1549380323-Statistical Mechanics Theory and Molecular Simulation

(jair2018) #1
Examples 145

We now extend this derivation to the case ofNparticles in three dimensions, i.e.,
an ideal gas ofNparticles in a cubic box of sideL(volumeV=L^3 ), for which the
Hamiltonian is


H=

∑N


i=1

p^2 i
2 m

. (4.5.5)


Since each momentum vectorpihas three components, we may also write the Hamil-
tonian as


H=

∑N


i=1

∑^3


α=1

p^2 αi
2 m

, (4.5.6)


whereα= (x,y,z) indexes the Cartesian components ofpi. The sum in eqn. (4.5.6)
contains 3Nterms. Thus, the partition function is given by


Q(N,V,T) =


1


N!h^3 N


D(V)

dNr


dNpexp

[


−β

∑N


i=1

p^2 i
2 m

]


. (4.5.7)


Since the Hamiltonian is separable in the each of theN coordinates and momenta,
the partition function can be simplified according to


Q(N,V,T) =


1


N!


[


1


h^3


D(V)

dr 1


dp 1 e−βp

(^21) / 2 m


][


1


h^3


D(V)

dr 2


dp 2 e−βp

(^22) / 2 m


]


···


[


1


h^3


D(V)

drN


dpNe−βp

(^2) N/ 2 m


]


. (4.5.8)


Since each integral in brackets is the same, we can write eqn. (4.5.8)as


Q(N,V,T) =


1


N!


[


1


h^3


D(V)

dr


dpe−βp

(^2) / 2 m


]N


. (4.5.9)


The six-dimensional integral in brackets is just


1
h^3


D(V)

dr


dpe−βp

(^2) / 2 m


1


h^3

∫L


0

dx

∫L


0

dy

∫L


0

dz

×


∫∞


−∞

dpxe−βp

(^2) x/ 2 m


∫∞


−∞

dpye−βp

(^2) y/ 2 m


∫∞


−∞

dpze−βp

(^2) z/ 2 m


. (4.5.10)


Eqn. (4.5.10) can also be written as


1
h^3


D(V)

dr


dpe−βp

(^2) / 2 m


[


1


h

∫L


0

dx

∫∞


−∞

dpe−βp

(^2) / 2 m


] 3


, (4.5.11)

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