Minimization - Vibrational
Calculations
Contents
The vibrational frequencies and modes of a molecule are strictly
dynamic properties. However, it is possible to calculate the harmonic
vibrational frequencies of a molecule from just information at its
equilibrium geometry by expanding the potential energy surface as a
Taylor series, truncating after the second term, and considering
infinitesimal displacements. This harmonic approximation usually gives
a good description of the true frequencies and normal modes and can be
quite valuable for tasks ranging from evaluating the quality of a
forcefield to understanding vibrational shifts induced by
conformational changes or other interactions. The harmonic vibrational
frequencies also can be used for zero-point vibrational corrections
and for deriving vibrational free energy contributions. These effects
can be important in comparing conformational energies and rotational
barrier heights.
Following Wilson et
al. (1955), the kinetic energy of the nuclei is:
- Eq. 4-11:
-
where the coordinates represent displacements from an equilibrium
structure. If the 3N Cartesian coordinates are replaced with
3N mass-weighted coordinates as follows:
- Eq. 4-12:
-
where m
is the mass of
the atom associated with the
coordinate,
and
x
runs over the y and z coordinates, as well
as x, then the kinetic energy has the following simple form:
- Eq. 4-13:
-
When the potential energy of the system is expanded as a Taylor series
in the same coordinates, it yields:
- Eq. 4-14:
-
V0 is simply a constant--the energy scale can be
chosen so that V0 = 0. The definition of an
equilibrium structure is that the force on each atom is zero. The
second term in Eq. 4-14 also is zero, leaving
the following second-order approximation of the potential energy:
- Eq. 4-15:
-
Using this approximation of the potential energy in Newton's equations
of motion yields the following simultaneous second-order differential
equations:
- Eq. 4-16:
-
The solution to these equations can be of the form:
- Eq. 4-17:
-
where the Ai are related to the relative
amplitudes of the vibrational motion,
1/2 is proportional to the
vibrational frequency, and
is a
phase. Substituting Eq. 4-17 in Eq. 4-16 yields a set of algebraic equations:
- Eq. 4-18:
-
where
ij is a Kronecker
delta, which equals one if i = j and zero
otherwise. This is an eigenvalue problem that is readily solved
numerically by standard techniques. The second derivatives of the
potential energy, often called the force constants, can be
analytically evaluated for most energy expressions used in molecular
mechanics, in terms of the Cartesian coordinates of the atoms. A
simple transformation to the mass-weighted coordinates then gives the
values needed in Eq. 4-18.
The Discover program calculates the vibrational frequencies by
calculating the second derivative matrix, mass weighting it, and then
diagonalizing it to obtain the eigenvalues. These eigenvalues are then
converted to vibrational frequencies in wavenumbers as follows:
- Eq. 4-19:
-
where the conversion factor F converts the units from kcal
mol-1 to wavenumbers. Of the 3N coordinates used to
calculate the energy and vibrational frequencies, six correspond to
net translations and rotations of the molecule (five for linear
systems). These six modes have no restoring force and therefore have
vibrational frequencies of zero for a minimized structure. Due to
numerical inaccuracies, the Discover program reports these
frequencies with small values, which are typically less than 0.1
cm-1. If the structure is not
perfectly minimized, the first-order terms in the Taylor expansion of
the potential surface in Eq. 4-14 do not
vanish. In turn, they introduce terms that couple the net rotations of
the molecule with the internal motions and both perturb the internal
vibrational frequencies and give apparent frequencies for the three
rotations. Thus, the magnitude of the six "zero" frequencies is a good
indication of the quality of the calculation.
For calculating vibrational frequencies, the structure must be
minimized and the gradients must be zero. This does not mean that the
configuration of the molecule must be at a minimum, but rather that it
must be at a stable point on the surface. If the structure is not at a
minimum, but rather is at a saddle point or transition state in one or
more directions, this is reflected in the eigenvalues and the reported
vibrational frequencies. For a saddle point, at least one eigenvalue
is negative, which means that the curvature of the surface along at
least one normal mode is negative. By convention, the imaginary
frequencies for such modes are reported as negative. Therefore, the
reported vibrational frequencies describe the character of the stable
point on the surface. If all frequencies are real, it is a minimum; if
one frequency is imaginary, the structure is in a simple transition
state; if two or more frequencies are imaginary, a double or more
complicated transition state is indicated. The normal modes
corresponding to the frequencies can be analyzed to understand the
reaction path going through such a transition state.
