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3 which corresponds to the infinitesimal transformation 15.8.1.2, is called an infinitesimal operator.* THEOREMLIE.. In this book, we call an operator 15.8.1.3 an infinitesimal operator

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Remark In the special case of transformations in the plane, the functions ϕ1 and ϕ2 in (15.8.1.1) are

independent of w, and ψ = w (i.e., w¯= w).

The expansion of (15.8.1.1) into truncated Taylor series in ε about ε = 0 to linear terms gives

¯x  x + εξ(x, y, w), ¯y  y + εη(x, y, w), w ¯  w + εζ(x, y, w), (15 8 1 2 ) where

ξ (x, y, w) = ∂ϕ1

∂ε





ε=0, η (x, y, w) =

∂ϕ2

∂ε





ε=0, ζ (x, y, w) =

∂ψ

∂ε





ε=0.

The linear first-order differential operator

X = ξ(x, y, w) ∂

∂x + η(x, y, w) ∂

∂y + ζ(x, y, w) ∂

∂w , (15 8 1 3 )

which corresponds to the infinitesimal transformation (15.8.1.2), is called an infinitesimal

operator.*

THEOREM(LIE) Suppose the coordinates ξ(x, y, w), η(x, y, w), ζ(x, y, z) of the

in-finitesimal operator (15.8.1.3) are known Then the transformation (15.8.1.1), having the group property, can be completely recovered by solving the Lie equations

1

dε = ξ(ϕ1, ϕ2, ψ), dϕ2

dε = η(ϕ1, ϕ2, ψ), dψ

dε = ζ(ϕ1, ϕ2, ψ)

with the initial conditions

ϕ1|ε=0= x, ϕ2|ε=0= y, ψ |ε=0= w.

15.8.1-2 Invariant of an infinitesimal operator Transformations in the plane.

An invariant of the operator (15.8.1.3) is a function I(x, y, w) that satisfies the condition

I ( ¯x, ¯y, ¯ w ) = I(x, y, w).

Let us expand this equation in Taylor series in the small parameter ε, divide the resulting relation by ε, and the proceed to the limit as ε → 0 to obtain a linear partial differential

equation for I:

XI = ξ(x, y, w) ∂I

∂x + η(x, y, w) ∂I

∂y + ζ(x, y, w) ∂I

∂w = 0 (15 8 1 4 ) Let the associated characteristic system of ordinary differential equations (see Paragraph 13.1.1-3)

dx

ξ (x, y, w) =

dy

η (x, y, w) =

dw

ζ (x, y, w) (15. 8 1 5 )

* In the literature, it is also known as an infinitesimal generator or a group generator In this book, we call

an operator (15.8.1.3) an infinitesimal operator, a group generator, or, for short, an operator.

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TABLE 15.7 One-parameter transformations in the plane

Name Transformation Transformation Invariant

Translation in the x-axis ¯x = x + ε, ¯y = y X = ∂x ∂ I1= y

Translation along the straight line

ax + by =0 ¯x = x + bε, ¯y = y – aε X = b ∂x ∂ – a ∂y ∂ I1= ax + by

Rotation ¯x = x cos ε + y sin ε,

¯y = y cos ε – x sin ε X = y ∂x ∂ – x ∂y ∂ I1= x2+ y2

Galileo transformation ¯x = x + εy, ¯y = y X = y ∂x ∂ I1= y

Lorentz transformation ¯x = x cosh ε + y sinh ε,

¯y = y cosh ε + x sinh ε X = y ∂x ∂ + x ∂y ∂ I1= y2– x2

Uniform extension ¯x = xe ε, ¯y = ye ε X = x ∂x ∂ + y ∂y ∂ I1= y/x

Nonuniform extension ¯x = xe aε, ¯y = ye bε X = ax ∂x ∂ + by ∂y ∂ I1 =|y|a|x|–b

have the functionally independent integrals

I1(x, y, w) = C1, I2(x, y, w) = C2, (15. 8 1 6 )

where C1and C2are arbitrary constants Then the general solution of equation (15.8.1.4) has the from

I = Ψ(I1, I2), (15. 8 1 7 ) where Ψ(I1, I2) is an arbitrary function of two arguments, I1= I1(x, y, w) and I2= I2(x, y, w).

This means that the operator (15.8.1.3) has two functionally independent invariants,

I1and I2, and any function Φ(x, y, w) invariant under the operator (15.8.1.3) can be

repre-sented as a function of the two invariants.

