Hamiltonian Perturbation Theory
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Questions and Answers

What is the general form of the total Hamiltonian in time-independent perturbation theory?

H = H0 + V

What is the physical significance of the first-order energy correction ΔE_n^1 in perturbation theory?

The expectation value of the perturbation V in the unperturbed state |n^0>

What is the formula for the first-order correction to the wave function |n^1> in perturbation theory?

|n^1> = Σ_(m≠n) [(V_nm) / (E_n^0 - E_m^0)] |m^0>

What is the assumption behind non-degenerate perturbation theory?

<p>The unperturbed states are non-degenerate (i.e., distinct energies)</p> Signup and view all the answers

What is the condition for the perturbation V to be considered small in perturbation theory?

<p>The perturbation V must be small compared to the energy level spacing of the unperturbed system</p> Signup and view all the answers

How can higher-order corrections be calculated in perturbation theory?

<p>Using similar formulas to calculate corrections of any order</p> Signup and view all the answers

What is the purpose of time-independent perturbation theory?

<p>To calculate the effects of a small perturbation on the energy levels and wave functions of a system</p> Signup and view all the answers

Study Notes

Hamiltonian Perturbation

Time-Independent Perturbation Theory

Perturbed Hamiltonian

  • The total Hamiltonian (H) is split into an unperturbed part (H0) and a perturbation (V):
    • H = H0 + V
  • The unperturbed Hamiltonian (H0) has known eigenvalues (E_n^0) and eigenfunctions (|n^0)

First-Order Perturbation Theory

First-Order Energy Correction

  • The first-order correction to the energy (ΔE_n^1) is given by:
    • ΔE_n^1 =
  • This represents the expectation value of the perturbation (V) in the unperturbed state |n^0>

First-Order Wave Function Correction

  • The first-order correction to the wave function (|n^1>) is given by:
    • |n^1> = Σ_(m≠n) [(V_nm) / (E_n^0 - E_m^0)] |m^0>
  • This represents the correction to the unperturbed wave function due to the perturbation (V)

Higher-Order Perturbation Theory

  • Higher-order corrections can be calculated using similar formulas
  • The process can be extended to calculate corrections of any order

Limitations and Validity

  • Non-degenerate perturbation theory assumes that the unperturbed states are non-degenerate (i.e., distinct energies)
  • The perturbation (V) must be small compared to the energy level spacing of the unperturbed system

Hamiltonian Perturbation

Time-Independent Perturbation Theory

  • The total Hamiltonian (H) is split into two parts: the unperturbed part (H0) and a perturbation (V)
  • The unperturbed Hamiltonian (H0) has known eigenvalues (E_n^0) and eigenfunctions (|n^0)

First-Order Perturbation Theory

First-Order Energy Correction

  • The first-order correction to the energy (ΔE_n^1) is the expectation value of the perturbation (V) in the unperturbed state |n^0>
  • ΔE_n^1 represents the energy shift due to the perturbation

First-Order Wave Function Correction

  • The first-order correction to the wave function (|n^1>) is a sum of corrections from other unperturbed states |m^0> (m ≠ n)
  • The correction is proportional to the matrix element (V_nm) and inversely proportional to the energy difference (E_n^0 - E_m^0)

Higher-Order Perturbation Theory

  • Higher-order corrections can be calculated using similar formulas
  • The process can be extended to calculate corrections of any order

Limitations and Validity

  • Non-degenerate perturbation theory assumes non-degenerate unperturbed states (i.e., distinct energies)
  • The perturbation (V) must be small compared to the energy level spacing of the unperturbed system

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Description

Learn about time-independent perturbation theory, including the perturbed Hamiltonian and first-order energy correction. Understand the concepts of unperturbed Hamiltonian and perturbation.

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