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Simultaneous bifurcation of limit cycles for Piecewise Holomorphic systems

Armengol Gasull1, Gabriel Rondón1 and Paulo R. da Silva2 1Departament de Matemàtiques, Edifici Cc, Universitat Autònoma de Barcelona, 08193 Bellaterra, Barcelona, Spain. 2São Paulo State University (Unesp), Institute of Biosciences, Humanities and Exact Sciences. Rua C. Colombo, 2265, CEP 15054–000. S. J. Rio Preto, São Paulo, Brazil. [email protected] [email protected] [email protected]
Abstract.

Let z˙=f(z)\dot{z}=f(z) be a holomorphic differential equation with center at pp. In this paper we are concerned about studying the piecewise perturbation systems z˙=f(z)+ϵR±(z,z¯),\dot{z}=f(z)+\epsilon R^{\pm}(z,\overline{z}), where R±(z,z¯)R^{\pm}(z,\overline{z}) are complex polynomials defined for ±Im(z)>0.\pm\operatorname{Im}(z)>0. We provide an integral expression, similar to an Abelian integral, for the period annulus of p.p. The zeros of this integral control the bifurcating limit cycles from the periodic orbits of this annular region. This expression is given in terms of the conformal conjugation between z˙=f(z)\dot{z}=f(z) and its linearization z˙=f(p)z\dot{z}=f^{\prime}(p)z at pp. We use this result to control the simultaneous bifurcation of limit cycles of the two annular periods of z˙=i(z21)/2\dot{z}={\rm i}(z^{2}-1)/2, after both complex and holomorphic piecewise polynomial perturbations. In particular, as far as we know, we provide the first proof of the existence of non nested limit cycles for piecewise holomorphic systems.

Key words and phrases:
Piecewise polynomial complex systems, holomorphic systems, limit cycles, averaging method, simultaneous bifurcation
2020 Mathematics Subject Classification:
32A10, 34A36, 34C07, 37G15

1. Introduction

There are several important aspects to understand the dynamics of planar differential systems such as knowledge of the existence and number of limit cycles. In fact, the famous Hilbert’s 16th problem is one of the main open problems in the qualitative theory of planar polynomial vector fields. Finding good upper or lower bounds for the maximum number of limit cycles of particular families of such systems in terms of their degrees, or other characteristics, constitute challenging problems. Of course, the existence of upper bounds, explicit or not, are the more difficult questions. In this work we will concentrate on lower bounds.

In recent years, great interest has arisen in the study of limit cycles of piecewise holomorphic systems, which is a subfamily of piecewise smooth systems. This is because holomorphic functions have many applications in various areas of applied science, such as the study of fluid dynamics [1, 5, 6]. Furthermore, the study and properties of holomorphic systems z˙=f(z)\dot{z}=f(z) make them interesting and beautiful but the absence of limit cycles makes them dynamically poor. Interestingly, in [13] and [14] the authors showed that there are piecewise holomorphic systems that have limit cycles. More precisely, in [14] the authors have used the intrinsic properties of holomorphic functions, such as their integrability, to construct limit cycles, whereas in [13] Gasull et al. approach this problem with different points of view: study of the number of zeros of the first and second order averaged functions, and with the control of the limit cycles appearing from a monodromic equilibrium point via a degenerated Andronov–Hopf type bifurcation.

Consider the piecewise polynomial complex systems (PWCS),

(1) z˙=f(z)+{ϵRm+(z,z¯), when Im(z)>0,ϵRm(z,z¯), when Im(z)<0,\displaystyle\dot{z}=f(z)+\left\{\begin{array}[]{l}\epsilon R^{+}_{m}(z,\overline{z}),\text{ when }\operatorname{Im}(z)>0,\\[5.0pt] \epsilon R^{-}_{m}(z,\overline{z}),\text{ when }\operatorname{Im}(z)<0,\end{array}\right.

where z˙=f(z)\dot{z}=f(z) has a center at p,p, 0<ϵ1,0<\epsilon\ll 1, z=x+iyz=x+iy\in\mathbb{C} and Rm±(z,z¯)R_{m}^{\pm}(z,\overline{z}) are complex polynomial functions with degree m.m. Notice that the straight line Σ={z:Im(z)=0}\Sigma=\{z\in\mathbb{C}:\operatorname{Im}(z)=0\} divides the plane in two halfplanes Σ±={z:±Im(z)>0}.\Sigma^{\pm}=\{z\in\mathbb{C}:\pm\operatorname{Im}(z)>0\}. As usual, the orbits on Σ\Sigma are defined following the Filippov convention, see [8] for more details.

When in system (1), f(z)=iz,f(z)={\rm i}z, in the (r,θ)(r,\theta)-polar coordinates z=reiθz=re^{i\theta}, r>0r>0 and θ𝕊1,\theta\in\mathbb{S}^{1}, it is converted into

(2) drdθ={F+(θ,r,ϵ)=ϵF1+(θ,r)+𝒪(ϵ2), if 0θπ,F(θ,r,ϵ)=ϵF1(θ,r)+𝒪(ϵ2), if πθ2π,\dfrac{dr}{d\theta}=\begin{aligned} \left\{\begin{array}[]{l}F^{+}(\theta,r,\epsilon)=\epsilon F_{1}^{+}(\theta,r)+\mathcal{O}(\epsilon^{2}),\text{ if }0\leq\theta\leq\pi,\\[5.0pt] F^{-}(\theta,r,\epsilon)=\epsilon F_{1}^{-}(\theta,r)+\mathcal{O}(\epsilon^{2}),\text{ if }\pi\leq\theta\leq 2\pi,\end{array}\right.\end{aligned}

where ϵ>0\epsilon>0 is a sufficiently small parameter and 𝒪\mathcal{O} represents terms of order at least two in ε\varepsilon for the functions F±.F^{\pm}. By using the theory of averaging in this context (see [15]), it is well-known that each simple zero r=r0r=r_{0} of

(3) M1(r)=M1+(r)M1(r)whereM1±(r)=0±πF1±(θ,r)𝑑θ,M_{1}(r)=M_{1}^{+}(r)-M_{1}^{-}(r)\quad\mbox{where}\quad M_{1}^{\pm}(r)=\displaystyle\int_{0}^{\pm\pi}F_{1}^{\pm}(\theta,r)d\theta,

provides, for ϵ\epsilon small enough, a hyperbolic limit cycle of the piecewise smooth system (2) that tends to r=r0r=r_{0} when ϵ\epsilon tends to 0. The function M1M_{1} is called the first order averaged function and sometimes it is also called the first order Melnikov function.

Our first aim is to use expression (3) to obtain a general closed expression for the Melnikov function of system (1) for a general ff such that z˙=f(z)\dot{z}=f(z) has a center at p.p. From [3, 10], we know that there exists a conformal map w=ϕ(z)w=\phi(z) such that this differential equation can be written as w˙=iw\dot{w}=-{\rm i}w (or w˙=iw\dot{w}={\rm i}w). The map ϕ\phi is called the linearizing change of z˙=f(z)\dot{z}=f(z) at pp. Our approach works on the largest open set where this conformal map is well defined. In what follows, we state our first main result.

Theorem A.

Consider the piecewise complex system (1). Suppose that ϕ\phi is the linearizing change of z˙=f(z)\dot{z}=f(z) at pp such that ϕ(Σ)Σ\phi(\Sigma)\subset\Sigma. Then, its first order Melnikov function is M1(r)=M1+(r)M1(r),M_{1}(r)=M_{1}^{+}(r)-M_{1}^{-}(r), where

(4) M1±(r)=Im(0±πϕ(ϕ1(reiθ))Rm±(ϕ1(reiθ),ϕ1(reiθ¯))¯ieiθ𝑑θ).M_{1}^{\pm}(r)=-\operatorname{Im}\left(\displaystyle\int_{0}^{\pm\pi}\overline{\phi^{\prime}(\phi^{-1}(re^{{\rm i}\theta}))R_{m}^{\pm}\left(\phi^{-1}(re^{{\rm i}\theta}),\overline{\phi^{-1}(re^{{\rm i}\theta}})\right)}\,{\rm i}e^{{\rm i}\theta}d\theta\right).

In particular, each simple zero r=r0r=r_{0} of M1M_{1} provides, for ϵ\epsilon sufficiently small, a hyperbolic limit cycle of (1) that tends to r=r0r=r_{0} when ϵ\epsilon tends to 0.

The above results is an extension to the discontinuous case to the one obtained in [11] in the smooth situation.

We will employ Theorem A to study PWCS (1) for f(z)=i(z21)/2f(z)={\rm i}(z^{2}-1)/2 and

(5) Rm±(z,z¯)=l=0mk=0la¯k,l±zlkz¯k,ak,landm=0,1,2,3.R_{m}^{\pm}(z,\overline{z})=\sum_{l=0}^{m}\sum_{k=0}^{l}\overline{a}^{\pm}_{k,l}z^{l-k}\overline{z}^{k},\,\,a_{k,l}\in\mathbb{C}\,\,\text{and}\,\,m=0,1,2,3.

In fact, this unperturbed system has been also the one considered in [11] in the smooth perturbations context.

We emphasize that z˙=f(z)=i(z21)/2\dot{z}=f(z)={\rm i}(z^{2}-1)/2 has 2 centers at -1 and 1, separated by the invariant straight line Re(z)=0.\operatorname{Re}(z)=0. Each of the punctured halfplanes {z:±Re(z)>0}{±1}\{z\in\mathbb{C}:\pm\operatorname{Re}(z)>0\}\setminus\{\pm 1\} is filled by periodic orbits of the system. To carry out this study, we explicitly use the linearization change w=ϕ(z)=(1+z)/(1z)w=\phi(z)=(1+z)/(1-z) of z˙=f(z)\dot{z}=f(z) at 1-1, which we employ to find the bifurcation function at z=1z=-1. Thus, by changing variables and time we will obtain the bifurcation function at z=1.z=1. It is worth noting that this linearizing is specially simple and has also a simple inverse but, unfortunately, for most holomorphic vector fields ff, the calculations can be much more complicated.

This type of problem has been addressed in several papers. Specifically, in [11] Garijo et al. study the smooth case, that is, Rm=Rm+=RmR_{m}=R^{+}_{m}=R^{-}_{m}, providing an integral expression for the differential equation z˙=f(z)+ϵRm(z,z¯)\dot{z}=f(z)+\epsilon R_{m}(z,\overline{z}) and use this formula to control the simultaneous bifurcation of limit cycles of the two annular periods of z˙=iz+z2\dot{z}={\rm i}z+z^{2}, after a polynomial perturbation. Also, in [7] the authors investigate the number of bifurcating periodic orbits of a cubic polynomial vector field having two period rings using piecewise perturbations. They study, up to first-order averaging analysis, the bifurcation of periodic orbits of the two annular periods, the first separately and the second simultaneously. There are other works that consider the problem of simultaneous bifurcation such as [4, 12, 19] although in the context of piecewise systems the type of bifurcation that we consider in this paper is a complete novelty.

Before stating our second main result, we introduce some notations. We denote by M1M_{1} and N1N_{1} the first order averaged functions at 1-1 and 11, respectively. In addition, we say that system (1) presents the configuration of limit cycles [i,j][i,j] if M1M_{1} and N1N_{1} have simultaneously ii and jj simple zeros in the interval (0,1),(0,1), respectively. Our definition is motivated from the theory of averaging of first order, because as we will see in this case, for ε\varepsilon small enough, the differential system has ii limit cycles surrounding 1-1 and jj limit cycles surrounding 1.1. Obviously, by the symmetry of the problem if the configuration [i,j][i,j] holds the configuration [j,i][j,i] also does. For short we will say that the configuration [[i,j]][[i,j]] is realizable.

For m3,m\leq 3, we will prove that both functions, multiplied by r,r, belong to the vectorial space \mathcal{F} generated by the functions

=[r,r2,r3,r4,(r21)2arctanh(r),(r41)arctanh(r),r2arctanh(r)],\mathcal{F}=[r,r^{2},r^{3},r^{4},(r^{2}-1)^{2}\operatorname{arctanh}(r),(r^{4}-1)\operatorname{arctanh}(r),r^{2}\operatorname{arctanh}(r)],

where recall that

arctanh(r)=tanh1(r)=12ln(1+r1r).\operatorname{arctanh}(r)=\tanh^{-1}(r)=\frac{1}{2}\ln\left(\frac{1+r}{1-r}\right).

As we will prove, the above ordered set of functions forms an extended complete Chebyshev system (ECT-system) on (0,1),(0,1), see Section 2.2 for more details. This property will allow to control the exact number of zeros of each of the functions, separately.

For bigger mm the number of monomials rk,r^{k}, as well as the number of functions of the form Sl(r)arctanh(r)S_{l}(r)\operatorname{arctanh}(r) for some fixed increasing degree polynomials SlS_{l} in M1M_{1} and N1N_{1} will grow, but our approach also would apply. In short, for a fixed mm the control of the maximum number of zeros of M1M_{1} and N1N_{1} seems that could be completely understood, but would need much more computational effort. For this reason we have restricted most of our attention to the case m3.m\leq 3. On the other hand, the knowledge of the maximum number that both functions can have simultaneously is a difficult and challenging problem. All results that we have obtained in this direction are resumed in next theorems.

