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math problem L(rinv)=4pid(x)d(y)

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Math working document by Phil, dated January 2011 and written while studying Stakgold's Green's function methods. It tests candidate operators, comparing the 3D radial operator with the 2D Laplacian, and works through the 2D divergence theorem, a paradox for 1/r, and the 2D fundamental solution. A phone call to Jim Ball leads to two solutions, one of which matches Phil's early candidate up to a factor of -r.

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Math Problem L(1/r)=4 π δ(x)δ(y) PhL 1.4.11 Summary: This doc comes right after the v1,v2,v3 series. It is the first doc where I really try to solve the problem Lr(1/r) = δ(r) in 2D as an isolated problem. I wrongly assume this is the same as the real problem I need solved which is Lr(1/R) = δ(r-r'), so I focus on Lr(1/r) = δ(r). This is all before Shankar and Jim Ball involvement. Early on I identify L = 23D,radial = r-2∂r(r2∂r..) as a possible candidate solution. I show that 22D,radial does not work since it gives 1/r3 when acting on (1/r). I don't know about ε regulation, I don't even know that δ(x)δ(y) = δ(r)/2πr, and I am not thinking about the Stakgold Theorem -- these ideas are all in the future. I understand perhaps for the first time in a long time the 2D divergence theorem, but I cannot make φ = 1/r satisfy it (later ε regulation fixes this problem). Late on this day 1/4 I call Jim Ball, and we eventually come up with two solutions to Lr(1/r) = δ(r), after much labor and learning on my part. It turns out that one of these solutions is exactly -r23D,radial so my initial candidate was pretty close to a solution. But I have no solutions to Lr(1/R) = δ(r-r') which is what I need to convert my 2D integral equation Ku=μu into a PDE EV problem. ___________________________________________________________________________________ Overview ( 1 page, written 1.18.11) 1 1. Statement of the Problem: 2 2. A similar problem 3 3. Back to our 2D problem 3 4. Question 1: how to you write 2 in polar coordinates? 3 (d) Example C: 2D Cartesian to Polar coordinates 4 5. Status at this point: 4 6. Question 2: what is the 2D divergence theorem? 4 7. Digression on a Paradox 5 8. A reminder of the 2D Fundy Solution of Stak Vol II p 50 6 9. Resume our problem. 6 10. What happens when we try L = 23D,radial using Jim regulation? 7 11. Email to Jim with this attachment called "jim delta 1_18_11.doc". 9 __________________________________________________________________________________ Overview ( 1 page, written 1.18.11) In Section 1 I state "my problem" L(1/) = 4πδ(x)δ(y). In Section 2 I consider the 3D problem L(1/r) = 4πδ(3)(r) and show how the 3D divergence theorem confirms that L = -2 . Since this is similar to my problem, maybe it will help. In Section 3 I propose Lf = r-2∂r(r2∂rf ) as a candidate solution for my problem, on the grounds that I can see that L(1/r) = 0 for r > 0, and because this is 23D,radial which did well in Section 2. But I have no idea whether or not it is a solution (see Section 10 below) . In Section 4 I derive the fact that 22D = r-1∂r(r ∂rf) + r-2∂θ2f in polar coordinates. I then note that the L = 22D,radial = r-1∂r(r ∂r...) is not a viable candidate solution to my problem because for this L we get L(1/r) = 1/r3 which fails to vanish for r > 0. In Section 5 I note that L = 23D,radial = r-2∂r(r2∂r..) is still a candidate, and I decide I should examine the 2D divergence theorem. In Section 6 I write the 2D divergence theorem as ∫dA 2φ = C dl φ = C dl ∂nφ. In Section 7 