Kramers' Relation

Proving ⟨1/r³⟩ for the hydrogen atom using Kramers' relation — brutal-looking but apparently the least painful option, thanks Uncle Griffiths T_T

The integrals are back, so Isaac Newton is back in the firing line too. I am joking, of course—but this is one of those derivations that makes the invention of calculus feel personal.

In the previous post on the Feynman–Hellmann theorem, I obtained the first two inverse-power expectation values for hydrogen:

The previously derived hydrogen expectation values for one over r and one over r squared

Here the target is the next member of the sequence:

The target hydrogen expectation value of one over r cubed

Kramers’ relation gives the cleanest route to that result. Unfortunately, getting the relation itself is the long part.

1. Kramers’ relation

Problem 6.34

For an electron in the hydrogen eigenstate $\psi_{n\ell m}$,

Kramers’ relation connecting the expectation values of r to the powers s, s minus one, and s minus two

prove

$$ \boxed{ \frac{s+1}{n^2}\langle r^s\rangle -(2s+1)a\langle r^{s-1}\rangle {}+\frac{s}{4}\left[(2\ell+1)^2-s^2\right]a^2 \langle r^{s-2}\rangle=0 }. $$

The state is labeled in the usual way:

Hydrogen eigenstate label psi sub n ell m

The hint introduces the three moments

The three radial moments r to the s, r to the s minus one, and r to the s minus two

and asks us to evaluate a radial integral involving $u''$ in two ways.

Source-image correction. The preserved source image below fixes the power at $r^2$, but the recurrence needs an arbitrary real power $r^s$. The equation used in this proof is the native equation immediately below the image.

Preserved source image with r squared; for the recurrence this is corrected below to the arbitrary power r to the s

$$ I_s\equiv\int_0^\infty u(r)\,r^s u''(r)\,dr. $$

It looks brutal, but it is still the least painful way to reach

The desired inverse-cube radial expectation value

for the hydrogen atom.

2. Start from the reduced radial equation

Write

$$ \psi_{n\ell m}(r,\Omega)=\frac{u_{n\ell}(r)}{r}Y_{\ell m}(\Omega), \qquad \int |Y_{\ell m}|^2\,d\Omega=1. $$

The bound-state radial function may be chosen real, and I make that choice throughout. Then

$$ \int_0^\infty |u|^2\,dr=1, \qquad M_q\equiv\langle r^q\rangle =\int_0^\infty |u(r)|^2r^q\,dr. $$

For a finite-mass electron–proton system, let $\mu$ be the reduced mass and define

$$ a=\frac{4\pi\epsilon_0\hbar^2}{\mu e^2}, \qquad E_n=-\frac{\hbar^2}{2\mu a^2n^2}. $$

The fixed-proton approximation is recovered by taking $\mu\approx m_e$. The same mass convention must be used in both $a$ and the radial Hamiltonian.

Source-image correction. The preserved source equation below prints the centrifugal denominator as $r$. It must be $r^2$.

Preserved reduced radial equation whose centrifugal denominator r is corrected below to r squared

Source-image correction. The following rearrangement inherits that same $r$-instead-of-$r^2$ error. The corrected reduced equation is given natively after it.

Preserved rearrangement of the hydrogen radial equation whose centrifugal denominator is corrected below

The notation $u''$ means the second derivative of $u$ with respect to $r$:

Explanation that u double prime denotes the second derivative with respect to r

The dimensionally consistent reduced equation used below is

$$ u''(r)=\left[ \frac{\ell(\ell+1)}{r^2} -\frac{2}{ar} {}+\frac{1}{a^2n^2} \right]u(r). $$

Source-image correction. The preserved multiplication step below again prints $\ell(\ell+1)/r$ even though its next line uses the $M_{s-2}$ moment. Replace that denominator by $r^2$ as in the native calculation that follows.

Preserved multiplication step with a centrifugal denominator corrected below from r to r squared

Expansion of the radial integral into the moments r to the s minus two, s minus one, and s

Multiplying the corrected radial equation by $u r^s$ and integrating gives the first evaluation:

$$ \begin{aligned} I_s &=\int_0^\infty u r^s \left[\frac{\ell(\ell+1)}{r^2}-\frac{2}{ar} {}+\frac{1}{a^2n^2}\right]u\,dr\\ &=\ell(\ell+1)M_{s-2} -\frac{2}{a}M_{s-1} {}+\frac{1}{a^2n^2}M_s. \end{aligned} $$

Boundary conditions and domain

For a regular hydrogen bound state,

$$ u(r)\sim r^{\ell+1},\qquad u'(r)\sim r^\ell \quad (r\to0), $$

while $u$ and $u'$ decay exponentially as $r\to\infty$. Thus the moments, derivative integral, and all origin boundary terms used below converge and vanish for

$$ s>-2\ell-1. $$

The intermediate calculation of $K_s$ divides by $s+1$, so the derivation at first also assumes $s\ne-1$. We will recover $s=-1$ for $\ell\ge1$ by a limit after proving the recurrence on this domain.