Theorem B.

Consider PWCS (1) with f(z)=i(z21)/2f(z)={\rm i}(z^{2}-1)/2. If m=0,m=0, the unique realizable configurations are [[i,j]],[[i,j]], with 0i+j10\leq i+j\leq 1. When 1m3,1\leq m\leq 3, if [[i,j]][[i,j]] is a realizable configuration then i,jm+3.i,j\leq m+3. Moreover the following configurations, of course satisfying i,jm+3,i,j\leq m+3, are realizable:

  • (a)

    [[i,j]][[i,j]] with 0i+j40\leq i+j\leq 4 when m=1.m=1.

  • (b)

    [[i,j]][[i,j]] with 0i+j6,0\leq i+j\leq 6, when m=2.m=2.

  • (c)

    [[i,j]][[i,j]] with 0i+j80\leq i+j\leq 8 when m=3.m=3.

As a very particular subcase in the proof of Theorem B there appears the situation when both M1M_{1} and N1N_{1} are polynomials. In this situation the question of the simultaneous number of zeros in (0,1)(0,1) of both functions can be approached with much more detail. We believe that this is a problem that is interesting by itself. All our results in this subcase are resumed in Proposition 8.

At this point another natural question arises: What happens if the complex perturbation function Rm±R^{\pm}_{m} in PWCS (1) is holomorphic? For short we will call these systems PWHS. For them both Rm±R^{\pm}_{m} depend only on zz. As we will see, the fact that the perturbation is holomorphic greatly simplifies the calculations and it is not surprising that the number of cycles that arise is less than in the above more general situation.

As we will prove, in this case and for m3,m\geq 3, the functions M1(r)M_{1}(r) and N1(r),N_{1}(r), multiplied by (r21)m3,(r^{2}-1)^{m-3}, belong to the vectorial space 𝒢\mathcal{G} generated by the functions

𝒢=[1,r,r2,,r2(m2),r(r21)m3arctanh(r)],\mathcal{G}=[1,r,r^{2},\ldots,r^{2(m-2)},r(r^{2}-1)^{m-3}\operatorname{arctanh}(r)],

that is also an ECT-system on (0,1).(0,1). We only have tackled the problem of simultaneous bifurcations when m3.m\leq 3. Our main result for PWHS is:

Theorem C.

Consider piecewise holomorphic systems of the form (1), with f(z)=i(z21)/2,f(z)={\rm i}(z^{2}-1)/2, where Rm±R^{\pm}_{m} depend only on zz. The following holds:

(a) When m=0m=0 the unique realizable configurations are [[i,j]],[[i,j]], with 0i+j10\leq i+j\leq 1 and when m{1,2}m\in\{1,2\} the unique realizable configurations are [[i,j]][[i,j]] with i+j2.i+j\leq 2.

(b) When m=3,m=3, if [[i,j]][[i,j]] is a realizable configuration then i,j3.i,j\leq 3. Moreover the following configurations, of course satisfying i,j3,i,j\leq 3, are realizable: [[i,j]][[i,j]] with 0i+j4.0\leq i+j\leq 4.

(c) When m>3,m>3, if [[i,j]][[i,j]] is a realizable configuration then i,j2m3.i,j\leq 2m-3.

In item (c) we only give an upper bound for the values ii and j.j. We believe that this upper bound is reached, as happens when m=3.m=3. To prove this fact we should develop in more detail our computations but we have decided do not face this question here. Similarly, we think that the value i+ji+j must have an upper bound smaller that 2(2m3),2(2m-3), because the functions M1M_{1} and N1N_{1} are strongly dependent, see the proof of Proposition 9.

It is well known that smooth quadratic systems can have nested limit cycles, formed by 1,21,2 or 33 limit cycles and also limit cycles forming two disjoint nests with configurations {1,1},\{1,1\}, {2,1}\{2,1\} and {3,1},\{3,1\}, see [18] and its references. Moreover, people believe that these are the only possible configurations. Until now, all examples with PWHS having limit cycles present them in a single nest and, already in the degree 1 case, there were linear PWHS examples with 1,21,2 or 33 nested limit cycles, see [13]. In this paper we present the first examples of PWHS with two different nests of limit cycles. Moreover for quadratic PWHS we obtain the following result:

Corollary 1.

There are quadratic PWHS of the form (1), with Rm±R^{\pm}_{m} depending only on zz and m{1,2},m\in\{1,2\}, having two limit cycles with configuration [[1,1]].[[1,1]]. For cubic PWHS of the same form but with m=3,m=3, there are configurations with two nests of the types [[1,1]],[[1,1]], [[2,1]],[[2,1]], [[3,1]][[3,1]] and [[2,2]].[[2,2]].

The paper is organized as follows. In Section 2 we present some basic results and the proof of Theorem A. Then we dedicate next two sections to prove Theorems B, and C. The most tedious computations, devoted to obtain the first order averaged functions M1M_{1} and N1,N_{1}, are deferred to the Appendix 5.

2. Preliminaries and proof of Theorems A

In this section first we recall some results that will be used throughout the paper. Then we prove Theorem A and by using it and the computations of Appendix 5 we obtain the explicit expressions of first order averaged functions M1M_{1} and N1.N_{1}.

2.1. The averaging method

We briefly recall some basic results of the averaging theory for piecewise smooth systems written in polar coordinates. An overview on this subject can be found in [15], and the reader can see the details of the proofs there. Consider the piecewise smooth systems of the form

(6) drdθ={F+(θ,r,ϵ) if 0θπ,F(θ,r,ϵ) if πθ2π,\dfrac{dr}{d\theta}=\begin{aligned} \left\{\begin{array}[]{l}F^{+}(\theta,r,\epsilon)\text{ if }0\leq\theta\leq\pi,\\[5.0pt] F^{-}(\theta,r,\epsilon)\text{ if }\pi\leq\theta\leq 2\pi,\end{array}\right.\end{aligned}

where F±(θ,r,ϵ)=j=1kϵjFj±(θ,r)+ϵk+1R±(θ,r,ϵ),F^{\pm}(\theta,r,\epsilon)=\sum_{j=1}^{k}\epsilon^{j}F_{j}^{\pm}(\theta,r)+\epsilon^{k+1}R^{\pm}(\theta,r,\epsilon), with θS1,\theta\in S^{1}, r>0r>0 and ϵ>0\epsilon>0 is a sufficiently small parameter.

The following result can be found in [15, Theorem 1]:

Theorem 2.

Let M1M_{1} be the averaged function of order 1 given by (3). Then, each simple zero r=r0r=r_{0} of M1M_{1} provides, for ϵ\epsilon small enough, a hyperbolic limit cycle of the piecewise smooth system (6) that tends to r=r0r=r_{0} when ϵ\epsilon tends to 0.

2.2. A miscellany of results

A very useful and well-kown characterization of extended complete Chebyshev system (ECT-system) is the following:

Lemma 3.

[f0,,fn][f_{0},\cdots,f_{n}] is an ECT-system on I,I\subset\mathbb{R}, an open interval, if and only if for all k=0,1,,n,k=0,1,\cdots,n, Wk(x)0W_{k}(x)\neq 0 for all xIx\in I, where

Wk(x)=W[f0,,fk](x)=det(fj(i)(x))0i,jkW_{k}(x)=W[f_{0},...,f_{k}](x)=\det\left(f^{(i)}_{j}(x)\right)_{0\leq i,j\leq k}

is the Wronskian of f0,,fkf_{0},\cdots,f_{k} at xIx\in I.

This result allows us to estimate the number of real zeros of any non-zero function FSpan{f0,,fn}F\in\operatorname{Span}\{f_{0},\cdots,f_{n}\}, where Span()\operatorname{Span}(\mathcal{F}) denotes the set of all functions given by linear combinations of the functions of \mathcal{F}. In what follows, we state a classical result related to the ECT-system, whose proof can be found in [16].

Theorem 4.

Let =[f0,,fn]\mathcal{F}=[f_{0},...,f_{n}] be an ECT-system on II. Then, the number of isolated zeros for every element of Span()\operatorname{Span}(\mathcal{F}) does not exceed nn. Moreover, for each configuration of mnm\leq n zeros in I,I, taking into account their multiplicity, there exists FSpan()F\in\operatorname{Span}(\mathcal{F}) with this configuration of zeros.

In what follows, we provide a simple result for finding the zeros of kk-parameter families of polynomials in one variable.

Let Fλ(x)F_{\lambda}(x) be a kk-parametric family of polynomials. We denote the discriminant of a polynomial p(x)=anxn++a1x+a0p(x)=a_{n}x^{n}+\cdots+a_{1}x+a_{0} as Δx(p)\Delta_{x}(p), i.e.

Δx(p)=(1)n(n1)21anRes(p(x),p(x)),\Delta_{x}(p)=(-1)^{\frac{n(n-1)}{2}}\frac{1}{a_{n}}\operatorname{Res}(p(x),p^{\prime}(x)),

where Res(p,p)\operatorname{Res}(p,p^{\prime}) is the resultant of pp and p0.p_{0}.

Using the same ideas as in [9, Lemma 8.1], it is easy to prove the following result, which will be used throughout the paper.

Lemma 5.

Let Fλ(x)=fn(λ)xn+fn1(λ)xn1++f1(λ)x+f0(λ)F_{\lambda}(x)=f_{n}(\lambda)x^{n}+f_{n-1}(\lambda)x^{n-1}+\cdots+f_{1}(\lambda)x+f_{0}(\lambda), n>1n>1, be a family of real polynomials depending continuously on a parameter λk\lambda\in\mathbb{R}^{k} and set Ωλ=(a(λ),b(λ))\Omega_{\lambda}=(a(\lambda),b(\lambda)), for some continuous functions a(λ)a(\lambda) and b(λ)b(\lambda). Assume that there exists an connected open set 𝒰k\mathcal{U}\subset\mathbb{R}^{k} such that:

  • (i)

    For some λ0𝒰\lambda_{0}\in\mathcal{U}, Fλ0F_{\lambda_{0}} has exactly mm zeros in Ωλ0\Omega_{\lambda_{0}} and all of them are simple.

  • (ii)

    For all λ𝒰\lambda\in\mathcal{U}, Fλ(a(λ))Fλ(b(λ))0F_{\lambda}(a(\lambda))\cdot F_{\lambda}(b(\lambda))\neq 0.

  • (iii)

    For all λ𝒰\lambda\in\mathcal{U}, Δx(Fλ)0\Delta_{x}(F_{\lambda})\neq 0.

Then for all λ𝒰\lambda\in\mathcal{U}, FλF_{\lambda} has also exactly mm zeros in Ωλ\Omega_{\lambda} and all of them are simple.

To finish this section we state the well-known Descartes Theorem, which provides information about the number of positive zeros of a real polynomial based on the sign changes and the number of terms. For further details, see, for example, [2]. Given an ordered list of p+1p+1 non-zero real numbers [a0,a1,,ap][a_{0},a_{1},\ldots,a_{p}], we define the number of sign variations, denoted by mm with 0mp0\leq m\leq p, as the number of indices jp1j\leq p-1 for which ajaj+1<0a_{j}a_{j+1}<0.

Theorem 6 (Descartes Theorem).

Consider the real polynomial P(x)=a0xi0++apxipP(x)=a_{0}x^{i_{0}}+\dots+a_{p}x^{i_{p}} with 0i0<<ip0\leq i_{0}<\dots<i_{p} and aja_{j} non-zero real constants for j{0,,p}.j\in\{0,\ldots,p\}. If the number of sign variations of [a0,a1,,ap][a_{0},a_{1},\ldots,a_{p}] is mm, then P(x)P(x) has exactly m2nm-2n positive real zeros counting their multiplicities, where nn is a non negative integer number.

2.3. Proof of Theorem A

Since pp is a center of z˙=f(z)\dot{z}=f(z), then from [3, 10] we know that there exists ϕ\phi conformal map such that ϕ(z)f(z)=iϕ(z).\phi^{\prime}(z)f(z)=-{\rm i}\phi(z). Using this on z˙=f(z)+ϵR±(z,z¯),\dot{z}=f(z)+\epsilon R^{\pm}(z,\overline{z}), we get

(7) w˙=iw+ϵL±(w,w¯),\dot{w}=-{\rm i}w+\epsilon L^{\pm}(w,\overline{w}),

where L±(w,w¯)=ϕ(ϕ1(w))Rm±(ϕ1(w),ϕ1(w)¯).L^{\pm}(w,\overline{w})=\phi^{\prime}(\phi^{-1}(w))R^{\pm}_{m}(\phi^{-1}(w),\overline{\phi^{-1}(w)}). In the (r,θ)(r,\theta)-coordinates w=reiθw=re^{i\theta}, (7) is converted into

(8) drdθ=rϵ(Re(L±(reiθ,reiθ))cos(θ)+Im(L±(reiθ,reiθ))sin(θ))r+ϵ(Im(L±(reiθ,reiθ))cos(θ)Re(L±(reiθ,reiθ))sin(θ))=F±(r,θ,ϵ).\frac{dr}{d\theta}=\frac{r\epsilon\Big{(}\operatorname{Re}(L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta}))\cos(\theta)+\operatorname{Im}(L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta}))\sin(\theta)\Big{)}}{-r+\epsilon\Big{(}\operatorname{Im}(L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta}))\cos(\theta)-\operatorname{Re}(L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta}))\sin(\theta)\Big{)}}=F^{\pm}(r,\theta,\epsilon).

