|
History and Origins
of the
Korteweg-de Vries Equations
Eduard de Jager
Korteweg-de Vries Institute
University of Amsterdam, the Netherlands
(translated from Dutch by Hinke Osinga, University of Bristol,
UK) |
Professor Eduard de Jager. |
Introduction
Korteweg and De Vries gained international
recognition for their model equation of shallow-water waves that now
bears their name. However, their fame rose only seventy years after
the journal publication on the Korteweg-de Vries (KdV) equation,
caused by a rediscovery of the KdV equation by Zabusky and
Kruskal [23] and the many
applications that followed [9].
The mathematical literature usually refers to a
simplified form of the KdV equation, but there is actually little
difference with the formulations given in the PhD thesis of De Vries
from 1894 [22] or the famous paper
by Korteweg and De Vries in the Philosophical Magazine of
1895 [12]. Historically, however,
the origins of the KdV equation are to be found much earlier, starting
with the experiments of Scott Russell in 1834 [21] and the subsequent theoretical
research, mainly by Boussinesq in 1871-1877 [1]-[4],
Raleigh (Strutt, J.W.) in 1876 [18], and Saint Venant in 1885 [20]. This article considers aspects of the
research by Boussinesq, on the one hand, and by Korteweg and De Vries,
on the other hand, particularly focusing on the most accessible paper
by Boussinesq [3] and the paper in
the Philosophical Magazine of Korteweg and De Vries [12]. As we shall see, it is Boussinesq who
deserves the honour of having formulated the first satisfactory
mathematical description of long waves and is, therefore, actually
the true discoverer of the KdV equation, albeit in a disguised way;
see also R. Pego [17]. For many
historical details, including later developments, the reader is
referred to A.C. Newell [15],
R.K. Bullough [6],
J.W. Miles [14],
O. Darrigol [7], and
KdV'95 [7].
Problem formulation
In 1834 the Scottish naval architect Scott Russell
on horseback followed a towboat, pulled by a pair of horses along the
Union Canal, connecting Edinburgh and Glasgow. The boat was suddenly
stopped in its speed -- presumably by some obstacle -- but not the
mass of water that it had put in motion. Scott Russell observed a very
peculiar phenomenon: a nice round and smooth wave -- a well-defined
heap of water -- loosened itself from the stern and moved off in
forward direction without changing its form with a speed of about
eight miles per hour; the wave was about thirty feet long and one or
two feet high. He followed the wave on his horse and after a chase of
one or two miles he lost the heap of water in the windings of the
channel [21]. Many a physicist
would not be inclined to analyze this phenomenon and leave it as it
was, but Scott Russell recognised the peculiarity of the phenomenon in
this seemingly ordinary event. He designed experiments generating long
waves in long shallow basins filled with a layer of water and he
investigated the phenomenon he had observed. He studied the form of
the waves, their speed of propagation and stability. A schematic view
of these experiments is shown in Figure 1.
For a detailed historical study of Scott Russell's work we refer to
the overview paper by R.K. Bullough [6].
Figure 1:
Schematic view of the experiments by Scott Russell; adapted from
M. Remoissenet [19].
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In the 19th century in England and France there
existed a rich tradition in the mathematical description of
hydrodynamic phenomena, in particular of wave motions in
incompressible fluids without friction; famous names are Airy, Stokes,
Rayleigh, Lamb, Lagrange, Saint Venant, and Boussinesq, to name a
few. Scott Russell challenged the mathematical community to prove
theoretically the existence of his solitary wave and to give an a
priori demonstration a posteriori. His challenge did not fail to
have an effect. From a mathematical and physical point of view he
asked to show the existence of a stable solitary wave that propagates
without changing form. In stark contrast with the experimental results
of Scott Russell, Airy was of the opinion that this was not possible:
a propagating wave would necessarily be steeper at the front and less
steep at the back; he was supported in this view by Lamb (1879),
Bassett (1888) and McCowan (1892); see [12,22].
Initially, Stokes objected to the well-defined heap of water,
because he believed that the only stable wave should be sinusoidal,
but later he admitted that he was mistaken.
The a priori demonstration a posteriori, as
requested by Scott Russell, was first provided by Boussinesq [1]-[4] in
1871-1877, some time later by Raleigh [18] in 1876, and in order to remove all
existing doubts over the existence of the solitary wave, by Korteweg
and De Vries [12,22] in 1894. In many ways, Rayleigh used
the same methods in his mathematical analysis as Boussinesq and later
Korteweg and De Vries. Since Rayleigh's explanation is less detailed,
we will not consider it here; see [10] instead.
