Abstract
The equation of Camassa and Holm [2]2 is an approximate description of long waves in shallow water.
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- 1.
See also Camassa, Holm, and Hyman [3].
- 2.
I recall H. Flaschka’s definition of integrability, the only honest one around: “You didn’t think I could integrate that, but I can!”
- 3.
0 is not in the spectrum.
- 4.
The indexing will be explained later.
- 5.
The computation can be found in McKean [12] I repeat it here for the reader’s convenience.
- 6.
The individual flows commute so the order of the product is immaterial.
- 7.
McKean and Trubowitz [13] encountered similar theta-like determinants in connection with the isospectral class of the quantum-mechanical oscillator − D 2 + x 2 − 1.
- 8.
m +∕m − is the positive/negative part of m.
- 9.
\(f_{n}(x) \simeq\) a “norming constant” × e −x∕2 at \(+\infty.\)
- 10.
\(A^{\mathfrak{p}}\) inverse is \(A^{-\mathfrak{p}}\), in which \(-\mathfrak{p}\) is \(\mathfrak{p}\) with signature reversed.
- 11.
\(G = (1 - D^{2})^{-1} = \frac{1} {2}\exp (-\vert x - y\vert )\) as before.
- 12.
Here and below f n is always normalized as in \(\|f_{n}\|^{2} =\int [(f_{n}^{{\prime}})^{2} + \frac{1} {4}f_{n}^{2}] = \lambda _{n}\int mf_{n}^{2} = 1.\)
- 13.
J = mD + Dm as before.
- 14.
mD + Dm is skew.
- 15.
The computation is the same.
- 16.
The preliminary evaluation of J from the previous display is used.
- 17.
\(\lambda _{0}m_{0}f_{0} = (\frac{1} {4} - D^{2})f_{0}\) is used to reduce the integrals to their final form.
- 18.
\(-\varLambda \int _{-\infty }^{+\infty }mf_{-}^{2} = 1\).
- 19.
f −(−1) = 0 implies f − ≡ 0. which is not so.
- 20.
f ⊗ f is the matrix \([f_{i}f_{j}: i,j \in \mathbb{Z} - 0]\).
- 21.
t is the diagonal matrix \(t_{n}: n \in \mathbb{Z} - 0\), and similarly for \(\lambda\).
- 22.
1 − M(1 + CM)−1 C = (1 + MC)−1, (1 + CM)−1 C being symmetric.
- 23.
Q −1(e t − 1) is symmetric and \(\eta = (e^{t} - 1)\xi\).
- 24.
See Sect. 9.5.2.
- 25.
Q −1 = 1 − (Q − 1)Q −1.
- 26.
PQ −1 is bounded.
- 27.
Q −1 = 1 − (Q − 1)Q −1.
- 28.
\(G = (1 - D^{2})^{-1} = \frac{1} {2}\exp (-\vert x - y\vert )\) as before.
- 29.
You may think line 3 is a little shaky but you can check line 4 directly from line 2.
- 30.
\(\lambda \int _{-\infty }^{\infty }mf \otimes f = \text{the identity}\).
- 31.
\(C\int _{-\infty }^{x}mf \otimes fC\) is compact with finite absolute trace; compare Sect. 9.5.3.
- 32.
\(\langle f_{1},f_{2}\rangle\) is the inner product \(\int _{-\infty }^{\infty }(f_{1}^{{\prime}}f_{2}^{{\prime}} + \frac{1} {4}f_{1}f_{2})\).
- 33.
The rest cancels.
- 34.
The rest cancels.
- 35.
\((1 +\xi \otimes \eta )^{-1} = 1 - (1+\xi \bullet \eta )^{-1}\xi \otimes \eta\).
- 36.
\(K\,K^{\dag } = e^{-\frac{1} {2} \vert x-y\vert }\).
- 37.
- 38.
\(q(0) =\ln \mathop{ \mathrm{ch}}\nolimits (T\sqrt{H/2})\) is used; it comes from the second version of T.
- 39.
If you think of the two solitons as particles, you might prefer to say they “bounce off each other,” but all such descriptions are just a manner of speaking, not the thing itself.
- 40.
Change n to − n and use \(\lambda \int _{-\infty }^{\infty }mf \otimes f = 1\).
- 41.
m ≠ 0 on any interval, so the functions \(f_{n}: n \in \mathbb{Z} - 0\ \mathop{ \mathrm{span}}\nolimits H^{1}\); see Sect. 9.2.2.
- 42.
The spectrum is odd.
- 43.
\(q =\ln c^{2}\).
- 44.
[a, b] is the Wronskian \(a^{{\prime}}b - ab^{{\prime}}\).
- 45.
The scale \(\overline{x}\) must be adjusted by an additive \(-\ln (-\varLambda )\) before making \(\varLambda \uparrow 0\).
- 46.
\(\overline{x}^{{\prime}} = me^{x}/e^{\overline{x}}\).
- 47.
\(m/\overline{y}^{{\prime}} = -(e^{{\prime}2} -\frac{1} {4}e^{2})/\varLambda e^{2}\).
- 48.
McKean and Trubowitz [13] served as a model.
- 49.
\(\overline{x}^{{\prime}} =\vartheta ^{2}/\vartheta _{-}\vartheta _{+}\).
- 50.
(1 + cM)−1 C is symmetric.
- 51.
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McKean, H.P. (2015). Fredholm Determinants and the Camassa-Holm Hierarchy. In: Grünbaum, F., van Moerbeke, P., Moll, V. (eds) Henry P. McKean Jr. Selecta. Contemporary Mathematicians. Birkhäuser, Cham. https://doi.org/10.1007/978-3-319-22237-0_9
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