Blue moon ensemble calculations
The information needed to determine the blue moon ensemble averages within a Constrained molecular dynamics can be obtained by setting LBLUEOUT=.TRUE., cf. blue moon ensemble for details of the theory. 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.
Mind: is defined as in the REPORT file. This is an arbitrary character and has no relation to Green's functions, reciprocal lattice vectors, etc. |
Note that one line introduced by the string 'b_m>' is written for each constrained coordinate. With this output, the free energy gradient with respect to the fixed coordinate can conveniently be determined (by the equation given above) as a ratio between averages of the last and the second numerical terms. In the simplest case when only one constraint is used, the free energy gradient can be obtained as follows:
grep b_m REPORT |awk 'BEGIN {a=0.;b=0.} {a+=$5;b+=$3} END {print a/b}'
As an example of a blue moon ensemble average, let us consider the calculation of an unbiased potential energy average from constrained MD. For simplicity, only a single constraint is assumed. Here we extract for each step and store the data in an auxiliary file zet.dat:
grep b_m REPORT |awk '{print $3}' > zet.dat
Here we extract potential energy for each step and store the data in an auxiliary file energy.dat:
grep e_b REPORT |awk '{print $3}' > energy.dat
Finally, the weighted average is determined according to the first formula shown above:
paste energy.dat zet.dat |awk 'BEGIN {a=0.;b=0.} {a+=$1*$2;b+=$2} END {print a/b}'