Hence, expanding F±(r,θ,ϵ)F^{\pm}(r,\theta,\epsilon) around ϵ=0\epsilon=0, (8) is written as

drdθ=ϵF1±(θ,r)+𝒪(ϵ2),\frac{dr}{d\theta}=\epsilon F_{1}^{\pm}(\theta,r)+\mathcal{O}(\epsilon^{2}),

where F1±(θ,r)=Re(L±(reiθ,reiθ))cos(θ)Im(L±(reiθ,reiθ))sin(θ)F_{1}^{\pm}(\theta,r)=-\operatorname{Re}(L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta}))\cos(\theta)-\operatorname{Im}(L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta}))\sin(\theta). Computing the first averaged function

M1±(r)\displaystyle M_{1}^{\pm}(r) =0±πF1±(θ,r)𝑑θ\displaystyle=\displaystyle\int_{0}^{\pm\pi}F_{1}^{\pm}(\theta,r)d\theta
=0±πIm(iL±(reiθ,reiθ)¯)cos(θ)Im(L±(reiθ,reiθ)¯)sin(θ)dθ\displaystyle=-\displaystyle\int_{0}^{\pm\pi}\operatorname{Im}({\rm i}\overline{L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta})})\cos(\theta)-\operatorname{Im}(\overline{L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta})})\sin(\theta)d\theta
=0±πIm(L±(reiθ,reiθ)¯(icos(θ)sin(θ)))𝑑θ\displaystyle=-\displaystyle\int_{0}^{\pm\pi}\operatorname{Im}\Big{(}\overline{L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta})}({\rm i}\cos(\theta)-\sin(\theta))\Big{)}d\theta
=Im(0±πL±(reiθ,reiθ)¯ieiθ𝑑θ)\displaystyle=-\operatorname{Im}\left(\displaystyle\int_{0}^{\pm\pi}\overline{L^{\pm}(re^{{\rm i}\theta},re^{-{\rm i}\theta})}\,{\rm i}e^{{\rm i}\theta}d\theta\right)
=Im(0±πϕ(ϕ1(reiθ))Rm±(ϕ1(reiθ),ϕ1(reiθ¯))¯ieiθ𝑑θ).\displaystyle=-\operatorname{Im}\left(\displaystyle\int_{0}^{\pm\pi}\overline{\phi^{\prime}(\phi^{-1}(re^{{\rm i}\theta}))R^{\pm}_{m}\left(\phi^{-1}(re^{{\rm i}\theta}),\overline{\phi^{-1}(re^{{\rm i}\theta}})\right)}\,{\rm i}e^{{\rm i}\theta}d\theta\right).

From Proposition 2 the result follows.

2.4. The bifurcations functions M1M_{1} and N1N_{1}

The following proposition gives us the expressions of the Melnikov functions M1M_{1} and N1N_{1} as well as the maximum number of zeros that each on of these functions separately can have when f(z)=i(z21)/2.f(z)={\rm i}(z^{2}-1)/2. The starting point is to obtain first an explicit expression for M1M_{1} by doing a detailed study around z=1z=-1. Then, the analysis around z=1z=1 will be reduced from the previous one. All these results are detailed in the Appendix 5.

Proposition 7.

For system (1) with f(z)=i(z21)/2f(z)={\rm i}(z^{2}-1)/2 and m3,m\leq 3, it holds that

M1(r)\displaystyle M_{1}(r) =1r(ar+br2+cr3+dr4+α(r21)2arctanh(r)+β(r41)arctanh(r)\displaystyle=\frac{1}{r}\Big{(}ar+br^{2}+cr^{3}+dr^{4}+\alpha(r^{2}-1)^{2}\operatorname{arctanh}(r)+\beta(r^{4}-1)\operatorname{arctanh}(r)
+γr2arctanh(r)),\displaystyle\qquad\quad+\gamma r^{2}\operatorname{arctanh}(r)\Big{)},
N1(r)\displaystyle N_{1}(r) =1r(cr+(b+2dκ+ρ)r2+ar3+(d+κ)r4+α(r21)2arctanh(r)\displaystyle=\frac{1}{r}\Big{(}cr+(b+2d-\kappa+\rho)r^{2}+ar^{3}+(-d+\kappa)r^{4}+\alpha(r^{2}-1)^{2}\operatorname{arctanh}(r)
β(r41)arctanh(r)+γr2arctanh(r)),\displaystyle\qquad\quad-\beta(r^{4}-1)\operatorname{arctanh}(r)+\gamma r^{2}\operatorname{arctanh}(r)\Big{)},

where, for m=3,m=3, the variables a,b,c,d,α,β,γ,κ,ρa,b,c,d,\alpha,\beta,\gamma,\kappa,\rho can take any real value and depend linearly of the coefficients ak,l±.a^{\pm}_{k,l}. When m<3m<3 only appear the following restrictions: γ=ρ=0\gamma=\rho=0 when m=2;m=2; γ=β=κ=ρ=0\gamma=\beta=\kappa=\rho=0 when m=1;m=1; and γ=β=α=κ=ρ=d=0\gamma=\beta=\alpha=\kappa=\rho=d=0 and c=ac=-a when m=0.m=0. More specifically, the values of these constants are given in Remarks 11 and 13 in the Appendix.

Moreover, the maximum number of zeros of each M1M_{1} and N1N_{1} in (0,1)(0,1) is 1 when m=0m=0 and it is m+3m+3 when 1m3.1\leq m\leq 3.

Proof.

The expression of M1M_{1} is given in Proposition 10 and Remark 11 of the Appendix 5. We remark that we use the linearizing change w=(1+z)/(1z).w=(1+z)/(1-z). To get the expression of N1N_{1} in terms of the coefficients of M1M_{1}, it is enough to use Proposition 12 and Remark 13 of that Appendix, by changing ak,l±a_{k,l}^{\pm} in M1M_{1} by (1)lak,l,(-1)^{l}a_{k,l}^{\mp}, for all 0kl0\leq k\leq l and 0l3.0\leq l\leq 3. Then we arrive to the expression of N1N_{1} of the statement and all the restrictions given there. We skip the details.

Let us study the maximum number of zeros of each of the functions M1M_{1} and N1N_{1} in (0,1),(0,1), separately, in terms of m.m.

The case m=0m=0 is simpler and we study it in a different way. In this situation

M1(r)=a+brar2,N1=a+br+ar2,M_{1}(r)=a+br-ar^{2},\qquad N_{1}=-a+br+ar^{2},

for arbitrary values a=Im(a0,0+)Im(a0,0)a=\operatorname{Im}(a_{0,0}^{+})-\operatorname{Im}(a_{0,0}^{-}) and b=π(Re(a0,0)+Re(a0,0+))b=-\pi(\operatorname{Re}(a_{0,0}^{-})+\operatorname{Re}(a_{0,0}^{+})). It is easy to see each of the functions has at most one zero in (0,1).(0,1).

Let us continue by studying the case m=3.m=3. We want to prove that the ordered set of functions

=[r,r2,r3,r4,(r21)2arctanh(r),(r41)arctanh(r),r2arctanh(r)]\mathcal{F}=[r,r^{2},r^{3},r^{4},(r^{2}-1)^{2}\operatorname{arctanh}(r),(r^{4}-1)\operatorname{arctanh}(r),r^{2}\operatorname{arctanh}(r)]

is an ECT-system in (0,1).(0,1). Notice that M1,N1Span(M_{1},N_{1}\in\operatorname{Span}(\mathcal{F}) . We will use Theorem 4 together with Lemma 3. So, we need to compute several Wronkskians and prove that they do not vanish on (0,1).(0,1). We get, W0(r)=r,W_{0}(r)=r, W1(r)=r2,W_{1}(r)=r^{2}, W2(r)=2r3,W_{2}(r)=2r^{3}, W3(r)=12r4,W_{3}(r)=12r^{4},

W4(r)\displaystyle W_{4}(r) =96(r(5r23)+3(r21)2arctanh(r))(r21)2,\displaystyle=\frac{96(r(5r^{2}-3)+3(r^{2}-1)^{2}\operatorname{arctanh}(r))}{(r^{2}-1)^{2}},
W5(r)\displaystyle W_{5}(r) =3072(15r+22r33r5+3(r21)2(5+r2)arctanh(r))(r21)6,\displaystyle=\frac{3072(-15r+22r^{3}-3r^{5}+3(r^{2}-1)^{2}(5+r^{2})\operatorname{arctanh}(r))}{(r^{2}-1)^{6}},
W6(r)\displaystyle W_{6}(r) =294912r(r(105145r2+15r4+9r6)+3(r21)2(35+10r2+3r4)arctanh(r))(r21)12.\displaystyle=\frac{294912r(-r(105-145r^{2}+15r^{4}+9r^{6})+3(r^{2}-1)^{2}(35+10r^{2}+3r^{4})\operatorname{arctanh}(r))}{(r^{2}-1)^{12}}.

Clearly, the Wronskians Wj(r)0W_{j}(r)\neq 0 at (0,1),(0,1), for all j{0,1,2,3}.j\in\{0,1,2,3\}. Let us prove that Wj(r)0,W_{j}(r)\neq 0, for j=4,5,6j=4,5,6 on (0,1).(0,1).

By computing the first derivative of W4W_{4} we obtain

W4(r)=768r4(1r2)3>0,W_{4}^{\prime}(r)=\frac{768r^{4}}{(1-r^{2})^{3}}>0,

for all r(0,1)r\in(0,1). Since W4(0)=0W_{4}(0)=0 and W4W_{4} is increasing at (0,1)(0,1), we conclude that W4(r)>0W_{4}(r)>0 for all r(0,1)r\in(0,1).

Similarly,

W5(r)\displaystyle W_{5}^{\prime}(r) =18432(U(r)+V(r)arctanh(r))(1r2)7>18432(U(r)+V(r)(r+r33+r55))(1r2)7\displaystyle=\dfrac{18432(U(r)+V(r)\operatorname{arctanh}(r))}{(1-r^{2})^{7}}>\dfrac{18432(U(r)+V(r)(r+\frac{r^{3}}{3}+\frac{r^{5}}{5}))}{(1-r^{2})^{7}}
=18432r6(16+r2+20r4+3r6)5(1r2)7>0,\displaystyle=\dfrac{18432r^{6}(16+r^{2}+20r^{4}+3r^{6})}{5(1-r^{2})^{7}}>0,

where U(r)=21r2+32r43r6U(r)=-21r^{2}+32r^{4}-3r^{6} and V(r)=3r(r21)2(7+r2)V(r)=3r(r^{2}-1)^{2}(7+r^{2}) and we have used that arctanh(r)>r+r3/3+r5/5,\operatorname{arctanh}(r)>r+{r^{3}}/{3}+{r^{5}}/{5}, for all r(0,1)r\in(0,1), which can be proven for instance by using Taylor’s formula. Again W5(0)=0W_{5}(0)=0 and W5(r)W_{5}(r) is increasing, and so we can also conclude that W5(r)>0W_{5}(r)>0 for all r(0,1)r\in(0,1).

Finally,

W6(r)\displaystyle W_{6}^{\prime}(r) =294912(U(r)+V(r)arctanh(r))(1r2)13>294912(U(r)+V(r)(r+r33+r55+r77))(1r2)13\displaystyle=\dfrac{294912\Big{(}U(r)+V(r)\operatorname{arctanh}(r)\Big{)}}{(1-r^{2})^{13}}>\dfrac{294912\Big{(}U(r)+V(r)(r+\frac{r^{3}}{3}+\frac{r^{5}}{5}+\frac{r^{7}}{7})\Big{)}}{(1-r^{2})^{13}}
=294912r9(255+1824r4+474r6+135r8)7(1r2)13>0,\displaystyle=\dfrac{294912r^{9}(255+1824r^{4}+474r^{6}+135r^{8})}{7(1-r^{2})^{13}}>0,

where U(r)=r(105+1910r22864r4+330r6+135r8)U(r)=-r(105+1910r^{2}-2864r^{4}+330r^{6}+135r^{8}) and V(r)=15(r21)2(7+139r2+37r4+9r6),V(r)=15(r^{2}-1)^{2}(7+139r^{2}+37r^{4}+9r^{6}), and this time we have used that arctanh(r)>r+r3/3+r5/5+r7/7,\operatorname{arctanh}(r)>r+{r^{3}}/{3}+{r^{5}}/{5}+{r^{7}}/{7}, for all r(0,1).r\in(0,1). As in the previous case we get that W6(r)>0W_{6}(r)>0 for all r(0,1)r\in(0,1).

