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8/4/2019 AsianOptions-ArithmeticAverage
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1
The Arithmetic Average Case
of Asian Options:Reducing the PDE to theBlack-Scholes Equation
Solomon M. Antoniou
SKEMSYS
S cientific Knowledge Engineering
and Management Systems
37 oliatsou Street, Corinthos 20100, [email protected]
Abstract
We consider the path-dependent contingent claims where the underlying assetfollows an arithmetic average process. Considering the no-arbitrage PDE of these
claims, we first determine the underlying Lie Point Symmetries. After
determination of the invariants, we transform the PDE to the Black-Scholes (BS)
equation. We then transform the BS equation into the heat equation and we
provide some general solutions to that equation. This procedure appears for the
first time in the finance literature.
Keywords: Path-Dependent Options, Asian Options, Arithmetic Average Path-
Dependent Contingent Claims, Lie Symmetries, Exact Solutions.
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1. Introduction
A path-dependent option is an option whose payoff depends on the past history of
the underlying asset. In other words these options have payoffs that do not depend
on the assets value at expiry. Two very common examples of path-dependent
options areAsian options and lookback options.
The terminal payoff of an Asian option depends on the type of averaging of the
underlying asset price over the whole period of the options lifetime. According to
the way of taking average, we distinguish two classes of Asian options: arithmetic
andgeometric options.
A lookback option is another type of path-dependent option, whose payoff
depends on the maximum or minimum of the asset price during the lifetime of the
option.
The valuation of path-dependent (Asian) European options is a difficult problem
in mathematical finance. There are only some simple cases where the price of
path-dependent contingent claims can be obtained in closed-form (refs. [1]-[8]).
If the underlying asset price follows a lognormal stochastic process, then its
geometric average has a lognormal probability density and in this case there is a
closed-form solution (ref. [5]). This is not however the case by considering
arithmetic average. In this case there is no closed-form solution. However in both
cases there are some numerical procedures available (ref. [8]).
It is the purpose of this article to provide a closed-form general solution for the
arithmetic path-dependent options.
The paper is organized as follows: In Section 2 we consider the general problem of
pricing the path-dependent contingent claims. In Section 3 we consider the Lie
Point Symmetries of the Partial Differential Equation (equation (3.1)) for the path-
dependent arithmetic average options. Full details of the calculation are provided
in Appendix A. In Section 4, considering two invariants of the PDE, we convert
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the equation into the Black-Scholes equation. In section 5, we transform the BS
equation to the heat equation. We then find the general solution of our PDE
(Theorem 3). In section 6 we provide some solutions to the heat equation.
Because of the complexity of the calculations, we have included a great deal ofcalculation details, supplemented by many Appendices.
2. Path-Dependent Contingent Claims
Suppose that an option pays off at expiration time T an amount that is a function
of the path taken by the asset between time zero and T. This path-dependent
quantity can be represented by an integral of some function of the asset over the
time period 0 :
=T
0
d),S(f)( (2.1)
where )t,S(f is a suitable function. Therefore, for every t, t0 , we have
=t
0
d),S(f)t( (2.2)
or, in differential form,
dt)t,S(fdA = (2.3)
We have thus introduced a new state variable A, which will later appear in our
PDE.
We are now going to derive the PDE of pricing of the path-dependent option. To
value the contract, we consider the function )t,A,S(V and set up a portfolio
containing one of the path-dependent options and a number of the underlying
asset:
S)t,A,S(V = (2.4)
The change in the value of this portfolio is given by, according to Its formula, by
dSS
VdA
A
Vdt
S
VS
2
1
t
Vd
2
222
+
+
+
= (2.5)
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Choosing
S
V
= (2.6)
to hedge the risk and using (2.3), we find that
dtA
V)t,S(f
S
VS
2
1
t
Vd
2
222
+
+
= (2.7)
This change is risk-free and thus earns the risk-free rate of interest r,
dtrd = (2.8)
leading to the pricing equation
0VrSVSr
AV)t,S(f
SVS
21
tV 2
2
22 =+++(2.9)
combining (2.7), (2.8) and (2.4), where in (2.4) has been substituted by (2.6)
for the value of .
