOW: Its kinetic energy is exact for non-interacting or infinitely-slowly-moving electrons. That's a good approximation, because it gives most of the kinetic energy. The effects of correlated motion are very small in comparison.
Improving on it is of course the main deal with QC. For instance there's Møller-Plesset perturbation theory, which works by treating the correlation energy as a perturbation, and Configuration Interaction, which works by using multiple determinants.
Now you don't
have to do it this way. For instance, Hylleraas used the Ritz variational method very early, 1929, to find the ground-state energy of Helium, using a total wave function parametricized in terms of r_1, r_2, r_{12} (no spin coordinates!) directly, by re-expressing the Hamiltonian in these terms and solving the variational problem, with the symmetry requirement built in via constraints and integration limits. Very clever and extremely accurate. But that method is notoriously difficult to extend to systems of more than two electrons.
'Orbital-less' DFT methods (starting with the old Thomas-Fermi model) don't use single-electron descriptions either. But they tend to fail badly due to the difficulty of getting the kinetic energy. It was Kohn-Sham's Nobel-prize winning method that made DFT accurate enough to be usable, and that entailed re-using the Hartree-Fock approach to get the 'non-interacting' kinetic energy, and treating exchange and correlation as a pseudopotential. (and it's usually that single part that's referred to as a 'functional' now) Exchange was lost because you're not solving the Schrödinger equation; Kohn-Sham orbitals are not 'real' orbitals. (although debate rages over whether or not they can be ascribed
some physical significance or not)