GENERAL SIXTH PAINLEVÉ EQUATION
HUIZENG QIN AND YOUMIN LU
Received 9 May 2006; Revised 3 September 2006; Accepted 1 October 2006
We study the general sixth Painlev´e equation, develop, and justify the existence of several groups of asymptotics of its real solutions. Our methods also justify the differentiability of the asymptotics. Particular attention is paid to the solutions between 0 and 1. We find the asymptotics of all real solutions between 0 and 1 of the sixth Painlev´e equation as x→+∞.
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1. Introduction
The mathematical and physical significance of the six Painlev´e transcendents has been well established. In the last 20 to 30 years, many mathematicians have spent dramatic effort on studying the properties of these transcendents. Although it is the most com- plicated one among the six Painlev´e equations, there have been many results about the sixth Painlev´e transcendent. In fact, the asymptotics problem of the sixth Painlev´e tran- scendent has been studied in many papers such as [1,2,4–7,9–12], and the connection problem is also studied in the papers [1,4–7,10,11]. In this paper, we study the general sixth Painlev´e equation
d2y dx2 =
1 2
dy dx
21 y+ 1
y−1+ 1 y−x
− 1
x+ 1 x−1+ 1
y−x dy
dx + y(y−1)(y−x)
x2(x−1)2
α+βx
y2 +γ(x−1)
(y−1)2 +δx(x−1) (y−x)2
,
(PVI)
whereα,β,γ, andδare parameters. Heuristically, if yis a “small” solution of(PVI), the following equation truncated from(PVI)would be its “major” part asx→+∞:
d2y dx2 =
1 2
dy dx
21 y+ 1
y−1
−1 x
dy dx−
β(y−1) x2y −
γy
x2(y−1). (1.1)
Hindawi Publishing Corporation
International Journal of Mathematics and Mathematical Sciences Volume 2006, Article ID 69562, Pages1–10
DOI 10.1155/IJMMS/2006/69562
Lettingt=lnxand applying elementary techniques to (1.1), one may solve it to get three different solutions:
y=A+Bsin(alnx+b), (1.2)
whereA=1/2 + (β+γ)/a2andB2=(1/2 + (β+γ)/a2)2−2β/a2; y=b
2xa+B2
2bx−a+A, (1.3)
whereA=1/2−(β+γ)/a2andB2=2β/a2+ (1/2−(β+γ)/a2)2; and y=β+γ
2 (lnx+b)2+ β
β+γ. (1.4)
It is reasonable to expect that some solutions of(PVI) take (1.2), (1.3), or (1.4) as their asymptotics. Indeed, many authors [4–7,9–12] have obtained the corresponding asymptotics asx→0 that can be used to obtain (1.2), (1.3), and (1.4) by applying the well- known symmetry transformations. In this paper, we will prove the following theorems.
The differences of our results are pointed out following each theorem.
Theorem 1.1. Letβ >0 andγ <0. Ifx0>1, 0< y0<1, andyis a solution of(PVI)with y(x0)=y0, then 0< y <1 for allx > x0and it satisfies, asx→+∞,
y=A+Bcos(alnx+b) +Ox−1,
y= −aBx−1sin(alnx+b) +Ox−2, (1.5) whereA=1/2 + (β+γ)/a2andB2=(1/2 + (β+γ)/a2)2−2β/a2.
It is clear that the parameters need to satisfy the condition (1/2 + (β+γ)/a2)2≥2β/a2. The complex form of the asymptotics asx→0 corresponding to this asymptotics has been obtained in many papers [7,10], but our result provides the conditions on the coefficients of the equation for the real solutions to exist, together with the bound 0< y <1. Our proof of this theorem is also elementary and simple.
Theorem 1.2. Equation(PVI)has a group of solutions with the following asymptotics:
y=b
2xa+A+Ox(3/2)a−1/2), y=ab
2 xa−1+Ox(3/2)a−3/2), asx−→+∞,
(1.6)
where 0< a <1/4 or 3/4< a <1, andA=1/2−(β+γ)/a2.
We have noticed that it makes more sense for this result to be true when 0< a <1.