The previous PDE is solved by imposing the condition
)A,S()T,A,S(V = (2.10)
where T is the expiration time.
If A is considered to be an arithmetic average state variable,
=t
0
d)(S (2.11)
then PDE (2.9) becomes
0VrS
VSr
A
VS
S
VS
2
1
t
V
2
222 =
+
+
+
(2.12)
If A is considered to be a geometric average state variable,
=t
0
d)(Sln (2.13)
then PDE (2.9) becomes
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0VrS
VSr
A
V)S(ln
S
VS
2
1
t
V
2
222 =
+
+
+
(2.14)
We list below the payoff types we have to consider along with PDEs (2.12) and
(2.14).
For average strike call, we have the payoff )A,S(
)0,AS(max (2.15)
For average strike put, we have the payoff
)0,SA(max (2.16)
For average rate call, we have the payoff
)0,EA(max
(2.17)
For average rate put, we have the payoff
)0,AE(max (2.18)
where E is the strike price.
This is an introduction to the path-dependent options. Details can be found in
Wilmotts 3-volume set on Quantitative Finance (ref. [3]).
3. Lie Symmetries of the Partial Differential Equation
The technique of Lie Symmetries was introduced by S. Lie [11]-[12] and is best
described in refs [13]-[28]. This technique was for the first time used in partial
differential equations of Finance by Ibragimov and Gazizov [29]. The same
technique was also used by the author in solving the Bensoussan-Crouhy-Galai
equation [30] and the HJB equation for a portfolio selection problem [31]. There is
however a growing lists of papers in applying this method to Finance. For a non
complete set of references, see [29]-[40].
We consider the PDE (2.12)
0VrA
VS
S
VSr
S
VS
2
1
t
V
2
222 =
+
+
+
(3.1)
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We shall determine the Lie Point Symmetries of the previous equation.
We follow closely Olver (ref. [15]).
Let )V,t,A,S( )2( be defined by
VrA
VS
S
VSr
S
VS
2
1
t
V)V,t,A,S(
2
222)2(
+
+
+
= (3.2)
We introduce the vector field X (the generator of the symmetries) by
+
+
=A
)V,t,A,S(S
)V,t,A,S(X 21
V)V,t,A,S(
t)V,t,A,S(3
+
+ (3.3)
We calculate in Appendix A the coefficients 321 ,, and and we find that
the Lie algebra of the infinitesimal transformations of the original equation (3.1)
is spanned by the five vectors
tX1
= (3.4)
A
X2
= (3.5)
AA
SSX3
+
= (3.6)
VV)ArS(
2
AA
SAS2X
2
24
+
+
= (3.7)
V
VX5
= (3.8)
and the infinite dimensional sub-algebra
V)t,A,S(X
= (3.9)
where )t,A,S( is an arbitrary solution of the original PDE (3.1).
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4. Reduction of the equation to the BS equation
We shall now try to transform the pricing differential equation into another by
reducing the number of independent variables. We shall retain the time variable
and try to find a combination of the other two variables S and A. The best
candidate for this job is the generator 4X given by (3.7).
We state and prove the following Theorem:
Theorem 1. Any solution of the partial differential equation
0VrA
VS
S
VSr
S
VS
2
1
t
V
2
222 =
+
+
+
can be expressed into the form
=
A
Sbexp)t,x(uA)t,A,S(V n (4.1)
where the function )t,x(u satisfies the Black-Scholes equation
0uruxrux2
1u xxx
22t =++ (4.2)
with2A
Sx = , brn = and
2
2b = .
