The energy of the orbital of a one-electron atom depends on n only, but the shape depends on three quantum numbers: n, l, and ml. Where
When describing any element other than Hydrogen, the structure of that atom will by more complicated than the simple Bohr picture can predict.
We will treat the way in which the whole atom behaves as the cumulative behavior of each individual electron. Each individual electron is a 'wave' and has a wavefunction, which may be described approximately with at orbitals of Hydrogen. The energy of each of these wavefunctions (orbitals) is qualitatively different from that of the one-electron atom, however, because of the discriminatory effects of electron-electron repulsion.
We can now 'build' atoms by filling the orbitals expected from a one-electron model 'perturbed' by what we know about electron-electron repulsion. This is called atomic 'Aufbau'. The first elements are easy if we postulate two 'rules':
If it were not for the spin (the 'up' or 'down' flavor) of the electron, many electron atoms would be filled by putting one electron in each hydrogen-like orbital, to satisfy the Pauli exculsion principle. But, as it is, each spatial orbital can two electrons in it, as long as they are spin paired (one up, one down)
Be aware of the notation that explicitly ignores closed inner shells. As these orbitals deep in the atom are significantly more stable than the frontier or valence orbitals, they do not significantly contribute to chemical bonding.
In general we fill orbitals with electrons from the lowest energy (most satble) orbitals up. We put electrons in singly at first when degenerate orbitals are being filled as this minimized electron electron repulsion. Electrons are paired in degenerate orbitals only when there is no room to put any more in unpaired. The energy of an atom with several unpaired electrons in degenerate orbitals is lowered when the unpaired spins are parallel.
Half-filled and completely filled subshells are particularly stable due to
a Quantal phenomena called 'exchange'.
This phenomenon contributes to the stability of parallel unpaired spins in
degenerate orbitals as well as leads to some filling 'exceptions'
in the middle and end of the first transition
period. Check out Cr and Cu, for example: You can still see these type of exceptions higher still in atomic number
(and thus total number of electrons in the atom
The electron configuation of the elements are what give rise to the shape of the
periodic table and the names of the blocks that compose it.
The filling exceptions due to the stability of half filled and completely
filled subshells leads to some elements at the middle (Cr) and the end of the
transition blocks (Cu) having chemistry somewhat like the alkali metals, but for odd
exceptions like this it is not worth rearranging the traditional the Periodic Table.
It is expected that you be able to determine the lowest energy electronic
configuration of any neutral atom in the Periodic Table.
Let's go crazy and list all the elements...
PJ Brucat ||
University of Floridai