Normalization condition for free & spherically symmetric

zhaos
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Homework Statement



I think, to normalize a wavefunction, we integrate over the solid angle ##r^2 dr d\theta d\phi##. Typically we have ## R(r)Y(\theta, \phi) ## as solutions. If ##Y## is properly normalized, then the normalization condition for ##R(r)## ought to be

$$ \int_0^\infty dr r^2 |R(r)|^2 = 1$$

Homework Equations



Now I am trying to develop a general normalization condition for the spherical Bessel functions, which are solutions to the free particle in free space, but solved using spherical symmetry. For example the 0th solution is

$$ R(r) = \sin (kr)/r $$

where ## k = \sqrt{2mE/\hbar} ##.

Now if I were to normalize with integration over ## r^2 dr ##, the normalization integral will not converge. Google searching has been unhelpful so far, but I've tended to see just integration over ## dr ##. So I'm conceptually unsure why this would be the case.

The Attempt at a Solution



The end goal is to have a general normalization factor for the spherical Bessel functions. If I normalize

$$ \int_0^\infty dr | A R_0(r)|^2 = 1 $$

In this case, ## A = \sqrt{2/\pi k} ##.

In fact I found by just doing the normalization for the first few functions, sqrt(2l+1) works as the additional normalization factor.
But the current sticking point is the integration over dr or r^2 dr.

Thanks.
 
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Free particle states aren't normalizable. You can see this pretty quickly in cartesian coordinates (showing one dimension for simplicity):
<br /> \psi_k(x) = Ne^{i k x}<br />
where k is a quantum number related to energy E = \hbar^2 k^2/2m. Since |\psi(x)|^2 = 1, clearly you can't normalize this state.

Instead, it's conventional to normalize the states as
<br /> \int dx \psi_{k&#039;}^*(x) \psi_{k}(x) = \delta(k - k&#039;)<br />
with the dirac delta function. Then you can show that N = 1/\sqrt{2 \pi}. This normalization is useful because you can then write down general normalizable states as
<br /> \Psi(x) = \int dk A(k) \psi_k(x)<br />
and now the normalization condition on \Psi becomes
<br /> \int dx |\Psi(x)|^2 = \int dk A(k) = 1.<br />
So A(k) is a normalized distribution over which k's contribute to the wave function. So a good choice for normalizing for your spherical problem would be to generalize the delta function normalization above.
 
I guess i have
$$
|A|^2 \int_0^\infty dr r^2 \psi^*_{0,k'}(r)\psi_{0,k}(r) = \delta(k-k')
$$
and ## \psi_0(r) = \sin(kr)/r = \frac{i}{r}( \exp(ikr) - \exp(-ikr))##, and the r^2 will cancel, and then one does the integral...
 
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Looks good. You'll need to use the integral I used above,
<br /> \int_{-\infty}^{\infty} dx e^{ikx} = 2 \pi \delta(k),<br />
and be careful with all of the algebra. A few points: you should actually have j_{0}(kr) = \sin(kr)/(kr), and you're missing some factors for the exponential form for \sin.
 
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