According to Lemma 3, \mathcal{F} is an ECT-system. Then, by Theorem 4, 6=m+36=m+3 is the maximum number of zeros for any element of Span()\operatorname{Span}(\mathcal{F}) in (0,1)(0,1) and there are choices for a,b,c,d,α,βa,b,c,d,\alpha,\beta and γ\gamma such that an element of Span()\operatorname{Span}(\mathcal{F}) has exactly jj simple zeros in (0,1)(0,1) for any j=0,1,,6.j=0,1,\ldots,6.

From the expressions of the involved constants, the results when m=1,m=1, (resp. m=2m=2) correspond to κ=ρ=β=γ=0\kappa=\rho=\beta=\gamma=0 (resp. ρ=γ=0\rho=\gamma=0) follow similarly. Moreover it is clear that the number of elements of \mathcal{F} is m+4,m+4, form an ECT-system on (0,1)(0,1) with at most m+3m+3 zeros, taking into account their multiplicities, and the result follows. ∎

3. Proof of Theorem B and the polynomial case

To study the number of zeros that the functions M1M_{1} and N1N_{1} can have in (0,1)(0,1) is a difficult question because of their transcendental nature. In Theorem B we only obtain partial results. In the first part of this section we will prove this theorem.

In the particular case α=β=γ=0\alpha=\beta=\gamma=0 both functions become polynomial and the study is much more affordable. Although this case gives less limit cycles we include a detailed study because we believe that itself provides an interesting problem.

Proof of Theorem B.

Recall that by Proposition 7, the bifurcation function of PWHS (1) associated to z=1z=-1 and z=1z=1 are given respectively by M1(r)=1rf(r)M_{1}(r)=\frac{1}{r}f(r) and N1(r)=1rg(r),N_{1}(r)=\frac{1}{r}g(r), where

f(r)\displaystyle f(r) =ar+br2+cr3+dr4+α(r21)2arctanh(r)\displaystyle=ar+br^{2}+cr^{3}+dr^{4}+\alpha(r^{2}-1)^{2}\operatorname{arctanh}(r)
+β(r41)arctanh(r)+γr2arctanh(r),\displaystyle\quad+\beta(r^{4}-1)\operatorname{arctanh}(r)+\gamma r^{2}\operatorname{arctanh}(r),
g(r)\displaystyle g(r) =cr+(b+2dκ+ρ)r2+ar3+(d+κ)r4+α(r21)2arctanh(r)\displaystyle=cr+(b+2d-\kappa+\rho)r^{2}+ar^{3}+(-d+\kappa)r^{4}+\alpha(r^{2}-1)^{2}\operatorname{arctanh}(r)
β(r41)arctanh(r)+γr2arctanh(r).\displaystyle\quad-\beta(r^{4}-1)\operatorname{arctanh}(r)+\gamma r^{2}\operatorname{arctanh}(r).

with a,b,c,d,α,β,γ,κa,b,c,d,\alpha,\beta,\gamma,\kappa and ρ\rho real coefficients, which depend of coefficients of the system and of m.m. Moreover, the maximum number of zeros that these functions separately can have is 11 when m=0m=0 and m+3m+3 otherwise. Let us study the number of simple simultaneous zeros that ff and gg possess in (0,1)(0,1) in several situations. Clearly, these zeros coincide with the of zeros in (0,1)(0,1) of M1M_{1} and N1,N_{1}, respectively. Recall that we denote these number of zeros as m1,n1,m_{1},n_{1}, respectively, and they give the realizability of the configuration [[m1,n1]][[m_{1},n_{1}]] for PWHS (1).

We will fix m{0,1,2,3}m\in\{0,1,2,3\} and prove the result case by case.

When m=0m=0 the proof is very simple. We know that M1(r)=a+brar2M_{1}(r)=a+br-ar^{2} and N1(r)=a+br+ar2,N_{1}(r)=-a+br+ar^{2}, for arbitrary values a,ba,b\in\mathbb{R}. Then, it is easy to see that either m1=n1=0m_{1}=n_{1}=0 or one of the values is 0 and the other one is 1.

For the cases 1m3,1\leq m\leq 3, we will not give all details, but a procedure that allows to control the number of zeros of ff and gg by forcing the existence of several zeros of them in (1,1).(-1,1).

(a) When m=1,m=1, then κ=ρ=β=γ=0.\kappa=\rho=\beta=\gamma=0. The case α=0\alpha=0 is much simpler and will be studied in next Proposition 8, so we consider α0\alpha\neq 0 and we can assume that α=1.\alpha=1.

Then, the main idea of our approach is to consider four different values r1,r2,r3r_{1},r_{2},r_{3} and r4r_{4} in (1,1)(-1,1) and then impose that four equations among the eight ones: f(rj)=0,g(rj)=0,j=1,2,3,4f(r_{j})=0,g(r_{j})=0,j=1,2,3,4 are fulfilled. Then these four equations fix the values of a,b,ca,b,c and dd and it is easy to obtain them even explicitly, because the eight equations are linear with unknowns a,b,c,d.a,b,c,d.

In this way, any of the configurations [[m1,n1]][[m_{1},n_{1}]] with m1+n14,m_{1}+n_{1}\leq 4, can be obtained. Notice that the negative values of rjr_{j} give zeros of ff or gg that do not contribute to any of the values m1m_{1} or n1,n_{1}, because only simple positive zeros give rise to limit cycles of PWHS (1).

Notice also that when all the procedure is applied, to be sure that a configuration happens we need to prove that the forced zeros are simple. This is not always an easy task but it can be done with a case by case study. For instance, if for 0<m3,0<m\leq 3, m1=m+3,m_{1}=m+3, then they are always simple zeros of ff because this function is an element of an ECT system. If m1<m+3m_{1}<m+3 and not all zeros were simple, then it is easy to perturb the function to have at least m1m_{1} simple zeros. Afterwards, one has to take care of the zeros of g.g. Each situation needs special tricks and sometimes some careful computations. Finally, it has to be studied if the given zeros are the only ones in (0,1)(0,1) or some extra zero does appear. Although this could be done, again by a case by case study, we do not give details on this matter. The main reason is that without studying this last question we already know that at least m1m_{1} limit cycles surrounding z=1z=-1 and n1n_{1} limit cycles surrounding z=1z=1 exist although, eventually, more limit cycles could also appear.

As an illustration we present a detailed study for the case (m1,n1)=(4,0).(m_{1},n_{1})=(4,0). Fix rj=j/5,r_{j}=j/5, for j=1,2,3,4j=1,2,3,4 and force that all these values are zeros of f.f. This completely fixes the parameters a,b,ca,b,c and d.d. Moreover, since we know that [r,r2,r3,r4,(r21)2arctanh(r)][r,r^{2},r^{3},r^{4},(r^{2}-1)^{2}\operatorname{arctanh}(r)] is an ECT in (0,1)(0,1) we can ensure that these zeros are simple for f.f. Then we have to prove that gg does not have zeros in (0,1).(0,1). With this aim, it can be seen that

(g(r)(r21)2)=P4(r)(r21)3,\left(\frac{g(r)}{(r^{2}-1)^{2}}\right)^{\prime}=\frac{P_{4}(r)}{(r^{2}-1)^{3}},

where P4P_{4} is a fixed polynomial of degree 4. It can be seen, by computing its Sturm’s sequence, that it is positive in [0,1].[0,1]. Since g(0)=0,g(0)=0, this shows that g(r)>0g(r)>0 in (0,1)(0,1) and n1=0,n_{1}=0, as we wanted to prove.

(b) When m=2,m=2, ρ=γ=0.\rho=\gamma=0. Recall that in this case the maximum number of zeros that the functions ff and gg separately can have in (0,1)(0,1) is five. We will look for new configurations not appearing when m<2.m<2. Similarly that in the case m=1,m=1, we can fix β=1,\beta=1, take six different values rj,j=1,,6r_{j},j=1,\ldots,6 in (1,1)(-1,1) and impose that six equations among the twelve ones: f(rj)=0,g(rj)=0,j=1,,6f(r_{j})=0,g(r_{j})=0,j=1,\ldots,6 are fulfilled. We remark that at most five of these equations can involve ff or g.g. Then from these six equations we obtain explicitly the values of a,b,c,d,κa,b,c,d,\kappa and α.\alpha. They provide all configurations with 0m1+n160\leq m_{1}+n_{1}\leq 6 with m1,n15.m_{1},n_{1}\leq 5.

(c) Case m=2.m=2. In this occasion we fix γ=1\gamma=1 and eight values between 1-1 and 11 fix the parameters a,b,c,d,κ,ρ,αa,b,c,d,\kappa,\rho,\alpha and β.\beta. By using this approach we obtain all configurations with 0m1+n180\leq m_{1}+n_{1}\leq 8 with m1,n16.m_{1},n_{1}\leq 6.

Next proposition fully characterizes the number of simultaneous zeros of M1M_{1} and N1N_{1} when both functions are polynomial.

Proposition 8.

For each m3,m\leq 3, set

M1(r)=a+br+cr2+dr3,andN1(r)=c+(b+2dκ+ρ)r+ar2+(d+κ)r3,\displaystyle M_{1}(r)=a+br+cr^{2}+dr^{3},\quad\mbox{and}\quad N_{1}(r)=c+(b+2d-\kappa+\rho)r+ar^{2}+(-d+\kappa)r^{3},

the functions given in Proposition 7 when α=β=γ=0.\alpha=\beta=\gamma=0. Let m13m_{1}\leq 3 and n13n_{1}\leq 3 be, respectively, their number of zeros in (0,1)(0,1) taking into account their multiplicities. Then the following holds:

  1. (i)

    When m=0,m=0, (κ=ρ=d=0,\kappa=\rho=d=0, c=ac=-a) then m1+n11.m_{1}+n_{1}\leq 1.

  2. (ii)

    When m=1,m=1, (κ=ρ=0\kappa=\rho=0) then m1+n14.m_{1}+n_{1}\leq 4.

  3. (iii)

    When m=2,m=2, (ρ=0\rho=0) then m1+n14.m_{1}+n_{1}\leq 4.

  4. (iv)

    When m=3,m=3, then m1+n15.m_{1}+n_{1}\leq 5.

Moreover, all values of m1m_{1} and n1n_{1} satisfying the above restrictions are attained, except (m1,n1){(3,0),(0,3)}(m_{1},n_{1})\in\{(3,0),(0,3)\} when m{1,2}.m\in\{1,2\}.

Proof.

(i) It is already proved in Theorem B.

When m0,m\neq 0, the most interesting and difficult case happens if either m1=3m_{1}=3 or n1=3.n_{1}=3. We will concentrate in the case m1=3,m_{1}=3, because the other situation can be reduced to this one.

In particular, dd must be non zero and without loss of generality we can assume that d=1.d=1. Since m1=3,m_{1}=3, M1M_{1} has all its roots r1,r2r_{1},r_{2} and r3r_{3} in (0,1),(0,1), we obtain that

M1(r)\displaystyle M_{1}(r) =r3+cr2+br+a=(rr1)(rr2)(rr3)\displaystyle=r^{3}+cr^{2}+br+a=(r-r_{1})(r-r_{2})(r-r_{3})
=r3(r1+r2+r3)r2+(r1r2+r1r3+r2r3)rr1r2r3.\displaystyle=r^{3}-(r_{1}+r_{2}+r_{3})r^{2}+(r_{1}r_{2}+r_{1}r_{3}+r_{2}r_{3})r-r_{1}r_{2}r_{3}.

Then,

N1(r)=(κ1)r3r1r2r3r2+(r1r2+r1r3+r2r3+2κ+ρ)r(r1+r2+r3).\displaystyle N_{1}(r)=(\kappa-1)r^{3}-r_{1}r_{2}r_{3}r^{2}+\big{(}r_{1}r_{2}+r_{1}r_{3}+r_{2}r_{3}+2-\kappa+\rho\big{)}r-(r_{1}+r_{2}+r_{3}).

Notice that

N1(0)=(r1+r2+r3)<0,N1(1)=(1r1)(1r2)(1r3)+ρ.\displaystyle N_{1}(0)=-(r_{1}+r_{2}+r_{3})<0,\quad N_{1}(1)=(1-r_{1})(1-r_{2})(1-r_{3})+\rho.

Let us prove item (ii). When r1,r2,r3(0,1)r_{1},r_{2},r_{3}\in(0,1) and κ=ρ=0,\kappa=\rho=0, then N1(0)<0,N_{1}(0)<0, N1(1)>0N_{1}(1)>0 and N1′′(r)=6r2r1r2r3<0N_{1}^{\prime\prime}(r)=-6r-2r_{1}r_{2}r_{3}<0 for r0.r\geq 0. Hence when m1=3,m_{1}=3, by Bolzano’s Theorem n11n_{1}\geq 1 and by Rolle’s Theorem n12n_{1}\leq 2 because N1′′|[0,1]<0.N_{1}^{\prime\prime}\big{|}_{[0,1]}<0. Moreover, the possibility n1=2n_{1}=2 is incompatible with N1(0)N1(1)<0N_{1}(0)N_{1}(1)<0 and it holds that (m1,n1)=(3,1).(m_{1},n_{1})=(3,1).