First integration by parts

The preserved source image records the first integration-by-parts step:

First integration by parts for the integral of u r to the s u double prime with blue and red terms

Its complete native form is

$$ \begin{aligned} I_s &=\left[u r^s u'\right]_0^\infty -\int_0^\infty r^s(u')^2\,dr -s\int_0^\infty u r^{s-1}u'\,dr\\ &=-K_s-s\int_0^\infty u r^{s-1}u'\,dr, \qquad K_s\equiv\int_0^\infty r^s(u')^2\,dr. \end{aligned} $$

For any needed power $p$, a second elementary integration by parts gives

Derivation of the integral of u r to the s minus one u prime from a vanishing boundary term

$$ \begin{aligned} \int_0^\infty u r^p u'\,dr &=\frac12\int_0^\infty r^p (u^2)'\,dr\\ &=\frac12\left[r^p u^2\right]_0^\infty -\frac{p}{2}\int_0^\infty r^{p-1}u^2\,dr\\ &=-\frac{p}{2}M_{p-1}. \end{aligned} $$

In particular,

Result for the integral of u r to the s minus one u prime in terms of the r to the s minus two moment

$$ \int_0^\infty u r^{s-1}u'\,dr =-\frac{s-1}{2}M_{s-2}, $$

and therefore

$$ I_s=-K_s+\frac{s(s-1)}{2}M_{s-2}. $$

The remaining derivative integral

The next preserved image encodes the derivative identity for $K_s$:

Second integration-by-parts identity relating the integral of r to the s times u prime squared to an integral containing u double prime

Written completely in native form,

$$ \begin{aligned} 0 &=\int_0^\infty\frac{d}{dr}\left[r^{s+1}(u')^2\right]dr\\ &=(s+1)\int_0^\infty r^s(u')^2\,dr {}+2\int_0^\infty r^{s+1}u'u''\,dr, \end{aligned} $$

so, for $s\ne-1$,

$$ K_s=-\frac{2}{s+1}\int_0^\infty r^{s+1}u'u''\,dr. $$

Source-image correction. This preserved substitution image prints the centrifugal denominator as $r$; the required denominator is $r^2$.

Preserved substitution of the reduced radial equation whose centrifugal denominator is corrected below to r squared

Source-image correction. The next preserved image also prints that denominator as $r$ and consequently writes $r^{s+1}$ in the centrifugal derivative integral. With $1/r^2$, the correct power is $r^{s-1}$. The complete corrected substitution is below.

Preserved derivative-integral substitution with r corrected to r squared and r to the s plus one corrected to r to the s minus one

$$ \begin{aligned} K_s &=-\frac{2}{s+1}\int_0^\infty r^{s+1}u' \left[\frac{\ell(\ell+1)}{r^2}-\frac{2}{ar} {}+\frac{1}{a^2n^2}\right]u\,dr\\ &=-\frac{2}{s+1}\left[ \ell(\ell+1)\int_0^\infty u r^{s-1}u'\,dr -\frac{2}{a}\int_0^\infty u r^s u'\,dr {}+\frac{1}{a^2n^2}\int_0^\infty u r^{s+1}u'\,dr \right]. \end{aligned} $$

Source-image correction. The preserved evaluated image gives the $M_s/(a^2n^2)$ term the wrong negative sign. Applying the identity above to all three integrals gives a positive sign:

Preserved evaluation of K sub s whose negative energy term is corrected below to positive

$$ \begin{aligned} K_s &=-\frac{2}{s+1}\left[ -\frac{\ell(\ell+1)(s-1)}{2}M_{s-2} {}+\frac{s}{a}M_{s-1} -\frac{s+1}{2a^2n^2}M_s \right]\\ &=\frac{\ell(\ell+1)(s-1)}{s+1}M_{s-2} -\frac{2s}{a(s+1)}M_{s-1} {}+\frac{1}{a^2n^2}M_s. \end{aligned} $$

The earlier integration-by-parts equation was

First expression for the central radial integral, ready to receive the evaluated derivative terms

and the corrected substitution gives

$$ \begin{aligned} I_s &=-K_s+\frac{s(s-1)}{2}M_{s-2}\\ &=\left[ \frac{s(s-1)}{2} -\frac{\ell(\ell+1)(s-1)}{s+1} \right]M_{s-2} {}+\frac{2s}{a(s+1)}M_{s-1} -\frac{1}{a^2n^2}M_s. \end{aligned} $$

Source-image correction. The preserved combination below carries the wrong negative sign from the preceding source step and then distributes the outer minus inconsistently. Those two errors compensate. The proof instead equates the two internally consistent native expressions above.