The equations of Boussinesq and Korteweg-de Vries
The derivations of the equations of Boussinesq and
of Korteweg and De Vries are very similar. Both authors consider long
waves in a shallow basin with rectangluar cross section; the fluid is
assumed incompressible and rotation free, and there is no friction,
also not along the boundaries of the basin.
Boussinesq
Boussinesq introduces coordinates \((x, y)\)
that represent the position of a fluid particle at time \(t\); the
pressure in the fluid is denoted \(p\), its density \(\rho\), and the velocity vector \((u, v)\). The height
of the water in equilibrium is denoted by the constant \(y = H\)
and the wave surface by the function \(y = H + h(x, t)\),
where the amplitude \(h\) of the wave is small compared
with \(H\); see Figure 2. Finally, he assumes that the wave length is large
with respect to \(H\).
Figure 2:
Mathematical representation of the wave surface.
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Since the fluid is rotation free the velocity
vector is equal to the gradient of a scalar field, the so-called
velocity potential \(\phi(x, y, t)\). Incrompessibility
implies that the velocity potential satisfies Laplace's equation, so
that we have the series expansions:
\(\phi\) |
\(=\) |
\( \int f \; dx - \frac{1}{2!} y^2 \frac{\partial
f}{\partial x} + \frac{1}{4!} y^4 \frac{\partial^3 f}{\partial x^3} - \dots,\) |
(1) |
\(u\) |
\(=\) |
\(\frac{\partial \phi}{\partial x} = f - \frac{1}{2!} y^2 \frac{\partial^2
f}{\partial x^2} + \frac{1}{4!} y^4 \frac{\partial^4 f}{\partial x^4} - \dots,\) |
|
\(v\) |
\(=\) |
\(\frac{\partial \phi}{\partial y} = -y \frac{\partial f}{\partial x} + \frac{1}{3!} y^3 \frac{\partial^3 f}{\partial x^3} - \frac{1}{5!} y^5 \frac{\partial^5 f}{\partial x^5} + \dots,\) |
|
where \(f\) is an as yet unknown function
of \(x\) and \(t\) that slowly
varies with \(x\) (the waves are long with respect to \(H\)). The boundary condition \(v = 0\) at \(y = 0\) is satisfied and the boundary condition on the wave
surface can be derived from the equations of motion and the kinematic
equation.
Integration of equation (1)
leads to the Bernoulli equation
\(\frac{p}{\rho} = -g y - \frac{\partial \phi}{\partial t}
- \frac{1}{2} \left( u^2 + v^2 \right) + \chi(t),\)
where \(g\) is the gravitational
acceleration constant and \(\chi\) is an arbitrary function
that only depends on \(t\). If the constant atmospheric
pressure is \(p_0\) then we also have
\(\frac{p}{\rho} = \frac{p_0}{\rho} + g (H + h - y)\)
and elimination of \(p/\rho\) gives
\(\frac{\partial \phi}{\partial t} + \frac{1}{2}
\left( u^2 + v^2 \right) + g h = \chi(t) - g H - \frac{p_0}{\rho} =: \tilde{\chi}(t).\) |
(2) |
Finally, if we assume that the fluid is at rest for \( x \to \infty\) (or \( x \to -\infty\)), the following boundary condition holds for the wave surface:
\(\frac{\partial \phi_s}{\partial t} + \frac{1}{2}
\left( u_s^2 + v_s^2 \right) + g h = 0,\) |
(3) |
where the subscript \(s\) indicates that for \(y\) the value \(y = H + h(x, t)\) was taken. A second boundary condition follows from the kinematic equation
\( v_s = \frac{d h}{d t} = \frac{\partial
h}{\partial t} + u_s \frac{\partial h}{\partial x}.\) |
(4) |
By expanding \(\phi_s\) and relations (3) and (4) in powers
of \((H + h)\) up to terms of order \(O(h^2)\), and after elimination of \(\phi_s\), \(u_s\), and \(v_s\), Boussinesq obtains the
following equation for the wave surface that is named after him:
\(\frac{\partial^2 h}{\partial t^2} = g H \frac{\partial^2 h}{\partial x^2} + g H \frac{\partial^2}{\partial x^2} \left( \frac{3 h^2}{2 H} + \frac{H^2}{3} \frac{\partial^2 h}{\partial x^2} \right).\) |
(5) |
This equation already gives a better approximation
than the one given by Lagrange in 1786, namely the wave equation
\(\frac{\partial^2 h}{\partial t^2} = g H \frac{\partial^2 h}{\partial x^2},\)
with general solution \(h(x, t) = h_1(x - \sqrt{g H} t) + h_2(x + \sqrt{g H}t)\).
Boussinesq subsequently restricts his analysis to
waves that propagate in the direction of the positive \(x\)-axis, that is, in the Lagrange approximation, waves of the form
\(h(x, t) = h_1(x - \sqrt{g H} t)\), with wave speed \(\omega_1 = \sqrt{g H}\).
