Rotational energy level
Molecular rotations require little energy to excite them. Pure rotation spectra occur in
the microwave region of the spectrum (~1 - 200 cm-1
). It is important to note that a molecule cannot rotate about some arbitrary axis - the principle of conservation of
angular momentum dictates that only a few rotations are possible. In general, rotation
must be about the centre of mass of a molecule, and the axis must allow for
conservation of angular momentum. In simple cases, this can often be recognised
intuitively through symmetry - such as with the water molecule.
A pure rotation spectrum can only arise when the molecule possesses a permanent
electric dipole moment. Like with vibrational spectroscopy, the physical effect that
couples to photons is a changing dipole moment. Since molecular bond lengths remain
constant in pure rotation, the magnitude of a molecule's dipole cannot change.
However, since electric dipole is a vector quantity (it has both size and direction)
rotation can cause a permanent dipole to change direction, and hence we observe its
spectra. Since homonuclear molecules such as dinitrogen N2
have no dipole moment
they have no rotation spectrum. Highly symmetric polyatomic molecules, such as
carbon dioxide, also have no net dipole moment - the dipoles along the C-O bonds are
always equal and opposite and cancel each other out. It is important to recognise also
that if a molecule has a permanent dipole, but this dipole lies along the main rotation
axis, then the molecule will not have a rotational spectrum - such as for a water
molecule.
In pure rotational spectroscopy for a simple diatomic molecule, the energy levels - as
displayed below - are given by EJ = BJ (J+1), where J is the rotational quantum
number, B is the rotational constant for the particular molecule given by
I
h
B 2
2
8
with the unit of Joules, where I is the moment of inertia, given by I = μr
2
- where r is
the bond length of this particular diatomic molecule and μ is the reduced mass, given
by μ = m1m2
/ m1 + m2
.
Most energy level transitions in spectroscopy come withselection rules. These rules
restrict certain transitions from occuring - though often they can be broken. In pure
rotational spectroscopy, the selection rule is ΔJ = ±1.
A vibrational spectrum would have the following appearence. Each line corresponds to
a transition between energy levels, as shown. Notice that there are no lines for, for
example, J = 0 to J = 2 etc. This is because the pure rotation spectrum obeys the
selection rule ΔJ = ±1. The energy gap between each level increases by 2B as the
energy levels we consider increase by J = 1. This leads to the line spacing of 2B in the
spectrum. Each transition has an energy value of 2B more than the previous transition.
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