Proof. Considering the generator 4X , we can determine two invariants of the
PDE. For this purpose we have to solve the following system
V)ArS(
dV
2
A
dA
AS2
dS 2
2 == (4.3)
The differential equation2
A
dA
AS2
dS= is equivalent to
A
dA2
S
dS= , which can be
integrated to give 12C
A
S= from which we can obtain our first invariant x:
2A
Sx = (4.4)
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The second differential equation
V)ArS(
dV
2
A
dA 2
2 =
can be written as (since 2AxS = )
V
dVdA
A
ArAxb
2
2
=
,
or
V
dVdA
A
rxb =
where 22b = . By integration of this equation we find
VlnC)AlnrAx(b 2 =+
from which there follows that Axbbr eACV= , where C is a constant.
Therefore another invariant of the PDE is the function )t,x(u , related to )t,A,S(V
by
= AS
bexp)t,x(uA)t,A,S(Vn
(4.5)
with2
r2brn == .
Upon substitution of )t,A,S(V given by (4.5) into equation (3.1), we find that the
function )t,x(u satisfies the BS equation
0uruxrux
2
1u xxx
22t =++ (4.6)
The proof is in Appendix B.
5. Transformation of the BS equation to the heat equation.
Under the substitution
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is transformed into the equation
yy2
2
1 = (5.11)
Introducing further a new independent variable by
2
y = (5.12)
equation (5.11) is transformed to the heat equation
ww = (5.13)
where
)y,(),(ww == (5.14)
We thus arrive at the following
Theorem 2. The solution to the BS equation (4.6) is given by
),(we)t,x(ur= (5.15)
where
)x(ln
2y
2 +== (5.16)
t
=(5.17)
and ),(w satisfies the heat equation ww = .
Using Theorems 1 and 2, we get the following
Theorem 3. The differential equation (3.1) has the general solution
= r
A
Sbexp),(wA)t,A,S(V
m (5.18)
where the function ),(w satisfies the heat equation ww = .
The variables and are defined by (5.16) and (5.17) respectively, while
brm = ,2
2b = , is given by (5.3) and x by (4.4).Therefore equation (5.18)
can be written in full notation as
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= r
A
S
2exp),(w
A
1)t,A,S(V
2
r22
where
+
=
2
1r
A
Sln
2
2
2
What we need now is some solutions to the heat equation, which are not singular
at 0 = ( Tt = ). We come to this point next.
6. General solutions of the heat equation
The Lie algebra of the infinitesimal symmetries of the heat equation ww = is
produced by the six vector fields
X1
=
2
X4
+
=
X2
= w
w
2X5
=
w
wX3
= w
w)2(
4
4X22
6
+
+
=
and the infinite dimensional sub-algebra
w ),(X =
where ),( is an arbitrary solution of the heat equation (refs. [15], [37]).
6.1. The solution that is invariant with respect to the generator
w2
2
362 w)a2()14(4XaXX +++=++
(a is a constant) is given by ([15], [37])
+
+
+
+=
14
2,
2
aWK
14
2,
2
aWK
14
1),(w
22
214 2
+
+ )2arctan(
2
a
14
exp
2
2
(6.1)
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where )z,a(W is the parabolic cylindrical function of imaginary argument
(Appendix D).
Note. The solution given by Olver [15] (Example 3.17, p.208) contains some
misprints. We have repeated the calculations [28] and we have found the solutiongiven by (6.1).
6.2. The solution that is invariant with respect to the generator
w52 w2XX +=
is given by ([15], [37])
++++=3
2exp})(BiK)(AiK{),(w
32
22
1 (6.2)
where )x(Ai and )x(Bi are the Airy functions (Appendix E).
Both solutions (6.1) and (6.2) we have considered, are not singular for 0 =
( Tt = ). This is because we want to take into account the payoff conditions (2.15)-
(2.18) valid for Tt = ( 0 = ).
Appendix A. Lie Symmetry Analysis of the pricing PDE.
We consider the PDE (3.1) :
0VrA
VS
S
VSr
S
VS
2
1
t
V
2
222 =
+
+
+
(A.1)
We shall determine the Lie Point Symmetries of the previous equation.
We follow closely Olver (ref. [15]).