I apply this theorem naively to (1/r) and find that both sides give -2π/a except the LHS also has an extra term +2π/0 which of course diverges, so this is a paradox. I test the 2D divergence theorem on the simple function φ = r2 and it works. Then in a noted added 1.18.11 I am able to resolve the paradox by using the regulated [1/r] = 1/, and then for the 2D divergence theorem I get LHS = RHS both before and after the ε→0 limit (which gives -2π/a on both sides). But when I wrote this section, I never though of doing such regulation ! In Section 8 I use the 2D divergence theorem to verify that -[r-1∂r(r ∂r )] [ -(1/2π) ln(r)] = δ2(r) which is the same as -22D [ -(1/2π) ln(r)] = δ2(r). Thus us Stak's 2D fundy solution of course. In Section 9 I am stalled on "my problem" and I call Jim on 1.4.11 and he will think about it. My gut feeling is that my problem in fact has no solution. I mourn that I cannot think of a good web handle and can therefore not do a successful web search for someone who has dealt with "my problem". As it turns out later, Jim will come up with both a regulation method and two proposed and successful solutions! Those solutions will be these, where I now have 2π on the RHS Lxy(1) [1/r] = - limε→0 ∂r2(r[1 /]) = + 2π δ(2)(r) Lxy(3)[1/r] = limε→0 (1/r)∂r(r [1/]) = + 2π δ(2)(r) In Section 10, which was added today 1.18.11, I show that my original candidate of Section 3 above, when multiplied by -r, also solves my problem: Lxy(4)[1/r] = - r 23D,radial[1/r] = - r-1∂r(r2∂r[1/r]) = + 2π δ(2)(r) and due to Jim's Theorem r-1∂r(r2∂rf) = ∂r2(rf) it turns out that Lxy(4) is the same as Lxy(1). And when written just in terms of r, it is totally obvious that cases (4) and (1) are the same equation. This same logic then shows there are two solutions to the 3D problem: - 23D,radial ([1/r]) = - r-2∂r(r2∂r[1/r]) = 4π δ(3)(r) // the well known 3D solution r-2∂r(r [1/r]) = 4π δ(3)(r) // the newly found 3D solution In Section 11 I paste an email I am sent to Jim today 1.18 in which I derive both his solutions without using the Stakgold theorem, and thank him for his contributions. _____________________________________________________________________________ I am still taking my Stakgold mid-term exam. Here is a simple exam problem: 1. Statement of the Problem: What 2D differential operator L causes this to be true: L(1/) = 4πδ(x)δ(y) Certainly this is a simply-stated problem. We might first wonder whether such an operator even exists. In attempting to solve a problem, it is always helpful to study any similar problem that you already know how to solve. 2. A similar problem. We know that this is true -2(1/) = 4π δ(x)δ(y)δ(z) = 4π δ(r) So how does one prove this is true? I quote first from my integral theorems page ∫V dV A = ∫S dSA // divergence theorem = Gauss's theorem (1) Schaum 22.59 ∫V dV 2φ = ∫S dSφ = ∫S dS ∂nφ // application of the above with A = φ Let's set φ = 1/r and set the volume to be a sphere of radius a. We have then ∫V dV 2(1/r) = ∫S dS ∂nφ = ∫ a2dΩ ∂r(1/r)|a = 4π a2 (-a-2) = -4π Using the spherical form of 2, it is trivial to show that 2(1/r)= 0 for r > 0. Therefore, in the volume integral on the left, all the contribution must come from the region at r = 0. In other words, this equation that ∫V dV 2(1/r) = -4π is true no matter how small we make our spherical radius a. Since it is true in the limit that a→0, we conclude that 2(1/r) can only be -4πδ(r). This is a viable definition of a delta function as we learned in Stak. 3. Back to our 2D problem. If we work by analogy, it seems that the first thing we need is to find an operator L such that L(1/r) = 0 for r > 0. This must be true for L, otherwise we don't stand a chance. Suppose we try Lf = r-2∂r(r2∂rf) where we are now in 2D polar coordinates. We know that L(1/r) = 0 for r>0, very obvious, same idea as in the 3D case, but this is not a 2D r. So this is a candidate at least. Lots of questions are arising now: 1. Is this L somehow 2 in 2D? 2. Is there a 2D version of our divergence theorem? 