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Volume 2009, Article ID 590856,11pages doi:10.1155/2009/590856

Research Article

The Return Map for a Planar Vector

Field with Nilpotent Linear Part: A Direct and

Explicit Derivation

Rodica D. Costin

Ohio State University, Columbus, OH 43210, USA

Correspondence should be addressed to Rodica D. Costin,[email protected]

Received 18 May 2009; Revised 4 July 2009; Accepted 24 August 2009

Recommended by Manfred H. Moller

Using a direct approach the return map near a focus of a planar vector field with nilpotent linear part is found as a convergent power series which is a perturbation of the identity and whose terms can be calculated iteratively. The first nontrivial coefficient is the value of an Abelian integral, and the following ones are explicitly given as iterated integrals.

Copyrightq2009 Rodica D. Costin. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

1. Introduction

The study of planar vector fields has been the subject of intense research, particularly in connection to Hilbert’s 16th Problem. Significant progress has been made in the geometric theory of these fields, as well as in bifurcation theory, normal forms, foliations, and the study of Abelian integrals1,2.

The Poincar´e first return maps have been studied in view of their relevance for establishing the existence of closed orbits, and also due to their large number of applications

see e.g.,3and references therein, and also in connection to o-minimality4.

The monodromy problemdetermining when the singularity is a center or a focus was solved by Andreev5.

A fundamental result concerns the asymptotic form of return maps states that if the singular points of aC∞ vector field are algebraically isolated, there exists a semitransversal arc such that the return map admits an asymptotic expansion is positive powers ofxand logswith the first term linear, or has its principal part a finite composition of powers and exponentials6,7.

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the other hand, there are few results available in the general setting18–20. The recent papers

21,22contain methods that can generate general return maps.

The present paper studies an example of a field with nilpotent linear part, near a focus. The main goal is to establish techniques that allow to deduce the return map as a suitable series which can be calculated algorithmically and can be used in numerical calculations.

2. Main Result

The paper studies the return map for the system

˙

XY, Y˙ X3−Y3, 2.1

which has a nilpotent linear part both eigenvalues are zero. This is one of the simplest examples of systems in this class23, and for which there areto the author’s knowledge no methods available to generate the return map.

The main result is the following.

Proposition 2.1. Letwith 0< < 0be small enough.

The solution of 2.1satisfyingX0 , Y0 0 first returns to the positiveX-axis at the valueXsatisfying

X

n1

Xn3n1, 2.2

which is a convergent series.

The coefficientsXncan be calculated iteratively. In particular,

X1 −23/2c1, X2 16c21, X3−23/2

20c2c18c349c31

, 2.3

wherecnvn1withvngiven by

v1ξ ξ−2

ξ

0

t4pt3/2 dt, v2ξ − 3 2ξ

−2

ξ

0

t4pt1/2v1tdt, 2.4

v3ξ ξ−2

ξ

0

t4

−3 2 pt

1/2

v2t 3 8

v12t

pt1/2

dt, 2.5

where

pt 4−6t24t4−t6. 2.6

3. Proof of

Proposition 2.1

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3.1. Normalization

It is convenient to normalize the variablesX, Y, t so that the constantappears as a small parameter in the equation with

Xx, Y 2−1/22y, τ 2−3/2t, 3.1

the system2.1becomes

dx −2y,

dy 4x

3αy3, 3.2

whereαis the small parameter

α21/23. 3.3

While the initial conditionX0 becomesx0 1, it is useful to study solutions of

3.2with the more general initial conditionx0 ηwithηin a neighborhood of 1.

Remark 3.1. System 3.2has the formdHαω 0 withH y2 x4,ω y3dxandαa small parameter. The recent result15gives a formalism for finding the return map for this type of systems; see also17. The present construction is concrete, explicit, and suitable for numerical calculations.

3.2. General Behavior of Solutions of

3.2

Letα >0.

