14.3 Physics applications 519
even)orungerade (German for odd) that indicates whether the wavefunction is even or
odd under the inversion σ : r (→−r.
The buckyball is roughly spherical, and the lowest 25 states can be thought of as being
derived from the L = 0, 1, 2, 3, 4 eigenstates, where L is the angular momentum quantum
number that classifies the energy levels for an electron moving on a perfect sphere. In
the many-electron ground-state, the 30 single-particle states with energy below E < 0
are each occupied by pairs of spin up/down electrons. The 30 states with E > 0 are
empty.
To explain, for example, why three copies of T
1
appear, and why two of these are T
1u
and one T
1g
, we must investigate the manner in which the 60-dimensional Hilbert space
decomposes into irreducible representations of the 120-element group Y
h
. Problem 14.23
leads us through this computation, and shows that no irrep of Y
h
occurs more than three
times. In finding the energy levels, we therefore never have to diagonalize a matrix
bigger than 3-by-3.
The equality of the energies of the h
g
and g
g
levels at E =−1isanaccidental
degeneracy . It is not required by the symmetry, and will presumably disappear in a
more sophisticated calculation. The appearance of many “accidental” degeneracies in an
energy spectrum hints that there may be a hidden symmetry that arises from something
beyond geometry. For example, in the Schrödinger spectrum of the hydrogen atom all
states with the same principal quantum number n have the same energy although they
correspond to different irreps L = 1, ..., n −1ofO(3). This degeneracy occurs because
the classical Kepler-orbit problem has symmetry group O(4), rather than the naïvely
expected O(3) rotational symmetry.
14.3.2 Vibrational spectrum of H
2
O
The small vibrations of a mechanical system with n degrees of freedom are governed by
a Lagrangian of the form
L =
1
2
˙x
T
M ˙x −
1
2
x
T
V x (14.47)
where M and V are symmetric n-by-n matrices, and with M being positive definite. This
Lagrangian leads to the equations of motion
M ¨x = V x. (14.48)
We look for normal mode solutions x(t) ∝ e
iω
i
t
x
i
, where the vectors x
i
obey
−ω
2
i
M x
i
= V x
i
. (14.49)
The normal-mode frequencies are solutions of the secular equation
det (V − ω
2
M ) = 0, (14.50)