Definitions

# Painlevé transcendents

In mathematics, Painlevé transcendents are solutions to certain nonlinear second-order ordinary differential equations in the complex plane with the Painlevé property (the only movable singularities are poles), but which are not generally solvable in terms of elementary functions. They are named for the French mathematican (and prime minister) Paul Painlevé who found them around 1900.

## History

Painlevé transcendents have their origin in the study of special functions, which often arise as solutions of differential equations, as well as in the study of isomonodromic deformations of linear differential equations. One of the most useful classes of special functions are the elliptic functions. They are defined by second order ordinary differential equations whose singularities have the Painlevé property: the only movable singularities are poles. This property is shared by all linear ordinary differential equations but is rare in nonlinear equations. Poincare and L. Fuchs showed that any first order equation with the Painlevé property can be transformed into the Weierstrass equation or the Riccati equation, which can all be solved explicitly in terms of integration and previously known special functions. Émile Picard pointed out that for orders greater than 1, movable essential singularities can occur, and tried and failed to find new examples with the Painleve property. (For orders greater than 2 the solutions can have moving natural boundaries.) Around 1900, Paul Painlevé studied second order differential equations with no movable singularities. He found that up to certain transformations, every such equation of the form

$y^\left\{primeprime\right\}=R\left(y^\left\{prime\right\},y,t\right)$

(with R a rational function) can be put into one of fifty canonical forms (listed in ). found that forty-four of the fifty equations are reducible in the sense that they can be solved in terms of previously known functions, leaving just six equations requiring the introduction of new special functions to solve them. (There were some computational errors in his work, which were fixed by B. Gambier and R. Fuchs.) It was a controversial open problem for many years to show that these six equations really were irreducible for generic values of the parameters (they are sometimes reducible for special parameter values; see below), but this was finally proved by and . These six second order nonlinear differential equations are called the Painlevé equations and their solutions are called the Painlevé transcendents.

The most general form of the sixth equation was missed by Painlevé, but was discovered in 1905 by Richard Fuchs (son of Lazarus Fuchs), as the differential equation satisfied by the singularity of a second order Fuchsian equation with 4 regular singular points on P1 under monodromy-preserving deformations. It was added to Painlevé's list by . tried to extend Painlevé's work to higher order equations, finding some third order equations with the Painlevé property.

## List of Painlevé equations

These six equations, traditionally called Painlevé I-VI, are as follows:

• I (Painlevé):

$frac\left\{d^2y\right\}\left\{dt^2\right\} = 6 y^2 + t$
• II (Painlevé):

$frac\left\{d^2y\right\}\left\{dt^2\right\} = 2 y^3 + ty + alpha$
• III (Painlevé):

$tyfrac\left\{d^2y\right\}\left\{dt^2\right\} =$
t left(frac{dy}{dt} right)^2 -yfrac{dy}{dt} + delta t + beta y + alpha y^3 + gamma ty^4
• IV (Gambier):

$yfrac\left\{d^2y\right\}\left\{dt^2\right\}=$
frac{1}{2} left(frac{dy}{dt} right)^2 +beta+2(t^2-alpha)y^2+4ty^3+frac{3}{2}y^4
• V (Gambier):

begin\left\{align\right\}
frac{d^2y}{dt^2}&= left(frac{1}{2 y }+frac{1}{ y -1}right) left(frac{dy}{dt} right)^2 -frac{1}{t} frac{dy}{dt} &quad+frac{(y -1)^2}{t}left(alpha y +frac{beta}{ y }right) +gammafrac{ y }{t}+deltafrac{ y (y +1)}{ y -1} end{align}
• VI (R. Fuchs):

begin\left\{align\right\}
frac{d^2y}{dt^2}&= frac{1}{2}left(frac{1}{y}+frac{1}{y-1}+frac{1}{y-t}right)left(frac{dy}{dt} right)^2 -left(frac{1}{t}+frac{1}{t-1}+frac{1}{y-t}right)frac{dy}{dt} &quad + frac{y(y-1)(y-t)}{t^2(t-1)^2} left(alpha+betafrac{t}{y^2}+gammafrac{t-1}{(y-1)^2}+deltafrac{t(t-1)}{(y-t)^2}right) end{align}

The numbers α, β, γ, δ are complex constants. By rescaling y and t one can choose two of the parameters for type III, and one of the parameters for type V, so these types really have only 2 and 3 independent parameters.