One can obtain a different form of the differential
equation (5) by utilizing the conservation law
\(\frac{\partial h}{\partial t} + \frac{\partial}{\partial x}(\omega h) = \frac{\partial h}{\partial t} + \omega \frac{\partial h}{\partial x} + h \frac{\partial \omega}{\partial x} = 0,\) |
(6) |
where \(\omega\) is the wave speed. Substitution in (5) and integration with
respect to \(x\), while using the condition that \(h\) and all its derivatives with respect to \(x\) go
to zero as \( x \to -\infty\), leads to the equation
\(\frac{\partial}{\partial t}(\omega h) + g H \frac{\partial}{\partial x}
\left(h + \frac{3 h^2}{2 H} + \frac{H^2}{3} \frac{\partial^2 h}{\partial x^2}\right) = 0.\) |
(7) |
Using (6) we can write this expression as
\(\frac{\partial}{\partial t}\left\{h \left(\omega-\sqrt{g H}\right)\right\}-\sqrt{g H}\frac{\partial}{\partial x}\left\{h\left(\omega-\sqrt{g H}\right)\right\}+g H \frac{\partial}{\partial x}\left(\frac{3 h^2}{2 H}+\frac{H^2}{3}\frac{\partial^2 h}{\partial x^2}\right)=0.\)
Without changing the order of the approximation, we may replace \(\partial / \partial t\) with \(-\sqrt{g H} \partial / \partial x\), so that after integration with respect to \(x\), we obtain the following important formula for the wave speed:
\(\omega = \sqrt{g H} +
\sqrt{g H} \left(\frac{3 h}{4 H} + \frac{H^2}{6 h} \frac{\partial^2
h}{\partial x^2} \right).\) |
(8) |
Substituting this value for \(\omega\) into the relation
\(h \frac{d h}{d t} = h \left( \frac{\partial h}{\partial t} + \omega\frac{\partial h}{\partial x}\right)= -h^2\frac{\partial \omega}{\partial x}= -\frac{\partial}{\partial x}(h^2 \omega) + 2 \omega h \frac{\partial h}{\partial x},\)
where \(d h / d t = \partial h / \partial t + \omega \partial h /
\partial x\) is the total differential with respect to \(t\), we obtain an alternative formulation of (7),
namely
\(\frac{d h}{d t} = - \frac{1}{4} \sqrt{\frac{g}{H}} \frac{1}{h} \frac{\partial}{\partial x}\left[h^3\left\{1+\frac{2 H^3}{3h}\left(\frac{\partial}{\partial x} \frac{1}{h} \frac{\partial h}{\partial x}\right)\right\}\right].\)
If we introduce the new variable \(\sigma\) with the definition \(h \; dx = -d \sigma\), this is equivalent to:
\(\frac{d h}{d t} = \frac{1}{4} \sqrt{\frac{g}{H}} \frac{\partial}{\partial \sigma} \left[h^3\left\{1+\frac{2H^3}{3}\frac{\partial}{\partial \sigma}\left(\frac{\partial h}{\partial \sigma}\right)\right\}\right].\) |
(9) |
Boussinesq does not immediately substitute (8) into (6); had he done this, the result would have become
\(\frac{\partial h}{\partial t} + \sqrt{\frac{g}{H}} \frac{3}{2} \frac{\partial}{\partial x}\left(\frac{2}{3}H h + \frac{1}{2} h^2 + \frac{H^3}{9} \frac{\partial^2 h}{\partial x^2} \right) = 0,\) |
(10) |
which is the KdV equation "avant la lettre" and
only differs from the well-known KdV equation because the coordinates \((x, t)\) refer to a fixed frame, while Korteweg and De Vries
used a moving frame. Boussinesq has given another derivation of (10) in a footnote on page 360 of his 680-pages
Mémoire "Essai sur la théorie des eaux courantes" [4]. He does not
use the wave speed \(\omega\) explicitly, but it can
easily be obtained from substitution of (6) in (10); see also R. Pego [17]. Finally, (8)
implies that the wave speed varies pointwise, which means that one
would expect the propagating wave to change form; this was the subject
of the discussion that followed after the discovery of the stationary
wave by Scott Russell.
Korteweg and De Vries
Korteweg and De Vries follow the same theoretical
arguments as Boussinesq and start with the same boundary value
problem. A difference in their treatise is that they take surface
tension into account so that the Bernoulli equation (2), when applied to the wave surface, becomes
\( \frac{\partial \phi_s}{\partial t} + \frac{1}{2}(u_s^2 + v_s^2) + g h - T \frac{\partial^2 h}{\partial x^2} = \tilde{\chi}(t).\)
A second more important difference is that Korteweg
and De Vries differentiate this boundary condition with respect to
\(x\), which removes the dependence on the arbitrary choice of
the function \(\tilde{\chi}\), so that the theory can also be applied to
periodic wave motions that do not vanish for \(x \to \pm \infty\); see the section on the
periodic stationary wave.