The quantum mechanical solution for the vibrational energy of a set of
uncoupled harmonic oscillators, which corresponds to the classical
treatment outlined above, is:
- Eq. 4-20:
-
where the summation is over all the vibrational frequencies,
ni is the vibrational quantum number for each
vibration, h is Planck's constant, and
i is the vibrational
frequency. This leads to the following correction to the classical
forcefield energy:
- Eq. 4-21:
-
where k is the Boltzmann constant and T is the
temperature. The first term, h
i / 2, is the zero-point
correction; the second term corrects for the average thermal
population of vibrational levels at the temperature T. This
leads to a vibrational free energy correction of:
- Eq. 4-22:
-
and a vibrational entropy of:
- Eq. 4-23:
-
Computation of the harmonic vibrational frequencies requires the
storage and diagonalization of the second-derivative matrix, which has
dimensions of 3N x 3N, where N is the number of
atoms. The work involved in the diagonalization scales as N
3 and quickly becomes prohibitively expensive for more than
a few hundred atoms. The frequencies are valid only for well minimized
structures having maximum derivatives no greater than approximately
0.001 kcal mol-1 Å-1.
The forcefield is a major consideration. Most forcefield development
has emphasized structures and energetics rather than vibrational
frequencies. As a result, the frequencies calculated with forcefields
such as AMBER, MM2, CHARMm and, to a lesser extent, CVFF, may often be
in error by several hundred wavenumbers. The inclusion of cross terms
such as bond-bond and bond-angle terms is crucial for the accurate
reproduction of experimental frequencies. The CVFF forcefield includes
such cross terms and was, in part, parameterized to reproduce
experimental frequencies, which explains its moderately good
performance for vibrational calculations. The recent Class II
forcefields MM3 and CFF91 were explicitly designed to evenly weight
vibrational frequencies as well as structural and energetic
properties. Therefore, they provide the most reasonable and consistent
results, usually within 50-100 cm-1. This error of up to
approximately 100 cm-1 appears to be the current limit of
general-purpose, transferable forcefields.
Beyond these considerations, the vibrational frequencies can be used
for two classes of problems. The first is for determining the shape of
the potential energy surface; that is, the characterization of stable
points as minima, transition states, or other points. For this
purpose, the question of forcefield accuracy is less important. The
qualitative, rather than quantitative, shape of the surface is all
that is important. The second use is for comparison with experimental
results. The vibrational frequencies and thermodynamic corrections
depend strongly on the forcefield as well as on the fundamental
harmonic approximation invoked. By nature, low-frequency modes are
less harmonic. The torsion and nonbond interactions, which dominate
low-frequency modes, are fundamentally anharmonic; hence the
interpretation of the calculated low-frequency modes should take this
into account. Unfortunately, these low-frequency modes make the
largest contributions to the vibrational entropy.
Hagler et al. (1979c)
investigated the stability of the
-helix
and C7 conformations of short polypeptides, explicitly
calculating the vibrational corrections to the enthalpy and free
energy. Their results show that, for the specific cases they examined,
the conformational difference in the vibrational contribution to the
enthalpy was essentially negligible. This result is not too
surprising, because the enthalpy contribution is dominated by the
high-frequency modes such as the C-H stretching frequencies. These
high-energy modes would not be expected to change much between
conformations differing primarily in torsional angles. In contrast,
the entropic contributions to the free energy differences were
substantial and approximately the same magnitude as the total enthalpy
differences. Essentially, the entropic contribution is significant for
the same reason that the vibrational contribution to the enthalpy is
small: the low-frequency modes, particularly the torsions, contribute
heavily to the free energy. For instance, for Boc-Met6-OMe
the forcefield energy of the minimized C7 conformation was
5.09 kcal mol-1 lower in energy than for the
-helical form. Correcting the difference in
enthalpies for the vibrations decreased the difference by only 0.05
kcal mol-1. The contribution to the change in entropy,
however, led to a further decrease in the free energy of 3.99 kcal
mol-1. Although the energy difference of the minimized
structures appeared to be 5.09 kcal mol-1, the estimated
difference of the free energies was only 1.05 kcal
mol-1. Several other polypeptides of varying lengths and
compositions were studied. In all cases, the results were similar to
those for the example given here, which clearly indicates that the
vibrational contributions to relative free energies can be
important.
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