|
|||||||||||||||||||||||||||||||||
AMBER Archive (2003)Subject: CCL: Amber free energy equation
From: Daquan Gao (d0gao001_at_gwise.louisville.edu)
Dear CCLers or AMBER users:
Having a question about the equation with free energy perpurbation:
The equation is , among other variations:
Delta G = -kT ln <exp(-(H(lambda + d lambda) - H (lambda))/kT) >
Now in gibbs, I used nstlim = 1, nrun = 100, almdel =0.01, isldyn = -3.
The reason I used nstlim =1 is I wanted to test the equation.
The isldym = -3 means I have a starting state at lambda = 1.0, and a
Now my questions:
After the first nrun, there is still only one set of energies, (either
At nrun = 2, I have lambda = 0.99, the previous state is lambda = 1.00.
What exactly is the equation that is being used in gibbs?
I have looked at the references, all says the above equation. Only
If any one knows the answer, please help. It may help me to improve my
I have posted once today, it did not appear, so again, sorry if you get
| |||||||||||||||||||||||||||||||||
|