A third difference in the derivation of the
differential equation is the wave speed \(\omega\) as a
function of \(h(x ,t)\). A wave that is propagating to the
right can be stopped approximately by letting the fluid move in the
opposite direction, or equivalently, by introducing a moving
coordinate frame that moves to the right, initially with uniform speed
\(\sqrt{g H}\), and more accurately with speed \(\sqrt{g H} - \alpha \sqrt{g / H}\), where \(\alpha\)
is a constant of the same order as \(h(x,t)\) that is to
be determined. In this moving frame
\(\xi = x - \left(\sqrt{g H} - \alpha \sqrt{\frac{g}{H}}\right) t, \quad \tau =
-t\) |
(11) |
the differential equation for the wave surface by Korteweg and De Vries becomes
\(\frac{d h}{d \tau} = \frac{3}{2} \sqrt{\frac{g}{H}} \frac{\partial}{\partial \xi}\left(\frac{h^2}{2} + \frac{2 \alpha h}{3} + \frac{\sigma}{3} \frac{\partial^2 h}{\partial \xi^2}\right).\) |
(12) |
Here, the parameter \(\sigma\) is defined as
\(\sigma = \frac{H^3}{3} - \frac{T H}{\rho g},\)
with \(T\) the surface tension of the wave
surface, which was not taken into account by Boussinesq. Equation (12) is the original KdV equation, as it appeared for
the first time in the PhD thesis of De Vries. For \(T = 0\) this equation is equivalent to (10), from which it
can be derived by applying the coordinate transformation (11).
The long solitary wave
If we assume that a solitary wave exists then the
equivalence of (10) and (12)
implies that both theories lead to the same formulation of the surface
wave in stationary state. For such a wave all points on its surface
must have the same propagation speed so that \(\omega\) must be constant. Using \(\omega = \sqrt{g H} +\) const\(=:
\sqrt{g H} + \frac{1}{2} \sqrt{g / H} , h_1\) in (8), we obtain
\(\frac{\partial^2 h}{\partial x^2} = \frac{3 h (2 h_1 - 3 h)}{2 H^3}.\)
Under the specific assumption that \(h \to 0\) and \(\partial h / \partial x \to 0\) as \(x \to -\infty\) we get
\(\left( \frac{\partial h}{\partial x} \right)^2 = \frac{3 h^2 (h_1 - h)}{H^3},\) |
(13) |
and the positive solution becomes
\(h(x, t) = h_1,\) sech\(^2 \left(\sqrt{\frac{3 h_1}{4 H^3}} (x - \omega t)\right)\) |
(14) |
with
\(\omega = \sqrt{g H} + \frac{h_1}{2} \sqrt{\frac{g}{H}}.\) |
(15) |
Equation (13) implies that the
amplitude of the wave is \(h_1\) and (15)
shows, furthermore, that the wave speed increases with the amplitude
of the wave. This means that, when there are several different
solitary waves of the form (14), higher waves that
start behind smaller ones will overtake them. Since there can be no
change in shape, the solitary waves behave like a row of rolling
marbles, where the faster marbles carry over their impulses to the
slower marbles. This is the reason why Zabusky and Kruskal called such
waves solitons [23]. For an
explicit calculation of this behaviour the interested reader may
consult [8, part II, 3.5].
Equations (14)-(15) were also
derived by Rayleigh, but he attributes the credit to
Boussinesq [18].
