Talk:Laplace–Runge–Lenz vector

SO(4)
Hi, I reverted the "burial" of SO(4). Its not that the Runge-Lenz is "related to SO(4)", its rather that the symmetry of planetary motion is SO(4). Its easy to understand the SO(3) part of planetary motion, and Runge-Lenz gives up the harder-to-see part of it. linas 17:08, 13 June 2006 (UTC)


 * In fact, the article already disucssses this, in the mis-titled section called "applications to quanum mechanics" In fact, the theory applies to the classical motion as well, not just the quantum motion. linas 17:30, 13 June 2006 (UTC)


 * I whacked on that section so as to give a name for the actual group that the commutators generate, and to make it clear that it applies to classical mechanics, not just to quantum mechanics. Perhaps you'll find these edits acceptable. linas 18:03, 13 June 2006 (UTC)

Explanation of edits (14 June 2006)
Hi Linas, I agree that the SO(4) pertains classically as well as quantum mechanically, and deserves mention in the introduction. However, I reduced it to a "teaser", for the following reasons.

My general approach to writing scientific articles is to "lay out a honey trail to enlightenment", that is, to begin very simply and gradually draw the reader onwards to ever greater complexity, all the while mixing the new with the familiar. This approach may be frustratingly slow for experts, but I believe that our target audience for this article consists mostly of people who are


 * interested in physics and/or astronomy
 * have a basic knowledge of algebra and calculus (~1 semester course)

Relatively few will have had any group theory, even fewer will understand the full Pioncare group and, I daresay, only experts will understand the SO(4) symmetry of the Lagrangian and how the LRL vector follows from it, especially given our (presently) terse explanation. I'm not saying that we shouldn't write for those few, on the contrary; however, I believe that we need to "ramp up" to that level gradually, to keep our non-expert readers engaged for as long as possible.

Does that seem sensible to you?

A few technical points
Strictly speaking, the LRL vector is not conserved exactly for real planetary motion. The orbit of every planet around a star precesses inevitably due to several factors, e.g., the corrections of general relativity, the imperfectly spherical distribution of mass in the star and the presence of mass (such as cosmic dust) between the star and the planet. Thus, the LRL vector is conserved exactly only in the two-body problem of classical gravity or electrostatics.

Your edit note suggests that SO(4) symmetry is the only reason for the importance of the LRL vector. I can't really agree with that, since the LRL was being used for planetary motion long before SO(4) was ever formulated. Perhaps that's not what you meant, though. Out of curiosity, when was the relationship between the LRL and SO(4) first pointed out explicitly? It'd be nice to find the original reference for the article. WillowW 09:59, 14 June 2006 (UTC)

So what is it?
So, what fundamentally does the Laplace-Runge-Lenz vector represent? Are there intuitive ways of thinking about it that the average person would understand? If so, they should be given in the first few sentences of the article. Mike Peel 19:08, 5 November 2006 (UTC)


 * Hi, Mike, thanks to your and Lambiam's suggestions, I tried to make the lead less math-y and more intelligible to the average reader.   Does it read better now, do you think?  Do you have any other suggestions before the article ventures out onto the dark, dangerous waters of peer review?  Thanks for your help! Willow 19:13, 9 November 2006 (UTC)


 * Much better, thanks. I've just moved some content from the start section to an Introduction section, as it was getting a bit long and complicated in places. I guess that the first couple of sections ideally want to be orientated at the lay person, providing a gradual buildup to the more complex stuff later on in the article. Mike Peel 08:55, 18 November 2006 (UTC)

Kepler's problem
What is "Kepler's problem"? Is it related to Kepler's laws of planetary motion, or the Kepler conjecture? Mike Peel 08:52, 18 November 2006 (UTC)

Symmetry

 * ''The vector A is constant, because the Kepler problem has an unusually high symmetry; it has SO(4) symmetry, whereas most central force problems of classical mechanics have only SO(3) symmetry.

I doubt this is true; there should be such vectors, differently defined, for most if not all central force problems. In any case, it does not belong in the introduction. Septentrionalis 23:06, 20 November 2006 (UTC)


 * Hi, Septentrionalis Nice name :) &mdash; "a person characterized by 73", did I guess right?


 * It is indeed true that the Kepler problem has a higher symmetry than most central-force problems, as I tried to describe later in the article. That's why, for instance, the energy levels of the hydrogen atom depend only on n and not on the other quantum numbers, l and m.  That is not true, for instance, if other potentials are added, such as those that cause level splitting in hydrogen.


 * I have to mention it in the introduction, because it is discussed at great length in the article itself (please see Lead section). I agree with the method of gradually working up to ever more complex concepts in a WP article, and I realize that the symmetry sentence might be daunting to beginners. But it might also lure them onwards with curiosity and, besides, it's only one sentence.  I hope that you'll understand my reasons and forgive my reversion. Willow 23:22, 20 November 2006 (UTC)


 * P.S. That reason also holds for including in the intro the precession of A under a perturbing potential, which is granted a whole section of the article, as requested in the scientific peer review. Secondly, the answer to the question "why should I care that A is constant?" &mdash; namely, that it lets one solve the Kepler problem by elementary geometry, rather than solving a differential or integral equation &mdash; also seems pertinent to the introduction.  Sincere apologies on our difference of opinion, Willow 23:44, 20 November 2006 (UTC)

Let me be clearer; it's the word because I don't believe. Septentrionalis 23:28, 20 November 2006 (UTC)


 * OK, I'm beginning to understand your point now; you're referring to the Fradkin (1967) paper referenced in the article and discussed in the scientific peer review? Namely, that other, possibly multi-valued functions can be defined for other central forces?  Would you please describe your objection in more detail, so that we can find a good way to resolve it?  Thanks! :) Willow 23:44, 20 November 2006 (UTC)

I didn't read Fradkin; I did the mathematics. As this article proves,
 * $$\frac{d}{dt} \left( \mathbf{p} \times \mathbf{L} \right) = -m f(r) r^{2} \left[ \frac{1}{r} \frac{d\mathbf{r}}{dt} - \frac{\mathbf{r}}{r^{2}} \frac{dr}{dt}\right] =