All the other cases satisfying m1<3m_{1}<3 or n1<3n_{1}<3 and 0m1+n140\leq m_{1}+n_{1}\leq 4 can be easily obtained by simple inspection. For instance, by taking r1=1/6r_{1}=1/6, r2=1/4r_{2}=1/4 and r3(0,1)r_{3}\in\mathbb{R}\setminus(0,1) as the roots of M1M_{1}, we get that for r3=2,1/5,21/20,r_{3}=-2,-1/5,21/20, it holds that m1=2m_{1}=2 and the values of n1n_{1} are 0,10,1 and 2,2, respectively. We omit the other examples.

(iii) By using item (ii) it is clear that all cases with 0m1+n140\leq m_{1}+n_{1}\leq 4 and m1<3m_{1}<3 and n1<3n_{1}<3 do happen. It is also clear that there are examples where (m1,n1)(m_{1},n_{1}) is (3,1)(3,1) or (1,3).(1,3). Let us prove that, as in the above case, when m1=3m_{1}=3 then n1=1.n_{1}=1. In this case the proof is more involved.

As in item (ii) we assume that m1=3m_{1}=3 and s1,s2,s3(0,1).s_{1},s_{2},s_{3}\in(0,1). In this case ρ=0\rho=0 and also happens that N1(0)N1(1)<0,N_{1}(0)N_{1}(1)<0, because it is independent of κ.\kappa. In particular we know that n11.n_{1}\geq 1. The difference with the above case is that N1′′(r)=6(κ1)r2r1r2r3N_{1}^{\prime\prime}(r)=6(\kappa-1)r-2r_{1}r_{2}r_{3} and when κ>1\kappa>1 this function can change sign in (0,1).(0,1). In any case, when κ1\kappa\leq 1 we know that n1=1n_{1}=1 and the result follows.

To prove that n1=1n_{1}=1 when κ>1,\kappa>1, we will apply Lemma 5. We fix the values r1,r2,r3(0,1),r_{1},r_{2},r_{3}\in(0,1), consider κ\kappa as a parameter and introduce the notation

Qκ(r):=N1(r)=(κ1)r3r1r2r3r2+(r1r2+r1r3+r2r3+2κ)r(r1+r2+r3).Q_{\kappa}(r):=N_{1}(r)=(\kappa-1)r^{3}-r_{1}r_{2}r_{3}r^{2}+\big{(}r_{1}r_{2}+r_{1}r_{3}+r_{2}r_{3}+2-\kappa\big{)}r-(r_{1}+r_{2}+r_{3}).

Notice that

Qκ(0)=N1(0)<0andQκ(1)=N1(1)>0.Q_{\kappa}(0)=N_{1}(0)<0\quad\mbox{and}\quad Q_{\kappa}(1)=N_{1}(1)>0.

To apply the lemma we first need to study the zeros of Δr(Qκ(r)).\Delta_{r}(Q_{\kappa}(r)). Some computations give that

Δr(Qκ(r))=4κ4+η3κ3+η2κ2+η1κ+η0,\Delta_{r}(Q_{\kappa}(r))=4\kappa^{4}+\eta_{3}\kappa^{3}+\eta_{2}\kappa^{2}+\eta_{1}\kappa+\eta_{0},

where the coefficients ηj=ηj(r1,r2,r3)\eta_{j}=\eta_{j}(r_{1},r_{2},r_{3}), j=0,1,2,3,j=0,1,2,3, are symmetric polynomials that we skip for the sake of shortness. It is well-know that given any real quartic polynomial P(κ)P(\kappa) such that Δκ(P(κ))<0\Delta_{\kappa}(P(\kappa))<0 it has two real roots and two complex ones, see [17]. Some tedious computations give that

Δκ(Δr(Qκ(r)))=256(r121)(r221)(r321)(r1+r2+r3)(E(r1,r2,r3))3,\Delta_{\kappa}\big{(}\Delta_{r}(Q_{\kappa}(r))\big{)}=-256(r_{1}^{2}-1)(r_{2}^{2}-1)(r_{3}^{2}-1)(r_{1}+r_{2}+r_{3})(E(r_{1},r_{2},r_{3}))^{3},

with

E(r1,r2,r3)\displaystyle E(r_{1},r_{2},r_{3}) =27(r2+r3)(1+r2r3)2+27r1(1+r23r32r32+r2r3(6+r32)\displaystyle=-27(r_{2}+r_{3})(1+r_{2}r_{3})^{2}+27r_{1}(-1+r_{2}^{3}r_{3}-2r_{3}^{2}+r_{2}r_{3}(-6+r_{3}^{2})
+r22(2+r32))+r13(27r2r327r32+r23r33+9r22(3+2r32))\displaystyle\quad+r_{2}^{2}(-2+r_{3}^{2}))+r_{1}^{3}(27r_{2}r_{3}-27r_{3}^{2}+r_{2}^{3}r_{3}^{3}+9r_{2}^{2}(-3+2r_{3}^{2}))
+9r12(3r2(2+r32)3r3(2+r32)+r23(3+2r32)+r22r3(3+2r32)),\displaystyle\quad+9r_{1}^{2}(3r_{2}(-2+r_{3}^{2})-3r_{3}(2+r_{3}^{2})+r_{2}^{3}(-3+2r_{3}^{2})+r_{2}^{2}r_{3}(3+2r_{3}^{2})),

which can be seen that is negative for all (r1,r2,r3)(0,1)3.(r_{1},r_{2},r_{3})\in(0,1)^{3}. This is so, because by studying the system

r1E(r1,r2,r3)=0,r2E(r1,r2,r3)=0,r3E(r1,r2,r3)=0,\frac{\partial}{\partial r_{1}}E(r_{1},r_{2},r_{3})=0,\quad\frac{\partial}{\partial r_{2}}E(r_{1},r_{2},r_{3})=0,\quad\frac{\partial}{\partial r_{3}}E(r_{1},r_{2},r_{3})=0,

we get that does not have solutions in (0,1)3.(0,1)^{3}. Hence, the maximum of the function EE on the box [0,1]3[0,1]^{3} is 0 and it is reached in the boundary at the point (0,0,0).(0,0,0). Furthermore, it is easy to see that the two real zeros of Δr(Qκ(r)),\Delta_{r}(Q_{\kappa}(r)), κ1\kappa_{1} and κ2\kappa_{2} satisfy

1<κ1<R<κ2,whereR=r1r2+r1r3+r2r3+2,1<\kappa_{1}<R<\kappa_{2},\quad\mbox{where}\quad R=r_{1}r_{2}+r_{1}r_{3}+r_{2}r_{3}+2,

because Δr(Qκ(r))|κ=1>0\Delta_{r}(Q_{\kappa}(r))|_{\kappa=1}>0 and Δr(Qκ(r))|κ=R<0.\Delta_{r}(Q_{\kappa}(r))|_{\kappa=R}<0.

Hence, if we define the three intervals K1=(1,κ1),K_{1}=(1,\kappa_{1}), K2=(κ1,κ2)K_{2}=(\kappa_{1},\kappa_{2}) and K3=(κ2,),K_{3}=(\kappa_{2},\infty), by Lemma 5 the value n1n_{1} (that is the number of roots of Qκ(r)Q_{\kappa}(r) in (0,1)(0,1)) when κKj,\kappa\in K_{j}, j=1,2,3j=1,2,3 does not depend on κ,\kappa, but on jj and maybe on the values of r1,r2r_{1},r_{2} and r3.r_{3}.

Similarly that in the quartic case, it is also well-know that given any real cubic polynomial P(r)P(r) it holds that:

  • If Δr(P(r))>0\Delta_{r}(P(r))>0 it has three simple real roots; and

  • If Δr(P(r))<0\Delta_{r}(P(r))<0 it has one simple real root and two simple complex roots.

Hence, if we take κK1,\kappa\in K_{1}, then Δr(Qκ(r))>0\Delta_{r}(Q_{\kappa}(r))>0 and QκQ_{\kappa} has three simple real roots. Let us prove that two of them are greater than 1.1. To ensure that κK1\kappa\in K_{1} we take κ=1+ε,\kappa=1+\varepsilon, for ε>0,\varepsilon>0, small enough. For this value of κ,\kappa, let us prove that QκQ_{\kappa} has a positive root that tends to infinite when ϵ\epsilon tends to 0. To prove this fact consider the new variable s=1/r,s=1/r, Then, when κ=1+ε,\kappa=1+\varepsilon,

Pε(s):=s3Qκ(1/s)=(r1+r2+r3)s3+(r1r2+r1r3+r2r3+1ε)s2r1r2r3s+ε.P_{\varepsilon}(s):=s^{3}Q_{\kappa}(1/s)=-(r_{1}+r_{2}+r_{3})s^{3}+\big{(}r_{1}r_{2}+r_{1}r_{3}+r_{2}r_{3}+1-\varepsilon\big{)}s^{2}-r_{1}r_{2}r_{3}s+\varepsilon.

By the implicit function Theorem PεP_{\varepsilon} has a zero s(ε)=ε/(r1r2r3)+O(ε2)s(\varepsilon)=\varepsilon/(r_{1}r_{2}r_{3})+O(\varepsilon^{2}) that tends to zero when ε\varepsilon tends to zero. This zero gives a positive zero r(ε)r(\varepsilon) of Q1+εQ_{1+\varepsilon} that tends to infinity when ε\varepsilon goes to zero. Moreover its asymptotic expansion at ε=0\varepsilon=0 is r(ε)r1r2r3/ε.r(\varepsilon)\sim r_{1}r_{2}r_{3}/\varepsilon. Hence, from the existence of two positive roots of Q1+ε,Q_{1+\varepsilon}, one in (0,1)(0,1) and a second one near infinity we deduce the existence of a third one, which moreover it is in (1,r(ε)),(1,r(\varepsilon)), as we wanted to prove.

If we take κK2,\kappa\in K_{2}, then Δr(Qκ(r))<0\Delta_{r}(Q_{\kappa}(r))<0 and QκQ_{\kappa} has a single real root. Since QκQ_{\kappa} has a root in (0,1)(0,1) then n1=1.n_{1}=1.

If we take κK3,\kappa\in K_{3}, then again Δr(Qκ(r))>0\Delta_{r}(Q_{\kappa}(r))>0 and QκQ_{\kappa} has three simple real roots. To know the localization of the roots it suffices to consider a value of κ\kappa big enough. Then the signs of the ordered coefficients of QκQ_{\kappa} are [+,,,][+,-,-,-] and by Descarte’s rule of signs (see Theorem 6) QrQ_{r} has exactly one positive root. Hence, as in the previous case n1=1.n_{1}=1.

In short, when κ{κ1,κ2}\kappa\not\in\{\kappa_{1},\kappa_{2}\} it holds that (m1,n1)=(3,1).(m_{1},n_{1})=(3,1). Otherwise, some multiple root of N1N_{1} appears but never in (0,1).(0,1).

(iv) We only need to take care of cases with at least five zeros. Let us assume that m1=3m_{1}=3 and n12n_{1}\geq 2 and prove that indeed n1=2.n_{1}=2. As in the previous case, the values 0<r1,r2,r3<10<r_{1},r_{2},r_{3}<1 fix M1.M_{1}. By imposing that 0<s1,s2<10<s_{1},s_{2}<1 and N1(s1)=N1(s2)=0N_{1}(s_{1})=N_{1}(s_{2})=0 we obtain that

κ\displaystyle\kappa =r1r2r3s1s2+s1s2(s1+s2)(r1+r2+r3)s1s2(s1+s2),\displaystyle=\frac{r_{1}r_{2}r_{3}s_{1}s_{2}+s_{1}s_{2}(s_{1}+s_{2})-(r_{1}+r_{2}+r_{3})}{s_{1}s_{2}(s_{1}+s_{2})},
ρ\displaystyle\rho =U(r1,r2,r3,s1,s2)s1s2(s1+s2),\displaystyle=\frac{U(r_{1},r_{2},r_{3},s_{1},s_{2})}{s_{1}s_{2}(s_{1}+s_{2})},
U(r1,r2,r3,s1,s2)\displaystyle U(r_{1},r_{2},r_{3},s_{1},s_{2}) =(r1+r2+r3)(s12+s22+s1s21)\displaystyle=(r_{1}+r_{2}+r_{3})(s_{1}^{2}+s_{2}^{2}+s_{1}s_{2}-1)
(r1r2+r1r3+r2r3+1)s1s2(s1+s2)+r1r2r3s1s2(s1s2+1).\displaystyle\quad-(r_{1}r_{2}+r_{1}r_{3}+r_{2}r_{3}+1)s_{1}s_{2}(s_{1}+s_{2})+r_{1}r_{2}r_{3}s_{1}s_{2}(s_{1}s_{2}+1).