Korteweg and De Vries do not have an explicit
expression for the wave speed. However, for a stationary wave in the
moving frame (11) we have \(\partial h / \partial \tau = 0\) so that equation (12) implies
\(\frac{d}{d \xi} \left(\frac{h^2}{2} + \frac{2 \alpha h}{3} + \frac{\sigma}{3} \frac{d^2 h}{d \xi^2} \right) = 0,\) |
(16) |
where the correction \(\alpha\) of the wave
speed \(\sqrt{g H}\) is still unknown. Assuming \(h\),
\(d h / d \xi\), \(d^2 h / d \xi^2 \to 0\) as \(\xi \to -\infty\), integration gives
\(\frac{d h}{d \xi} = \pm \sqrt{- \frac{h^2 (h + 2 \alpha)}{\sigma}}.\)
Korteweg and De Vries distinguish the two cases
\(\sigma > 0\) and \(\sigma < 0\); we only consider the case \(\sigma > 0\) so that we must have \(2 \alpha < 0\). Let us choose \(2 \alpha = -h_2\), where \(h_2\) is the wave amplitude. Then we get
\(h(\xi) = h_2\) sech\(^2 \left(\sqrt{\frac{h_2}{4 \sigma}} \xi \right).\) |
(17) |
If \(T = 0\) then \(\sigma = \frac{1}{3} H^3\) and (17) becomes
\(h(\xi) = h_2\) sech\(^2 \left(\sqrt{\frac{3 h_2}{4 H^3}}\xi \right),\) |
(18) |
which corresponds to equation (14) of Boussinesq. The wave speeds are also the same,
namely, using (11), we have
\(\omega = \sqrt{g H} - \alpha \sqrt{\frac{g}{H}}=\sqrt{g H} + \frac{h_2}{2} \sqrt{\frac{g}{H}}.\)
This approximation of the wave speed, which
improves the formula of Lagrange, was verified experimentially already
in 1844 by Scott Russell. Korteweg and De Vries also consider negative
amplitudes and easily show that such waves exist if \(H < \sqrt{3 T/(\rho g)}\), that is, approximately for water
with \(H < \frac{1}{2}\) cm.
The stationary wave surface satisfies equation (16), but the theory of Korteweg and De Vries does not require \(h\), \(d h / d \xi\), \(d^2 h / d \xi^2 \to 0\) for \(\xi \to +\infty\). Therefore, they do not need this
assumption. Integrating (16) twice leads to
\(c_1 + \frac{h^2}{2} + \frac{2 \alpha h}{3} + \frac{\sigma}{3}\frac{d^2 h}{d \xi^2} = 0\)
and
\(c_2 + 6
c_1 h + h^3 + 2 \alpha h^2 + \sigma \left( \frac{d h}{d \xi} \right)^2
= 0,\) |
(19) |
where \(c_1\) and \(c_2\)
are integration constants. If we assume that the \(y\)-coordinate at the minimum of the wave surface takes the value
\(H\) then the stationary wave surface satisfies \(y = H + h(\xi)\), with \(d h/ d \xi = 0\) and \(d^2 h / d \xi^2 > 0\) for \(h =
0\); see also Figure 3. Hence, \(c_2 = 0\) and if we
further assume \(\sigma > 0\), we also have \(c_1 < 0\).
Figure 3:
Formulation for wave with minimal height \(H\).
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This implies that the equation \(\mu^2 + 2 \alpha \mu + 6 c_1 = 0\) has a
positive root \(\bar{h}\) and a negative root
\(-k\), so that (19) reduces to
\(\frac{d
h}{d \xi} =
\pm \sqrt{\frac{1}{\sigma} h (\bar{h} - h) (h + k)}, \quad \bar{h}
> 0, \quad k > 0.\) |
(20) |
Using the substitution \(h = \bar{h} cos^2 \chi\) we obtain the periodic solution
\(h(\xi) =
\bar{h},\) cn\(^2 \left(\sqrt{\frac{\bar{h} + k}{4 \sigma}} \xi \right),\) |
(21) |
where cn denotes one of the Jacobian elliptic
functions with modulus \(M = \bar{h} / (\bar{h}
+ k)\) and period
\(4 K = 4 \int_0^1 (1 - t^2)^{- \frac{1}{2}}(1 - M^2 t^2)^{- \frac{1}{2}} \; d t.\)
Korteweg and De Vries called such waves cnoidal
waves and the wave surface forms a train of periodic waves with
wave length \(4 K \sqrt{\sigma / (\bar{h} + k)}\). If \(k = 0\) and \(M= 1\) then the
wave length becomes infinite and one obtains the stationary solitary
wave (17); if \(k \to \infty\) and \(M \to 0\) then the result is
approximately the sinusoidal wave
\(h(\xi) = \bar{h} cos^2{\chi}= \bar{h} cos^2{\left(\sqrt{\frac{\bar{h} + k}{4 \sigma}} \xi \right)}\)
where the wave length decreases with increasing
\(k\); this corresponds to the
result of Stokes [14]. Note that in this
case \(h(\xi)\) may be expanded in a
Fourier series; this may be the reason why Stokes at first believed
that the only permanent wave should be of sinusoidal type. Boussinesq
also considered in his Mémoire [4, pp 390-396]
the general case of a periodic stationary wave. However, he is forced
to use a different set of equations, because his assumption that \(h\) vanishes at infinity does not hold for periodic waves; see
also [20]. His result is, in
principle, the same as equation (20) but he does
not provide an explicit solution. It is the merit of Kortweg and De
Vries that they have given a unified treatment of the stationary
solitary wave, valid for waves vanishing at infinity as well as
periodic waves.