-m f(r) r^{2} \frac{d}{dt} \left( \frac{\mathbf{r}}{r}\right) $$. If the right-hand side is integrable to g(r), and in general it will be, consider the vector p x L - g(r). This will not be A; call it B. B will be a constant of the motion. Septentrionalis 23:58, 20 November 2006 (UTC)


 * Please allow me to encourage you to read the Fradkin reference, which treats this problem at length. The approach is valid, but g(r) is generally not a simple function of position.  Have to run now and stalk some hapless mountaineers, but I'll check in tomorrow. Thanks for your comments and insights! The Abominable Snowgirl 00:09, 21 November 2006 (UTC)

Improvements to the writing
Introducing bad writing because you think FA will require it is abominable. In fact, what WillowW cites is a suggestion from a guideline, not a requirement. FA requires that articles be comprehensible. Introducing SO(3) as though it were more than symmetry about a central point is jargon, justly deprecated. Septentrionalis 23:39, 20 November 2006 (UTC)


 * I'm speaking from my experience on Photon, in which I was required to add a paragraph to the lead to describe a section on the technological applications of photons. I believe that was right and a desirable thing to do, wouldn't you agree?  Here, we have more than one section on the SO(4) symmetry, which you'll find is very important to some mathematicians (see above).

In Photon, the added sentence is unobjectionable, and therefore a benefit to the article. Guidelines (and FA when it's working) impose things that should be done, unless there is a good reason not to.Septentrionalis 00:23, 21 November 2006 (UTC)


 * That said, I'm perfectly willing to replace SO(3) and SO(4) with more accessible language. Is that the main problem, or the Fradkin issue, or maybe both?  Just wondering, The Abominable Snowgirl ;) 23:50, 20 November 2006 (UTC)

You reverted edits intended to solve three problems.
 * The Fradkin issue, where the text was (at best) misleading, and I suspect false; if there is a constant vector B without SO(4), the text is wrong
 * "SO(3)" does not belong in the lead of an article, unless Lie group is preliminary reading; especially here, where "rotational symmetry of space" is so easy.
 * A should not be used before it is introduced. Septentrionalis 00:11, 21 November 2006 (UTC)

In this edit, I think "any" is what you want; but do think about it. Septentrionalis 00:15, 21 November 2006 (UTC)

Turning a new leaf
Hi Septentrionalis,

I couldn't resist flipping open my Lewis&Short as soon as my family was asleep, and discovering that your Latin name means "of or pertaining to the North", presumably due to the related word septentriones, the seven stars of the Big Dipper (Great Wain) and I guess Polaris. Fun name! :) I'm a Latin fan as well; you might enjoy some of my translations and original texts at Wikisource and Vicifons, although I know my own limitations and would welcome any suggestions on them.  I'll confess, though, that the music of Greek &mdash; especially Homer and Sappho &mdash; has always appealed to me more than any Latin text.

I probably won't have much time to edit today, but I thought we might turn over a new leaf. I really wasn't aware that I had destroyed your efforts to clarify the above three problems; from my perspective, I was adding back explanatory text that had been deleted from the lead section. I firmly agree with your goal of making the article as well-written, precise and accessible as possible, and I hope that we can work together to unite our differing perspectives.

My sense is that the because issue is semantic. My intended meaning was: "Given such-and-such a symmetry, such-and-such a quantity is conserved." It says nothing about what might be conserved under different symmetries. Perhaps we might eliminate the causal confusion by associative phrasing, e.g., "The conservation of A corresponds to (or is asociated with) a higher symmetry"?

I'm perfectly happy to remove the technical name SO(3) from the lead; it's much more accessible and less daunting without it.

I'm not sure about which A is being introduced before it is defined &mdash; do you mean Figure 1? It seems appropriate to mention in the caption, don't you agree?

Serenely, Willow 16:54, 21 November 2006 (UTC)
 * I have much Latin "and less Greek"; but I consider myself a Hellenist. As for the name, I mean Northerner in the strict American sense.


 * I have no problem with Figure I; but I hope what is now said about geometry in the lead is sufficient. Anything more definite belongs in Introduction, not the lead IMHO. Septentrionalis 18:14, 21 November 2006 (UTC)

Shakespeare is great, too! :) Happy to hear that Figure 1 is OK. :) Willow 20:51, 22 November 2006 (UTC)

Symmetry
I read Fradkin, and have good news and bad news. Septentrionalis 06:59, 22 November 2006 (UTC)
 * You don;t have worry about "multivalued"; what he means is that θ is multivalued as a function of r; i.e. that the period does not divide 2п.
 * On the other hand, he proves that all central forces have O(4) and SU(3) symmetry. This means that most of what this article says about symmetry is wrong.


 * I don't believe that what the article said was wrong per se, but I understand how the SO(4) arguments might be misconstrued. Please review the additions/corrections/refinements I made today and let me know what you all think.  We might be ready for FAC next week, do you all agree?  I'll probably be busy for the next few days with Thanksgiving, though.  See you all, Willow 20:51, 22 November 2006 (UTC)


 * I do think parts of the article are wrong, i.e. the sentence "The higher symmetry results in the conservation of both the angular momentum vector L and the Laplace-Runge-Lenz vector A." I thought that this was the case, and I might have misled you in this regard, but the fact that all central forces have O(4) symmetry means that it is at least more subtle than a simple application of Noether's theorem. I should have realized this immediately, because O(4) is six-dimensional so Noether's theorem would lead to six functionally independent conserved quantities, but there are only five. So, can you explain (or point to a reference explaining exactly how the O(4) symmetry leads to conservation of L and A?
 * Needless to say, this should be resolved before thinking of FAC. -- Jitse Niesen (talk) 22:39, 22 November 2006 (UTC)


 * You raise a really good point with the 5 vs. 6 conserved quantities. Of the five, four are defined by the energy and the angular momentum vector; so the LRL vector seems to correspond to only one additional symmetry.  What do you all think of the hodograph inversion/rotation mapping?  To me, the key is being able to find a mapping that transforms orbits of the same total energy but different angular momentum into one another; but whether that mapping will turn out to be SO(4), I haven't thought through yet.


 * In most papers, the identification of SO(4) seems to follow from the Lie algebra defined by the Poisson brackets; with the exception of the Rogers reference, no one seems to spell out the mapping explicitly. I'll keep looking, though; the 2nd external link is a promising review paper.