Note the following Lyapunov function for3.2

L x, yy2x4, with d

dτL xτ, yτ

−2αyτ4≤0. 3.4

Since the set {y 0} contains no trajectories besides the origin which is the only equilibrium point of3.2, then the origin is asymptotically stable by the Krasovskii-LaSalle principle.

Consider the solution of3.2with the initial conditionx0 η, y0 0 for some

η∈1/2,3/2.

Sincey0 > 0 andx0 0, x0 < 0 thenyincreases andxdecreases for small

τ > 0. This monotony must change due to3.4, and this can happen only at some point where y 0 or where 4x3 αy3, whichever comes first. Sincey increases, then the first occurrence is a point where 4x3 αy3. At this pointx<0 soxcontinues to decrease, while

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Denote by x0τ, y0τ the solution for α 0: x0 −2y, y0 4x30 and x00

η, y00 0. Thereforex40y20 η4. We have x0τ Oα, yτ y0τ thereforeηηOα.

Similar arguments show that the solutionxτ, yτof3.2continues to turn around the origin, crossing again the positivex-axis at a pointηηOα and, of course,η < ηby

3.4.

Solutionsxτ, yτof3.2provide smooth parametrizations for solutionsyxof

d dx

y2−4x3αy3. 3.5

Note that following the path xτ, yτ one full rotation around the origin corresponds to considering a positive solution of3.5, followed by a negative one.

3.3. Positive Solutions of

3.5

for

x >

0

Lemma 3.2shows that there exists a unique solution y ≥ 0 of 3.5 so that 0; this solution is defined forx ∈ 0, ηand establishes an iterative procedure for calculating this solution.

Substitutingyu1/2in3.5we obtain

du dx −4x

3αu3/2. 3.6

Lemma 3.2. There existsδ0>0 independent ofηandαso that the following holds.

Letη >0. For anyαwith|α|< α0≤δ0η−3/2,3.6with the conditionuη 0 has a unique solutionuux;α, ηforx∈0, η. One hasux;α, η>0 forx∈0, η,α >0 andux;α, ηis analytic inαandη for|α|< α0andη >0.

Remark 3.3. We will use the results ofLemma 3.2only forηsuch that 1/2≤η ≤3/2. In this caseby loweringα0we can takeα0ofLemma 3.2independent ofηby taking

α0≤ δ0 2 minη

−3 43/273δ0

2 ≡c0δ0. 3.7

Proof ofLemma 3.2. Local analysis shows that solutions of3.6satisfying 0 have an expansion in integer and half-integer powers ofηxand we have

ux η4−x4−16

5 αη

9/2 ηx5/2

1o1, x−→η, 3.8

which inspires the following substitutions. Denote

ξ

1−x

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with the usual branch of the square root forx/η <1and let

ux η4−x4−η3 ηxvξ. 3.10

Note that if 0 then necessarilyv0 0 by3.8. Equation3.6becomes

ξ d

dξvξ 2 δξ

3pξvξ3/2

, 3.11

where

δ2η3α, 3.12

and the polynomialpis given by2.6.Note that∈1,4forξ∈0,1. Lemma 3.2follows if we show the following.

Lemma 3.4. These exists δ0 > 0 so that for any δ with |δ| < δ0, 3.11 has a unique solution

vvξ;δforξ∈0,1so thatv0 0.

Moreover,vξis analytic forδ∈Cwith|δ|< δ0and the terms of its power series

;δ

n≥1

δnvnξ 3.13

can be calculated recursively; in particular, the first terms are2.4,2.5.

To proveLemma 3.4multiply3.11byξand integrate; we obtain thatvis a fixed point

vJvfor the operator

J δξ−2 ξ

0

t4ptvt3/2dtδξ3 1

0

s4pξsvξs3/2ds. 3.14

LetBbe the Banach space of functions;δcontinuous forξ ∈0,1and analytic on the

complexdisk|δ|< δ0, continuous on|δ| ≤δ0, with the norm

f sup

ξ∈0,1 sup

|δ|≤δ0

fξ;δ. 3.15

Letmbe a number with 0< m <1. Letδ0>0 be small enough, so thatδ0< m/

5 and

δ0<10/3/

5.

