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Time Dependent Perturbation Theory
-----------------------------------
Consider a small time dependent perturbation, ΔH, to the
Hamiltonian, H0. We assume that the system before the
perturbation is in an eigenstate. We can write this as:
H'|ψ> = H0|ψ> + ΔH|ψ> ... 1.
ψ = Σnan(t)un(k)exp(-iωnt)) where un(k) = exp(ikx)
Note that if ΔH is time-independent the sytem will only go into
energy states that have the same energy as the initial state.
These are referred to as stationary states. If ΔH is a function
of time then the system will go into energy states that differ
by hω from the energy of the initial state.
From the time dependent Schrodinger equation we get:
H'|ψ = ih∂/∂t|Ψ>
Expanding we get:
LHS of 1.
Σnih(∂an(t)/∂t)un(k)exp(-iωnt)) + Σnhωnan(t)un(k)exp(-iωnt))
RHS of 1.
Using H0|ψ> = hωn|ψ>
Σnhωnan(t)un(k)exp(-iωnt)) + ΣnΔHan(t)un(k)exp(-iωnt))
Equating the two gives:
Σnih(∂an(t)/∂t)un(k)exp(-iωnt)) = ΣnΔHan(t)un(k)exp(-iωnt))
If we multiply sides by ψ* = um*(k)(exp(iωmt) we get:
Σnih(∂an(t)/∂t)<um*(k)|un(k)>exp(i(ωmt - ωnt))
= Σn<um(k)|ΔH|un(k)>exp(i(ωmt - ωnt))
Which after applying the orthogonality condition gives:
ih(∂an(t)/∂t) = Σn<um(k)|ΔH|un(k)>exp(i(ωmt - ωnt))
Therefore,
an(t) = (-i/h)<um(k)|ΔH|un(k)>∫dt exp(i(ωmt - ωnt))
= (2/h)<um(k)|ΔH|un(k)>exp(iωt/2) sin(ωt/2)/ω
Where ω = (ωm - ωn)
The transition rate is then:
Γn->m = d|an(t)|2/dt = (2/h2)|<um(k)|ΔH|un(k)>|2sin(ωt)/ω
If there are a continuum of energy states close to ωn then:
+∞
Γi->f = (2/h)|<f|ΔH|i>|2 ∫dω ρ(ω)sin(ωt)/ω
-∞
Noting that E = hω and where ρ(ω) is the density of final states.
Γi->f = (2π/h)|<f|ΔH|i>|2 ρ(ω)
This is referred to as FERMI's GOLDEN RULE.
The transition probability is independent of time (constant).
The <f|ΔH|i> term is called the MATRIX ELEMENT for the transition.
The matrix element can be placed in the form of an integral as:
Mif = ∫ψf*ΔHψidV V = volume
This of the general form used to find the expectation value of
an operator (observable).
= <ψ|O|ψ> = ∫ψ*Oψ dV
Mif = ∫ψf*ΔHψidV