Undergrad Orthogonality of spherical Bessel functions

Click For Summary
The discussion focuses on determining the value of k at which the integral function I_{\ell}(k,k_{i}) peaks, suggesting it should peak at k = k_{i} due to the orthogonality of spherical Bessel functions. Participants explore the complexity of the integral, noting it appears to be a 3D integral dependent on the radial coordinate. Integration by parts is proposed as a method to simplify the integral, leading to an approximation involving the logarithmic function and the spherical Bessel functions. The conversation emphasizes the significance of higher-order integrals and their diminishing contributions, while also suggesting further examination of these integrals in computational analysis. Overall, the method of integration by parts is highlighted as a key approach to understanding the behavior of the integral.
sunrah
Messages
191
Reaction score
22
at what value of k should the following integral function peak when plotted against k?

<br /> I_{\ell}(k,k_{i}) \propto k_{i}\int^{\infty}_{0}yj_{\ell}(k_{i}y)dy\int^{y}_{0}\frac{y-x}{x}j_{\ell}(kx)\frac{dx}{k^{2}}<br />

This doesn't look like any orthogonality relationship that I know, it's a 2D integral for starters, but I'm told it should peak at k = ki due to orthogonality of the jl
 
Physics news on Phys.org
This integral is 3D if your integrand only depends on the radial coordinate, and not angular coordinates. Note it starts at 0 and goes outwards. What you need is a way to make this whole thing a single 3D integral. If you expand by parts, you should be able to isolate the integrand of the dx integral as a function of y inside the dy integral, and that should result in the orthogonality integral. If that wasn't clear let me know and I'll write up what I mean in detail.
 
Twigg said:
If that wasn't clear let me know and I'll write up what I mean in detail.

Thanks for replying.
If I understand correctly, I should try integrating by parts. So doing this I find my function can be approximated as
<br /> I_{\ell}(k,k_{i}) \approx \frac{k_{i}}{k^{2}}\int^{\infty}_{0} y^{2}(\ln{y} - 1)j_{\ell}(k_{i}y)j_{\ell}(ky)dy<br />

to do this I'v used j_{\ell}(0) = 0 for \ell &gt; 0 (I'm not interested in monopols) and that the value of higher-order integrals, e.g.
<br /> \int^{\infty}_{0}dz (\int^{z}_{0}dy\int^{y}_{0}j_{\ell}(x)dx)<br />

are progressively much smaller than first-order integrals (if that's clear??). My opinion is that for this function I_{\ell} to peak at k=ki then the approximation shown featuring the two un-integrated sph. Bessel functions must dominate. Also just plugging some values into python seems show that there are orders of magnitude difference between higher-order integrals of jl.

Is this what you meant?
 
That is what I had in mind, but to be honest I hadn't examined the remainders when I first replied. It might not be the best method, it's just what jumped out at me. After working it through on paper, I got the same approximation as you when I expanded the inner integral (the dx integral) to first order using integration by parts. When I did the second-order correction, I found that the next term in the part of the inner (dx) integral that is a multiple of the ##\ell##-th spherical bessel depends on ##\ell##, due to the recursion formulas. So when you run your Python calculations, you might want to examine those higher-order integrals for some high-order spherical bessels, like ##j_{10}(x)## and ##j_{100}(x)##, just to be on the safe side.

Here's what I got for the second-order integration by parts expansion:

##\int_{0}^{y} \frac{y-x}{x} j_{\ell}(kx)dx = [ y (\ln y - 1) - \ell y (\ln y - \frac{3}{2}) ]j_{\ell}(kx) - ky^{2} (\ln y - \frac{3}{2}) j_{\ell + 1}(kx) + ...##

By orthogonality, you can ignore the ##\ell + 1## term and higher in ##I_{\ell}##, but the coefficient on the first term will probably be an infinite series in ##\ell##. You might even be able to extrapolate the series.

To get the above result, I used the following recursion relation after the first integration by parts:

##j'_{\ell}(z) = \frac{\ell}{z} j_{\ell}(z) + j_{\ell + 1} (z)##

This is where I'm getting my series for the coefficient on the ##\ell##-th spherical bessel.

Hope this helps!
 
Relativistic Momentum, Mass, and Energy Momentum and mass (...), the classic equations for conserving momentum and energy are not adequate for the analysis of high-speed collisions. (...) The momentum of a particle moving with velocity ##v## is given by $$p=\cfrac{mv}{\sqrt{1-(v^2/c^2)}}\qquad{R-10}$$ ENERGY In relativistic mechanics, as in classic mechanics, the net force on a particle is equal to the time rate of change of the momentum of the particle. Considering one-dimensional...

Similar threads

  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 10 ·
Replies
10
Views
3K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 9 ·
Replies
9
Views
4K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
2
Views
3K
Replies
1
Views
2K
  • · Replies 14 ·
Replies
14
Views
2K