LetBmbe the ballBm{f ∈ Bm;fm}.

We haveJ:Bm → Bm. Indeed, note that forf ∈ Bmwe have

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therefore, sincef is analytic inδ, then so isptft;δ3/2, and therefore so isJf. Also, if

f∈ Bmthen alsoJf ∈ Bmbecause

Jfξ;δ≤ |δ| 1

0

s4|pξs||fξs;δ|3/2dsδ04m

3/2

5 < δ0 √

5< m. 3.17

Moreover, the operatorJis a contraction onBm. Indeed, using the estimate

pf1

3/2

pf2

3/2

f1−f2 3

2 |f|≤msuppf 1/2

f1−f2

34m1/2

2 3.18

we obtain

Jf1− Jf2cf1f2 withcδ03√5

10 <1. 3.19

Therefore the operatorJhas a unique fixed point, which is the solution;δ. To obtain the power series3.13substitute an expansion;δ v0ξ

n≥1δnvnξ

in3.11. It follows thatξv0 2v00 withv00 0, thereforev0ξ≡0.

Substitution of3.13inpv3/2followed by expansion in power series inδgives

pv3/2 p3/2

1−

n≥1

δnvn p

3/2 ≡p3/2

1

n≥1

δnRn

, 3.20

whereRnRnv1, . . . , vn, p. In particular,

R1− 3 2

v1

p, R2 −3 2 v2 p 3 8

v12

p2

. 3.21

From3.11we obtain the recursive system

ξd

dξvn2vnξ

3p3/2R

n−1, 3.22

forn≥1 and withR01, with the only solution withvn0 0 given recursively by

vnξ ξ−2

ξ

0

t4pt3/2Rn−1tdt. 3.23

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The following gathers the conclusions of the present section.

Corollary 3.5. There existsα0 >0 so that for anyη ∈ 1/2,3/2andαwith|α|< α0,3.5has a unique solutionyxon0, ηsatisfyingyη 0 andy >0 on0, ηforα >0.

Moreover, this solution has the form

x;α, η

η4−x4−η3 ηxv

1−x

η; 2η

3α

1/2

, 3.24

withvvξ, δa solution of3.11. The mapα; 2η3αis analytic for|α|< α 0.

3.4. Solutions of

3.5

in Other Quadrants and Matching

3.4.1. Solutions in Other Quadrants

We found an expression for the solutionyxof3.5forx > 0 andy >0. In a similar way, expressions in the other quadrants can be found. However, taking advantage of the discrete symmetries of3.5, these solutions can be immediately written down as follows.

Letη∈1/2,3/2,αwith|α|< α0.

iLety1 φx;α, ηbe the solution of3.24, defined forx ∈ 0, η, withy1η 0 andy1>0 forα >0,

Then:

iithe functiony2 φx;−α, ηis also a solution of3.5, defined forx∈−η,0; we havey2−η 0 andy2≥0 forα >0,

iiiThe functiony3−φx;α, ηis a solution of3.5, defined forx∈−η,0. We have

y3−η 0 andy3≤0 forα >0,

ivThe functiony4 −φx;−α, ηis a solution of3.5, defined forx ∈0, ηand we havey4η 0 andy4≤0 forα >0,

3.4.2. Matching at the Positive y-Axis

Letη,η∈1/2,3/4and lety1x φx;α, ηbe the solution of3.5as ini, forx∈0, η andy2x φx;−α,ηsolution as inii, forx∈−η, 0.

The following lemma finds η so that y10 y20, therefore so that y1 is the continuation ofy2

Lemma 3.6. Let|α|< α0withα0satisfying3.7. Letηso that|η−1|< c1|α|withα0small enough so thatc1α0≤1/2.