 * Terribly tired from cooking tonight, but looking forward to understanding this all, Willow 05:59, 23 November 2006 (UTC)

Fradkin derives L, A and the symmetries, both in the special case of (relativistic) inverse square forces and for general central forces. He doesn't expressly write the O(4) symmetry (and it must be O(4), not just SO(4); the reflection of any orbit is an orbit) but he sets up the Lie algebra. I'm not a physicist, and it's not clear to me what the rotation is; but it looks like it should be simple enough to explain if I really understood this.

I suspect, without reading everything (and I can't on Thanksgiving anyway) that five versus six is whether to count the energy as an invariant or take it for granted; so there should be two more after the energy and the angular momentum. Septentrionalis 17:02, 23 November 2006 (UTC)


 * The other review paper wasn't that helpful in understanding the O(4) rotation, unfortunately. :(


 * Six dynamically independent constants might be one too many for the six-dimensional phase space, being more than maximally superintegrable. The orbit would presumably be reduced to isolated points, right? That suggests two important considerations:


 * Maybe we're dealing with a restricted set of O(4) transformations? Presumably, there are other rotations of the orbits on the 4-sphere that change the energy of the stereographically projected orbits as well.


 * The vector A really adds only one dynamical constraint to those of E and L, which in turn suggests that we look for a single-parameter transformation that is independent of the normal O(3) spatial rotations. I like the Möbius transformation of the hodographs, but the Rogers reference has another type of pseudo-4-rotation.  I'll also go check out the old Fock and Bargmann papers, they probably have some good insights.


 * Talk to you all soon, Willow 16:37, 27 November 2006 (UTC)

Accessibility
I really think this article needs an explanation of the vector with as little technical machinery as possible. This includes such machinery as the angular momentum vector. Everybody writing this article knows what one is; but our readership doesn't. (For those who care about it, this will include the readership which is going to review any FA nomination, btw. See Featured article candidates/General relativity, where they are complaining of unit vector.)

If you don't think there can be such a thing as excessive precision, wait until we have the pedant who insists (correctly) that angular momentum is really not a vector, but a bivector.

Comments? Septentrionalis 23:42, 27 November 2006 (UTC)


 * I agree that we'll need to make the article more accessible to our readers, but first we should make it complete and correct, don't you agree? Then we can figure out how to lay out that "honey trail to enlightenment".  Along those lines...
 * We should make it correct; we can hardly make it complete. But the context section is correct now. It is also clear to you, me, Linas, and Jitse. Let me get back to you with a demonstration.... Septentrionalis 22:51, 28 November 2006 (UTC)

The O(4) symmetry
...I think I might understand the O(4) symmetry of the motion. The momentum hodograph approach was indeed correct, but the true mapping is much simpler and more direct than that cute little Möbius transformation. Rather, the mapping is a straightforward rotation of the 4d sphere that mixes the py and pw components. The key insight is that the 4d orbit is a great circle that intersects the px axis; thus, rotation about that axis, followed by stereographic projection, produces all the Apollonian circles directly. The foci px=±p0 are pinned throughout, lying as they do on the rotation axis. As in the original description, the normal O(3) rotational symmetry can be eliminated by choosing the Cartesian coordinates such that pz is aligned with the angular momentum vector L (and, thus, pz=0); by considering only the three-dimensional unit sphere defined by (pw, px, py), the symmetry also becomes more visualizable to the average reader. I'll try to add some Figures and text to explain this better over the next few days. Willow 19:18, 28 November 2006 (UTC)


 * Good. What is pw? Septentrionalis 22:51, 28 November 2006 (UTC)

Oops, sorry, I changed the variable names a few edits ago. I mean ηw; the w component is the fourth dimension in addition to the normal x, y, and z. Rotate a great circle on a 3d unit sphere that intersects the x-axis about the x axis, and project stereographically from the North pole unit vector w (1, 0, 0) onto the x-y plane and you produce a family of Apollonian circles with foci at x=±1. The eccentricity e of the orbit equals the sine of the dihedral angle between the great circle and the x-y plane. Hoping that this helps to clarify the transformation, Willow 23:24, 28 November 2006 (UTC)

Ummm...
...does anyone have any comments on all the material I've been adding &mdash; perhaps you're waiting until I've finished?

Confused by the silence, but still looking forward to FA status for our favorite vector, Willow 19:57, 1 December 2006 (UTC)


 * Just a short note that I'm still planning to look through your changes; unfortunately, I don't know when I'll find the time. -- Jitse Niesen (talk) 02:53, 6 December 2006 (UTC)

few quick comments
Sorry this isn't more thorough; I've been kind of pressed for unbroken blocks of time lately, and this article needs a bit of time to digest :)
 * These diagrams are exactly what people want converted to SVG. The current PNGs look quite pixelated on my screen; SVG will scale better.


 * I totally agree, but it's a little hard for me; my old version of Xfig doesn't do SVG (well). I'll try to figure something out.


 * Minor wording issue, but: for some reason, I don't like 'overview' and its variants in headings; an 'overview' is what the lead is for.
 * "The Laplace-Runge-Lenz vector A is defined below for a single point particle of mass m..." in the overview section - why not just put this in the mathematical definition section with the content it describes?
 * Does "Kepler problem" = "two-body problem", as suggested by the piped link in the Kepler orbits section? If so, explicitly say that, perhaps in the lead, where the linking goes to Kepler but not two-body problem.
 * In the 'conservation under inverse-square forces' section, the sentence 'none are as conserved as A' may be a bit ambiguous, since it's referring to the A defined immediately above rather than the general A used in the rest of the article. Maybe use a subscript?
 * Same section, 'these constant vectors are multivalued functions of the angle θ' - though it's not hard to figure out, θ hasn't been explicitly introduced in the preceding derivation.
 * I have a dim memory that the precession of Mercury agreeing with Einstein rather than Newton was a notable event. If what I'm thinking of is in fact what's described here, this section could be expanded to describe that discovery in more detail, which would also provide a bit of a practical touchstone for those who aren't just here for the vectors.


 * My memory is that the anomalous precession of Mercury was known well before Einstein did his calculations and, if I recall correctly, he cited it in an early paper on general relativity. I think the historical discovery that made the news was that Eddington expedition showing that the bending of starlight in a gravitational field was twice what Newtonian gravity would predict, and agreed with Einstein's predictions.