Table 15.7 lists the most common transformations in the plane and the corresponding operator (15.8.1.3) and invariants; only one invariant is specified, with the other being the

same: I2= w.

15.8.1-3 Formulas for derivatives Coordinates of the first and second prolongations.

In the new variables (15.8.1.1), the first derivatives become

∂ w ¯

∂ ¯x 

∂w

∂x + εζ1, ∂ w ¯

∂ ¯y 

∂w

∂y + εζ2 (15 8 1 8 )

Here, ζ1and ζ2are the coordinates of the first prolongation, which are found as

ζ1= Dx(ζ) – wxDx(ξ) – wyDx(η) = ζx+ (ζw– ξx)wx– ηxwy– ξww2x– ηwwxwy,

ζ2= Dy(ζ) – wxDy(ξ) – wyDy(η) = ζy– ξywx+ (ζw– ηy)wy – ξwwxwy– ηww2y,

(15 8 1 9 )

where Dxand Dyare the total differential operators with respect to x and y:

Dx= ∂x ∂ + wx∂w ∂ + wxx∂w ∂

x + wxy

∂wy + · · · ,

Dy = ∂y ∂ + wy∂w ∂ + wxy∂w ∂

y + wyy

∂wy + · · ·

(15 8 1 10 )

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Let us verify that the first formula in (15.8.1.8) holds Obviously,

¯

w x=w¯x¯¯x x+w¯y¯¯y x, w¯y=w¯x¯¯x y+w¯y¯¯y y (15.8.1.11)

Differentiating (15.8.1.2) with respect to x and y and retaining terms to the first order of ε, we have

¯x x=1+ εD x , ¯x y = εD y ,

¯y x = εD x η, ¯y y=1+ εD y η,

¯

w x = w x + εD x , w¯y = w y + εD y

(15.8.1.12)

In order to calculatew¯x¯, let us eliminatew¯¯yfrom (15.8.1.11) and then substitute the derivatives ¯x x, ¯x y, ¯y x,

¯y y,w¯x,w¯yfor their respective expression from (15.8.1.12) to obtain

¯

w¯x= w x + ε(D x + w x D y η – w y D x η ) + ε

2(D x ζD y η – D x ηD y )

1+ ε(D x + D y η ) + ε2(D x ξD y η – D x ηD y ) .

Expanding into a series in ε, we have

¯

w x¯ w x + εζ1, ζ1= D x – w x D x – w y D x η,

which was to be proved The coordinate ζ2is calculated likewise

The second derivatives in the new variables (15.8.1.1) are calculated as

2w ¯

∂ ¯x2  ∂2w

∂x2 + εζ11,

2w ¯

∂ ¯x∂¯y 

2w

∂x∂y + εζ12, 2w ¯

∂ ¯y2  ∂2w

∂y2 + εζ22. (15. 8 1 13 )

Here, the ζij are the coordinates of the second prolongation and are found as

ζ11= Dx1) – wxxDx(ξ) – wxyDx(η),

ζ12= Dy1) – wxxDy(ξ) – wxyDy(η),

ζ22= Dy2) – wxyDy(ξ) – wyyDy(η),

or, in detailed form,

ζ11 = ζxx+ ( 2ζwx– ξxx)wx– ηxxwy+ (ζww– 2ξwx)w2x– 2ηwxwxwy

– ξwww3

x– ηwww2

xwy + (ζw– 2ξx– 3ξwwx– ηwwy)wxx– 2 x+ ηwwx)wxy,

ζ12 = ζxy+ (ζwy– ξxy)wx+ (ζwx– ηxy)wy– ξwyw2

x

– (ζww– ξwx– ηwy)wxwy– ηwxw2

y– ξwww2

xwy– ηwwwxw2

y

– (ξy+ ξwwy)wxx+ (ζw– ξx– ηy– 2ξwwx– 2ηwwy)wxy– (ηx+ ηwwx)wyy,

ζ22 = ζyy– ξyywx+ ( 2ζwy– ηyy)wy– 2ξwywxwy+ (ζww– 2ηwy)w2y

– ξwwwxw2y– ηwww3y– 2 y+ ξwwy)wxy + (ζw– 2ηy– ξwwx– 3ηwwy)wyy.

(15 8 1 14 ) The above formulas for the coordinates of the first and second prolongation, (15.8.1.9) and (15.8.1.14), will be required later for the analysis of differential equations.

15.8.2 Symmetries of Nonlinear Second-Order Equations.

Invariance Condition

15.8.2-1 Invariance condition Splitting in derivatives.