The stability of the stationary solitary wave
The goal of the research by Boussinesq and Korteweg
and De Vries was the study of the behavior of long waves on the
surface of a fluid in a shallow basin. In general, wave propagation
involves a change of form, but by definition this does not occur in
the case of a steady wave and so the question arises why the steady
solitary wave is stable and an exception to the rule. For the possible
existence of the steady wave further investigation is required, in
particular with regard to the "parameters" determining the stable
behavior. This has been carried out by Boussinesq and Korteweg and De
Vries in quite different ways. The presence in (7)
and (12) of the non-linear term \(h , d h / d \xi\) and the dispersion term \(\frac{1}{3}\sigma , \partial^3 h / \partial \xi^3\) is already an indication for a possible balance, furthering the stability
of the wave.
Stability in the theory of Korteweg and De Vries
Korteweg and De Vries consider a wave form close to
that of the steady solitary wave
\(h(\xi,
0) = \bar{h},\) sech\(^2(p \xi),\) |
(22) |
where \(\bar{h}\) and \(p\) are as yet arbitrary constants. The deformation of \(h(\xi, \tau)\) is determined by equation (12) and substitution of (22)
leads to an equation for the wave surface \(h(\xi, \tau)\) as a function of \(\xi\) and \(\tau\):
\(\frac{\partial h}{\partial \tau} = -3 \sqrt{\frac{g}{H}} \bar{h}p(4\sigma p^2 - \bar{h})\left\{-\mbox{sech}^2(p \xi)+\frac{2(\alpha + 2\sigma p^2)}{3 (4 \sigma p^2 - \bar{h})}\right\}\mbox{sech}^2(p \xi)\mbox{tanh}(p \xi).\) |
(23) |
If we choose \(\alpha\) and \(p\) such that \(2 (\alpha + 2 \sigma p^2) = 3(4 \sigma p^2 - \bar{h})\), that is
\(\alpha = 4 \sigma p^2 - \frac{3}{2}\bar{h}\), then (23) becomes
\(\frac{\partial h}{\partial \tau} = -3 \sqrt{\frac{g}{H}} p \bar{h} (4 \sigma p^2 -
\bar{h})\mbox{sech}^2(p \xi) \mbox{tanh}^3(p \xi).\) |
(24) |
The choices \(p = \sqrt{\bar{h} / (4 \sigma)}\) and
\(\alpha = - \frac{1}{2} \bar{h}\) ensure that \(\partial h / \partial \tau = 0\) and we get the steady
wave (17).
Further numerical analysis of (24), using Table IX from Traité des fonctions
elliptiques (II) by Legrendre [13], shows that, in its
course, the wave
becomes steeper in front and less steep behind when \(\bar{h} > 4 \sigma p^2\) and, the converse when
\(\bar{h} < 4 \sigma p^2\). This result is in contradiction
with the assertion of Airy, among others, that a progressive wave
always gets steeper in front and less steep behind. This opinion is
conceivable given the fact that the KdV equation, when neglecting the
dispersion term \(\frac{1}{3} \sigma \partial^3 h / \partial \xi^3\), can be
reduced to \(\partial h / \partial \tau + h \partial h / \partial \xi =0\), which implies that particles on the wave surface
move faster to the right as they are higher on the wave's crest. In a
steady wave, the dispersion term \(\frac{1}{3}\sigma \partial^3 h / \partial \xi^3\)
compensates the nonlinear term \(h , \partial h / \partial \xi\).
Stability in the theory of Boussinesq
For studying stability, Boussinesq considers waves
with the same energy satisfying
\(\rho , g E = \frac{1}{2} \rho g \int_{-\infty}^\infty h^2 dx + \frac{\rho}{2} \int_{-\infty}^\infty dx \int_0^{H+h} (u^2 + v^2) \; dy = \rho g \int_{-\infty}^\infty h^2 \; dx.\)
Furthermore, he introduces the functional
\(M = \int_{-\infty}^\infty \left\{\left(\frac{\partial h}{\partial x}\right)^2 - \frac{3 h^3}{H ^3}\right\} dx,\)
which he calls the moment de
stabilité. Straightforward calculation shows that \(M\) is a conserved quantity,
that is, \(d M / dt = 0\) for any wave satisfying (7)
and (8). After the transformation
\(\varepsilon = \int_x^\infty h^2 \; dx,\)
the expression for \(M\) becomes
\(M = \int_0^E \left\{\left( \frac{1}{4} \frac{\partial h^2}{\partial \varepsilon}\right)^2 - \frac{3 h}{H^3}\right\} d \varepsilon.\)
Boussinesq uses the well-known Euler-Lagrange
method, without a reference, to obtain a condition for \(h(\varepsilon, t)\) such that \(M\) attains an extremal value. The result is
\(1 + \frac{2 H^3 h}{3}\frac{\partial}{\partial \varepsilon}\left(h , \frac{\partial h}{\partial \varepsilon}\right) = 0.\)
Using \(d \varepsilon = - h^2 \; d x = h \; d \sigma\) or
\(h \frac{\partial}{\partial \varepsilon} = \frac{\partial}{\partial \sigma}\) one obtains equation (9) with \(d h / d t = 0\). Therefore, only the stationary solitary wave
with given energy \(E\) yields an
extremum for \(M\). Variation of \(h\) with \(\Delta h\) gives
\(\Delta M > 0\) for all \(h(\varepsilon, t)\), so that \(M\) is a minimum
among all waves with given energy, provided the corresponding wave
\(h(\varepsilon, t)\) is stationary. The stability of the wave
is evident, because also \(\Delta M\) does not
depend on \(t\).