4. Question 1: how to you write 2 in polar coordinates? Answer: we go to our tensors doc. In Section 9b we see this section: (d) Example C: 2D Cartesian to Polar coordinates  There we compute the metric tensor and find it to be g'ab = = and we then identify Q1 = Qr = 1 and Q2 = Qθ = r. We then fast-forward to the Laplacian section where we have 2f = (1/ [Q1Q2]) { ∂1 [ (Q2/Q1 ) (∂1f)] +∂2 [ (Q1/Q2 ) (∂2f)] } so this says 2f = (1/ [r]) { ∂r [ (r) (∂rf)] +∂θ [ (1/r ) (∂θf)] } = r-1∂r(r ∂rf) + r-2∂θ2f and to no great surprise we see this is the non-z part of the cylindrical coordinates 2. Notice that 2(1/r) = r-1∂r(r ∂rr-1) = - r-1∂r(r r-2) = - r-1∂r(r-1) = + r-1r-2 = r-3 and that therefore this 2 is NOT a candidate for our L operator above! This being the case, I guess we won't bother with question 2 above. Note: I compute this 2 "the long way" in doc "polar coordinates.doc" in math misc. 5. Status at this point: We still have a candidate Lf = r-2∂r(r2∂rf) for L, but this is NOT 2 in polar coordinates. Thus even if there is a 2D divergence theorem, it won't help us out. So our analogy with the known 3D case seems not too helpful! But let's do Question 2 anyway! 6. Question 2: what is the 2D divergence theorem? I answer this question in doc "Proof of the Divergence Theorem.doc" in math misc, and I also prove it. The result is this (after I repaired my notation in that doc! ) ∫dA F = C dl F 2D where on the left we integrate over some 2D area, and on the right we go around its boundary. If we wanted, we could set F = φ and this would then say ∫dA 2φ = C dl φ = C dl ∂nφ 2D 7. Digression on a Paradox Let's apply our 2D divergence theorem above to φ = 1/r. We claimed earlier that 2(1/r) = r-3 where we use our 2D Laplacian. Then our theorem applied to a disk of radius a says ∫rdr ∫dθ r-3 = ∫adθ ∂r(1/r)|r=a We easily find that RHS = 2π a (-1/a2) = -2π/a LHS = 2π !Syntax Error, Idr r-2 = 2π [ -r-1]|a0 = -2π/a + 2π/0 So what is going on here? The divergence theorem fails for φ = 1/r, it would seem. Let's first make sure our divergence theorem works for a more reasonable φ. Try φ = r2 2(r2) = r-1∂r(r ∂rr2) = r-1∂r(r 2r) = 2 r-1∂r(r2) = 4 r-1r1 = 4 ∫dA 2φ = 4A = 4πa2 C dl ∂nφ = 2π a ∂r(r2)|r=a = 2π a 2a = 4πa2 I guess my conclusion is that a divergence theorem is not valid if one side or the other involves a divergent integral. I think the fact that 2(1/r) = r-3 is correct for all r, and there is no delta function here. Note added 1.18.11. What happens to our paradox if we regulate 1/r using 1/ ? We then have 2[1/r] ≡ 2(1/) = r-1∂r(r ∂r{1/}) = (r2-2ε2)/(r2+ε2)5/2 // Maple Then for LHS we then get !Syntax Error, Irdr ∫dθ 2[1/r] = 2π !Syntax Error, Irdr(r2-2ε2)/(r2+ε2)5/2 = -2πa2/(a2+ε2)3/2 → -2π/a // Maple For the RHS we first compute ∂r[1/r]|r=a = ∂r(1/)r=a = - r/(r2+ε2)3/2 = - a/(a2+ε2)3/2 Then RHS = ∫adθ ∂r(1/r)|r=a = 2πa [- a/(a2+ε2)3/2] = -2πa2/ (a2+ε2)3/2 → -2π/a Now we get LHS = RHS both before and after the limit, so the divergence theorem is happy again! 