We will consider second-order partial differential equations in two independent variables

F



x , y, w, ∂w

∂x , ∂w

∂y ,

2w

∂x2,

2w

∂x∂y ,

2w

∂y2



= 0 (15 8 2 1 )

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The procedure for finding symmetries* of equation (15.8.2.1) consists of several stages.

At the first stage, one requires that equation (15.8.2.1) must be invariant (preserve its form) under transformations (15.8.1.1), so that

F



¯x, ¯y, ¯ w , ∂ w ¯

∂ ¯x ,

∂ w ¯

∂ ¯y ,

2w ¯

∂ ¯x2,

2w ¯

∂ ¯x∂¯y ,

2w ¯

∂ ¯y2



= 0 (15 8 2 2 )

Let us expand this equation into a series in ε about ε = 0 , taking into account that the leading term vanishes, according to (15.8.2.1) Using formulas (15.8.1.2), (15.8.1.8), (15.8.1.13)

and retaining the terms to the first-order of ε, we obtain

X

2F



x , y, w, ∂w

∂x , ∂w

∂y ,

2w

∂x2,

2w

∂x∂y ,

2w

∂y2

 



F =0 = 0 , (15 8 2 3 ) where

X

2F = ξ ∂F

∂x +η ∂F

∂y +ζ ∂F

∂w +ζ1 ∂F

∂wx2

∂F

∂wy 11

∂F

∂wxx12

∂F

∂wxy22

∂F

∂wyy (15. 8 2 4 )

The coordinates of the first, ζi, and the second, ζij, prolongation are defined by formulas

(15.8.1.9) and (15.8.1.14) Relation (15.8.2.3) is called the invariance condition, and the

operator X

2 is called the second prolongation of the operator (15.8.1.3).

At the second stage, either the derivative ∂ ∂y2w2 or ∂ ∂x2w2 is eliminated from (15.8.2.3) using equation (15.8.2.1) The resulting relation is then written as a polynomial in the “inde-pendent variables,” the various combinations of the products of the derivatives (involving

various powers of wx, wy, wxx, and wxy):



Ak1 k2k3k4(wx)k1(wy)k2(wxx)k3(wxy)k4 = 0 , (15 8 2 5 )

where the functional coefficients Ak1 k2 k3k4 are dependent on x, y, w, ξ, η, ζ and the deriva-tives of ξ, η, ζ only and are independent of the derivaderiva-tives of w Equation (15.8.2.5) is satisfied if all Ak1k2k3 k4 are zero Thus, the invariance condition is split to an overdeter-mined determining system, resulting from equating all functional coefficients of the various

products of the remaining derivatives to zero (recall that the unknowns ξ, η, and ζ are independent of wx, wy, wxx, and wxy).

At the third stage, one solves the determining system and finds admissible coordinates

ξ , η, and ζ of the infinitesimal operator (15.8.1.3).

Remark 1 It should be noted that the functional coefficients A k1k2k3k4and the determining system are

linear in the unknowns ξ, η, and ζ.

Remark 2 An invariant I that is a solution of equation (15.8.1.4) is also a solution of the equation X

2I=0

The procedure for finding symmetries of differential equations is illustrated below by specific examples.

15.8.2-2 Examples of finding symmetries of nonlinear equations.

Example 1 Consider the two-dimensional stationary heat equation with a nonlinear source

2w

∂x2 +

2w

The corresponding left-hand side of equation (15.8.2.1) is F = w xx + w yy – f (w).

* A symmetry of an equation is a transformation that preserves its form

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Infinitesimal operators X admitted by the equations are sought in the form (15.8.1.4), where the coordinates

ξ = ξ(x, y, w), η = η(x, y, w), ζ = ζ(x, y, w) are yet unknown and are to be determined in the subsequent analysis.

In view of identity F = w xx + w yy – f (w), the invariance condition (15.8.2.3)–(15.8.2.4) is written as

ζ22+ ζ11 – ζf  (w) =0 Substituting here the expressions of the coordinates of the second prolongation (15.8.1.14) and then replacing

w yy by f (w) – w xx, which follows from equation (15.8.2.6), we obtain

–2ξ w w x w xx+2η w w y w xx–2η w w x w xy–2ξ w w y w xy–2(ξ x – η y )w xx–2(ξ y + η x )w xy

– ξ ww w3x – η ww w x2w y – ξ ww w x w y2– η ww w3y + (ζ ww–2ξ xw )w x2–2(ξ yw + η xw )w x w y+

