Chemistry Reference
In-Depth Information
Table B.1 Details of quantum numbers associated with energy levels of an isolated atom
Name
Symbol
Values allowed
Physical property
Principal
n
n = 1, 2, 3, ...
Determines radial extent and energy
Orbital
l
l = 0, 1, ... , ( n 1 )
Angular momentum and orbit shape
Magnetic m
l , l + 1, ... , l 1, l
Projection of orbital angular momentum
along quantisation axis
1
2
1
2
Spin
s z
and
Projection of electron spin
along quantisation axis
+
Table B.2 Spectroscopic labels associated with different orbital
quantum numbers (atomic subshells) in an isolated atom
Orbital quantum number l
0
1
2
3
4
5
Spectroscopic label
s
p
d
f
g
h
The degeneracy we have found for states with the same principal
quantum number n , but different orbital quantum numbers l ,isan
'accidental' consequence of the hydrogen atompotential V
(
r
)
, which varies
as 1
r . This 'accidental' l -degeneracy is removed when most other central
potentials are used in (B.11), including the potential of any multi-electron
atom. Each shell of states with particular principal quantum number n
therefore breaks up into a set of subshells in the multi-electron atom, with
a different orbital quantumnumber l associatedwith each subshell. Histor-
ically, the states in different subshells were identified using spectroscopic
techniques, and the different subshells were given the spectroscopic labels
shown in Table B.2. States with n
/
=
1and l
=
0 are referred to as 1s states,
while states with n
=
2and l
=
0 and 1 are referred to as 2s and 2p states,
respectively.
We recall from eq. (B.11) that the effect of increasing angular momentum
(increasing l ) is described by an increasingly strong centrifugal potential
barrier (proportional to l
r 2 ) which pushes the electron away from
the nucleus. As a consequence, the 2s wavefunction (with l
(
l
+
1
)/
0) will have
larger amplitude close to the nucleus than does the 2p wavefunction (with
l
=
. The 2s states therefore experience on average a stronger attrac-
tive potential, and so will be at a lower energy than the 2p states. The
energies of the different electron states in a multi-electron atom are clearly
affected by the presence of other electrons. The 1s orbital will always have
lowest energy and, because it largely experiences the full nuclear attrac-
tion (proportional to Ze for atomic number Z ), its binding energy will be
close to Z 4 times the binding energy of the 1s hydrogen state. The 1s states
will then partially screen the higher lying levels, modifying their energies
accordingly.
=
1
)
 
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