8. A reminder of the 2D Fundy Solution of Stak Vol II p 50 The claim is this: -[r-1∂r(r ∂r )] [ -(1/2π) ln(r)] = δ2(r) First, it is clear that the LHS is 0 for r>0. So then we have to apply our 2D divergence theorem: ∫dA 2φ = C dl φ We want to apply this to the case φ = -(1/2π) ln(r) and we apply it to a disk of radius a. For the RHS, we have is so φ = ∂rφ = ∂r [ -(1/2π) ln(r)] = -(1/2π)(1/r). Then C dl φ = ∫a dθ [-(1/2π)(1/r)]|a = 2π a [-(1/2π)(1/a)] = -1 We are claiming that -2φ = δ2(r) so inserting this on the LHS gives -1, QED. 9. Resume our problem. We seek L such that L(1/) = 4πδ(x)δ(y) If we had this, then we could say L(1/) = 4πδ(x-x')δ(y-y') which is what I am really after. In 2D polar coordinates we have then L(1/r) = 4π δ(2)(r) I just called Jim (1.4.11) and I think he understood the question. He babbled about strings and monopoles, but they I asked him just to tell me what L is. He said he would have to think about it. So maybe I will go do something else for a while. If there is no solution, I would like to know why? Later (1.5.11) I emailed Shankar with this same question. Maybe I will let it ride for a while and see if either of these people tells me the answer. I don't know how to look up this kind of problem on the web. Why? (1) the symbols in the above equation don't work well in web searches (2) there are many different ways the equation could be written (3) this is not a "standard problem". One usually has L and asks for g. (4) there is not much 2D work in the world (5) there is no phrase I can use as a handle, like "two dimensional delta function". I will let some days go by, and if I get no response, maybe I will continue some more on this problem. Shankar responded and I think convinced me that if there is some L, it is not something with constant coefficients, so it is not a "simple" differential operator. I could not get him to say more. Jim is still pending. 10. What happens when we try L = 23D,radial using Jim regulation? This section was added 1.18.11. If this were a solution, we would have to have 23D,radial[1/r] = r-2∂r(r2∂r[1/r]) = const * δ(2)(r) First off we have to knock out a power of r to get correct dimensions, so we would maybe expect (r) 23D,radial[1/r] = r-1∂r(r2∂r[1/r]) = const * δ(2)(r) = const δ(r)/(2πr) As usual, we start with Maple's help and compute r-1∂r(r2∂r[1/r]) = r-1∂r(r2∂r(1/)) = -3 rε2 / (r2+ε2)5/2 = ε-2 { -3 (r/ε) / [(r/ε)2 +1]5/2 } so we have shown that -K r-1∂r(r2∂r(1/)) = ε-2 g(r/ε) where g(x) = 3Kx/(x2+1)5/2 Our normalization in 2D then says 1/2π = !Syntax Error, Idx x g(x) = !Syntax Error, Idx x{3Kx/(x2+1)5/2} = 3K !Syntax Error, Idx x2/(x2+1)5/2 = 3K { 1/3 } so we find K = 1/2π and therefore we have shown that limε→0{ - r-1∂r(r2∂r(1/))} = 2π limε→0 { ε-2 g(r/ε)} = 2π δ(2)(r) (*) and therefore L = limε→0{ - r-1∂r(r2∂r(1/))} is a third solution to my problem! But probably we can see this another way. Recall Jim's Theorem r-2∂r(r2∂rf) = r-1∂r2(rf) // = 2r-1∂rf + ∂r2f , did this in Maple just now or r-1∂r(r2∂rf) = ∂r2(rf) Thus, we can take our conclusion (*) above limε→0{ - r-1∂r(r2∂r(1/))} = 2π δ(2)(r) (*) and restate it as limε→0{ - ∂r2(r(1/))} = 2π δ(2)(r) and this is the same as the first of our known two solutions Lxy(1) [1/r] = - limε→0 ∂r2(r[1 /]) = + 2π δ(2)(r) Lxy(3)[1/r] = limε→0 (1/r)∂r(r [1/]) = + 2π δ(2)(r) The solution we just showed is the same as the first is this Lxy(4)[1/r] = - r 23D,radial[1/r] = - r-1∂r(r2∂r[1/r]) In retrospect, my very first candidate with this extra factor of r is a solution to my problem. So here then are three operators which work: Lxy(4) = - r-1∂r(r2∂r..) = - r 23D,radial Lxy(1) = Lxy(4) Lxy(1) = - ∂r2(r...) Lxy(3) = (1/r)∂r(r..) and due to Jim's Theorem r-1∂r(r2∂r..) = ∂r2(r..), the first two are the same. So in the end we can compare these two results: -23D,radial ([1/r]) = 4πδ3(r) = δ(r)/r2 // the