+ (ζ ww–2η yw )w2y+ (2ζ xw – ξ xx – ξ yy – f ξ w )w x+ (2ζ yw – η xx – η yy–3f η w )w y+

+ ζ xx + ζ yy + f (ζ w–2η y ) – ζf =0,

where f = f (w) and f  = df /dw Equating the coefficients of all combinations of the derivatives to zero, we

have the system

w x w xx: ξ w=0,

w y w xx: η w=0,

w xx: ξ – η y=0,

w xy: ξ + η x=0,

w x2: ζ ww–2ξ wx=0,

w x w y: η wx + ξ wy=0,

w x: 2ζ wx – ξ xx – ξ yy – ξ w f (w) =0,

w2y: ζ ww–2η wy=0,

w y: 2ζ wy – η xx – η yy–3η w f (w) =0,

1: ζ xx + ζ yy – f  (w)ζ + f (w)(ζ w–2η y) =0

(15.8.2.7)

Here, the left column indicates a combination of the derivatives and the right column gives the associated

coefficient The coefficients of w y w xy , w x w xy , w3x , w x2w y , w x w2y , w3yeither are among those already listed

or are their differential consequences, and therefore they are omitted It follows from the first, second, and fifth equations and their consequences that

ξ = ξ(x, y), η = η(x, y), ζ = a(x, y)w + b(x, y). (15.8.2.8) The third and fourth equations of system (15.8.2.7) give

ξ xx + ξ yy=0, η xx + η yy=0 (15.8.2.9) Substituting (15.8.2.8) into the seventh and ninth equations of (15.8.2.7) and using (15.8.2.9), we find that

a x = a y=0, whence

In view of (15.8.2.8) and (15.8.2.10), system (15.8.2.7) becomes

ξ – η y=0,

ξ + η x=0,

b xx + b yy – awf  (w) – bf  (w) + f (w)(a –2η y) =0

(15.8.2.11)

For arbitrary f , it follows that a = b = η y=0, and then ξ = C1 y + C2, η = –C1 x + C3, and ζ =0 By setting one

of the constants to unity and the others to zero, we establish that the original equation admits three different operators:

X1= ∂ x (C2=1, C1= C3=0);

X2= ∂ y (C3=1, C1= C2=0);

X3= y∂ x – x∂ y (C1=1, C2 = C3=0)

(15.8.2.12)

The first two operators define a translation along the x- and y-axis The third operator represents a rotational

symmetry

Let us dwell on the third equation of system (15.8.2.11) If the relation

(aw + b)f  (w) – f (w)(a –2η y) =0 (15.8.2.13)

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holds, there may exist other solutions of system (15.8.2.11) that will result in operators other than (15.8.2.12).

Let us study two cases: a≠ 0and a =0

Case 1 If a≠ 0, the solution of equation (15.8.2.13) gives

f (w) = C(aw + b)1 2a γ,

where γ = η y = const and b = const Therefore, for f (w) = w k, equation (15.8.2.6) admits another operator,

X4= x∂ x + y∂ y+ 2

1– k w∂ w,

that defines a nonuniform extension

Case 2 If a =0, we have

f (w) = Ce λw,

where λ = const Then b = –2η y /λ , and the functions ξ and η satisfy the first two equations (15.8.2.11), which

coincide with the Cauchy–Riemann conditions for analytic functions The real and the imaginary part of any analytic function,Φ(z) = ξ(x, y) + iη(x, y), of the complex variable z = x + iy satisfies the Cauchy–Riemann conditions In particular, if b = const and f (w) = e w, the equation admits another operator,

X4= x∂ x + y∂ y–2∂ w,

which corresponds to extension in x and y with simultaneous translation in w.

Example 2 Consider the nonlinear nonstationary heat equation

∂w

∂t =

∂x

*

f (w) ∂w

∂x

+

In the invariance condition (15.8.2.3)–(15.8.2.4), one should set

y = t, F = w t – f (w)w xx – f  (w)w x2, ζ12= ζ22=0

The coordinates of the first and second prolongations, ζ1, ζ2, and ζ11, are expressed by (15.8.1.9) and (15.8.1.14)

with y = t In the resulting equation, one should replace w twith the right-hand side of equation (15.8.2.14) and equate the coefficients of the various combinations of the remaining derivatives to zero, thus arriving at the system of equations