Preserved combination with compensating sign errors; the consistent native coefficient equation is given below

Equating the radial-equation evaluation of $I_s$ to the integration-by-parts evaluation and multiplying by $2(s+1)$ gives

$$ \begin{aligned} 0={}& \left\{2(s+1)\ell(\ell+1) -(s-1)\left[s(s+1)-2\ell(\ell+1)\right]\right\}M_{s-2}\\ &-\frac{4(2s+1)}{a}M_{s-1} {}+\frac{4(s+1)}{a^2n^2}M_s\\ ={}& s\left[(2\ell+1)^2-s^2\right]M_{s-2} -\frac{4(2s+1)}{a}M_{s-1} {}+\frac{4(s+1)}{a^2n^2}M_s. \end{aligned} $$

Multiplying by $a^2/4$ produces the claimed recurrence:

Final Kramers recurrence relation after simplifying the radial-moment coefficients

$$ \boxed{ \frac{s+1}{n^2}\langle r^s\rangle -(2s+1)a\langle r^{s-1}\rangle {}+\frac{s}{4}\left[(2\ell+1)^2-s^2\right]a^2 \langle r^{s-2}\rangle=0 }. $$

That is Kramers’ relation for $s>-2\ell-1$ and $s\ne-1$ as derived above. Where the moments remain finite, the recurrence itself extends to $s=-1$ by continuity.

3. Useful special cases

Problem 6.35(a)

The immediate goal is still

Reminder that the calculation is seeking the expectation value of one over r cubed

but first the exercise proposes $s=0,1,2,3$ in

Kramers’ relation repeated for substitution of special integer values of s

I evaluate $s=0$ and $s=1$ here because they supply the moments used in this post. The $s=2$ and $s=3$ cases are intentionally skipped; they generate higher positive moments but are not needed for the inverse-cube result.

At $s=0$, normalization gives $M_0=1$, so

The s equals zero substitution yielding the hydrogen expectation value of one over r

and therefore

Kramers’ relation repeated after the s equals zero calculation

$$ \boxed{\left\langle\frac1r\right\rangle=\frac{1}{an^2}}. $$

At $s=1$,

The s equals one substitution and simplification leading toward the expectation value of r

the recurrence gives

$$ \frac{2}{n^2}\langle r\rangle-3a {}+a^2\ell(\ell+1)\left\langle r^{-1}\right\rangle=0. $$

Source-image correction. In the preserved handwritten simplification below, $-(4\ell^2+4\ell)$ is incorrectly changed to $-4\ell^2+4\ell$, leading temporarily to $\ell(\ell-1)$. The correct factor is $\ell(\ell+1)$, as shown by the native calculation.

Preserved handwritten s equals one calculation with the sign and ell times ell minus one errors corrected below

Using $\langle r^{-1}\rangle=1/(an^2)$,

$$ \begin{aligned} 2\langle r\rangle-3an^2+a\ell(\ell+1)&=0,\\ \therefore\qquad \boxed{\langle r\rangle =\frac{a}{2}\left[3n^2-\ell(\ell+1)\right]}. \end{aligned} $$

The inverse-cube result requires a different value, so let us return to

The inverse-cube radial expectation value highlighted as the remaining target

in the recurrence

Kramers’ relation repeated before taking the limit s to minus one

and now take $s\to-1$. This is not direct substitution into the intermediate $K_s$ equation, which divided by $s+1$. For $\ell\ge1$, an open interval around $s=-1$ lies inside $s>-2\ell-1$, and the convergent moments $M_s$, $M_{s-1}$, and $M_{s-2}$ are continuous—indeed analytic—in $s$ there. We may therefore take the limit of the already-proved recurrence. The first term tends to zero, leaving

The s equals minus one limiting recurrence deriving the inverse-cube moment from the inverse-square moment

$$ a\left\langle r^{-2}\right\rangle -a^2\ell(\ell+1)\left\langle r^{-3}\right\rangle=0. $$

Using the previous post’s result

$$ \left\langle r^{-2}\right\rangle =\frac{1}{a^2n^3\left(\ell+\tfrac12\right)}, $$

we finally obtain

$$ \boxed{ \left\langle\frac{1}{r^3}\right\rangle =\frac{1}{a^3n^3\ell(\ell+1)\left(\ell+\tfrac12\right)} },\qquad \ell\ne0. $$

The restriction $\ell\ne0$ matters. For an $s$ state, $u(r)\sim r$ near the origin, so the integrand $|u|^2r^{-3}\sim r^{-1}$ and $\langle r^{-3}\rangle$ diverges logarithmically. For $\ell\ge1$, the limit above is valid and the boxed result is finite.

Portrait of Isaac Newton closing the author’s calculus-heavy derivation

After a semester full of integrals, I think an Isaac Toast is the appropriate way to call it a day.

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