 * See Vulcan (hypothetical planet). Septentrionalis PMAnderson 22:55, 11 December 2006 (UTC)


 * Thank you, Septentrionalis, I do fondly recall Le Verrier's initial hypothesis for the anomalous precession; the planet Vulcan was a popular conceit of the science fiction of my youth. ;) There's also no doubting that Einstein's 1915 paper and the nearly exact agreement between his prediction and experiment did make a splash for general relativity. However, since the magnitude of the precession was known beforehand, an ungenerous scientist might have suspected that Einstein tinkered with his theory to produce the agreement.   The starlight bending was a more powerful result, since it was not known beforehand, don't you agree?  It seemed to get more press coverage, at any rate.  Willow 23:23, 11 December 2006 (UTC)


 * I think I had these two events conflated in my mind. I'm not familiar with the history, but just a bit more on this - ie, the fact that it was a notable 'post-diction' for general relativity - might be an interesting aside. Opabinia regalis 06:26, 13 December 2006 (UTC)


 * On that note, there's a lot of derivations in the middle (up to 'lie transformation') with little connection to their practical uses, ie, what is Noether's theorem used for? I think a bit more on what the practical applications of these vectors to physical problems would be useful, as several sections of the article seems to be spent going through alternative definitions and derivations, which can get rather abstract and cause the reader to forget why he wanted to read this article in the first place.


 * That is a crucial point; thanks! I'll work at making that part more sensible.

Opabinia regalis 06:06, 7 December 2006 (UTC)


 * I think I may have fixed some of those up &mdash; does it read better now? Thanks super-muchly for taking the time to review it! :D Willow 18:45, 7 December 2006 (UTC)


 * Looks nice! The main concern I have, I think, is that Noether's theorem and the Lie transformations both read as rather disconnected from the preceding and following sections. The Lie transformation in particular jumps back to Kepler's third law after some discussion of the applications of these vectors in QM. I can see that Noether's theorem comes into the conservation and symmetry section, but it might be better placed as a subsection? Or a reference in the Noether's theorem section to the fact that the implications are discussed further below? Opabinia regalis 06:58, 9 December 2006 (UTC)

New stuff
Separating this out for clarity (mostly nitpicky stuff, so the article must be good :)
 * Much prefer the current positioning of Noether's theorem and Lie transformations.
 * I'm not sure about the positioning of the Hamilton-Jacobi section. It comes between two sections discussing quantum, but the section itself only describes another way of deriving the vector's conservation. Seems like it might go more logically before the hydrogen atom section - possibly even before Poisson brackets, since that section follows rather clearly into the next.
 * Inconsistent wikilinking. Quantum number seems like an obvious candidate but isn't (perhaps because this text is new, I think?). Yet the rotational symmetry section wikilinks things like Cartesian coordinates (twice) and vector - subjects that no one who makes it that deep into the article will need clarification on.
 * I've never thought about this before, but do we have a label system for figures yet? I doubt this article will get too much editing after you guys are done with it, but it worries me to see things like "figure 7" in plain text, easily lost or obsoleted by the addition of a new figure or removal of an old one.
 * Picky writing question: was the Schrodinger equation "discovered" or "invented"? Opabinia regalis 06:26, 13 December 2006 (UTC)

More comments
I have some more comments, but no time now to write them down. Just quickly, it's much better now than two weeks ago. I didn't find any major issues However, I think the connection between the sections "Conservation and symmetry" and "Four-dimensional rotational symmetry" on the one hand and the rest on the other hand can still be tightened. More tomorrow. O yes, Willow, I have a recent version of XFig, so if you mail me the xfig files I can convert them easily to SVG. -- Jitse Niesen (talk) 12:09, 10 December 2006 (UTC)

I made some corrections, which I expect to be uncontroversial, myself. I split it in lots of small edits so that I could justify them individually; hope you don't mind. Here are some more comments:
 * In the first sentence, I think the fragment "a special case of the two-body problem" can be removed.


 * Umm, that one I'd like to keep, since it introduces the concept of "two body problem" and, indeed, clarifies that there are two bodies interacting. Forget that, you are totally right. It's much better this way.


 * In the first figure, use the proper symbol for the cross product, i.e., write p×L instead of pxL.


 * OK; did you fix this already?


 * This may be controversial, but in my opinion you should not include inline cites in the lead section. They distract the reader and they do not help with verifiability because the references are mentioned in the body of the article.


 * Maybe, I suppose; I don't have strong feelings about it. My thought was that the lead is meant to function as a "mini-article", so I thought that it should have the key references as well.  Let's both look into this, and find out what's customary!


 * The sentence "Similarly, there is not consensus for its symbol, although A is used most commonly." seems to be not important enough to appear in the lead.


 * Sure, that makes sense.


 * Typographical nitpicking: In my opinion, one should use en dashes as in Laplace–Runge–Lenz vector and not hyphens as in Laplace-Runge-Lenz vector (look at the length of the dashes).


 * My keyboard doesn't have an en-dash key; is there a simple way besides writing "& n d a s h ;"?
 * It's on the edit screen, above the Greek alphabet; look for Insert. Septentrionalis PMAnderson 22:50, 11 December 2006 (UTC)


 * Section "History of rediscovery": what is the word "anschaulich" doing here?


 * Intuitive clarification without intuitive clarification. ;) (apologies to J. A. Wheeler)


 * Section "Mathematical definition": I think it's clearer to write $$ \mathbf{A} = \mathbf{p} \times \mathbf{L} - mk\hat\mathbf{r} $$ for the definition without using the middle expression. The middle expression is not needed, and the two equal signs in $$ \mathbf{A} = \mathbf{p} \times \mathbf{L} - m k \frac{\mathbf{r}}{r} = \mathbf{p} \times \mathbf{L} - m k \mathbf{\hat{r}} $$ have a slightly different meaning (definition and equality, respectively).


 * Sure, that's fine; I introduced the longer equation back when I hadn't defined the unit vector, as I recall.


