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10
Elements of Rayleigh-
Schroedinger Perturbation
Theory
In this chapter we present a few elements of RS stationary perturbation
theory, where a stationary system acted upon by an external perturbation
will change by a small amount its energy levels and eigenstates. It consists
essentially in relating the actual eigenvalue problem to be solved to one for
which a complete solution is exactly known, and in treating the difference
between the two Hamiltonian operators as a small perturbation.
10.1 RAYLEIGH-SCHROEDINGER PERTURBATION
EQUATIONS UP TO THIRD ORDER
We want to solve the Schroedinger eigenvalue equation
ð H E Þc ¼ 0
ð 10
:
1 Þ
for a Hermitian decomposition of the Hamiltonian H into:
H ¼ H 0 þ l H 1
ð 10
:
2 Þ
is a parameter giving the orders in perturbation theory, 1 (ii) H 0
is the unperturbed Hamiltonian, namely the Hamiltonian of an already
where (i)
l
1 Orders are here carried by the suffixes or their sum.
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