We particularly mention this result, because \(M\) inherits several properties from the Hamiltonian that
appears in the formulation of the KdV equation as a Hamiltonian
system. The theory of continuous Hamiltonian systems has been
investigated only recently and the first fundamental results have been
established in the late sixties by P. Lax in 1968 [11], Zacharov in 1969 [24], and L.J.F. Broer in
1974 [5]. We further refer to
P.J. Olver [16] and
E. van Groesen and E.M. de Jager [8, part I, Ch. 1, 2, part II,
Ch. 5], where the theory of infinite-dimensional continuous
dynamical systems is considered in detail.
The KdV equation can be represented as a
Hamiltonian system in the form
\(\frac{\partial h}{\partial t}= -\sqrt{g H}\frac{\partial }{\partial x} , \delta_h ({\mathcal{H}}),\)
where
\({\mathcal{H}}(h) = \int_{-\infty}^\infty \left[ \frac{h^2}{2}+ \varepsilon \left\{-\frac{H^2}{12}\left(\frac{\partial h}{\partial x}\right)^2 + \frac{h^3}{4 H}\right\}\right] dx.\)
Here, \(\delta_h ({\mathcal{H}})\) is the variational derivative of
the Hamiltonian \({\mathcal{H}}\) and \(\varepsilon\) is a scale parameter. The first term of
\({\mathcal{H}}\) is the Hamiltonian for waves in the Lagrange
approximation and the second term is the Boussinesq correction, given
by \(M\), the moment de stabilité. Hamilton's theory for finite discrete systems
dates from about 1835 and it was a century after Boussinesq that this
theory has been generalized for continuous systems. By using
functionals, Boussinesq has set a first step into the direction of
this generalization.
Other interesting topics
We only discussed the most important aspects of the
work of Boussinesq and Korteweg and De Vries. The authors further
consider in detail the velocity field in the fluid, the paths of the
fluid particles, the motion of the centre of gravity of a solitary
wave, and a number of characteristic quantities such as the potential
and kinetic energy of a wave. Boussinesq ends his article in [3] with a qualitative study of
the change
of form of long non-stationary waves. Obviously, the wave speed \(\omega\) (8) is important here. The signs
of \(h\) and \(h_{xx}\) determine the relative speed of a particle on the wave surface with respect to
the base speed \(\sqrt{g h}\). Boussinesq gives heuristic arguments for the
possibility that a positive solitary wave splits into several other
positive solitary waves, and that negative solitary waves cannot occur
(NB \(T = 0\)).
Korteweg and De Vries wanted to show that their
approximation of the surface of a steady wave may be improved
indefinitely, resulting in a convergent series. Their starting point
is the first approximation given in (21) and the
equalities
\(\left( \frac{d h}{d \xi}\right)^2 = a h (\bar{h} - h) (h + k)(1 + b h + c h^2 + \cdots)\)
and
\(f(\xi) = q + r h + s h^2 + \cdots,\)
where \(f\) is defined in (1); see also equation (20). The
coefficients \(a\), \(b\), \(c, \dots\) and \(q\), \(r\), \(s, \dots\) are determined by the boundary conditions that are
imposed on the wave surface. Namely,
\(v_s(h) = u_s(h) \frac{d h}{d \xi}\)
and
\(u_s(h)^2 + v_s(h)^2 + 2 g h =\) constant.
The result is a series expansion with general term
\(O(\bar{h}^m)\). While the calculations are elementary, they
are so complicated and tedious that one does not expect them to have
received much attention. Even the second approximation following (21) already requires so much effort that it is
commendable to content with the first approximation (21) only.
Concluding remarks
It is somewhat surprising that Korteweg and De
Vries only cite Boussinesq's short communication in the Comptes
Rendus of 1871 [1] and not the
extensive papers in the J. Math. Pures et Appl. [3] and the Mémoire [4] that appeared in 1872 and 1877,
respectively.