 * I'm used to adding a full stop after formulas if they end the sentence, e.g., the formula $$ E = \frac{p^{2}}{2m} - \frac{k}{r} = \frac{1}{2} mv^{2} - \frac{k}{r} $$. However, I have a vague memory that this is an instance where different conventions are followed in maths in physics.


 * I would really prefer to not punctuate the indented equations, since it might confuse lay-readers, rather than edifying them, which is the purpose of punctuation.


 * Section "Alternative scalings ...": Is it necessary to say "However, the choice of scaling and symbol for the Laplace-Runge-Lenz vector do not affect its conservation"? Perhaps somebody who made it this far will realize this themselves?


 * It is ghastly, I know, but I felt that it had to go in there, since even college students (such as me, once upon a time &mdash; how embarassing! ;) don't always "get" this, to say nothing of lay-readers.


 * The phrase "dyadic tensor" sounds rather quaint and outdated to me. Is it still being used in physics?


 * Indeed it is, albeit rarely. I used "dyadic" and the corresponding notation to clarify the relationship between W, A and B.


 * In the last formula in this section, you take the inner product of L with both W and A. Do you consider L as a dyadic tensor on the left-hand side and as a vector on the right-hand side? If yes, that's rather confusing, if no, I don't know what L ⋅ W is supposed to mean.


 * In a dyad, the two vectors stand "next" to each other in a specific order., e.g., X Y. Taking the right dot product with another vector Z results in the vector X scaled by the dot product Y⋅ Z, that is, X (Y⋅ Z).  Conversely, the left dot product of the dyadic tensor X Y with Z results in the vector Y scaled by the dot product Z⋅ X, that is, (Z⋅ X) Y.  That's why dyadic tensors are still around; they're useful for presenting some tensor calculations (contractions) in a brief way.


 * Section "Evolution under perturbing potentials": I'd call them perturbed potentials.


 * OK &mdash; did I fix it correctly?


 * Section "Poisson brackets": Are you sure that the sign of [D_i,D_j] depends on the energy? I find that rather odd. It also raises the question what happens what the energy is zero.


 * Yes, it's odd but I'm sure that it's true; it's because of the absolute value in the denominator or, seen another way, because of the radical in the denominator. The E=0 case is annoying but I know of no other definition.  The hodograph argument still works, though; the circles are tangential to the px axis.


 * Section "Quantum mechanics ...": Is it necessary to use the same symbol for the ladder operator as for the Laplace-Runge-Lenz vector?


 * No, but it's customary, along with the subscripts. What letter would you prefer?  I'm game. ;) (Added later: do you like J?)


 * What does "the eigenstates of the first Casimir operator are n^2-1" mean?


 * Oops, I mean, the "eigenvalues of the"; that's how we derive the Rydberg formula.


 * Section "Lie transformation": It's not clear what "the above equation" refers to.


 * It's that formula for A2 in terms of L and E that follows immediately; should I re-word that for clarity? (Added later: did so &mdash; is it any better?)


 * Section "Rotational symmetry ...": If the problem has an easy formulation in action-angle variables, perhaps you could include it in the article. I'm intrigued by this remark.


 * I'd be happy to, but I do give the reference and the article is already somewhat long and technical. I'm sensitive to Septentrionalis' criticism that the article is too technically exalted to make it as a FA, and would prefer to keep such details to a minimum.


 * How come that the coordinates x, y and z are not symmetric in the action-angle variables?


 * If I recall correctly, symmetry is broken by aligning z with the angular momentum, as in the above derivation.


 * You use &beta; at three places: when defining the rank-2 tensor W, when discussing the Hamilton-Jacobi equations, and in the action-angle variables. Are they the related?


 * They're totally unrelated, and you raise a very good point. I'll try to replace them with disambiguous symbols.

That brings me to the end. I trust you're not too disheartened by the length of the list ;) -- Jitse Niesen (talk) 12:55, 11 December 2006 (UTC)


 * Not at all disheartened! I'm very appreciative of the time and care you took with it, and for your fresh insights.  If we do ever make it to FA, it will be in good part thanks to your efforts! :) Willow 18:01, 11 December 2006 (UTC)

Include reflection symmetry?
Am I wrong in thinking the symmetry groups should be O(4), O(3,1), and O(3) throughout? The difference is not much if so, and they have the same Lie algebras; but I don't see why reflection is excluded. Septentrionalis PMAnderson 23:02, 11 December 2006 (UTC)


 * I have no real objection to including them if you'd like. It's just that the conservation laws are derived from continuous infinitesimal symmetry transformations (check out the Noether and Lie sections), whereas reflection is a discontinuous operation.  To me, that suggests that the reflection symmetry is irrelevant for showing that the Laplace-Runge-Lenz vector is conserved, and therefore a distraction. But what do you think?  Willow 23:12, 11 December 2006 (UTC)
 * Yes, the conservation laws derive from the Lie algebras, which are the results of the principal component of the Lie groups; and so the improper component makes no difference there. But it seems to me we will have two classes of readers;
 * Those who don't know exactly what SO(3) is, who won't care.
 * Those who do, who will see that O(3) is more than necessary for the proof, which depends on o(3); but who may wonder why we exclude improper rotations. I think the article on the groups is less than clear on this point. Septentrionalis PMAnderson 06:12, 12 December 2006 (UTC)


 * Hi, Septentrionalis, do you like new paragraph? Your point is very well-taken, and I tried to address it there.  Willow 20:07, 12 December 2006 (UTC)


 * Well, I was thinking of just dropping the S's, but flattery will get you everywhere. I think I've simplified things a bit; but feel free to revert. Septentrionalis PMAnderson 04:35, 13 December 2006 (UTC)


 * Well, let me flatter you some more &mdash; they were excellent edits! :)


 * Compliments aren't flattery if they're sincerely meant, no? You've made some excellent additions and changes to the article over the past month, making it much more accessible, insightful and accurate than it was earlier.  Doesn't it seem like we've all blended the best parts of our differing perspectives, in the best tradition of Wikipedia?  I tend to be over-enthusiastic and warmly approving, but I suspect that even the worst curmudgeon would concede that we've all done well with this article.  We might do better still; but I think we can pause for a moment and be proud of our work. :) Willow 15:45, 13 December 2006 (UTC)

Definition
This definition
 * Laplace-Runge-Lenz vector is a constant of motion in a key problem of classical mechanics: Kepler's problem...

