Talk:Solid harmonics: Difference between revisions

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|                abc = Solid harmonics
|                cat1 = Physics
|                cat2 = Mathematics
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|                  by = --[[User:Paul Wormer|Paul Wormer]] 04:18, 22 August 2007 (CDT)
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This article (my own article from Wikipedia) gave LaTeX errors which I worked around.
This article (my own article from Wikipedia) gave LaTeX errors which I worked around.
Added to WP version section on relation to regular and irregular solid harmonics and references.  --[[User:Paul Wormer|Paul Wormer]] 04:18, 22 August 2007 (CDT)
Added to WP version section on relation to regular and irregular solid harmonics and references.  --[[User:Paul Wormer|Paul Wormer]] 04:18, 22 August 2007 (CDT)


:Hi Paul. Is the definition of the orbital angular momentum <math>\mathbf{L}</math> (second displayed equation) correct? The factor <math>\hbar</math> seems out of place. -- [[User:Jitse Niesen|Jitse Niesen]] 08:01, 24 August 2007 (CDT)
== Hbar ==


::Hallo Jitse, I don't see what is wrong. Classically :
Hi Paul. Is the definition of the orbital angular momentum <math>\mathbf{L}</math> (second displayed equation) correct? The factor <math>\hbar</math> seems out of place. -- [[User:Jitse Niesen|Jitse Niesen]] 08:01, 24 August 2007 (CDT)
::::<math> \mathbf{L} = \mathbf{r}\times \mathbf{p}
 
:Hallo Jitse, I don't see what is wrong. Classically :
:::<math> \mathbf{L} = \mathbf{r}\times \mathbf{p}
</math>
</math>
::QM:
:QM:
::::<math>
:::<math>
\mathbf{p} \rightarrow - i\hbar \mathbf{\nabla}, \qquad \mathbf{r} \rightarrow \mathbf{r}
\mathbf{p} \rightarrow - i\hbar \mathbf{\nabla}, \qquad \mathbf{r} \rightarrow \mathbf{r}
</math>
</math>
::What do you think it should be? --[[User:Paul Wormer|Paul Wormer]] 09:21, 24 August 2007 (CDT)
:What do you think it should be? --[[User:Paul Wormer|Paul Wormer]] 09:21, 24 August 2007 (CDT)
 
::I may well be misunderstanding what the article is saying. My issue is that you say first that, in spherical coordinates,
:::<math> \nabla^2 =  \frac{1}{r} \frac{\partial^2}{\partial r^2}r - \frac{L^2}{r^2} </math>.
::If I try to substitute
:::<math> \mathbf{L} = -i\hbar\, (\mathbf{r} \times \mathbf{\nabla}), </math>
::then I get
:::<math> \nabla^2 =  \frac{1}{r} \frac{\partial^2}{\partial r^2}r + \frac{\hbar^2}{r^2} (\mathbf{r} \times \mathbf{\nabla}) \cdot (\mathbf{r} \times \mathbf{\nabla}). </math>
::But the Laplacian should be independent of hbar. Perhaps the problem is in the first formula, and it should be
:::<math> \nabla^2\Phi(\mathbf{r}) =  \left(\frac{1}{r} \frac{\partial^2}{\partial r^2}r - \frac{L^2}{\hbar^2r^2}\right)\Phi(\mathbf{r}) = 0 , \qquad \mathbf{r} \ne \mathbf{0}. </math>
::I hope you can make sense of it. It's ten years ago that I did this stuff, and I never did it properly. -- [[User:Jitse Niesen|Jitse Niesen]] 09:53, 24 August 2007 (CDT)
 
::Looking at the dimensions (sorry, I should have started with that; but I'm only a mathematician), it's indeed the formula for the Laplacian that's weird (or, more likely, me!). -- [[User:Jitse Niesen|Jitse Niesen]] 10:09, 24 August 2007 (CDT)
 
:::You are right wrt to the Laplacian. My problem is that I 've worked my whole life with atomic units (<math>\hbar = 1</math>). I have to be more careful with hbar, I'm a bit sloppy with it. I'm working on an article on [[spherical harmonics]] right now and there I specifically stated that I take hbar = 1. Maybe you can have a look at this article and also at [[Legendre polynomials]], which is more up your street? --[[User:Paul Wormer|Paul Wormer]] 10:35, 24 August 2007 (CDT)
 
::::Okay, at least I now understand the first bit. However, I still feel uncomfortable with physical constants floating around in this article. I know where you're coming from and I've only seen these functions in QM, so I'm happy to concede if you think it's better to leave them in. But this is how I'd write the first couple of sentences (caution: probably contains some sign errors):
 
:::::{| style="border: 1px solid; width: 75%; "
|
Introducing ''r'', &theta;, and &phi; for the spherical polar coordinates of the 3-vector '''r''', we can write the Laplace equation  in the following form
:<math> \nabla^2\Phi(\mathbf{r}) =  \left(\frac{1}{r} \frac{\partial^2}{\partial r^2}r + \frac{1}{r^2} (\mathbf{r} \times \nabla)^2 \right)\Phi(\mathbf{r}) = 0 , \qquad \mathbf{r} \ne \mathbf{0}.
</math>
The differential operator <math>\mathbf{r} \times \nabla</math> equals the [[orbital angular momentum]]
:<math> \mathbf{L} = -i\hbar\, (\mathbf{r} \times \mathbf{\nabla})
</math>
up to a constant.
 