Let )V,t,A,S()2(
be defined by
VrA
VS
S
VSr
S
VS
2
1
t
V)V,t,A,S(
2
222)2( +
+
+
= (A.2)
We introduce the vector field X (the generator of the symmetries)
by
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+
+
+
=t
)V,t,A,S(A
)V,t,A,S(S
)V,t,A,S(X 321
V)V,t,A,S(
+ (A.3)
The second prolongation is defined in our case by the equation
SS
SS
t
t
A
A
S
S)2(
V
V
V
VXXpr
+
+
+
+= (A.4)
The Lie point symmetries of the equation are determined by
0)]V,t,A,S([Xpr)2()2( = as long as 0)V,t,A,S( )2( = .
We implement next the equation 0)]V,t,A,S([Xpr)2()2( = .We have
0)]V,t,A,S([Xpr)2()2( =
0VrVSVSrVS2
1VXpr ASSS
22t
)2( =
+++
++++ )r(]VVrVS[ ASSS2
1
0S2
1)S()Sr(
SS22tAS =++++ (A.5)
We have the following expressions for the coefficients S , A ,t
and SS
+= tS32SV1SS1VS
S VVV)(
ASV2tSV3AS2 VVVVV
+= tA32AV2AA2VA
A VVV)(
tAV3SAV1SA1 VVVVV
+= St12tV3tt3Vt
t VVV)(
tSV1tAV2At2 VVVVV
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++= 2SSV1VVtSS3SSS1SVSSSS
V)2(VV)2(
+ SSS1Vt2SVV3
3SVV1tSSV3
V)2(VVVVV2
StSV3SSAV2SSSV1SAS2
VV2VVVV3V2
SStV3SASV2StS3SASV2 VVVV2V2VV2
ASS2A2SVV2 VVV
Using the previous expressions for S , A ,t and SS we get from
the equation (A.5) that
+++ r]VVrVS[ ASSS2
1
++ AS2tS32SV1SS1VS VVVV)({Sr
+ }VVVV ASV2tSV3
++ SA1tA32AV2AA2VA VVVV)({S
+ }VVVV tAV3SAV1
++ At2St12tV3tt3Vt VVVV)(
+ tSV1tAV2 VVVV
+++ 2SSV1VVtSS3SSS1SVSS22 V)2(VV)2({S
2
1
+ SSS1Vt2SVV3
3SVV1tSSV3
V)2(VVVVV2
StSV3SSAV2SSSV1SAS2 VV2VVVV3V2
SStV3SASV2StS3SASV2 VVVV2V2VV2
0}VVV ASS2A2SVV2 = (A.6)
We have now to take into account condition 0)V,t,A,S()2( = .
For this purpose we substitute tu by
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VrVSVSrVS2
1ASSS
22 +
into (A.6). We thus derive the equation
+++ r]VVrVS[ ASSS2
1
+++ }VVVVV)({Sr ASV2AS22SV1SS1VS
+
++ VrVSVSrVS
2
1}V{Sr ASSS
22SV3S3
+++ }VVVVV)({S SAV1SA12AV2AA2VA
+
++ VrVSVSrVS
2
1}V{S ASSS
22AV3A3
+++ VrVSVSrVS
2
1)( ASSS
22t3Vt
+
+ At2St1
2
ASSS22
V3 VVVrVSVSrVS2
1
+
++ VrVSVSrVS
2
1}VV{ ASSS
22SV1AV2
++++ }V)2(V)2({S21 2SSV1VVSSS1SVSS22
+ }VV2{S2
1 2SVV3SSV3SS3
22
+
+ VrVSVSrVS
2
1ASSS
22
++ SAS2SSS1V3SVV1
22V2V)2(V{S
2
1
StSV3SSAV2SSSV1 VV2VVVV3
+ }VV2V2VV2 SASV2StS3SASV2
+
++ VrVSVSrVS
2
1}V{S
2
1ASSS
22SSV3
22
0}VVV{S2
1ASS2A
2SVV2
22 =+ (A.7)
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Equate all the coefficients of the partial derivatives of the function V to zero. We
are then going to obtain a system of partial differential equations of the unknown
coefficients 321 ,, and of the vector field (A.3). Before that, and just for the
economy of the calculations, we observe that we can get some simple expressions,
by first looking at the coefficients of the mixed partial derivatives.