does not look complete. May be it is better to write
 * Laplace-Runge-Lenz vector is a constant of motion for a particle moving in Kepler or Coulomb potential.

or similar to that. Alexander Mayorov 21:45, 16 December 2006 (UTC)

I would leave it at Kepler's problem (or maybe the Kepler problem). There are many other examples besides Coulomb potential problems that could be added but this would just make it too busy and unreadable.--Filll 21:57, 16 December 2006 (UTC)

Unreferenced sections
The Derivation of the Kepler orbits, Circular momentum hodographs, and Poisson brackets sections contain no references. Could you please add references that show the derivations (just to demonstrate that the derivations are not original derivations)? Thank you, Dr. Submillimeter 12:19, 31 December 2006 (UTC)

"which closely matches the observed orbital precession of Mercury"
This phrase is not correct, because the observed precession of Mercury is about 5600" per 100 years, but the value 43" per 100 years which we are interested is just a general relativity correction unexplained by Newtonian gravitation. Alexander Mayorov 11:59, 13 January 2007 (UTC)

three and four dimensional spheres; Kepler problem
I know there is some confusion about the terminology in the physics literature, but the 'four-dimensional sphere' mentioned throughout the article (starting from the lead) is really a three-dimensional sphere (in the four-dimensional space). This actually becomes rather confusing around the point where the stereographic projection is discussed.

An unrelated question: since this article is a de facto authoritative source on the Kepler problem, should the results of Moser (in the classical case) and Simms (in the quantum case) be mentioned? They really clarify the role played by the group O(4) in the integrability of the system. And of course, there is the larger hidden symmetry group O(4,2), for those who wonder how to reconcile the O(4) symmetry for negative energies with the O(1,3) symmetry for positive energies. Arcfrk 00:45, 5 May 2007 (UTC)


 * Hi Arcfrk! :)


 * It's so nice that our paths have crossed again. I'm sorry that I didn't notice your comment until just now, but I'll try to answer, as gamely as I can.


 * I skimmed the Moser references cited in the Guillemin reference when I wrote the article. However, I was too dim to see how his work contributed anything to the solution; they seemed just to restate the old stereoprojection results in a new language.  But surely that's my failing; I'm aware of Moser's other contributions, and would be surprised indeed if he were serving warmed-up leftovers. ;)   Could you please explain what his work adds to the Apollonian circle argument used here?  The same goes for the Simms results.


 * I'm not sure if I understand our differences in sphere-dimensionality nomenclature. Do we agree that



x^{2} + y^{2} + z^{2} + w^{2} = 1 $$


 * defines a four-dimensional sphere, despite its being a three-dimensional manifold? Similarly, don't most lay-people understand a "three-dimensional sphere" to mean the two-dimensional manifold embedded in three-space, as defined by



x^{2} + y^{2} + z^{2} = 1 $$


 * Consequently, I'm concerned that the phrase "three-dimensional sphere" might make them imagine the latter (which is by far more customary) than the former. Do you see the danger?


 * All that aside, I would be delighted with a no-holds-barred final section that discusses the Kepler problem in the latest terminology. It would be a glorious conclusion and if you'd like to write that section, that'd be great! :)  My suggestion would be to keep it brief, summarizing the highlights without trying to explaining them from scratch.  Talk to you soon, Willow 03:35, 10 May 2007 (UTC)


 * No, the four-dimensional sphere is a four-dimensional manifold, and the three-dimensional sphere is a three-dimensional manifold. There is a method to (t)his madness. I firmly believe that if a misconception exists, then encyclopaedias should dispel it, rather than propagate it. However, it's a valid concern, which I've tried to address by (1) mentioning that the sphere is situated in the four-dimensional space, and (2) linking to the article three-sphere. If anyone still chooses to be confused then as far as I can tell there is very little we can do, but if you can think of something else to unconfuse those lost souls, go ahead with it! Unfortunately, at the moment I don't have time to address your other points, let me just say that Moser's paper established a regularization of the Kepler's problem (in n dimensions), and this is definitely a worthwhile contribution. Arcfrk 04:59, 10 May 2007 (UTC)


 * Sorry, I'm not sure whether I followed that. Do you mean to say that the manifold defined by



x^{2} + y^{2} + z^{2} + w^{2} = 1 $$


 * is a three-dimensional sphere and that



x^{2} + y^{2} + z^{2} = 1 $$


 * is a two-dimensional sphere? I understand the sense of that, but I'm sincerely worried about how it will be understood.    Please consider the typical reader, who has not been trained in manifolds and who may honestly prefer to use the words "three-dimensional sphere" to describe a soap-bubble.  It may not be a case of "confusion", exactly ;)  Perhaps we can find some elegant finesse to the nomenclature? Willow 07:45, 10 May 2007 (UTC)
 * May I suggest the good old nineteenth-century words volume and surface respectively? if it is useful, we can link to three-sphere and sphere. Septentrionalis PMAnderson 17:19, 10 May 2007 (UTC)

Switching conventions
I found the Poisson bracket formula

$$ [ D_i, L_j ] = \epsilon_{ijs} D_s $$

confusing at first. I had expected

$$ [ L_i, D_j ] = \epsilon_{ijs} D_s $$

since this says (to those who know how to read it) that the Runge--Lenz vector transforms like a vector under rotations. A moment's scribbling convinced me that the formulas are equivalent. But, I think mine would be clearer to people in the know.

Also, why not use the usual notation for Poisson brackets? Why Lie brackets? Maybe 'cause nobody knows how to draw curly brackets on this system?

John Baez (talk) 17:46, 6 March 2008 (UTC)

Why not geometric algebra ?
I would not dare to add something to such a distinguished article, but for the fun and the readers interested in geometric algebra (see Hestenes "New Foundations for Classical Mechanics") I would like to show how easy and instructive is the manipulation of the LRL vector with that mathematical tool.

First some self explaining definitions and relations :


 * $$r=\rho r \qquad \qquad \dot r=\dot\rho \hat{r}+\rho \dot \hat{r} \qquad \qquad \hat{r} \cdot \dot{\hat{r}}=0$$


 * $$r \wedge \dot r=\rho^2\hat{r} \wedge \dot{\hat{r}}=\rho^2\hat{r} \dot{\hat{r}}$$

Then we show that the bivector $$L$$ is constant.