B. Willink (Erasmus University Rotterdam) provided
this author with a copy of an abstract written by De Vries of a paper
by Saint Venant [20] from
1885. This copy shows that De Vries was certainly aware of the
"Essai sur la théorie des eaux courantes." Hence, one
may ask why Korteweg and De Vries revisited the research by Boussinesq
only in 1894. The answer is clarified in the introduction of their
paper in the Philosophical Magazine [12]. They write that Lamb and Basset still
believe that propagating waves must change shape, steeper at the front
and less steep behind. Furthermore, the research of Boussinesq, Lord
Rayleigh, and Saint Venant appear to corroborate this assumption, even
though it is difficult to see why the solitary wave would be an
exception. Therefore, they decided to re-examine this research. Maybe
it was not customary in the nineteenth century, as it is now, to cite
all relevant publications by other authors; moreover, communications
cannot have been so easy as they are nowadays. Finally, there is a
principle difference between the research on stationary waves by
Boussinesq and by Korteweg and De Vries: namely, Boussinesq takes the
conservation law (6) and the wave speed \(\omega\) (8) as the starting point of his
theory, while Korteweg and De Vries consider the famous KdV equation
as "This very important equation, to which we shall have
frequently to revert in the course of this paper." The
presentation of the two treatises differ enormously: Boussinesq is
rather elaborate, while Korteweg and De Vries remain direct and to the
point.
The honor of the discovery of the mathematical
formulation of the stationary solitary wave and, thus, the KdV
equation undoubtedly should go to Boussinesq. However, Korteweg and De
Vries did add several new aspects to the theory and were instrumental
in removing all doubt with respect to the existence of a stationary
solitary wave.
The author is indebted to the grandsons of Gustav de
Vries for presenting him with a copy of the doctoral thesis of their
grandfather and for the records of the handwritten correspondence
between Korteweg and De Vries. The author likes to thank
dr. B. Willink (Erasmus University, the Netherlands) for discussions
on who first discovered the KdV equation and for copies of some of the
work of Boussinesq and Saint Venant. He also thanks dr. F. van Beckum
(University of Twente, the Netherlands) for a program to illustrate
the interaction of solitons and for his help in the preparation of
this article. He is very much indebted to dr. H. Osinga of the
University of Bristol, who took great care to translate the original
Dutch text into English and to publish this historical essay in DSWeb
Magazine.
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About the author
The author was born in 1927 and started his
mathematical career at the University of Groningen in the Netherlands. In 1953,
after his masters degree in mathematics and physics, he joined the
National Aerospace
Laboratory (NLR) in Amsterdam, an excellent environment to
acquire experience in solving initial boundary value problems in
models for the flow around wings. To broaden his horizon he accepted
in 1960 a position at the Mathematical Centre (CWI) in Amsterdam where he
worked in different areas: theory of generalized functions, singular
perturbations and applications of mathematics. Shortly after his
Ph.D. in 1964 he was appointed as full professor at the University of Twente
and he changed this position four years later for a chair at
the University of
Amsterdam where he served until his retirement in 1992. In between
he was a guest professor at the University of Cologne in 1976 and 1992. He enjoys a
happy family life with his wife and two sons. In his younger years he
was an enthousiastic sailor and nowadays he finds his pleasure in
drawing and painting.
Selected publications
1. |
Oscillating Rectangular Wings in
Supersonic Flow with Arbitrary Bending and Torsion Mode
Shapes. Transactions NLR, Amsterdam, XXVI
(1959). |
2. |
Applications of Distributions in
Mathematical Physics. Mathematical Centre Tracts
10, Amsterdam, pp 1-182 (1964), Sec. Ed. (1969). |
3. |
Lorentz Invariant Solutions of the
Klein-Gordon Equation. SIAM J. Appl. Math.
15, no 1 (1967). |
4. |
with W.Eckhaus, Asymptotic Solutions
of Singular Perturbation Problems for Linear Differential Equations of
Elliptic Type. Arch. Rat. Mech. and Anal. 23,
no 1 (1966). |
5. |
with Jiang Furu, The Theory
of Singular Perturbations. Series in Appl. of Math. and Mech.
42, North-Holland Publ. Cy, Amsterdam, pp 1-340
(1996). |
6. |
with E.van Groesen, Mathematical
Structures in Continuous Dynamical Systems. Studies in
Math. Phys. 6, North-Holland Publ. Cy, Amsterdam, pp 1-617 (1994). |
7. |
with S.Spannenburg and M.H.Sitters,
Baecklund Transformations of Solutions of Nonlinear Evolution
Equations and the Lie-Bianchi Transformation. Physica A
228 (1996). |