Blue-moon ensemble: Difference between revisions

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with the four numerical terms indicating <math>\lambda_{\xi_k}</math>, <math>|Z|^{-1/2}</math>,  
with the four numerical terms indicating <math>\lambda_{\xi_k}</math>, <math>|Z|^{-1/2}</math>, <math>\frac{k_B T}{2 |Z|} \sum_{j=1}^{r}(Z^{-1})_{kj} \sum_{i=1}^{3N} m_i^{-1}\nabla_i \xi_j \cdot \nabla_i |Z| </math>, and , respectively.





Revision as of 15:40, 18 April 2022

In general, constrained molecular dynamics generates biased statistical averages. It can be shown that the correct average for a quantity can be obtained using the formula:

where stands for the statistical average of the quantity enclosed in angular parentheses 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 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:

Note that as the free-energy is a state quantity, the choice of path connecting (1) with (2) is irrelevant.

How to

The information needed to determine the blue moon ensemble averages within a Constrained molecular dynamics can be obtained by setting LBLUEOUT=.TRUE. The following output is written for each MD step in the file REPORT:

>Blue_moon
       lambda        |z|^(-1/2)    GkT           |z|^(-1/2)*(lambda+GkT)
  b_m>  0.585916E+01  0.215200E+02 -0.117679E+00  0.123556E+03


with the four numerical terms indicating , , , and , respectively.


References