About time-independent non-degenerate perturbation expansion

  • I
  • Thread starter Ishika_96_sparkles
  • Start date
In summary, time-independent non-degenerate perturbation expansion is a mathematical approach used in quantum mechanics to approximate the energy levels and wave functions of a quantum system that is subject to a small perturbation. This method builds upon the known solutions of a solvable Hamiltonian by systematically incorporating the effects of the perturbation, allowing for the calculation of corrections to energy levels and state functions. It is particularly applicable when the perturbation does not lead to degeneracy in the energy levels, enabling a straightforward application of perturbative techniques to derive useful physical insights.
  • #1
Ishika_96_sparkles
57
22
TL;DR Summary
Confusion regarding the state vector expansion over a set of basis functions and the perturbative expansion in the powers of $lambda$.
We know that any state vector in Hilbert space can be expanded as
$$ \Psi = \sum_{n=1}^{\infty} \alpha_i \psi_i $$

However, when we start the perturbation expansion of the eigenvalues and the eigenfunctions as
$$E_a = \lambda^0 E_a^0+\lambda^1 E_a^1+\lambda^2 E_a^2+\lambda^3 E_a^3+...+\lambda^n E_a^n+...$$
and
$$\psi_a = \lambda^0 \psi_a^0+\lambda^1 \psi_a^1+\lambda^2 \psi_a^2+\lambda^3 \psi_a^3+...+\lambda^n \Psi_a^n+...$$
respectively, is it the single state being expanded over its basis set or what? What exactly is this set ##{\psi_a^i}_{i=1}^n##?
How should I differentiate between the two?

PS: If my question is not clear, then please help me refine it as I really want to understand the basics of perturbation theory.
 
Physics news on Phys.org
  • #2
To reduce confusion, don't reuse the same symbols. For instance, consider
$$ \Psi = \sum_{n=1}^{\infty} \alpha_i \phi_i $$
where the ##\{ \phi_i \}## form some basis.

Then, in
Ishika_96_sparkles said:
$$\psi_a = \lambda^0 \psi_a^0+\lambda^1 \psi_a^1+\lambda^2 \psi_a^2+\lambda^3 \psi_a^3+...+\lambda^n \Psi_a^n+...$$
##\psi_a^0## would usually be an eigenstate of the unperturbed Hamiltonian ##\hat{H}_0##, and the other ##\psi_a^i## more generic functions (such that ##\psi_a## looks more and more like an eigenstate of the full Hamiltonian).

All the ##\psi_a^i## could be expressed in terms of basis states ##\{ \phi_i \}## (which would typically be the eigenstates of ##\hat{H}_0##, but could also be the eigenstates of the full Hamiltonian, or any other basis functions).
 
  • Care
Likes Ishika_96_sparkles
  • #3
Thank you @DrClaude! for a clear writeup and reply.
DrClaude said:
ψai more generic functions (such that ψa looks more and more like an eigenstate of the full Hamiltonian).
which probably are the "first-order... second-order...correction" terms that modify the unperturbed eigenfunction to match the eigenfunction of the full Hamiltonian. did i get that right?

Furthermore, all the ##\psi_a^i## are expandable in the original basis set ##\{\phi_i\}##.
 
  • #4
Ishika_96_sparkles said:
Thank you @DrClaude! for a clear writeup and reply.

which probably are the "first-order... second-order...correction" terms that modify the unperturbed eigenfunction to match the eigenfunction of the full Hamiltonian. did i get that right?

Furthermore, all the ##\psi_a^i## are expandable in the original basis set ##\{\phi_i\}##.
Correct.
 
  • Like
Likes Ishika_96_sparkles

FAQ: About time-independent non-degenerate perturbation expansion

What is time-independent non-degenerate perturbation theory?

Time-independent non-degenerate perturbation theory is a method used in quantum mechanics to find an approximate solution to the Schrödinger equation for a system where the Hamiltonian can be divided into a solvable part and a small perturbing part. It assumes that the unperturbed system has non-degenerate energy levels, meaning each energy level is uniquely associated with a single eigenstate.

How is the perturbation expansion formulated?

The perturbation expansion is formulated by expressing the perturbed quantities, such as the energy and wavefunctions, as power series in terms of a small parameter, typically denoted by λ. The zeroth-order terms correspond to the unperturbed system, while the first-order and higher-order terms account for the effects of the perturbation.

What are the first-order corrections in perturbation theory?

In first-order perturbation theory, the correction to the energy of the nth state is given by the expectation value of the perturbing Hamiltonian with respect to the unperturbed state. Mathematically, it is expressed as E_n^(1) = ⟨ψ_n^(0) | H' | ψ_n^(0)⟩, where E_n^(1) is the first-order energy correction, ψ_n^(0) is the unperturbed wavefunction, and H' is the perturbing Hamiltonian.

What are the second-order corrections in perturbation theory?

The second-order correction to the energy involves a sum over all states excluding the state of interest. It is given by E_n^(2) = Σ_m≠n |⟨ψ_m^(0) | H' | ψ_n^(0)⟩|^2 / (E_n^(0) - E_m^(0)), where E_n^(2) is the second-order energy correction, and the sum is over all unperturbed states m. This accounts for the interaction between the nth state and all other states due to the perturbation.

What are the limitations of time-independent non-degenerate perturbation theory?

Time-independent non-degenerate perturbation theory is limited by the requirement that the perturbation must be small compared to the unperturbed Hamiltonian. Additionally, it only applies to systems with non-degenerate energy levels. If the perturbation is too large or if the system has degenerate states, the method may not provide accurate results or may require modifications, such as degenerate perturbation theory.

Similar threads

Replies
8
Views
1K
Replies
10
Views
1K
Replies
3
Views
782
Replies
3
Views
3K
Replies
2
Views
1K
Replies
3
Views
888
Replies
1
Views
803
Back
Top