But, it seems to be impossible to prove it using our method. This asymptotics is actually a well-known result [4–6,9–12], but our result here also estimates the second term of the leading behavior of the solution as well as the differentiability of the asymptotics.
Theorem 1.3. Ifγ+β=0, then(PVI)has a group of solutions with the following asymp- totics:
y∼β+γ
2 (lnx+b)2+ β β+γ, y∼(β+γ)x−1(lnx+b), asx−→+∞.
(1.7)
Various forms of this result occur in the literature. For example, in [7] Guzzetti has the following result forx→0:
y(x)∼
⎧⎪
⎪⎪
⎨
⎪⎪
⎪⎩ x
θx2−θ20
4
lnx+4r+ 2θ0
θ02−θ2x 2
+ θ20
θ02−θx2
, θ0= ±θx,
x(r±θ0lnx), θ0= ±θx.
(1.8)
The coefficientsθ0andθxcome from the isomonodromy deformation theory andris a free complex parameter. Applying the symmetry transformations y(x)=xz(t) andx= t−1to this result, our result inTheorem 1.3can be obtained.
It is well known that the transformation y=x/z transforms (PVI) to itself with (α,β,γ,δ) changed to (−β,−α, 1/2−δ, 1/2−γ). Hence, based on the previous theorems, one may easily obtain the following one.
Theorem 1.4. Equation(PVI)has solutions with the following asymptotics:
y∼ x
A+Bsin(alnx+b), asx−→+∞, provided thatα <0,δ >1
2, (1.9) whereA=1/2 + (1−2α−2δ)/2a2andB2=(1/2 + (1−2α−2δ)/2a2)2+ 2α/a2, and
y∼ 2x
(1/2−α−δ)(lnx+b)2, asx−→+∞, provided that 1
2=α+δ. (1.10) 2. Proof of Theorems1.2and1.3
In this section, we use the classical successive approximation method to proveTheorem 1.2. The proof ofTheorem 1.3is similar. In fact, Shimomura [12] studied a more general nonlinear ordinary differential equation, applied the successive approximation method to it, and obtained the result as an application. We first denote the functions (1.2), (1.3),
and (1.4) asy0and substitutet=lnxandy=y0+y1into(PVI). The new equation is d2y1
dt2 − 1
y0
+ 1
y0−1 dy0
dt dy1
dt + β
y20
− γ y0−12
y1+1
2 dy0
dt 2
1 y02
+ 1
y0−12
y1
=Gy0,y1
y21+Hy0,y1
y1dy1
dt +Ky0,y1
dy1
dt 2
+e−tIy0,y1
dy1
dt +e−tFy0,y1,t, (2.1) where
Gy0,y1
=
1 2y20
y0+y1
+ 1
2y0−12y0+y1−1 dy0
dt 2
+ β
y02
y0+y1
− γ
y0−12y0+y1−1, Hy0,y1
= − 1
y0
y0+y1
+ 1
y0−1y0+y1−1) dy0
dt , Ky0,y1
=1 2
1
y0+y1+ 1 y0+y1−1
+1
2
e−t y0+y1
e−t−12, Iy0,y1
= 1 y0+y1
e−t−12 dy0
dt − 1
y0+y1
e−t−11−e−t, Fy0,y1,t=1
2 1
y0+y1
e−t−12 dy0
dt 2
− 1
y0+y1
e−t−11−e−t dy0
dt +αy0+y1
y0+y1−1y0+y1
e−t−1
1−e−t2 +βy0+y1−1y0+y1−2+e−t y0+y1
1−e−t2 +γy0+y1
1−e−t ±
δy0+y1
y0+y1−1 1−e−ty0+y1
e−t−1.
(2.2) As a routine, we introduce a new functionzby using the standard transformation
y1= y0
y0−1z. (2.3)
Now, (2.1) is changed to d2z
dt2 +
β3/2−y0
y02
−γy0+ 1/2 y0−12
z
=My0,y1
z2+Ny0,y1
zdz
dt +Py0,y1
dz dt
2
+e−tQy0,y1
z+e−tIy0,y1
dz
dt+ e−t y0
y0−1Fy0,y1,t,
(2.4)
where My0,y1
= y0
y0−1Gy0,y1
+ 2y0−1 2y0
y0−1Hy0,y1
+
2y0−12
4y3/20 (y0−1)3/2Ky0,y1
,
Ny0,y1
= y0
y0−1Hy0,y1
+ 2y0−1
y0
y0−1Ky0,y1
,
Py0,y1
= y0
y0−1Ky0,y1 , Qy0,y1
= 2y0−1 2y0
y0−1 dy0
dt Iy0,y1
.
