1549380323-Statistical Mechanics Theory and Molecular Simulation

(jair2018) #1

182 Canonical ensemble


s 0 = e(E−H(r,p)−p

(^2) s/ 2 Q)/gkT


1


|f′(s 0 )|

=


1


gkT

e(E−H(r,p)−p

(^2) s/ 2 Q)/gkT


. (4.8.7)


Substituting eqn. (4.8.7) into eqn. (4.8.4) yields


Ω =


1


gkT


dNpdNrdpse(dN+1)(E−H(r,p)−p

(^2) s/ 2 Q)/gkT


. (4.8.8)


Thus, if the parametergis chosen to bedN+ 1, then, after performing thepsinte-
gration, eqn. (4.8.8) becomes


Ω =


eE/kT


2 πQkT
(dN+ 1)kT


dNpdNre−H(r,p)/kT, (4.8.9)

which is the canonical partition function, apart from the prefactors. Our analysis
shows how a microcanonical distribution of the Nos ́e HamiltonianHNis equivalent to
a canonical distribution in the physical Hamiltonian. This suggests that a molecular
dynamics calculation performed usingHNshould generate sampling of the canonical
distribution exp[−βH(r,p)] under the usual assumptions of ergodicity. Because the
Nos ́e Hamiltonian mimics the effect of a heat bath by controlling the fluctuations
in the kinetic energy, the mechanism of the Nos ́e Hamiltonian is also known as a
thermostattingmechanism.
The equations of motion generated byHNare


r ̇i=

∂HN


∂pi

=


pi
mis^2

p ̇i=−

∂HN


∂ri

=Fi

s ̇=

∂HN


∂ps

=


ps
Q

p ̇s=−

∂HN


∂s

=


∑N


i=1

p^2 i
mis^3


gkT
s

=


1


s

[N



i=1

p^2 i
mis^2

−gkT

]


. (4.8.10)


Ther ̇iand ̇psequations reveal that the thermostatting mechanism works on anun-
conventional kinetic energy



ip
2
i/(2mis

(^2) ). This form suggests that the more familiar
kinetic energy can be recovered by introducing the following (noncanonical) change of
variables:
p′i=
pi
s
, p′s=
ps
s
, dt′=
dt
s


. (4.8.11)


When eqn. (4.8.11) is substituted into eqns. (4.8.10), the equationsof motion become

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