In fact the coefficient of the derivative SAV is )2(S2
1S2
22 and that of
SAS VV is )2(S2
1V2
22 which means that 0 S2 = and 0 V2 = .
Therefore the coefficient 2 does not depend either on S or V:
)t,A( 22 = (A.8)
The coefficient of the derivative StS VV is )2(S2
1V3
22 and that of StV is
)2(S2
1S3
22 which means that 0 V3 = and 0 S3 = . Therefore the
coefficient 3 does not depend neither on V nor on S:
)t,A( 33 = (A.9)
Because of (A.8) and (A.9), equation (A.7) becomes
+++ r]VVrVS[ ASSS2
1
+++ }VV)({Sr 2SV1SS1VS
+++ }VVVV)({S SAV1SA1AA2VA
+
++ VrVSVSrVS
2
1)(S ASSS
22A3
+++ VrVSVSrVS
2
1)( ASSS
22t3Vt
+
++ VrVSVSrVS
2
1)V(VV ASSS
22SV1At2St1
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++++ }V)2(V)2({S2
1 2SSV1VVSSS1SVSS
22
0}VV3V)2(V{S2
1SSSV1SSS1V
3SVV1
22 =++ (A.10)
The coefficient of SSSVV is the sum of the terms
22V1 S
2
1)( and )3(S
2
1V1
22
and therefore 0 V1 = , which means that
)t,A,S( 11 = (A.11)
Therefore (A.10) becomes
+++ r]VVrVS[ ASSS2
1
+++++ }VV)({S}V)({Sr SA1AA2VASS1VS
+
++ VrVSVSrVS
2
1)(S ASSS
22A3
+++ VrVSVSrVS
2
1)( ASSS
22t3Vt
++++ }VV)2({S2
1VV 2
SVVSSS1SVSS
22
At2St1
0V)2(S2
1SSS1V
22 =+ (A.12)
From (A.12) we get the following coefficients, which have to be zero:
Coefficient of 2SV :
0S2
1VV
22 = (A.13)
Coefficient of AV :
0)(SS t212t332 =++ (A.14)
Coefficient of SSV :
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0S2
1)2(S
2
1S A3
32S1t3
221
2 =++ (A.15)
Coefficient of SV :
+++ A32A1S1t31 SrS)(Srr
0)2(S2
1t1SS1SV
22 =+ (A.16)
Zero-th order coefficient
++++ t3AS VSrSSrr
0S2
1V)(r SS
22t3V =++ (A.17)
We have now to solve the system of PDEs (A.13)-(A.17).
From (A.13) we get 0VV = and therefore is a linear function with respect to
V:
)t,A,S(V)t,A,S( += (A.18)
From (A.15) we get
A3t31S1 S2
1
2
1
S
1 += (A.19)
which is a linear differential equation with unknown function 1 .
The solution of the previous differential equation is
)t,(SS2
1)SlnS(
2
1 A3
2t31 ++= (A.20)
where )t,( is a function to be determined.
From (A.14), using the expression (A.20) for the function 1 , we derive the
equation
++ )SlnS(2
1S
2
3t3
23
0S)]t,([ t22t3 =++ (A.21)
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Since the previous equation should hold for every S, each one of the coefficients
has to be zero. Therefore we obtain the following four equations:
0 3 = (A.22)
0 t3 = (A.23)0)t,( 2t3 =+ (A.24)
0 t2 = (A.25)
From the equations (A.22) and (A.23) and taking into account (A.9),we get that 3
is a constant:
13 a = (A.26)
From equation (A.25) there follows that 2 is independent of the time t and so
)A(f2 = (A.27)
Therefore equation (A.24) gives us
)A(f)t,( = (A.28)
The function 1 becomes, as follows from (A.20),
)(fS1 = (A.29)
From the above equation we get the following expressions to be used later on.