Then

N1(r)=(rs1)(rs2)s1s2(s1+s2)((r1r2r3s1s2r1r2r3)r(s1+s2)(r1+r2+r3))N_{1}(r)=\frac{(r-s_{1})(r-s_{2})}{s_{1}s_{2}(s_{1}+s_{2})}\big{(}(r_{1}r_{2}r_{3}s_{1}s_{2}-r_{1}-r_{2}-r_{3})r-(s_{1}+s_{2})(r_{1}+r_{2}+r_{3})\big{)}

and the third root of N1N_{1} is

r3=(s1+s2)(r1+r2+r3)r1r2r3s1s2r1r2r3<0,r_{3}=\frac{(s_{1}+s_{2})(r_{1}+r_{2}+r_{3})}{r_{1}r_{2}r_{3}s_{1}s_{2}-r_{1}-r_{2}-r_{3}}<0,

because r1r2r3s1s2<r1r_{1}r_{2}r_{3}s_{1}s_{2}<r_{1} and so r1r2r3s1s2r1r2r3<(r2+r3)<0.r_{1}r_{2}r_{3}s_{1}s_{2}-r_{1}-r_{2}-r_{3}<-(r_{2}+r_{3})<0. Hence, since r3(0,1),r_{3}\notin(0,1), n1=2.n_{1}=2.

4. Proof of Theorem C

The next result provides us with the expressions of the Melnikov functions M1M_{1} and N1N_{1} as well as the maximum number of zeros that these functions separately can have in the PWHS case when f(z)=i(z21)/2,f(z)={\rm i}(z^{2}-1)/2, and m3.m\geq 3.

Proposition 9.

Let Rm±R^{\pm}_{m} be a holomorphic polynomial of degree mm in (1) when f(z)=i(z21)/2,f(z)={\rm i}(z^{2}-1)/2, and m3.m\geq 3. Then, the Melnikov functions M1M_{1} and N1N_{1} on -1 and 1 associated to it are:

M1(r)\displaystyle M_{1}(r) =1(r21)m3[n=02(m2)anrn+αr(r21)m3arctanh(r)],\displaystyle=\displaystyle\frac{1}{(r^{2}-1)^{m-3}}\left[\sum_{n=0}^{2(m-2)}a_{n}r^{n}+\alpha r(r^{2}-1)^{m-3}\operatorname{arctanh}(r)\right],
N1(r)\displaystyle N_{1}(r) =1(r21)m3[n=02(m2)bnrn+αr(r21)m3arctanh(r)],\displaystyle=\displaystyle\frac{1}{(r^{2}-1)^{m-3}}\left[\sum_{n=0}^{2(m-2)}b_{n}r^{n}+\alpha r(r^{2}-1)^{m-3}\operatorname{arctanh}(r)\right],

where an,a_{n}, bnb_{n} and α\alpha depend of the coefficients a0,l±a^{\pm}_{0,l} for l={0,,m}.l=\{0,\dots,m\}. Moreover there are several linear relations among the values ana_{n} and the values bnb_{n} as can be seen in the proof.

Proof.

Since the functions Rm±R_{m}^{\pm} are holomorphic, then a¯k,l=0\overline{a}_{k,l}=0 for all 1kl1\leq k\leq l and 0lm0\leq l\leq m. Thus, from the formula (11) we get that

(9) M1±(r)=l=0m[k=0lIk,l±(r)]=l=0mI0,l±(r).M_{1}^{\pm}(r)=\sum_{l=0}^{m}\left[\sum_{k=0}^{l}I_{k,l}^{\pm}(r)\right]=\sum_{l=0}^{m}I_{0,l}^{\pm}(r).

The expressions of I0,l±I_{0,l}^{\pm} when l3l\leq 3 are already detailed in the proof of Proposition 10 in the general situation and can be easily particularized to the holomorphic case. Straightforward calculations allows us to get that for l3,l\geq 3,

I0,l±(r)=Im(a0,l±)(P2(l2)(r)(r21)l3+η(l)rarctanh(r))±(1)lRe(a0,l±)(l1)πr,I^{\pm}_{0,l}(r)=-\operatorname{Im}(a^{\pm}_{0,l})\left(\frac{P_{2(l-2)}(r)}{(r^{2}-1)^{l-3}}+\eta(l)r\operatorname{arctanh}(r)\right)\pm(-1)^{l}\operatorname{Re}(a^{\pm}_{0,l})(l-1)\pi r,

where P2(l2)P_{2(l-2)} is a polynomial function of degree 2(l1),2(l-1), with rational coefficients, and η(l)=2(1l)(1(1)l).\eta(l)=2(1-l)\big{(}1-(-1)^{l}\big{)}. Then,

M1±(r)\displaystyle M_{1}^{\pm}(r) =l=02I0,l±(r)+l=3mI0,l±(r)=l=02Im(a0l±)((1)l+1+r2)±l=0m(1)lRe(a0,l±)(l1)πr\displaystyle=\displaystyle\sum_{l=0}^{2}I_{0,l}^{\pm}(r)+\displaystyle\sum_{l=3}^{m}I_{0,l}^{\pm}(r)=-\displaystyle\sum_{l=0}^{2}\operatorname{Im}(a_{0l}^{\pm})((-1)^{l+1}+r^{2})\pm\displaystyle\sum_{l=0}^{m}(-1)^{l}\operatorname{Re}(a^{\pm}_{0,l})(l-1)\pi r
l=3mIm(a0,l±)(P2(l2)(r)(r21)l3+η(l)rarctanh(r))\displaystyle\quad-\displaystyle\sum_{l=3}^{m}\operatorname{Im}(a^{\pm}_{0,l})\left(\frac{P_{2(l-2)}(r)}{(r^{2}-1)^{l-3}}+\eta(l)r\operatorname{arctanh}(r)\right)
=1(r21)m3(l=02Im(a0l±)((1)l+1+r2)(r21)m3\displaystyle=\dfrac{1}{(r^{2}-1)^{m-3}}\left(-\displaystyle\sum_{l=0}^{2}\operatorname{Im}(a_{0l}^{\pm})((-1)^{l+1}+r^{2})(r^{2}-1)^{m-3}\right.
±l=0m(1)lRe(a0,l±)(l1)πr(r21)m3\displaystyle\quad\qquad\qquad\qquad\pm\displaystyle\sum_{l=0}^{m}(-1)^{l}\operatorname{Re}(a^{\pm}_{0,l})(l-1)\pi r(r^{2}-1)^{m-3}
l=3mIm(a0,l±)(P2(l2)(r)(r21)ml+η(l)r(r21)m3arctanh(r))).\displaystyle\quad\qquad\qquad\qquad\left.-\displaystyle\sum_{l=3}^{m}\operatorname{Im}(a^{\pm}_{0,l})\left(P_{2(l-2)}(r)(r^{2}-1)^{m-l}+\eta(l)r(r^{2}-1)^{m-3}\operatorname{arctanh}(r)\right)\right).

Thus,

M1(r)\displaystyle M_{1}(r) =M1+(r)M1(r)=1(r21)m3[n=02(m2)anrn+αr(r21)m3arctanh(r)],\displaystyle=M_{1}^{+}(r)-M_{1}^{-}(r)=\displaystyle\frac{1}{(r^{2}-1)^{m-3}}\left[\sum_{n=0}^{2(m-2)}a_{n}r^{n}+\alpha r(r^{2}-1)^{m-3}\operatorname{arctanh}(r)\right],

where α=l=3m(Im(a0,l+)Im(a0,l))η(l)\alpha=-\sum_{l=3}^{m}(\operatorname{Im}(a^{+}_{0,l})-\operatorname{Im}(a^{-}_{0,l}))\eta(l) and ana_{n} depends of the coefficients a0,l±a^{\pm}_{0,l} for l={0,,m}l=\{0,\dots,m\}.

To obtain the expression of N1N_{1} of the statement in terms of the coefficients of M1M_{1}, it is enough to use Proposition 12 of Appendix 5. ∎

Proof Theorem C.

(a) In the case m=0m=0 the PWCS is indeed holomorphic and the proof is the same as that given in Theorem B(a).

From Proposition 9, when m{1,2},m\in\{1,2\}, the bifurcation function of PWHS (1) associated to z=1z=-1 and z=1z=1 are given respectively by M1(r)=a+br+cr2M_{1}(r)=a+br+cr^{2} and N1(r)=c+br+ar2=r2(M1(1/r))N_{1}(r)=c+br+ar^{2}=r^{2}\big{(}M_{1}(1/r)\big{)} where a,b,ca,b,c are arbitrary real numbers. Hence if r=rr=r^{*} is root of M1M_{1} then r=1/rr=1/r^{*} is a root of N1N_{1} and vice versa because M1M_{1} and N1N_{1} are reciprocal polynomials. Hence the only possible configurations are [[i,j]][[i,j]] with i+j2i+j\leq 2 and i,j2i,j\leq 2 and all them are realizable.

(b) When m=3,m=3, according Proposition 9, the bifurcation functions of the PWHS (1) associated to z=1z=-1 and z=1z=1 are given respectively by

M1(r)\displaystyle M_{1}(r) =a+br+cr2+αrarctanh(r),\displaystyle=a+br+cr^{2}+\alpha r\operatorname{arctanh}(r),
N1(r)\displaystyle N_{1}(r) =c+(bκ)r+ar2+αrarctanh(r),\displaystyle=c+(b-\kappa)r+ar^{2}+\alpha r\operatorname{arctanh}(r),

where a,b,c,αa,b,c,\alpha and κ\kappa are arbitrary real coefficients, which depend of the real and imaginary parts of a0,l±a^{\pm}_{0,l}, for all l=0,1,2,3l=0,1,2,3. Even more, the maximum number of zeros that these functions separately can have is 3, because it can be seen that the functions [1,r,r2,rarctanh(r)][1,r,r^{2},r\operatorname{arctanh}(r)] form an ECT-system in (0,1).(0,1). Indeed this property also follows from the computations done in next item (c) by taking m=3.m=3. By using the same tools that in the proof of item (b) of Theorem B we obtain that all configurations [[i,j]][[i,j]] with i,j3,i,j\leq 3, and i+j4,i+j\leq 4, are realizable.

(c) By Proposition 9, the first order averaged functions M1M_{1} and N1,N_{1}, multiplied by (r21)m3,(r^{2}-1)^{m-3}, belong to the vectorial space 𝒢\mathcal{G} generated by the ordered set of functions

𝒢=[1,r,r2,,r2(m2),r(r21)m3arctanh(r)].\mathcal{G}=[1,r,r^{2},\ldots,r^{2(m-2)},r(r^{2}-1)^{m-3}\operatorname{arctanh}(r)].

Let us prove that they form an ECT-system on (0,1).(0,1). Their Wronskians, defined in Lemma 3, are Wj(r)=k=0jk!0W_{j}(r)=\prod_{k=0}^{j}k!\neq 0 for all j{0,1,2,,2(m2)}j\in\{0,1,2,\dots,2(m-2)\} and

W2(m2)+1(r)=(1)mξmr(r21)m0,W_{2(m-2)+1}(r)=\frac{(-1)^{m}\xi_{m}r}{(r^{2}-1)^{m}}\neq 0,

at (0,1),(0,1), where ξm\xi_{m} is an increasing sequence of positive real numbers. Then, according to this lemma, 𝒢\mathcal{G} is an ECT-system formed 2m42m-4 elements. Then, by Theorem 4, 2m32m-3 is the maximum number of roots in (0,1)(0,1) for any element of Span(𝒢),\operatorname{Span}(\mathcal{G}), taking into account their multiplicities, as we wanted to prove. Notice that at this point, to prove that there are values of a0,l±a^{\pm}_{0,l} for l={0,,m},l=\{0,\dots,m\}, for which the corresponding piecewise holomorphic system has 2m32m-3 nested limit cycles surrounding z=1z=-1 it would suffice to show that there is a choice of these parameters such that ana_{n}, and α\alpha, n{0,,2(m2)+1}n\in\{0,\dots,2(m-2)+1\} can take arbitrary values. ∎

5. Appendix

This appendix is devoted to find the explicit expressions of the first order averaged functions M1M_{1} and N1N_{1} for PWCS (1) when f(z)=i(z21)/2f(z)={\rm i}(z^{2}-1)/2 when m3.m\leq 3. We will start by doing a detailed study of M1M_{1} around z=1z=-1. The analysis of N1N_{1} around z=1z=1 will be deduced from the previous one.

Proposition 10.

For system (1) when f(z)=i(z21)/2f(z)={\rm i}(z^{2}-1)/2 and m3,m\leq 3, it holds that

M1(r)\displaystyle M_{1}(r) =1r(ar+br2+cr3+dr4+α(r21)2arctanh(r)\displaystyle=\frac{1}{r}\Big{(}ar+br^{2}+cr^{3}+dr^{4}+\alpha(r^{2}-1)^{2}\operatorname{arctanh}(r)
+β(1+r4)arctanh(r)+γr2arctanh(r)),\displaystyle\qquad+\beta(-1+r^{4})\operatorname{arctanh}(r)+\gamma r^{2}\operatorname{arctanh}(r)\Big{)},

where the variables a,b,c,d,α,βa,b,c,d,\alpha,\beta and γ\gamma can take any real value for m=3m=3. When m<3m<3 only appear the following restrictions: γ=0,\gamma=0, when m=2;m=2; γ=β=0\gamma=\beta=0 when m=1;m=1; and γ=β=α=0\gamma=\beta=\alpha=0 and c=ac=-a when m=0.m=0. More specifically, the values of these constants are given in Remark 11.

