QM time independent perturbation theory

In summary, QM time independent perturbation theory is a mathematical approach used in quantum mechanics to analyze the behavior of a quantum system when subjected to small disturbances or perturbations. It builds on the solution of a solvable Hamiltonian (the unperturbed system) and introduces a perturbing Hamiltonian, allowing for the calculation of energy levels and states of the perturbed system. The theory typically involves expanding the energy and wave function in terms of a small parameter related to the strength of the perturbation, leading to a series of corrections that improve the accuracy of the predictions for the system's properties. This method is particularly useful for understanding the effects of external fields and interactions in quantum systems.
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Marco99
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Homework Statement
Hello everyone,
So I have a QM assignment in which I have a s=1/2 particle with an unperturbed hamiltonian H diagonal in the |l,l_{z}>|s, s_{z}> base of the form H = A*L^2 + B*S_{z} (with 0 < B << A), and a perturbation term H' of the form H'=const * < L | S >, which can be shown to be diagonal in the |l, s; j, j_{z}> base. I am asked to calculate the energy corrections for the three lowest energy levels in the presence of the perturbation, and I applied time independent perturbation theory.
Relevant Equations
None
The lowest two energy level corrections (l=0, s_{z}=-1/2 and l=0, s_{z}=1/2) are easy to work out since the eigenvalues are not degenerate and the unperturbed energy levels also happen to be eigenstates of H'.

However I have three degenerate energy levels for the third eigenvalue of the form |l=1, l_{z}=0, +1, -1>|s=1/2, s_{z}=-1/2>. The l_{z}=-1 case is trivial, since it corresponds to the |l=1, s=1/2; j=3/2, j_{z}=-3/2> state, which is also an eigenstate of H'.

The l_{z}=0 and l_{z}=1 case is less trivial, so I used time independent perturbation theory in the degenerate case to diagonalise the H' matrix in the unperturbed state base |l=1, l_{z}=0, +1>|s=1/2, s_{z}=-1/2>.

The thing is in this base H' is already represented by a diagonal matrix since, calling |n_0}> and |n_1}> the two unperturbed states with l_{z}=0 and l_{z}=1 and expressing these in the |j, j_{z}> base, it happens that the off-diagonal terms <n_0 | H' | n_1> = <n_1 | H' |n_0> = 0, because |j, j_{z}> states with different j_{z} values are orthonormal.

Which means that the unperturbed states |n_0> and |n_1> already correspond to the perturbed eigenstates, which makes no sense since these two are not H' eigenstates at all. What am I missing?
 
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  • #2
I do not understand the perturbation "H'=const * < L | S >". Did you mean $$H'=\text{(const.)}~ \mathbf L\cdot \mathbf S~~?$$
 
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FAQ: QM time independent perturbation theory

What is time-independent perturbation theory in quantum mechanics?

Time-independent perturbation theory is a mathematical framework used in quantum mechanics to approximate the eigenstates and eigenvalues of a quantum system that is subject to a small perturbation. It is applicable when the Hamiltonian of the system can be expressed as a sum of an unperturbed Hamiltonian and a small perturbing Hamiltonian. This approach allows physicists to understand how small changes in the system affect its energy levels and wave functions.

When is time-independent perturbation theory applicable?

Time-independent perturbation theory is applicable when the perturbation is small compared to the main Hamiltonian, allowing for a perturbative expansion of the eigenstates and eigenvalues. It is typically used when the unperturbed system's eigenstates are known, and the perturbation does not lead to significant changes in the system's overall behavior. It is most effective when the perturbation does not mix states of very different energies.

How do you calculate the first-order energy correction using time-independent perturbation theory?

The first-order energy correction for a state |n⟩ in time-independent perturbation theory is given by the expectation value of the perturbing Hamiltonian H' in that state. Mathematically, it is expressed as E_n^(1) = ⟨n|H'|n⟩, where E_n^(1) is the first-order correction to the energy of the state |n⟩. This calculation involves integrating the product of the wave function, the perturbing Hamiltonian, and the complex conjugate of the wave function over the entire space.

What is the significance of the second-order energy correction?

The second-order energy correction provides a more refined estimate of the energy levels of the system when the first-order correction is insufficient due to the perturbation's influence on multiple states. It accounts for the contributions from all other states that can couple to the state |n⟩ through the perturbation. The second-order correction is given by E_n^(2) = Σ_{m≠n} |⟨m|H'|n⟩|² / (E_n^(0) - E_m^(0)), where E_n^(0) and E_m^(0) are the unperturbed energies of states |n⟩ and |m⟩, respectively.

What are the limitations of time-independent perturbation theory?

The limitations of time-independent perturbation theory include its reliance on the perturbation being small and the assumption that the unperturbed Hamiltonian's eigenstates are well-defined and non-degenerate. If the perturbation is not small or if it causes significant mixing of states, the perturbative approach may fail, leading to inaccurate results. Additionally

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