Blue moon ensemble

From VASP Wiki

In general, constrained molecular dynamics generates biased statistical averages. The blue moon ensemble average, also known as constrained-reaction-coordinate-dynamic (CRCD) ensemble, connects constrained and unconstrained molecular dynamics, cf. blue moon ensemble calcuations. It shows that the correct average for a quantity can be obtained using the formula:

where is the reaction coordinate, restrains the reference coordinate, e.g. to a transition state, where the associate velocity is , the stands for the statistical average of the quantity enclosed in angle brackets computed for a constrained ensemble, and is a mass metric tensor defined as:

It can be shown that the free energy gradient can be computed using the equation:[1][2][3][4]

where is the free energy, is the Boltzmann constant, is the temperature, and is the Lagrange multiplier associated with the parameter used in the SHAKE algorithm.[5]

The free-energy difference between states (1) and (2) can be computed by integrating the free-energy gradients over a connecting path, e.g. using the Simpson method[6]:

Note that as the free energy is a state quantity, the choice of path connecting (1) with (2) is irrelevant. As an example, when calculating the transition state, if (1) were set to the reactant and (2) to the transition state, then would be the activation free energy for the reaction.

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