Proof.

To employ Theorem A to (1) at z=1z=-1 we must first linearize z˙=i(z21)/2\dot{z}={\rm i}(z^{2}-1)/2. It is easy to verify that if

(10) ϕ(z)=1+z1z,ϕ(z)=2(z1)2andϕ1(w)=w1w+1,\phi(z)=\frac{1+z}{1-z},\quad\phi^{\prime}(z)=\frac{2}{(z-1)^{2}}\quad\text{and}\quad\phi^{-1}(w)=\frac{w-1}{w+1},

and by taking w=ϕ(z)w=\phi(z) the differential equation writes as w˙=iw.\dot{w}=iw. See the behaviour of the conformal map ϕ\phi in Figure 1.

\begin{overpic}[scale={0.5}]{conformal_map_simul.pdf} \put(102.0,15.0){$\phi(\Sigma)$} \put(38.0,15.0){$\Sigma$} \put(24.0,0.0){$\mathbb{S}^{1}$} \put(74.0,-3.0){$\phi(\mathbb{S}^{1})$} \put(49.0,27.0){$\phi$} \end{overpic}
Figure 1. Conformal map ϕ(z)=1+z1z\phi(z)=\frac{1+z}{1-z}.

In addition, from (10), we have that

ϕ(ϕ1(w))=12(w+1)2,ϕ1(w)¯=w¯1w¯+1,\phi^{\prime}\left(\phi^{-1}(w)\right)=\frac{1}{2}(w+1)^{2},\qquad\overline{\phi^{-1}(w)}=\frac{\overline{w}-1}{\overline{w}+1},

and ϕ(Σ)=Σ\phi(\Sigma)=\Sigma and ϕ(𝕊1)={(0,y):y}\phi(\mathbb{S}^{1})=\{(0,y):y\in\mathbb{R}\}.

From Theorem A with R±(z,z¯)=Rm±(z,z¯)R^{\pm}(z,\overline{z})=R_{m}^{\pm}(z,\overline{z}) given in (5) and f(z)=i(z21)/2f(z)={\rm i}(z^{2}-1)/2 we get that

(11) M1(r)=M1+(r)M1(r),whereM1±(r)=l=0m(k=0lIk,l±(r)),M_{1}(r)=M_{1}^{+}(r)-M_{1}^{-}(r),\quad\mbox{where}\quad M_{1}^{\pm}(r)=\sum_{l=0}^{m}\Big{(}\sum_{k=0}^{l}I_{k,l}^{\pm}(r)\Big{)},

and

Ik,l±(r)=Im(ak,l±0±πϕ(ϕ1(reiθ))¯(ϕ1(reiθ))k(ϕ1(reiθ)¯)lkieiθ𝑑θ).I^{\pm}_{k,l}(r)=-\operatorname{Im}\left(a_{k,l}^{\pm}\displaystyle\int_{0}^{\pm\pi}\overline{\phi^{\prime}(\phi^{-1}(re^{{\rm i}\theta}))}\left(\phi^{-1}(re^{{\rm i}\theta})\right)^{k}\left(\overline{\phi^{-1}(re^{{\rm i}\theta})}\right)^{l-k}{\rm i}e^{{\rm i}\theta}d\theta\right).

Thus, using (11) we get

Ik,l±(r)\displaystyle I^{\pm}_{k,l}(r) =Im(ak,l±0±π12(reiθ+1)2(reiθ1reiθ+1)k(reiθ1reiθ+1)lkieiθ𝑑θ)\displaystyle=-\operatorname{Im}\left(a_{k,l}^{\pm}\displaystyle\int_{0}^{\pm\pi}\frac{1}{2}(re^{-{\rm i}\theta}+1)^{2}\left(\frac{re^{{\rm i}\theta}-1}{re^{{\rm i}\theta}+1}\right)^{k}\left(\frac{re^{-{\rm i}\theta}-1}{re^{-{\rm i}\theta}+1}\right)^{l-k}{\rm i}e^{-{\rm i}\theta}d\theta\right)\vspace{.3cm}
=12Im(ak,l±0±π(reiθ+1)kl+2(reiθ1)k(reiθ1)lkieiθ(reiθ+1)k𝑑θ).\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{k,l}^{\pm}\displaystyle\int_{0}^{\pm\pi}\dfrac{(re^{-{\rm i}\theta}+1)^{k-l+2}(re^{{\rm i}\theta}-1)^{k}(re^{-{\rm i}\theta}-1)^{l-k}{\rm i}e^{{\rm i}\theta}}{(re^{{\rm i}\theta}+1)^{k}}d\theta\right).

To arrive to the final expression of M1M_{1} we have to compute each of the functions Ik,l±.I^{\pm}_{k,l}. When l=0,l=0,

I0,0±(r)\displaystyle I^{\pm}_{0,0}(r) =12Im(a0,0±0±π(reiθ+1)2ieiθ𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{0,0}^{\pm}\displaystyle\int_{0}^{\pm\pi}(re^{-{\rm i}\theta}+1)^{2}{\rm i}e^{{\rm i}\theta}d\theta\right)\vspace{0.3cm}
=Im(a0,0±)(r21)πRe(a0,0±)r.\displaystyle=-\operatorname{Im}\left(a_{0,0}^{\pm}\right)(r^{2}-1)\mp\pi\operatorname{Re}\left(a_{0,0}^{\pm}\right)r.

For l=1l=1 we obtain,

I0,1±(r)\displaystyle I^{\pm}_{0,1}(r) =12Im(a0,1±0±π(reiθ+1)(reiθ1)ieiθ𝑑θ)=Im(a0,1±)(1+r2),\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{0,1}^{\pm}\displaystyle\int_{0}^{\pm\pi}(re^{-{\rm i}\theta}+1)(re^{-{\rm i}\theta}-1){\rm i}e^{{\rm i}\theta}d\theta\right)=-\operatorname{Im}\left(a_{0,1}^{\pm}\right)(1+r^{2}),\vspace{0.3cm}
I1,1±(r)\displaystyle I^{\pm}_{1,1}(r) =12Im(a1,1±0±π(reiθ+1)2(reiθ1)ieiθreiθ+1𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{1,1}^{\pm}\displaystyle\int_{0}^{\pm\pi}\frac{(re^{-{\rm i}\theta}+1)^{2}(re^{{\rm i}\theta}-1){\rm i}e^{{\rm i}\theta}}{re^{{\rm i}\theta}+1}d\theta\right)\vspace{0.3cm}
=Im(a1,1±)r(r(1+r2)+2(r21)2arctanh(r))πRe(a1,1±)r(r21).\displaystyle=-\dfrac{\operatorname{Im}\left(a_{1,1}^{\pm}\right)}{r}\Big{(}-r(1+r^{2})+2(r^{2}-1)^{2}\operatorname{arctanh}(r)\Big{)}\mp\pi\operatorname{Re}\left(a_{1,1}^{\pm}\right)r(r^{2}-1).

When l=2l=2 we arrive to

I0,2±(r)\displaystyle I^{\pm}_{0,2}(r) =12Im(a0,2±0±π(reiθ1)2ieiθ𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{0,2}^{\pm}\displaystyle\int_{0}^{\pm\pi}(re^{-{\rm i}\theta}-1)^{2}{\rm i}e^{{\rm i}\theta}d\theta\right)\vspace{0.3cm}
=Im(a0,2±)(r21)±πRe(a0,2±)r,\displaystyle=-\operatorname{Im}\left(a_{0,2}^{\pm}\right)(r^{2}-1)\pm\pi\operatorname{Re}\left(a_{0,2}^{\pm}\right)r,\vspace{0.3cm}
I1,2±(r)\displaystyle I^{\pm}_{1,2}(r) =12Im(a1,2±0±π(reiθ+1)(reiθ1)(reiθ1)ieiθreiθ+1𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{1,2}^{\pm}\displaystyle\int_{0}^{\pm\pi}\frac{(re^{-{\rm i}\theta}+1)(re^{{\rm i}\theta}-1)(re^{-{\rm i}\theta}-1){\rm i}e^{{\rm i}\theta}}{re^{{\rm i}\theta}+1}d\theta\right)\vspace{0.3cm}
=Im(a1,2±)r(rr3+2(1+r4)arctanh(r))πRe(a1,2±)r3,\displaystyle=-\dfrac{\operatorname{Im}\left(a_{1,2}^{\pm}\right)}{r}\Big{(}r-r^{3}+2(-1+r^{4})\operatorname{arctanh}(r)\Big{)}\mp\pi\operatorname{Re}\left(a_{1,2}^{\pm}\right)r^{3},
I2,2±(r)\displaystyle I^{\pm}_{2,2}(r) =12Im(a2,2±0±π(reiθ+1)2(reiθ1)2ieiθ(reiθ+1)2𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{2,2}^{\pm}\displaystyle\int_{0}^{\pm\pi}\frac{(re^{-{\rm i}\theta}+1)^{2}(re^{{\rm i}\theta}-1)^{2}{\rm i}e^{{\rm i}\theta}}{(re^{{\rm i}\theta}+1)^{2}}d\theta\right)\vspace{0.3cm}
=Im(a2,2±)r(5r(r21)4(1+r4)arctanh(r))πRe(a2,2±)r(12r2).\displaystyle=-\dfrac{\operatorname{Im}\left(a_{2,2}^{\pm}\right)}{r}\Big{(}5r(r^{2}-1)-4(-1+r^{4})\operatorname{arctanh}(r)\Big{)}\mp\pi\operatorname{Re}\left(a_{2,2}^{\pm}\right)r(1-2r^{2}).

Finally, for l=3,l=3,

I0,3±(r)\displaystyle I^{\pm}_{0,3}(r) =12Im(a0,3±0±π(reiθ1)3reiθ+1ieiθ𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{0,3}^{\pm}\displaystyle\int_{0}^{\pm\pi}\frac{(re^{-{\rm i}\theta}-1)^{3}}{re^{-{\rm i}\theta}+1}{\rm i}e^{{\rm i}\theta}d\theta\right)\vspace{0.3cm}
=Im(a0,3±)((1+r2)8rarctanh(r))2πRe(a0,3±)r,\displaystyle=-\operatorname{Im}(a_{0,3}^{\pm})\Big{(}(1+r^{2})-8r\operatorname{arctanh}(r)\Big{)}\mp 2\pi\operatorname{Re}(a_{0,3}^{\pm})r,\vspace{0.3cm}
I1,3±(r)\displaystyle I^{\pm}_{1,3}(r) =12Im(a1,3±0±π(reiθ1)(reiθ1)2ieiθreiθ+1𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{1,3}^{\pm}\displaystyle\int_{0}^{\pm\pi}\frac{(re^{{\rm i}\theta}-1)(re^{-{\rm i}\theta}-1)^{2}{\rm i}e^{{\rm i}\theta}}{re^{{\rm i}\theta}+1}d\theta\right)\vspace{0.3cm}
=Im(a1,3±)r(r(1+r2)+2(1+r2)2arctanh(r))πRe(a1,3±)r2(1+r2),\displaystyle=-\dfrac{\operatorname{Im}\left(a_{1,3}^{\pm}\right)}{r}\Big{(}-r(1+r^{2})+2(1+r^{2})^{2}\operatorname{arctanh}(r)\Big{)}\mp\pi\operatorname{Re}\left(a_{1,3}^{\pm}\right)r^{2}(1+r^{2}),\vspace{0.3cm}
I2,3±(r)\displaystyle I^{\pm}_{2,3}(r) =12Im(a2,3±0±π(reiθ+1)(reiθ1)2(reiθ1)ieiθ(reiθ+1)2𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{2,3}^{\pm}\displaystyle\int_{0}^{\pm\pi}\frac{(re^{-{\rm i}\theta}+1)(re^{{\rm i}\theta}-1)^{2}(re^{-{\rm i}\theta}-1){\rm i}e^{{\rm i}\theta}}{(re^{{\rm i}\theta}+1)^{2}}d\theta\right)\vspace{0.3cm}
=Im(a2,3±)r(5r(1+r2)4(1+r4)arctanh(r))±2πRe(a2,3±)r4,\displaystyle=-\dfrac{\operatorname{Im}\left(a_{2,3}^{\pm}\right)}{r}\Big{(}5r(1+r^{2})-4(1+r^{4})\operatorname{arctanh}(r)\Big{)}\pm 2\pi\operatorname{Re}\left(a_{2,3}^{\pm}\right)r^{4},
I3,3±(r)\displaystyle I^{\pm}_{3,3}(r) =12Im(a3,3±0±π(reiθ+1)2(reiθ1)3ieiθ(reiθ+1)3𝑑θ)\displaystyle=-\dfrac{1}{2}\operatorname{Im}\left(a_{3,3}^{\pm}\displaystyle\int_{0}^{\pm\pi}\frac{(re^{-{\rm i}\theta}+1)^{2}(re^{{\rm i}\theta}-1)^{3}{\rm i}e^{{\rm i}\theta}}{(re^{{\rm i}\theta}+1)^{3}}d\theta\right)\vspace{0.3cm}
=Im(a3,3±)r(5r(1+r2)+(64r2+6r4)arctanh(r))πRe(a3,3±)r2(1+3r2).\displaystyle=-\dfrac{\operatorname{Im}\left(a_{3,3}^{\pm}\right)}{r}\Big{(}-5r(1+r^{2})+(6-4r^{2}+6r^{4})\operatorname{arctanh}(r)\Big{)}\mp\pi\operatorname{Re}\left(a_{3,3}^{\pm}\right)r^{2}(-1+3r^{2}).

