Molecular Simulation and Statistical Mechanics

 

·     The energy calculated by molecular mechanics or quantum mechanics corresponds to a state in which the nuclei are at rest. 

 

·     In reality, we need to take into account the effects of temperature, and zero-point energy.

 

·     In addition, laboratory measurements are obviously not carried out at absolute zero on single molecules.  Experiments are done at higher temperatures on large numbers of molecules. 

 

·     We ideally need to include the vibrational, translational and rotational energy at a particular temperature to compare with experimental results. 

 

·     To do this, the techniques of statistical mechanics are used. Central to statistical mechanics is the partition function.

 

The vibrational frequencies from a normal mode analysis can be used to find the zero-point energy of a molecule, as we have already seen. More fundamentally, the calculated frequencies can be used to calculate the (vibrational) partition function. All thermodynamic properties can be calculated from the partition function, q:

 

 

Where ei is the energy of state i.

We can usually write the total energy as the sum of translational, vibrational, rotational and electronic contributions (see Prof. Balint-Kurti’s course, or Atkins Physical Chemistry, 6th edn., Chapter 20)

 

U = Utrans + Urot + Uvib + Uelec

 

which means that the partition function can be factorized:

 

q = qtransqrotqvibqelec

 

and so we can treat each contribution separately. 

 

·     The translational partition function can be calculated using the fact that the separation of translation energy levels is small.

 

·     Usually for polyatomic molecules, the rotational partition function can be found by similarly assuming the gaps between rotational energy levels are small, and using the moments of inertia of the structure.

 

·     Unlike the rotational and vibrational energy levels, the gaps between the vibrational energy levels are not small compared to kT.  We know that the vibrations of the molecule can be found by a normal mode analysis - treating them as independent harmonic oscillators.  The energy levels of each mode are given by the frequency, Ev = (v + ½)hn.  For a single harmonic oscillator. 

 

(because  ). 

 

Each normal mode contributes a partition function of this type, so the overall vibrational partition function for a polyatomic molecule is the product of all of them: 

 

 

From a frequency calculation, we can calculate the vibrational partition function of a molecule, and we can then use this to calculate the thermodynamic properties of the molecule. 

 

The electronic partition function involves summing over electronic quantum states (i.e. the lowest electronic state and all excited states). Usually the gap between the electronic states is very large, so only the ground state needs to be considered.

 

Next: calculating rate constants