Perturbation Theory - First Order Approximation

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SUMMARY

Perturbation Theory's First Order Approximation involves expanding the disturbed eigenfunction ##\psi (x)## and eigenvalue ##E## using Taylor series. The disturbed Hamiltonian is expressed as ##\hat{H} = \hat{H_0} + \epsilon \hat{V}##, where ##\hat{H_0}## is the undisturbed Hamiltonian and ##\hat{V}## is the potential. The expansions yield ##\psi (x) = \psi_0 (x) + \epsilon \psi_1 (x) + \epsilon^2 \psi_2 (x) + ...## and ##E = E_0 + \epsilon E_1 + \epsilon^2 E_2 + ...##. The coefficients in these expansions are defined such that ##E^{(n)}## corresponds to the coefficient of ##\epsilon^n## in the power series, clarifying the roles of each term in the perturbation series.

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Sunnyocean
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If:

##\hat{H} \psi (x) = E \psi (x)##

where E is the eigenvalue of the *disturbed* eigenfunction ##\psi (x)##

and ##E_n## are the eigenvalues of the *undisturbed* Hamiltonian ##\hat{H_0}##

and the *disturbed* Hamiltonian is of the form:

##\hat{H} = \hat{H_0} +{\epsilon} \hat{V} ##

where ## \hat{V} ## is the potential and

then we can expand, using a Taylor expansion, ##\psi (x) ## and ##\epsilon## is a very small (positive?) number

##\psi (x) = {\psi}_0 (x) + {\epsilon}{\psi}_1 (x) + {\epsilon}^2 {\psi}_2 (x) + ... ## (1)

where ##{\psi}_k (x)## is the eigenfunction of ##\hat{H}## corresponding to the eigenvalue ##E_n## (eigenvalues are assumed to be non-degenerate)

We also get, using a Taylor expansion:

##E = E_0 +{\epsilon}{E_1} + {\epsilon}^2 {E_2} + ...## (2)

MY QUESTIONS:

I tried deriving formulae (1) and (2) - i.e. the expansions - on my own but I was unable to do it. Could anyone please show me *in detail* how to obtain those expansions?

Another question is:
How do we know that, when using the Taylor expansion, the coefficient ## {\epsilon} ## applies to ##{\psi}_1 (x)## and not to some other eigenfuncion, the coefficient ## {\epsilon}^2 ## applies to ##{\psi}_2 (x)## and not to some other eigenfuncion, and so on? The same question for eigenvalues.
 
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Sunnyocean said:
Another question is:
How do we know that, when using the Taylor expansion, the coefficient ## {\epsilon} ## applies to ##{\psi}_1 (x)## and not to some other eigenfuncion, the coefficient ## {\epsilon}^2 ## applies to ##{\psi}_2 (x)## and not to some other eigenfuncion, and so on? The same question for eigenvalues.

##E^{(n)}## is *defined* as the coefficient of ##\epsilon^n## in the power series expansion of ##E##. Same for ##\psi^{(n)}##.

Note that the ##E^{(n)}##'s and ##\psi^{(n)}##'s are *not* eigenvalues and eigenfunctions, except for ##E^{(0)}## and ##\psi^{(0)}## which are an eigenvalue and eigenfunction of ##H_0##.
 
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Thank you The_Duck, that clarifies it. I was obviously misled by the confusing notation. You made it clear, so thank you again :)
 

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