It is [[Angular momentum#Relation to spherical harmonics|known]] that [[spherical harmonics]] Y<sup>m</sup><sub>l</sub>  are eigenfunctions <math>(\mathbf{r} \times \nabla)^2</math>:
 
:<math>
(\mathbf{r} \times \nabla)^2 Y^m_{\ell} = -\ell(\ell+1) Y^m_{\ell}.
</math>
|}
 
::::I'll definitely have a look at [[Legendre polynomials]]. I regret that I've learnt so little about special functions. Oh, I suppose you read on my user talk page that \begin{align} now works (thanks to Greg). -- [[User:Jitse Niesen|Jitse Niesen]] 23:27, 24 August 2007 (CDT)
 
== Laplace operator ==
 
Hi Jitse, I start a new section, that indentation is driving me crazy. I believe I see your point: a mathematical article should stick to math and not be partly physics. Only in passing one can refer to the physics meaning of some math result. I agree with that. I have only one problem with your reasoning (a friend of mine calls this a matter of Kindergarten): your way of writing the Laplace operator is a bit foreign to me. The way I got to this result is: from Laplace-Beltrami in spherical polars and orbital angular momentum in spherical polars, comparison gives "your" Laplacian. I have seen your way before in Messiah p. 347 (that book is now in Dover, if you don't own it already it is worth buying). So, I would prefix your text with Messiah's outline of the way of writing the Laplacian. What do you think? PS. I would write the square of a vector(operator) always as a dot product. --[[User:Paul Wormer|Paul Wormer]] 03:03, 25 August 2007 (CDT)
 
:Yes, that my point. However, I'm afraid you're on your own here. Laplace-Beltrami is one of the things that I partially understand on a theoretical level, but I'd be completely lost if I'd actually have to do any computations with it. Put Messiah's outline there if you think it's a good idea (I don't have the book, but I'll consider getting it; thanks for the hint). I agree with your PS; I was just mirroring the <math>\textbf{L}^2</math> notation. -- [[User:Jitse Niesen|Jitse Niesen]] 05:59, 25 August 2007 (CDT)

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This article (my own article from Wikipedia) gave LaTeX errors which I worked around. Added to WP version section on relation to regular and irregular solid harmonics and references. --Paul Wormer 04:18, 22 August 2007 (CDT)

Hbar

Hi Paul. Is the definition of the orbital angular momentum (second displayed equation) correct? The factor seems out of place. -- Jitse Niesen 08:01, 24 August 2007 (CDT)

Hallo Jitse, I don't see what is wrong. Classically :
QM:
What do you think it should be? --Paul Wormer 09:21, 24 August 2007 (CDT)
I may well be misunderstanding what the article is saying. My issue is that you say first that, in spherical coordinates,
.
If I try to substitute
then I get
But the Laplacian should be independent of hbar. Perhaps the problem is in the first formula, and it should be
I hope you can make sense of it. It's ten years ago that I did this stuff, and I never did it properly. -- Jitse Niesen 09:53, 24 August 2007 (CDT)
Looking at the dimensions (sorry, I should have started with that; but I'm only a mathematician), it's indeed the formula for the Laplacian that's weird (or, more likely, me!). -- Jitse Niesen 10:09, 24 August 2007 (CDT)
You are right wrt to the Laplacian. My problem is that I 've worked my whole life with atomic units (). I have to be more careful with hbar, I'm a bit sloppy with it. I'm working on an article on spherical harmonics right now and there I specifically stated that I take hbar = 1. Maybe you can have a look at this article and also at Legendre polynomials, which is more up your street? --Paul Wormer 10:35, 24 August 2007 (CDT)
Okay, at least I now understand the first bit. However, I still feel uncomfortable with physical constants floating around in this article. I know where you're coming from and I've only seen these functions in QM, so I'm happy to concede if you think it's better to leave them in. But this is how I'd write the first couple of sentences (caution: probably contains some sign errors):

Introducing r, θ, and φ for the spherical polar coordinates of the 3-vector r, we can write the Laplace equation in the following form

The differential operator equals the orbital angular momentum

up to a constant.

It is known that spherical harmonics Yml are eigenfunctions :

I'll definitely have a look at Legendre polynomials. I regret that I've learnt so little about special functions. Oh, I suppose you read on my user talk page that \begin{align} now works (thanks to Greg). -- Jitse Niesen 23:27, 24 August 2007 (CDT)

Laplace operator

Hi Jitse, I start a new section, that indentation is driving me crazy. I believe I see your point: a mathematical article should stick to math and not be partly physics. Only in passing one can refer to the physics meaning of some math result. I agree with that. I have only one problem with your reasoning (a friend of mine calls this a matter of Kindergarten): your way of writing the Laplace operator is a bit foreign to me. The way I got to this result is: from Laplace-Beltrami in spherical polars and orbital angular momentum in spherical polars, comparison gives "your" Laplacian. I have seen your way before in Messiah p. 347 (that book is now in Dover, if you don't own it already it is worth buying). So, I would prefix your text with Messiah's outline of the way of writing the Laplacian. What do you think? PS. I would write the square of a vector(operator) always as a dot product. --Paul Wormer 03:03, 25 August 2007 (CDT)

Yes, that my point. However, I'm afraid you're on your own here. Laplace-Beltrami is one of the things that I partially understand on a theoretical level, but I'd be completely lost if I'd actually have to do any computations with it. Put Messiah's outline there if you think it's a good idea (I don't have the book, but I'll consider getting it; thanks for the hint). I agree with your PS; I was just mirroring the notation. -- Jitse Niesen 05:59, 25 August 2007 (CDT)