## Singularities

The possible singularities of these equations are

• Movable poles
• The point ∞
• The point 0 for types III, V, and VI
• The point 1 for type VI

For type I, the singularities are (movable) double poles or residue 0, and the solutions all have an infinite number of such poles in the complex plane. The functions with a double pole at z0 have the Laurent series expansion

$\left(z-z_0\right)^\left\{-2\right\}-frac\left\{z_0\right\}\left\{10\right\}\left(z-z_0\right)^2-frac\left\{1\right\}\left\{6\right\}\left(z-z_0\right)^3+h\left(z-z_0\right)^4+frac\left\{z_0^2\right\}\left\{300\right\}\left(z-z_0\right)^6+cdots$
converging in some neighborhood of z0 (where h is some complex number). The location of the poles was described in detail by . The number of poles in a ball of radious R grows roughly like a constant times R5/2.

For type II, the singularities are all (movable) simple poles.

## Degenerations

The first five Painlevé equations are degenerations of the sixth equation. More precisely, some of the equations are degenerations of others according to the following diagram, which also gives the corresponding degenerations of the Gauss hypergeometric function

 III Bessel $nearrow$ $searrow$ VI Gauss → V Kummer II Airy → I None $searrow$ $nearrow$ IV Hermite-Weber

## Hamiltonian systems

The Painlevé equations can all be represented as Hamiltonian systems.

Example: If we put

$displaystyle q=y,quad p=y^\left\{prime\right\}+y^2+t/2$
then the second Painlevé equation
$displaystyle y^\left\{primeprime\right\} =2y^3+ty+b-1/2$
is equivalent to the Hamiltonian system
$displaystyle q^\left\{prime\right\}=frac\left\{partial H\right\}\left\{partial p\right\} = p-q^2-t/2$
$displaystyle p^\left\{prime\right\}=-frac\left\{partial H\right\}\left\{partial q\right\} = 2pq+b$
for the Hamiltonian
$displaystyle H=p\left(p-2q^2-t\right)/2 -bq.$

## Symmetries

A Bäcklund transformation is a transformation of the dependent and independent variables of a differential equation that transforms it to a similar equation. The Painlevé equations all have discrete groups of Bäcklund transformations acting on them, which can be used to generate new solutions from known ones.

#### Example

The set of solutions of the type I Painlevé equation
$y^\left\{primeprime\right\}=6y^2+t$
is acted on by the order 5 symmetry y→ζ3y, t→ζt where ζ is a fifth root of 1. There are two solutions invariant under this transformation, one with a pole of order 2 at 0, and the other with a zero of order 3 at 0.

#### Example

In the Hamiltonian formalism of the type II Painlevé equation
$displaystyle y^\left\{primeprime\right\}=2y^3+ty+b-1/2$
with
$displaystyle q=y,p=y^prime+y^2+t/2$
two Bäcklund transformations are given by
$displaystyle \left(q,p,b\right)rightarrow \left(q+b/p,p,-b\right)$
and
$displaystyle \left(q,p,b\right)rightarrow \left(-q, -p+2q^2+t,1-b\right).$
These both have order 2, and generate an infinite dihedral group of Bäcklund transformations (which is in fact the affine Weyl group of A1; see below). If b=1/2 then the equation has the solution y=0; applying the Bäcklund transformations generates an infinite family of rational functions that are solutions, such as y=1/t, y=2(t3−2)/t(t3−4), ...

Okamoto discovered that the parameter space of each Painlevé equation can be identified with the Cartan subalgebra of a semisimple Lie algebra, such that actions of the affine Weyl group lift to Bäcklund transformations of the equations. The Lie algebras for PI, PII, PIII, PIV, PV, PVI are 0, A1, A1⊕A1, A2, A3, and D4,

## Relation to other areas

The Painlevé equations are all reductions of integrable partial differential equations; see .

The Painlevé equations are all reductions of the self dual Yang-Mills equations.

## References

• See sections 7.3, chapter 8, and the Appendices
• .