1549380323-Statistical Mechanics Theory and Molecular Simulation

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Numerical evaluation 479

×exp

{


−β

∑P


k=1

[


p^2 k
2 m′k

+


1


2


mkω^2 Pu^2 k+

1


P


U(xk(u))

]}


. (12.6.9)


In eqn. (12.6.9), the parametersmkare defined to be


m 1 = 0, mk=

k
k− 1

m, k= 2,...,P, (12.6.10)

andm′ 1 =m,m′k=mk. The notationxk(u) indicates the inverse transformation in
eqn. (12.6.6) or (12.6.7). In order to evaluate eqn. (12.6.9), we canemploy a classical
Hamiltonian of the form


H ̃cl(u,p) =

∑P


k=1

[


p^2 k
2 m′k

+


1


2


mkω^2 Pu^2 k+

1


P


U(xk(u))

]


, (12.6.11)


which leads to the equations of motion


u ̇k=

pk
m′k

p ̇k=−mkω^2 Puk−

1


P


∂U


∂uk

. (12.6.12)


From the chain rule, the forces on the staging variables can be expressed recursively
as


1
P

∂U


∂u 1

=


1


P


∑P


l=1

∂U


∂xl

1
P

∂U


∂uk

=


1


P


[


∂U


∂xk

+


k− 2
k− 1

∂U


∂uk− 1

]


. (12.6.13)


The recursive staging force calculation is performed starting withk= 2 and using
the first expression for∂U/∂u 1. Eqns. (12.6.12) need to be thermostatted to ensure
that the canonical distribution is generated. The presence of thehigh-frequency force
on each staging variable combined with the 1/Pfactor that attenuates the potential-
energy derivatives leads to a weak coupling between these two forces. Therefore, it is
important to have as much thermalization as possible in order to achieve equiparti-
tioning of the energy. It is, therefore, strongly recommended (Tuckermanet al., 1993)
that path-integral molecular dynamics calculations be carried out using the “massive”
thermostatting mechanism described in Section 4.10. This protocolrequires that a
separate thermostat be attached to each Cartesian componentof every staging vari-
able. Thus, for the single-particle one-dimensional system described by eqns. (12.6.12),
if Nos ́e–Hoover chain thermostats of lengthMare employed, the actual equations of
motion would be

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