Perturbation Method#

What you need to know

  • Perturbation method, attempts to solve analytically intractable problems by idintifying an exactly sovable part and a “small” pertrubation to it.

  • The method is similair in spirit to taylor expansion of continuous functions familiar to us from calculus. Just like in taylor expansion in pertrubation expansion the key is identifying the relatively small parameter in the problem to expand.

  • Application of pertrubation theory proceeds in two steps. Step one identify solvable part and perturbation. Part two expand energy and eigenfunctions as series of corrections of increasing order. In practice first and second order corrections to energy are sufficient to get quantiatively accurate results.

  • Perturbation theory allows writing down expressions entirely in terms of eigenfunctions and eigenvalues of exactly solved problem!

pertrub

Fig. 88 Pertrubation theory quantifies how much energy levels get pertrubed by adding “small” deviation of the exactly solvable Hamiltonian. For many problems which are impossibvle to solve exactly one can still identify part of the hamiltonian as exactly solvable H^0 with the rest being treated as pertrubation#

Time independent perturbations#

  • We have hamiltonian H^0 for some exactly solvable problem think particle in a box, harmonic oscilator, etc:

H^0n0=En0n0
  • Note the 0 superscript: It indicates exactly solvable hamitlonian, eigenfunctions and eigenvalues. The n0 is the eigenfunction corepsonding to the nth eigenvalue En0.

  • Consider a problem where we have a hamitlonian which is similiar to an exactly solvable problem differing only by a “small” pertrubation H1^. Small means that eiganvalues should of two systems are close relative to spacing.

  • The parameter λ turns perturbation on λ=1 and off λ=0.

H^=H^0+λH^1
  • The objective of perturbation theory is to solve the problem with new hamiltonian expressed entirely in terms of eigenvalues and eigenfunctions of exactly solvable problems.

H^n=Enn

It’s just like Taylor expansions!#

  • We assume that eigenvalues and eigenfunctions can be expanded in power series in the parameter λ to be set to 1 in the end.

En=En0+λEn1+λ2En2+...
n=n0+λn1+λ2n2...
  • Pluggin in the expansions into H^n=Enn we get expression involving various terms with λ. Next step is to expand brackets and group terms according to λ0, λ1, and λ2,

(H^0+λH^1)(n0+λn1+λ2n2)=(En0+λEn1+λ2En2)(n0+λn1+λ2n2)

Pertubation equations of order 0, 1 and 2.#

  • Opening the brackets and collecting different orders of λ we have 0, 1 and 2nd order perturbation equations:

H^0n0=En0n0
H^0n1+H1^n0=En0n1+En1n0
H0^n2+H1^n1=En0n2+En1n1+En2n0
  • Note how the sum of upstairs indeces determines the order of perturbation expansion

  • The 0 order is just the exact solution.

  • Hamitonian only has first order expansion while eigenfunctions and eigenvalues are expanded to infinite terms. Usually going to second order is enough for most problems.

Computing pertrubation correction to energy levels#

Perturbation Approximation to Energies

En=En0+Hnn+knHnk2En0Ek0
  • **n and k: Quantum numbers running from groun to excited states, e.g n=0,1,2...

  • Matrix Elements of pertrubation

Hnk=n0H1k0
Hnn=n0H1n0

First and second order corrections to the ground state#

  • The first order correction to the ground state requires computing diagonal matrix elements only:

E0(1)=0|H^1|0
  • 2nd order correction to the ground state requires calculating off-diagonal elements H0k where n=0 and k runs over all excited states.

E0(2)=k0H0k2E00Ek0
  • Note how the energy in the denominator of 2nd order term involves difference between energy of a given state En from all other states Ek denoted by k the summation index.

  • Key insight If the matrix elements are of comparable magnitude the neighbouring energy levels make larger contributions to pertrubation expression.

Derivations of 1st and 2nd order corrections#

Applications#

Example-1: Estimate ground state with second order pertrubation

Write second order correction explicitely for the ground state for some exactly solvable hamiltonian H0^ pertrubed by H1^

En=En0+Hnn+knHnk2En0Ek0
E0=E00+H00+H012E00E10+H022E00E20+H032E00E30+...
  • Notice that for the ground state the second order correction thereofre will always be negative because ΔE0k=E0Ek<0

Example-2: Magnetic field

Hydrogen atom in magnetic field problem can be seen as as a hamitonian of H atom to which we have added a small pertrubation in the form of interation with magnetic field.

H^=H^0+e2meBL^z=H^0+H^1
  • Using 1st order pertrubation expression we can calculate for instance how ground state energy will be perturbed. Where on right hand side we define RH as Rydberg’s and βB as Bohr’s magneton, both constants.

E0=E00+0H^10=RHn2+mlβBB

  • In a similiar way the effect of spin orbit coupling (LS)

H^=H^0+ASOL^S^
E=E0+ASO0L^S^0

Example-3: Perturbing particle in a box

Estimate the energy of the ground-state and first excited-state wavefunction within first-order perturbation theory of a system with the following potential energy:

V(x)=V00x
V(x)=+x, x

This problem can be seen as a particle in a box pertrubed by the presence of a potential energy V0

En1=nV0n=V02L0Lsin2nπxLdx=V0

Thus we find that energy level of PIB are pertrubed by a constant shift up term:

En=En0+En1n2h28mL2+V0

Example-4 Anharmonic oscillator

  • Anharmonic oscillator problem can be seen as a problem fo harmonic oscillator + pertrubation in the form of unharmonic term:

H^=K^+kx22+γx3=H^0+γx3
  • Using first order pertrubation we find an interesting result after evaluating the integral to by using simple symmetry arguments.

En1=0γx3n=even/oddoddeven/odd=0
  • But energy levels surely must experience change since we added a new term to hamitlonian. To see the change we must therefore turn to second order and use ground state as an example

E02=k00γx3k2E00Ek0=0γx312E00E10+nγx332E00E30+...
E0=E0+E1+E2=ω2+0+H012ω+H0322ω+...

Thus we see that only terms odd terms of the sum contribute. The matrix elements need to be evaluated explicitly using Hermite polynomials.