There exists a uniqueηηOαso that

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andηdepends analytically onηandαfor|α|< α1forα1being small enough. One has|η−1| ≤c2|α| for somec2>0 and

ηηη4c1α2α2η7c21α3η10

4c321 2 c

3

110c2c1

4, 3.26

wherecnvn1withvnξgiven by2.4,2.5.

Proof. Let

F η, η, α φ 0;−α,ηφ 0;α, η, 3.27

which is a function analytic inη, η, α byLemma 3.2and relation3.12. We haveFη, η,0 0 and

∂F ∂η η, η,0

−4η31−v1; 0 −4η3/0, 3.28

therefore the implicit equationFη, η, α 0 determinesηηη, αas an analytic function of

α,ηforαsmall. We have

ηη≤ |α| sup

|α|<α1,|η|<c1α1

∂αηc1|α|, 3.29

therefore

η−1≤ηηη−1≤ c1c1

|α| ≡c2|α|. 3.30

The expansion ofηin power series of αis found as follows. By using3.24,3.25 becomes

η4−η4v1;−2η3αη4−η4v1; 2η3α, 3.31

where by substituting3.13andηn≥0δnηnfollowed by power series expansion inαwe

obtain3.26.

3.4.3. Matching at the Negative y-Axis

Letη,η∈1/2,3/4andηgiven byLemma 3.6. Consider the solutiony3 −φx;α,ηas in

iii, forx∈−η, 0, withy3−η 0. Thereforey3is the continuation ofy2. Lety4xφx;−α,ηbe a solution of3.5as iniv, forx∈0.

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Lemma 3.7. Let|α|< α1and|η−1| ≤c2|α|withα1small enough so thatη∈1/2,3/2.

There exists a uniqueη >0 so thatφ0;−α,η φ0;α,ηandηdepends analytically onη

andαfor|α|< α2forα2small enough. One has|η−1| ≤c3|α|for somec3>0 and

ηηη4c1α2α2η7c21−α3η10

4c3 21

2 c 3

110c2c1

4, 3.32

wherecnvn1withvnξgiven by2.4,2.5.

Proof. We need to findηηη, α so that

Fη,η, α φ0;−α,ηφ 0;α,η0. 3.33

Note that the functionFabove is the same as3.27. ByLemma 3.6the present lemma follows.

3.5. The First Return Map

Letη∈1/2,3/2andα2as inLemma 3.7. Thenηgiven byLemma 3.7is the first return to the positivex-axis of the solution withx0 η, y0 0 and it is analytic inαandη, therefore, by3.12, it is analytic infor fixedη.

Combining 3.26 and 3.32 we obtain η as a convergent power series in η, with coefficients dependent onη, whose first terms are

ηη−2η4c1α8η7c21α2−η10

20c2c18c349c31

α34. 3.34

To obtain the pointX where the solution of2.1withX0 >0 andY0 0 first returns to the positiveX-axis letα21/23and multiply3.34bysince we haveXx

and, finally, letη1. We obtain thatXis analytic infor smalland

X−23/2 c1416c217−23/2

20c2c18c349c31

10O13, 3.35

wherecnvn1withvngiven by2.4,2.5.

Remark 3.8. The first coefficient of the return map3.34is, up to a sign, the Melnikov integral of the system3.2, see15; of course, the present results are in agreement with this factsee the appendix for details.

Appendix

With the notationH y2x4 andω y3dxthe Melnikov integral of3.2is the quantity

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x >0which means, in the notations used in the present paper, thatT η4then the return map of3.2has the formTTαMT 2 15.

For the present system we have

MT

y2x4Ty 3dx4

T1/4

0

Tx43/2dx4T

7 4

1

0

1−s43/2ds8T7/4c1. A.1

Taking the fourth root in the return map ofTwe obtain3.34.

Acknowledgment

The author is grateful to Chris Miller for suggesting the problem.

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