By adding all the above expressions we obtain M1±M_{1}^{\pm} and then the final expression of M1.M_{1}.

Remark 11.

Values of the parameters appearing in the expression of M1M_{1} given in Proposition 10 when m3.m\leq 3.

a\displaystyle a =Im(a0,0+)Im(a0,0)Im(a0,1+)+Im(a0,1)+Im(a11+)Im(a11)+Im(a0,2+)Im(a0,2)\displaystyle=\operatorname{Im}(a_{0,0}^{+})-\operatorname{Im}(a_{0,0}^{-})-\operatorname{Im}(a_{0,1}^{+})+\operatorname{Im}(a_{0,1}^{-})+\operatorname{Im}(a_{11}^{+})-\operatorname{Im}(a_{11}^{-})+\operatorname{Im}(a_{0,2}^{+})-\operatorname{Im}(a_{0,2}^{-})
Im(a1,2+)+Im(a1,2)+5Im(a2,2+)5Im(a2,2)Im(a0,3+)+Im(a0,3)+Im(a1,3+)\displaystyle\quad-\operatorname{Im}(a_{1,2}^{+})+\operatorname{Im}(a_{1,2}^{-})+5\operatorname{Im}(a_{2,2}^{+})-5\operatorname{Im}(a_{2,2}^{-})-\operatorname{Im}(a_{0,3}^{+})+\operatorname{Im}(a_{0,3}^{-})+\operatorname{Im}(a_{1,3}^{+})
Im(a1,3)5Im(a2,3+)+5Im(a2,3)+5Im(a3,3+)5Im(a3,3),\displaystyle\quad-\operatorname{Im}(a_{1,3}^{-})-5\operatorname{Im}(a_{2,3}^{+})+5\operatorname{Im}(a_{2,3}^{-})+5\operatorname{Im}(a_{3,3}^{+})-5\operatorname{Im}(a_{3,3}^{-}),
b\displaystyle b =πRe(a0,0+)πRe(a0,0)+πRe(a11+)+πRe(a11)+πRe(a0,2)+πRe(a0,2+)πRe(a2,2+)\displaystyle=-\pi\operatorname{Re}(a_{0,0}^{+})-\pi\operatorname{Re}(a_{0,0}^{-})+\pi\operatorname{Re}(a_{11}^{+})+\pi\operatorname{Re}(a_{11}^{-})+\pi\operatorname{Re}(a_{0,2}^{-})+\pi\operatorname{Re}(a_{0,2}^{+})-\pi\operatorname{Re}(a_{2,2}^{+})
πRe(a2,2)2πRe(a0,3)2πRe(a0,3+)πRe(a1,3+)πRe(a1,3)\displaystyle\quad-\pi\operatorname{Re}(a_{2,2}^{-})-2\pi\operatorname{Re}(a_{0,3}^{-})-2\pi\operatorname{Re}(a_{0,3}^{+})-\pi\operatorname{Re}(a_{1,3}^{+})-\pi\operatorname{Re}(a_{1,3}^{-})
+πRe(a3,3+)+πRe(a3,3),\displaystyle\quad+\pi\operatorname{Re}(a_{3,3}^{+})+\pi\operatorname{Re}(a_{3,3}^{-}),
c\displaystyle c =Im(a0,0+)+Im(a0,0)Im(a0,1+)+Im(a0,1)+Im(a11+)Im(a11)Im(a0,2+)\displaystyle=-\operatorname{Im}(a_{0,0}^{+})+\operatorname{Im}(a_{0,0}^{-})-\operatorname{Im}(a_{0,1}^{+})+\operatorname{Im}(a_{0,1}^{-})+\operatorname{Im}(a_{11}^{+})-\operatorname{Im}(a_{11}^{-})-\operatorname{Im}(a_{0,2}^{+})
+Im(a0,2)+Im(a1,2+)Im(a1,2)5Im(a2,2+)+5Im(a2,2)+Im(a1,3+)Im(a1,3)\displaystyle\quad+\operatorname{Im}(a_{0,2}^{-})+\operatorname{Im}(a_{1,2}^{+})-\operatorname{Im}(a_{1,2}^{-})-5\operatorname{Im}(a_{2,2}^{+})+5\operatorname{Im}(a_{2,2}^{-})+\operatorname{Im}(a_{1,3}^{+})-\operatorname{Im}(a_{1,3}^{-})
5Im(a2,3+)+5Im(a2,3)+5Im(a3,3+)5Im(a3,3),\displaystyle\quad-5\operatorname{Im}(a_{2,3}^{+})+5\operatorname{Im}(a_{2,3}^{-})+5\operatorname{Im}(a_{3,3}^{+})-5\operatorname{Im}(a_{3,3}^{-}),
d\displaystyle d =πRe(a11+)πRe(a11)πRe(a1,2+)πRe(a1,2)+2πRe(a2,2+)+2πRe(a2,2)\displaystyle=-\pi\operatorname{Re}(a_{11}^{+})-\pi\operatorname{Re}(a_{11}^{-})-\pi\operatorname{Re}(a_{1,2}^{+})-\pi\operatorname{Re}(a_{1,2}^{-})+2\pi\operatorname{Re}(a_{2,2}^{+})+2\pi\operatorname{Re}(a_{2,2}^{-})
πRe(a1,3+)πRe(a1,3)+2πRe(a2,3+)+2πRe(a2,3)3πRe(a3,3+)3πRe(a3,3),\displaystyle\quad-\pi\operatorname{Re}(a_{1,3}^{+})-\pi\operatorname{Re}(a_{1,3}^{-})+2\pi\operatorname{Re}(a_{2,3}^{+})+2\pi\operatorname{Re}(a_{2,3}^{-})-3\pi\operatorname{Re}(a_{3,3}^{+})-3\pi\operatorname{Re}(a_{3,3}^{-}),
α\displaystyle\alpha =2Im(a11+)+2Im(a11)2Im(a1,3+)+2Im(a1,3)+4Im(a2,3+)4Im(a2,3)\displaystyle=-2\operatorname{Im}(a_{11}^{+})+2\operatorname{Im}(a_{11}^{-})-2\operatorname{Im}(a_{1,3}^{+})+2\operatorname{Im}(a_{1,3}^{-})+4\operatorname{Im}(a_{2,3}^{+})-4\operatorname{Im}(a_{2,3}^{-})
6Im(a3,3+)+6Im(a3,3),\displaystyle\quad-6\operatorname{Im}(a_{3,3}^{+})+6\operatorname{Im}(a_{3,3}^{-}),
β\displaystyle\beta =2Im(a1,2+)+2Im(a1,2)+4Im(a2,2+)4Im(a2,2),\displaystyle=-2\operatorname{Im}(a_{1,2}^{+})+2\operatorname{Im}(a_{1,2}^{-})+4\operatorname{Im}(a_{2,2}^{+})-4\operatorname{Im}(a_{2,2}^{-}),
γ\displaystyle\gamma =Im(a0,3+)+Im(a0,3)+Im(a1,3+)Im(a1,3)Im(a2,3+)+Im(a2,3)+Im(a3,3+)Im(a3,3).\displaystyle=-\operatorname{Im}(a_{0,3}^{+})+\operatorname{Im}(a_{0,3}^{-})+\operatorname{Im}(a_{1,3}^{+})-\operatorname{Im}(a_{1,3}^{-})-\operatorname{Im}(a_{2,3}^{+})+\operatorname{Im}(a_{2,3}^{-})+\operatorname{Im}(a_{3,3}^{+})-\operatorname{Im}(a_{3,3}^{-}).

In what follows, we establish a connection between the coefficients of the bifurcation functions M1M_{1} and N1N_{1} of -1 and 1, respectively. This relation allow us to study the simultaneous zeros of these functions.

Proposition 12.

Let M1(r)=M1(r;ak,l±)M_{1}(r)=M_{1}(r;a^{\pm}_{k,l}) and N1(r)=N1(r;ak,l±)N_{1}(r)=N_{1}(r;a^{\pm}_{k,l}) be the bifurcation functions of PWCS (1) with f(z)=i(z21)/2f(z)={\rm i}(z^{2}-1)/2 associated to z=1z=-1 and z=1,z=1, respectively. Then

N1(r)=N1(r;ak,l±)=M1(r;(1)lak,l),N_{1}(r)=N_{1}(r;a^{\pm}_{k,l})=M_{1}(r;(-1)^{l}a^{\mp}_{k,l}),

that is, the expression of N1(r)N_{1}(r) coincides with the expression of M1(r)M_{1}(r) given in Proposition 10 and Remark 11 where each ak,l±a_{k,l}^{\pm} is changed by (1)lak,l,(-1)^{l}a_{k,l}^{\mp}, for all 0kl0\leq k\leq l and 0lm.0\leq l\leq m.

Proof.

Using the change of variables and time w(t)=z(t),w(t)=-z(-t), we transform PWCS (1) with f(z)=i(z21)/2f(z)={\rm i}(z^{2}-1)/2 into

(12) w˙=i(w21)/2+{ϵRm(w,w¯), when Im(w)>0,ϵRm+(w,w¯), when Im(w)<0.\dot{w}={\rm i}(w^{2}-1)/2+\left\{\begin{array}[]{l}\epsilon R_{m}^{-}(-w,-\overline{w}),\text{ when }\operatorname{Im}(w)>0,\\[5.0pt] \epsilon R_{m}^{+}(-w,-\overline{w}),\text{ when }\operatorname{Im}(w)<0.\end{array}\right.

Hence, the zeros of the bifurcation function N1(r)N_{1}(r) of PWCS (1) are the zeros of the bifurcation function associated to z=1z=-1 of (12). Then

(13) Rm(w,w¯)=l=0mk=0la¯k,l(w)lk(w¯)k=l=0mk=0l(1)la¯k,lwlkw¯k,R_{m}^{\mp}(-w,-\overline{w})=\sum_{l=0}^{m}\sum_{k=0}^{l}\overline{a}^{\mp}_{k,l}(-w)^{l-k}(-\overline{w})^{k}=\sum_{l=0}^{m}\sum_{k=0}^{l}(-1)^{l}\overline{a}^{\mp}_{k,l}w^{l-k}\overline{w}^{k},

as we wanted to prove. ∎

From the above proposition we obtain the expression of the function N1N_{1} in Proposition 7 and also next remark.

Remark 13.

Values of the parameters appearing in the expression of N1N_{1} given in Proposition 7 when m3.m\leq 3.

κ\displaystyle\kappa =2π(2Re(a2,2)+2Re(a2,2+)Re(a1,2)Re(a1,2+)),\displaystyle=2\pi\big{(}2\operatorname{Re}(a_{2,2}^{-})+2\operatorname{Re}(a_{2,2}^{+})-\operatorname{Re}(a_{1,2}^{-})-\operatorname{Re}(a_{1,2}^{+})\big{)},
ρ\displaystyle\rho =4π(Re(a0,3+)+Re(a0,3)+Re(a1,3+)+Re(a1,3)Re(a2,3+)Re(a2,3)\displaystyle=4\pi\big{(}\operatorname{Re}(a_{0,3}^{+})+\operatorname{Re}(a_{0,3}^{-})+\operatorname{Re}(a_{1,3}^{+})+\operatorname{Re}(a_{1,3}^{-})-\operatorname{Re}(a_{2,3}^{+})-\operatorname{Re}(a_{2,3}^{-})
+Re(a3,3+)+Re(a3,3)).\displaystyle\quad\quad\quad+\operatorname{Re}(a_{3,3}^{+})+\operatorname{Re}(a_{3,3}^{-})\big{)}.

6. Acknowledgements

This article was possible thanks to the scholarship granted from the Brazilian Federal Agency for Support and Evaluation of Graduate Education (CAPES), in the scope of the Program CAPES-Print, process number 88887.310463/2018-00, International Cooperation Project number 88881.310741/2018-01.

Armengol Gasull is partially supported supported by the Ministry of Science and Innovation–State Research Agency of the Spanish Government through grants PID2022-136613NB-I00 and by the grant 2021-SGR-00113 from AGAUR of Generalitat de Catalunya.

Gabriel Alexis Rondón Vielma is supported by São Paulo Research Foundation (FAPESP) grants 2020/06708-9 and 2022/12123-9.

Paulo Ricardo da Silva is also partially supported by São Paulo Research Foundation (FAPESP) grant 2019/10269-3 and 2023/02959-5, CNPq grant 302154/2022-1 and ANR-23-CE40-0028.

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