(2.5) To proveTheorem 1.2, we assume thaty0takes the function in (1.3). Then, there exist constantsLandt0such that, for|a|<1,t > t0, and|y1| |y0|, the following estimates are true:
My0,y1< L, Ny0,y1< L, Py0,y1< L,
Fy0,y1,t y0
y0−1 < eatL, Qy0,y1< eatL, Iy0,y1
|< eatL.
(2.6)
We convert (2.4) into the following integral equation:
z1
z2
= ∞
t
t−τ 1
Rτ,z1(τ),z2(τ)dτ, (2.7)
wherez1=z,z2=z, and
R(τ,z,z)=
γy0+1/2 y0−12 −
β3/2−y0
y20
z+My0,y1
z2+Ny0,y1
zdz
dt+Py0,y1
dz dt
2
+e−tQy0,y1
z+e−tIy0,y1
dz
dt+ e−t y0
y0−1Fy0,y1,t.
(2.8) In order to apply the successive approximation method to (2.7), we rewrite it as
Z(t)=Lt,Z(t), (2.9)
whereZ(t)=(zz12) andL(t,τ,z) is the right-hand side of (2.7). Now, we can define the sequence
Z−1(t)=0,
Zn(t)=Lt,Zn−1(t), n=0, 1, 2,.... (2.10) We first take care of the case when|a|<1/4. Lett0be large enough such that, when t≥t0,
y0
y0−1e−(1/2−a/2)t<1
2, 5L
(1−a)2e−(1/2−a/2)t<1 6, 4e−at<1
6, 8Le−at<1
6, 4L
3(a−1)2e(a−1)t<1 6, 2
(1−a)2e−at<1
6, 8L
9(a−1)2e(a−1)t≤1 6.
(2.11)
Then,
Z1(t)≤
∞
t
τ−t 1
e−τ y0
y0−1Fy0, 0,τdτ
≤ L
(1−a)2e−(1−a)t≤1
2e(a/2−1/2)t, fort≥t0, Z1(t)−Z0(t)≤1
2e(a/2−1/2)t, fort≥t0.
(2.12)
Assume that
Zn(t)≤1
2e(a/2−1/2)t, Zn(t)−Zn−1(t)≤
1 2
n−1
e(a/2−1/2)t, fort≥t0.
(2.13)
Then, fort≥t0, Zn+1(t)≤
∞
t
τ−t 1
5Le(a−1)τ+1
2e−((a+1)/2)τ+ 2Le(3/2)(a−1)τ
dτ
≤1
2e(a/2−1/2)t.
(2.14)
Using the mean value theorem, we can also get Zn+1(t)−Zn(t)≤
∞
t
τ−t 1
e−aτ+ 2Le−aτ+ 3Le(a−1)τZn(τ)−Zn−1(τ)dτ
≤ 1
2
n−1∞
t
τ−t 1
e−((a+1)/2)τ+ 2Le−((a+1)/2)τ+ 3Le(3/2)(a−1)τdτ
≤ 1
2 n
e(a/2−1/2)t.
(2.15) Therefore, the sequence{Zn(t)}converges uniformly toZ(t) and
Z(t)≤1
2e(a/2−1/2)t ∀t≥t0. (2.16)
Hence, we have proved that(PVI)has a solution satisfying y=b
2eat+A+Oe((3/2)a−1/2)t=b
2xa+A+Ox(3/2)a−1/2, y=ab
2 xa−1+Ox(3/2)a−3/2), asx−→ ∞, 0< a <1 4.
(2.17)
Applying the transformationy=x/zto(PVI)and using the result we have obtained, we can get the asymptotics for 3/4< a <1 and finish the proof ofTheorem 1.2.