w x w xx: 2f (w)[η wx f (w) + ξ w ] + f  (w)η x=0,

w xx: ζf  (w) – f2(w)η xx – f (w)(2ξ – η t) =0,

w x w xt: f (w)η w=0,

w xt: f (w)η x=0,

w4x: f  (w)η w + f (w)η ww=0,

w3x: 2[f  (w)]2η x + f (w)ξ ww + f  (w)ξ w+2f (w)f  (w)η wx=0,

w2x: f (w)ζ ww + f  (w)ζ –2f (w)ξ wx – f  (w)(2ξ – η t ) + f  (w)ζ w – f (w)f  (w)η ww=0,

w x: 2f (w)ζ wx+2f  (w)ζ x – f (w)ξ xx + ξ t=0,

1: ζ t – f (w)ζ xx=0

Here, the left column indicates a combination of the derivatives, and the right column gives the associated

equation (to a constant factor); identities and differential consequences are omitted Since f (w)0, it follows

from the third and fourth equations of the system that η = η(t) Then from the first and second equations, we

have

ξ = ξ(x, t), ζ= f (w)(2ξ – η t)

f  (w) .

With these relations, the remaining equations of the system become

[f f  f  – f (f )2+ (f )2f ](2ξ – η t) =0,

f[4f f –7(f )2]ξ xx – (f )2ξ t=0,

2f ξ xxx–2ξ xt + η tt=0;

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the equations have been canceled by nonzero factors In the general case, for arbitrary function f , from the

first equation it follows that2ξ – η t=0and from the second it follows that ξ t=0 The third equation gives

ξ = C1 + C2 x , and then η =2C2t + C3 Therefore, for arbitrary f , equation (15.8.2.14) admits three operators

X1= ∂ x (C1=1, C2 = C3=0);

X2= ∂ t (C3=1, C1= C2=0);

X3=2t∂ t + x∂ x (C2=1, C1 = C3=0)

Similarly, it can be shown that the following special forms of f result in additional operators:

1 f = e w: X4= x∂ x+2∂ w;

2 f = w k , k≠ 0, –4/3: X4= kx∂ x+2w∂ w;

3 f = w–4/3: X4=2x∂ x–3w∂ w, X5 = x2∂ x–3xw∂ w

Example 3 Consider now the nonlinear wave equation

2w

∂t2 =

∂x

*

f (w) ∂w

∂x

+

In the invariance condition (15.8.2.3)–(15.8.2.4), one should set

y = t, F = w tt – f (w)w xx – f  (w)w2x, ζ2= ζ12=0,

and use the coordinates of the first and second prolongations, ζ1 , ζ11, and ζ22, expressed by (15.8.1.9) and (15.8.1.14) with y = t In the resulting equation, one should replace w ttwith the right-hand side of equation (15.8.2.15) and equate the coefficients of the various combinations of the remaining derivatives to zero, thus arriving at the system of equations

w x w xx: f (w)ξ w=0,

w t w xx: f (w)η w=0,

w xx: f  (w)ζ +2f (w)(η t – ξ x) =0,

w xt: f (w)η x – ξ t=0,

w3x: f  (w)ξ w + f (w)ξ ww =0,

w2x w t: f (w)η ww – f  (w)η w=0,

w2x: f (w)ζ ww + f  (w)ζ w + f  (w)ζ –2f (w)ξ wx–2f  (w)(ξ x – η t) =0,

w x w t: 2f  (w)η x+2f (w)η wx–2ξ wt =0,

w x: 2f  (w)ζ x – f (w)ξ xx+2f (w)ζ wx + ξ tt=0,

w t2: ζ ww–2η wt =0,

w t: f (w)η xx+2ζ wt – η tt=0,

1: ζ tt – f (w)ζ xx=0

Identities and differential consequences have been omitted Since f (w)≠const, it follows from the first two

equations that ξ = ξ(x, t) and η = η(x, t) The tenth equation of the system becomes ζ ww=0, thus giving

ζ = a(x, t)w + b(x, t) As a result, the system becomes

wf  (w)a(x, y) + f  (w)b(x, y) +2f (w)(η t – ξ x) =0,

f  (w)a(x, y) + wf  (w)a(x, y) + f  (w)b(x, y) –2f  (w)(ξ x – η t) =0,

2f  (w)(a x w + b x ) – f (w)ξ xx+2f (w)a x=0,

2a t – η tt=0,

a tt w + b tt – f (w)(a xx w + b xx) =0

For arbitrary function f (w), we have a = b =0, ξ xx=0, η tt=0, and ξ x – η t =0 Integrating yields three operators:

X1= ∂ x, X2= ∂ t, X3= x∂ x + t∂ t

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