)(f S1 = (A.30a)
0 SS1 = (A.30b)
)A(fS A1 = (A.30c)
0 t1 = (A.30d)
Equation (A.16), using the expressions (A.18)-(A.20), takes the form
0S)A(fS)A(fSr)A(fSr S222
=+Solving the previous equation with respect to S , we find
)A(f S2 = (A.31)
and therefore
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)t,A(S)A(f2 += (A.32)
where )t,A( is a function to be determined.
We also find from (A.31) that
0S SS2 = (A.33)
an expression we shall need later on.
From (A.32) we also get
)t,A( tt2 = (A.34)
and
)t,A(S)A(f AA2 += (A.35)
From (A.17), using (A.18) we obtain the equation
++++++ )V(S)V(Sr)V(r ASS
0)V(S2
1V)(r)V( SSSS
22t3tt =+++++ (A.36)
Equating the coefficients of V to zero, we get from the previous equation the
following two equations:
+++ AS SSrr
0S2
1)(r SS
22t3t =+++ (A.37)
and
0S2
1SSrr SS
22tS =++++ (A.38)
Equation (A.38) expresses the fact that the function introduced in (A.14) is a
solution of the original PDE.Equation (A.37) can be expressed as
+++ )}t,A(S)A(f{
1S)A(f
1Sr A22
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0)t,A(
1t2
=+ (A.39)
The previous equation can be written in equivalent form
0S)A(fS)}A(fr)t,A({)t,A(2
At =+++ (A.40)
Since the previous equation should hold for any value of S, we get the following
equations:
0)A(f = (A.41)
0)A(fr)t,A(A =+ (A.42)
0)t,A( t = (A.43)
From (A.41) we conclude that )A(f is a second degreepolynomial with respect to A:
2
432 AaAaa)A(f ++= (A.44)
From (A.43), we obtain that )t,A( does not depend on t. Therefore
)A(g)t,A( = (A.45)
and so equation (A.42) becomes, because of (A.45) and (A.44)
0a2r)A(g4=+
from which we determine the function )A(g :
54 aAar2)A(g += (A.46)
Therefore
54 aAar2)t,A( += (A.47)
Le us collect now everything together.
We find from (A.29) and (A.44) that
)Aa2a(S 431 += (A.48)
From (A.27) and (A.44) we find that
2
4322 AaAaa ++= (A.49)
We also have from (A.26)
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Using the transformation (4.5), we can express the various partial derivatives of
the function )t,A,S(V in terms of the partial derivatives of the function )t,x(u .
We find that
=
ASbexpAuV ntt
+=
A
Sbexp)AubAu(V 1n2nxS
++=
A
Sbexp)AubAub2Au(V 2n23nx
4nxxSS
+=
A
Sbexp)ASubAunASu2(V 2n1n3nxA
Substituting the above expressions into the original equation (3.1), we obtain
++++ )AubAub2Au(S2
1uA 2n23nx
4nxx
22t
n
+++ )AubAu(Sr 1n2nx
++ )ASubAunASu2(S 2n1n3nx
0Aur n =
The previous equation can be put into the form
++ xx4n22
tn u)AS(
2
1uA
+
++ x
3n22n3n22 u)AS(2)AS(r)AS(b22
1
+++
)AS(n)AS(br)AS(b2
1 1n1n2n222
] 0uAr)AS(b n2n2 = (B.1)We now have to simplify the expressions appearing within the brackets of the
previous equation. We have
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25
C1. Lie Symmetry Analysis of the equationAfter performing a Lie symmetry analysis, we have found that the above equation
has the six symmetry generators (six vector fields)
tX1
= (C.1)
uutc
a4
bx
a4
b
tt
xx
2
1X
2
2
22
+
+
= (C.2)
+
+
= 2xa8
1t2x
a4
b
tt
xtxX 2
22
23
uut
2
1tc
a4
b 22
2
(C.3)
xX4
= (C.4)
uut
a2
bx
a2
1
xtX
225
+
= (C.5)
uuX6
= (C.6)
and the infinite dimensional sub-algebra
u)t,x(X
= (C.7)
where )t,x( is an arbitrary solution of the original equation (ref. [37])
C.2. Transformation of the equation to the heat equation
We shall consider a linear combination of generators such as to convert the BS
equation to the heat equation. For this reason, we consider
uu
x
1
t
1X
+
+
= (C.8)
where and are constants to be determined.