 * $$L=m r\wedge v=m r \wedge \dot r=m \rho^2\hat{r} \dot{\hat{r}}\qquad \qquad \ddot{r}=-k m^{-1}\rho^{-2}\hat{r}\qquad \qquad \dot L=m(\dot r \wedge \dot r+r \wedge\ddot{r})=0$$

And finally we find the eccentricity vector :


 * $$\dot(Lv)=L \dot{v}=[m \rho^2\hat{r} \dot{\hat{r}}][-k m^{-1}\rho^{-2}\hat{r}]=-k\hat r \dot \hat r \hat r=k\dot \hat r $$


 * $$\dot (L v-k\hat r)=0\qquad \qquad Lv=k(\hat{r}+e)\qquad \qquad L=\lambda \hat L\qquad \qquad L^2=-\lambda^2$$

And now we can do something which is not possible in classical vector algebra ; we can immediately calculate $$v$$ :


 * $$v=k L^{-1}(\hat{r}+e)=-k\lambda^{-1}\hat L(\hat{r}+e)$$

Of course that gives us immediately a coordinate free equation of the hodograph. One interesting feature, seldom cited, is the fact that apart of a dilatation factor the velocity vector $$v$$ is deduced from the vector $$(\hat{r}+e)$$ by a 90 degrees rotation, where $$\hat L$$ acts as the rotation operator. That is a lot more illustrative than trying to visualize the cross product ...

Chessfan (talk) 10:00, 29 May 2010 (UTC)


 * It is plainly unsound to claim that a direct calculation of the momentum is inaccessible to standard vector algebra: you simply take the cross product of the first eqn in the Circular momentum hodographs section with L; and use the textbook identity to obtain an eqn for p L2. That hodographic equation is coordinate independent. I fear you are rewriting the equations of the article in a language whose obscurity prevents you from identifying the underlying transcriptive identity of the two.             Cuzkatzimhut (talk) 15:16, 2 June 2010 (UTC)

Dont worry. I meant only it is easier with GA. That language which I learned when I was almost 70 is not obscure for me :)Chessfan (talk) 22:50, 2 June 2010 (UTC) Transcriptive identity is far from an adequate description of the relation between GA and Gibbs vector algebra. But I am aware that Hestenes already has lost the battle ; every time when I try to use GA I get negative reactions, kind ones like yours, very aggressive ones often (see Talk:Rotation representation (mathematics) ‎ ). Chessfan (talk) 10:01, 3 June 2010 (UTC)

Clarification needed on Laplace–Runge–Lenz vector
Hi, I'm sincerely confused by this article, and I'd be grateful if you could answer a question or two. Thanks!

My question is whether this template is working? Thanks! Willow (talk) 00:58, 11 July 2010 (UTC)


 * I've removed it and said why here. -- JohnBlackburne wordsdeeds 01:02, 11 July 2010 (UTC)

Feature failure
Wikipedia has featured many great articles about technical matters, but I'm afraid this isn't one of them. As I look over this for the first time, I think...

Sorry - I know I've inevitably made some errors in the above. But when you want to put an article like this in front of a broad audience you need some ignorant feedback, IMHO. Wnt (talk) 02:45, 31 December 2010 (UTC)
 * 1) The lead tells us that "the Kepler problem is mathematically equivalent to a particle moving freely on the boundary of a four-dimensional ball,", which is really kewl, if only I understood it or the section that explains it.  But... the lead does not tell us what the LRL vector is, mathematically speaking.  Might I suggest something like "A vector directed along the major axis of an ellipse, pointing in the direction toward which the central body is displaced relative to the center of the ellipse"?
 * 2) The next section tells us that "Whereas for typical conserved quantities, there is a corresponding cyclic coordinate in the three-dimensional Lagrangian of the system, there does not exist such a coordinate for the LRL vector."  WETF that means.  But where's the explanation?  Oh, yeah, and where's the inline citation if I wanted to go hunting for the explanation?
 * 3) After that we finally get the mathematical derivation.  It might be a bit simpler in spots - it might be worth saying p x (r x p) - mkr/|r| - oh, yeah, but there's a trouble.  What is k?  Does it say anywhere in the article how to calculate k?
 * 4) The figure is a noble effort but falls short - for example, where the legend says that the angular momentum vector L is perpendicular to the orbit, and people look and see that p x L is perpendicular to the orbit at each spot (in 2-D), they're going to get confused.  And the figure shows just one orbit - the question is, how does A vary over all orbits?  I assume that for an elliptical (i.e. inverse square) orbit that A will be a vector related to the displacement of the focus to one side of the center of the ellipse.  (Hmmm, is there some simple way to calculate A as a scalar function of this displacement?)
 * 5) There's an effort here to express the generality of this to non inverse square forces, but is there any tangible example to give?  Does someone actually work this out with a deuterium nucleus and the strong force or something?  Can we see an example of how A varies under a situation more radical than a gradually advancing perhelion?
 * 6) Question: in political articles people are eager to farm out "details" to additional articles.  Here, why can't we displace the whole part about how the elliptical orbit is a four dimensional symmetry to some other article?
 * 7) It would be useful to say when A is zero.  Is it accurate to say that this is true for any perfectly circular orbit?


 * Agreed, mostly. I'm literate enough to follow, for example, a proof o Kepler's laws from Newton's laws (at ODE or [US] "calculus II" level), and I kinda intuited that something else is conserved in there. Eventually I found Laplace name-droped in a book as the other thing conserved... and I found this article... but it's anything but clear to me. The writing in it seems to go around in circles. 188.25.77.29 (talk) 14:02, 14 January 2016 (UTC)

boundary of a sphere???
The article states "the Kepler problem is mathematically equivalent to a particle moving freely on the boundary of a four-dimensional sphere". But this is nonsense. A sphere, four-dimensional or otherwise, has no boundary. Do you mean four-dimensional ball? -lethe talk [ +] 06:17, 5 December 2012 (UTC)

WP:PHYSICS review: A-level article
I'm beginning a sort of WP:Expert review process for articles independent of the featured article system which I've realized has problems. As such, I've rated this article a level 'A' which means it is of the quality that would be expected from a professional reference work on the subject. I say this as a person with graduate degrees in astrophysics, but I encourage others who have similar qualifications to make comments if they believe my judgement to be incorrect.