famous 3D result -r 23D,radial ([1/r]) = 2πδ2(r) = δ(r)/r // one of our 2D results and, when expressed just in terms of r, these two equations are really the same equation. What this then tells us is that we also have a second solution to the 3D problem as follows: Our second solution to the 2D problem is this: Lxy(3)[1/r] = limε→0 (1/r)∂r(r [1/]) = + 2π δ(2)(r) = δ(r)/r Divide both sides by 1/r to get limε→0 (1/r2)∂r(r [1/]) = δ(r)/r2 = 4π δ(3)(r) Therefore we have these two 3D solutions r-2∂r(r [1/r]) = 4π δ(3)(r) // the newly found 3D solution - 23D,radial ([1/r]) = - r-2∂r(r2∂r[1/r]) = 4π δ(3)(r) // the well known 3D solution What happens if we subtract these two solutions? The difference should say r-2∂r(r [1/r]) + r-2∂r(r2∂r[1/r]) = 0 (*) or ∂r(r [1/r]) + ∂r(r2∂r[1/r]) = 0 or [ ∂r(r..) + ∂r(r2∂r..)] [1/r] = 0 or [ r2∂r2 + 3r∂r + 1] [1/r] = 0 // says Maple and in fact, if we just write [1/r] as r-1, this last equation is true for all r (Maple). This then verifies our second 3D solution. Line (*) by Jim's Theorem r-2∂r(r2∂rf) = r-1∂r2(rf) can be written this way r-2∂r(r [1/r]) + r-1∂r2(r[1/r])) = 0 or r-1∂r(r [1/r]) + ∂r2(r[1/r])) = 0 which says that when you subtract our known 2D solutions, you properly get 0. 11. Email to Jim with this attachment called "jim delta 1_18_11.doc". Jim, I'm sure you are pretty bored by now with the problem I proposed, but here is simple way to verify the two solutions you came up with, where there is no need for Stakgold's Theorem and all that stuff. If you don't want to look at equations, at least jump down to item 3. 1. Use this shorthand notation: [1/r] ≡ limε→0 1/ . (0) We have this 3D known fact that - 23D,radial ([1/r]) = - r-2∂r(r2∂r[1/r]) = 4π δ(3)(r) (1) and we know that δ(3)(r) = δ(r)/[4πr2] so the above says - r-2∂r(r2∂r[1/r]) = δ(r)/r2 (2) Multiply both sides by r - r-1∂r(r2∂r[1/r]) = δ(r)/r (3) Use the fact that δ(2)(r) = δ(r)/[2πr] so the above says - r-1∂r(r2∂r[1/r]) = 2π δ(2)(r) (4) Now use "Jim's Theorem" which says this r-2∂r(r2∂rf) = r-1∂r2(rf) // = 2r-1∂rf + ∂r2f (5) and multiply it by r to get r-1∂r(r2∂rf) = ∂r2(rf) (6) and install this into (4) to get - ∂r2(r[1/r]) = 2π δ(2)(r) (7) and this then gives your first solution to my posed problem L([1/r]) = 2π δ(2)(r) 2. Your second solution is this: (1/r)∂r(r[1/r]) = 2π δ(2)(r) (8) If this is correct, then if we subtract (7) from (8) we should get zero, (1/r)∂r(r[1/r]) + ∂r2(r[1/r]) = 0 (9) We shall now show that this is in fact zero and in this way we verify your second solution. For the first step we have Maple show this fact, (1/r)∂r(rf(r)) + ∂r2(rf(r)) = (1/r) [ r2∂r2+ 3r∂r + 1]f(r) (10) If we take f(r) = (1/r), this thing is trivially true: [ r2∂r2+ 3r∂r + 1](1/r) = 2/r - 3/r + 1/r = 0 (11) Not surprisingly, if we take f(r) = [1/r], it is still true. Maple gives [ r2∂r2+ 3r∂r + 1][1/r] = -ε2 (2r2-ε2)/(r2+ε2)5/2 → ε2 2/r3 → 0 (12) Setting f(r) = [1/r] in (10) and using (12) we conclude that (1/r)∂r(r[1/r]) + ∂r2(r[1/r]) = 0 which is the fact (9) we sought to show, and your second solution is then verified. 3. I wish to give proper acknowledgement to Jim for solving this problem and, in doing so, pointing out these useful facts: (a) The fact that δ(n)(r) = δ(r)/[Sn(1)rn-1] where Sn(1) is the surface area of a sphere in n dimensions. (b) That the proper way to regulate 1/r is to say [1/r] ≡ limε→0 1/ . Other methods I tried did not work, such as [1/r] ≡ limε→0 1/(r+ε) or [1/r] ≡ limε→0 1/r1+ε . (c) The fact that ∂r(r2∂rf) = r-1∂r2(rf) which I used above. (d) for coming up with both solutions noted above. When I asked Jim about this problem, I had no solutions at all.