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form of the system's Hamiltonian from the initial state (
λ =
0) to the
final state (
λ =
1).
4.1.1. Free energy perturbation
By inserting a unity factor in the form e H A ( r , p ) e −β H A ( r , p ) into the numerator
of Eq. (12); we get
-
b
Hrp
(, )
+
b
H rp
(, )
-
b
H rp
(, )
Ú
e
e
e
dd
r
p
B
A
A
.
D Gk T
=-
ln
AB
B
Z
A
This can be seen as a phase space average of the quantity e −β [ HB HA ]
in
state A :
-
b [
HH
-
]
.
D Gk T
=-
ln
e
BA
(13)
AB
B
A
This approach is generally attributed to Zwanzig. 23 In practice, a single sim-
ulation in the reference state A is performed, during which the above phase
space average is converged. The accuracy of the free energy evaluation can
be improved if one can perform a simulation in state B as well. In such a
case, the FEP from A to B and from B to A can be optimally combined in
a single expression using the so-called Bennett acceptance ratio 27 :
(
)
-
b
[
HH
-
]
min
1
,
e
BA
.
A
D Gk T
=-
1
AB
B
(
)
-
b
[
HH
-
]
min
1
,
e
BA
B
The FEP method can give meaningful results only if the two states
A and B overlap in phase space, meaning that configurations are sampled
in which the difference H B
H A is smaller than k B T . Often, for transfor-
mations of practical interest, this is not the case. The solution is to intro-
duce n intermediate states between A and B , such that the overlap
between successive states is good. The Hamiltonian H ( r , p ,
λ
) is made a
function of a parameter
λ
which characterizes the intermediate states,
such that H ( r , p ,
λ Α )
=
H A ( r , p ) and H ( r , p ,
λ Β )
=
H B ( r , p ). One is free
 
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