I am, in full generality, confused about perturbation theory in quantum mechanics.
My textbook and Wikipedia have the same general approach to explaining it: given some Hamiltonian H=H(0)+H′, we can break down each eigenfunction |n⟩ into a power series in an invented constant λ and the eigenenergies likewise:
|n⟩=∑λi|n(i)⟩
En=∑λiE(i)n
(H(0)+H′)(|n(0)⟩+λ|n(0)⟩+⋯)=(E(0)+λE(1)+⋯)(|n(0)⟩+λ|n(1)⟩+⋯)
... and then they take λ→1.
My question is - what's the logic here? Where did this come from? What purpose does λ serve, given that the actual size of each contribution will be determined by the E(i)'s and |n(i)⟩'s?
Answer
Firstly, I refer you to Prof. Binney's textbook (see below) which covers perturbation theory in quantum mechanics in explicit detail. When doing perturbation theory, we perturb the Hamiltonian H(0) of a system which has been solved analytically, i.e. the eigenstates and eigenvalues are known. Specifically,
H(0)→H(0)+λH′
where H′ is the perturbation, and λ is a coupling constant. Why include such a constant? As Binney says, it provides us a 'slider' which when gradually increased to unity increases the strength of the perturbation. When λ=0, the system is unperturbed, and when λ=1 we 'fully perturb the system.'
Introducing a coupling constant λ also provides us with a manner to refer to a particular order of perturbation theory; O(λ) is first order, O(λ2) is second order, etc. As we increase in powers of the coupling constant, we hope the corrections decrease. (The series may not even converge.)
A caveat: the demand that a coupling λ≪1 may not be sufficient or correct to ensure that the coupling is small; this is only the case when the coupling is dimensionless. For example, if the coupling, in units where c=ℏ=1, had a mass (or equivalently energy) dimension of +1, then to ensure a weak coupling we would need to demand, λ/E≪1, where E had dimensions of energy. Such couplings are known as relevant as at low energies they are high, and at high energies the coupling is low.
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