In order to determine the invariants corresponding to the symmetry (C.8), we
consider the system
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u
du
1
dx
1
dt == (C.9)
From the equation1
dx
1
dt = we get by integration xCt 1 =+
or 1Ctx += and hence one invariant of the equation is
txy = (C.10)
From the equationu
du
1
dt = we get by integration )uCln(t 2=
or uCe 2t = and hence another invariant is
teu= (C.11)
Therefore
teu = (C.12)
Using (C.12) and (C.10) we find that
tytt e)(u +=
tyx eu =
tyyxx eu =
Therefore the equation ucubuau xxx2
t ++= transforms to the equation
(divided by the factort
e )
cba yyy2
yt ++=+
from which we get
)c()b(a yyy2t +++= (C.13)
We determine now and such as to become zero the coefficients
of y and :
0b =+
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0c =
Therefore we should have b = and c= , and hence the two
invariants will be
tbxy += and ue tc = Therefore we arrive at the following
Lemma
The substitution
)btyx,t(ue tc ==
converts the equation ucubuau xxx2
t ++= to the heat equation
yy2
t a =
Appendix D. Webers Differential Equation
Abramowitz and Stegun ([41], 19.17) define as standard solutions of Webers
equation
yx4
1ay 2
=
the functions )x,a(W where
)yG2yG(2
)a(cosh)x,a(W 2311
4/1 =with
+= ai
2
1
4
1G1
+= ai
2
1
4
3G3
and 1y , 2y are defined by
+
+
++=
!6
xa
2
7a
!4
x
2
1a
!2
xa1y
63
42
2
1
+
++
++
!8
xa
4
211a25a
!8
x
4
15a11a
835
824
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28
and
+
+
++=
!7
xa
2
13a
!5
x
2
3a
!3
xaxy
73
52
3
2
+
++
++
!11
xa
4
531a35a
!9
x
4
63a17a
1135924
respectively.
In the previous expressions, the non-zero coefficients na of!n
xn
are connected by
2nn2n a)1n(n4
1
aaa + =
It is also worth noting that )x,a(W can be expressed in terms of the Confluent
Hypergeometric functions ([41], 19.25)
= 2
3
14/3 x4
1,a
2
1,
4
3H
G
G2)x,a(W
21
3 x
4
1,a
2
1,
4
1Hx
G
G2
where
=++= )xi2;2m2;ni1m(Fe)x,n,m(H 11xi
)xi2;2m2;ni1m(Me xi ++=
Note. Webers equation can be obtained by separation of variables for the Laplace
equation in parabolic cylindrical coordinates (ref [42], Chapter 10).
Appendix E. The Airy equation
The differential equation ofAiry
0wzw =
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29
has as solutions the linearly independent solutions
)z(Ai and )z(Bi
(Abramowitz and Stegun [41], 10.4).
These functions are defined by
)z(gc)z(fc)z(Ai 21 =
)]z(gc)z(fc[3)z(Bi 21 +=
where
!)k3(
z
3
13z
!9
741z
!6
41z
!3
11)z(f
k3
k0k
k963
=
=+
+
++=
and
!)1k3(
z
3
23z
!10
852z
!7
52z
!4
2z)z(g
1k3
k0k
k1074
+
=+
+
++=
+
=
respectively.
The constants 1c and 2c are given by
)3/2(3
1
3
)0(Bi)0(Aic
3/21===
and
)3/1(3
1
3
)0(iB)0(iAc
3/12=
==
They also can be expressed in terms ofBessels functions of fractional order:
)(K3
z
1)z(Ai 3/1= ([41], 10.4.14)
)}(I)(I{3z)z(Bi 3/13/1 += ([41], 10.4.18)
where zz3
2 =
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