Environmental Engineering Reference
In-Depth Information
the external force is applied.
When the system is in thermal equilibrium, it is characterized by
the density operator
1
Z e −βH 0
Z =Tr e −βH 0 ,
ρ 0 =
;
(3 . 1 . 1)
where
H 0 is the (effective) Hamiltonian, Z is the (grand) partition func-
tion, and β =1 /k B T . Since we are only interested in the linear part of
the response, we may assume that the weak external disturbance f ( t )
gives rise to a linear time-dependent perturbation in the total Hamilto-
nian
H
:
Af ( t )
H 1 , (3 . 1 . 2)
where A is a constant operator, as for example i J zi , associated with
the Zeeman term when f ( t )= B H z ( t ) (the circumflex over A or B
indicates that these quantities are quantum mechanical operators). As
a consequence of this perturbation, the density operator ρ ( t ) becomes
time-dependent, and so also does the ensemble average of the operator
B :
H 1 =
;
H
=
H 0 +
B ( t )
ρ ( t ) B
=Tr
{
}
.
(3 . 1 . 3)
The linear relation between this quantity and the external force has the
form
= t
−∞
B ( t )
B
t ) f ( t ) dt ,
φ BA ( t
(3 . 1 . 4)
B
B ( t =
ρ 0 B
;here f ( t ) is assumed to vanish
for t →−∞ . This equation expresses the condition that the differential
change of
−∞
{
}
where
=
)
=Tr
B ( t ) is proportional to the external disturbance f ( t )and
the duration of the perturbation δt , and further that disturbances at
different times act independently of each other. The latter condition
implies that the response function φ BA
mayonlydependonthetime
t . In (3.1.4), the response is independent of any future per-
turbations. This causal behaviour may be incorporated in the response
function by the requirement
difference t
t )=0
for t >t,
φ BA ( t
(3 . 1 . 5)
in which case the integration in eqn (3.1.4) can be extended from t to
+
.
Because φ BA depends only on the time difference, eqn (3.1.4) takes
a simple form if we introduce the Fourier transform
f ( ω )=
−∞
f ( t ) e iωt dt,
(3 . 1 . 6 a )
Search WWH ::




Custom Search