jps (talk) 02:18, 12 September 2013 (UTC)
 * It might contain a collection of correct statements, but it's not an article for someone who doesn't already know the topic to learn much from. 188.25.77.29 (talk) 14:15, 14 January 2016 (UTC)

Bad dimensions
Philosophaies revisions of today are wrong, and have spoilt dimensional consistency. e should be dimensionles. They have been reverted. Please discuss misgivings before incorrect edits. Cuzkatzimhut (talk) 14:48, 25 September 2013 (UTC)

Big Scary Red Error Messages
I have spotted three Big Scary Red Error Messages on the page, the first being under heading "Rotational symmetry in four dimensions"

Failed to parse(syntax error): \begin{align} \boldsymbol\eta & = \displaystyle \frac{p^2 - p_0^2}{p^2 + p_0^2} \mathbf{\hat{w}} + \frac{2 p_0}{p^2 + p_0^2} \mathbf{p} \\[1em] & = \displaystyle \frac{mk — r p_0^2}{mk} \mathbf{\hat{w}} + \frac{rp_0}{mk} \mathbf{p} \end{align}

I suspect that they are both on the server end, as I found them in both Firefox (26.0) and IE 11.0.9600.16476. Simon Crase. — Preceding unsigned comment added by 118.93.231.190 (talk) 23:36, 16 December 2013 (UTC)

A Commons file used on this page or its Wikidata item has been nominated for deletion
The following Wikimedia Commons file used on this page or its Wikidata item has been nominated for deletion: Participate in the deletion discussion at the. —Community Tech bot (talk) 23:37, 9 February 2020 (UTC)
 * Relativistic precession.svg

abstract math geekery
If one ever wanted to kick this into the domain of abstract mathematics, one could tie this into the theory of symmetric spaces. It goes something like this: this article already explains that SO(4)/Z_2 = SO(3) x SO(3) but one could also write this as saying SO(4)/SO(3)= S^3 the three-sphere and the three-sphere is the Lie group manifold of SU(2) and of course SU(2)/Z_2 = SO(3) so that's just an alternative factorization of "the same stuff". The Z_2 is the involution. So the sphere is a symmetric space and symmetric spaces have an involution, the Cartan involution. The Cartan involution has two eigenvalues, +1 and -1. Now, if I recall correctly (its been a while) the -1 eigenvalue corresponds to the bound orbits and the eigenvalue +1 to the ionized orbits. The involution corresponds to a factorization of $$\mathfrak{g} = \mathfrak{k}\oplus\mathfrak{p}$$. Now, if you look at this article, and look at the part that says "Poisson bracket" -- "unscaled functions" you will see commutators that are effectively the same as those for "symmetric space -- algebraic definition" (which uses different notation $$\mathfrak{g} = \mathfrak{h}\oplus\mathfrak{m}$$ but its the same thing).

Then $$\mathfrak{p}$$ can be further factorized to pieces corresponding to different orbital angular momentum (for the hydrogen atom). This is the same factorization as for Riemanninan manifolds, where each distinct factor of $$\mathfrak{p}$$ has a distinct eigenvalue for the Killing form (the quadratic  Casimir invariant) which for this particular example is just the total orbital angular momentum $$L^2$$ (of the hydrogen atom; don't know how this works for the non-quantized version). The spaces here are the spherical harmonics; the spherical harmonics generalize to arbitrary symmetric spaces as eigenvalues of $$\nabla^2$$ on whatever symmetric space you're interested in. So "hydrogen atom" in a generic setting.

But wait, there's more (for the low, low price of $12.99 you also get ...) an extended bilinear form $$ds^2$$ that is a sum of the metric on the underlying space, plus the sum of weighted Killing forms on each of the $$\mathfrak{p}$$ factors... just like in this article, subsection titled "Conservation and symmetry".

I think I've spewed enough key-words here that your favorite search engine will find more detailed expositions of this stuff ... I think it would be cool to articulate this stuff ... somewhere if not here ... (because otherwise its just dry, dusty, pointless and dead abstractions in textbooks on Riemannian geometry)

p.s. Going through the article edit history, someone else (not me) attempted to wikilink this to potential theory which is the theory where the eigenvalues of the Laplacian for symmetric spaces are studied (even though our wikipedia article never quite comes out and says this). I have no clue if there is a generic LRL vector for these generic cases, but maybe there is one, any time you take a quotient G/H !??? That would also be cool to articulate, if it was true... it seems believable ... 67.198.37.16 (talk) 04:16, 7 November 2020 (UTC)

Featured article concerns
Looking at this as part of the ongoing FA sweeps. Currently, there is a very large amount of uncited text in here, which is problematic against the FA criteria. While some of it may not need a citation under WP:WTC as self-proving math stuff, the very high percentage of uncited text is problematic and may require a featured article review if not addressed. Hog Farm Talk 05:23, 17 April 2021 (UTC)

Dear editor Septentrionalls Pmanderson
Could you get my message on page User:Pmanderson (talk).What is a reason to remove the article: Fock symmetry in theory of hydrogen.

And, what is essential here, the operator of Laplace-Runge-Lenz vector doesn't exist in the momentum space ! So, Fock's symmetry found in momentum space, has nothing to do with that article.

Sincerely Yours

EfimovSP (talk) 11:27, 6 September 2021 (UTC)

"Mathematically equivalent"
This could be misleading to some readers:


 * This conclusion does not imply that our universe is a three-dimensional sphere; it merely means that this particular physics problem (the two-body problem for inverse-square central forces) is mathematically equivalent to a free particle on a three-dimensional sphere.

The mathematical equivalence is subtle:

1) It only holds for elliptical orbits of the two-body problem, not parabolic or hyperbolic orbits.

2) In this case the Hamiltonian of two-body problem is minus the inverse of the Hamiltonian of the free particle on the three-dimensional sphere.

Thanks to 2), solutions of the two-body problem where the particle has a very large negative energy and orbit very rapidly correspond to solutions of the free particle on the sphere where the particle has a small positive energy and moves around the sphere very slowly.

It's possible a slightly different wording would better hint at these issues, without sinking into details.