3. Proof ofTheorem 1.1
We can easily prove Theorems1.2and1.3using the successive approximation method since the corresponding homogeneous equation is easy to solve. When y0takes the ex- pression in (1.2), the corresponding homogeneous equation to (2.4) becomes one of the famous Hill equations [3] whose solutions are very hard to analyze. Thus, we have dif- ficulties to apply the successive approximation method to this case. Fortunately, we can manage to manipulate(PVI)a little bit and apply a method used by Hastings and McLeod [8] to it.
We first prove the first part of the theorem. Suppose that y(x1)=0 for somex1> x0. Sincey(x) is analytic nearx1, we have the expansion
y(x)=cx−x1
n
+Ox−x1
n+1
, (3.1)
wherec=0 andn >0. Substituting (3.1) into(PVI), we get the equation cn(n−1)x−x1
n−2
+Ox−x1
n−1
=c
2n2x−x1
n−2
+Ox−x1
n−1
+ β
cx1−12
x−x1−n+Ox−x1−n+1 .
(3.2)
Thus, we haven=1 andc/2 +β/c(x1−1)2=0. This is impossible whenβ >0 and there- fore,y(x)>0 for allx > x0. Similarly, we can prove thaty(x)<1 for allx > x0whenγ <0.
This result enables us to assume thatyis a solution between 0 and 1 in this section. We first apply the transformation
t=lnx (3.3)
to(PVI)and obtain d2y
dt2 = 1 2
1 y+ 1
y−1 dy
dt 2
+β(1−y)
y + γy
1−y +e−t
1 2ye−t−1
dy dt
2
− y−1 1−e−tye−t−1
dy
dt +αy(y−1)ye−t−1 1−e−t2 +β(y−1)y−2 +e−t
y1−e−t2 + γy
1−e−t+ δ y(y−1) 1−e−tye−t−1
.
(3.4) Since 0< y <1, we can rewrite (3.4) into
d dt
y(1−y)−1/2dy dt
·2y−1/2(1−y)−1/2dy dt
= 2 y(1−y)
β(1−y)
y + γy
1−y dy
dt + 2e−t
y(1−y)Q(y,t)dy dt.
(3.5)
Integrating both sides of (3.5), we get 1
y(1−y) dy
dt 2
+2β y −
2γ
1−y=C+ 1
y(1−y)Oe−t. (3.6) Sinceβ >0,γ <0, and 2β/y−2γ/(1−y) dominates (1/y(1−y))O(e−t) whentis large, C=a2>0, 1/y, 1/(1−y), anddy/dt are all bounded astgoes to infinity. Multiplying both sides of (3.6) byy(1−y) and lettingy=z+rwhereris a constant to be determined later, we get
dz dt
2
+a2z2+2ra2−2β−2γ−a2z+ 2β−
2β+ 2γ+a2r+a2r2=Oe−t. (3.7) We selectr=1/2 + (β+γ)/a2=A, then
dz dt
2
+a2z2=a2B2+Oe−t. (3.8) To solve (3.8), we let
z(t)=ρ(t) cosφ(t),
z(t)=aρ(t) sinφ(t). (3.9)
We are using two functionsρ(t) andφ(t) inz(t) andz(t) to describe the relationship of the functionz(t) and its derivative. Because of this relationship, one ofρ(t) andφ(t) should be depending on another as the product rule of derivatives prescribes. Substituting (3.9) into (3.8), one first gets
ρ2(t)=B2+Oe−t. (3.10)
Following (3.8), we may also get dφ
dt = −a+azz+a2z2
ρ2(t) = −a+Oe−t. (3.11) Integrating (3.11) and combining the result with (3.9) and (3.10), one gets
z(t)=
B+Oe−tcosat+b+Oe−t,
z(t)=aB+Oe−tsinat+b+Oe−t, (3.12) and finishes the proof ofTheorem 1.1.
Acknowledgment
The authors are deeply grateful to the referee for his/her valuable comments and sugges- tions.
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Huizeng Qin: Department of Mathematics and Information Science, Shandong University of Technology, ZiBo, Shandong 255049, China
E-mail address:qinhz [email protected]
Youmin Lu: Department of Mathematics and Computer Science, Bloomsburg University, Bloomsburg, PA 17815, USA
E-mail address:[email protected]