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thanks: Work performed under the auspices of the Gruppo Nazionale per l’Analisi Matematica, la Probabilità e le loro Applicazioni (GNAMPA) of the Istituto Nazionale di Alta Matematica (INdAM) and supported by the project PRID SiDiA – Sistemi Dinamici e Applicazioni of the DMIF, University of Udine. The first author is supported by INdAM–GNAMPA project “Problemi ai limiti per l’equazione della curvatura media prescritta”. This work was preliminarily announced on the occasion of the workshop “Recent Advances on Dynamical Equations” in honor of Professor Luisa Malaguti, held in Ancona, October 24–25, 2019.
Preprint – December 2020

Bound sets for a class of ϕ\phi-Laplacian operators

Guglielmo Feltrin Department of Mathematics, Computer Science and Physics, University of Udine
Via delle Scienze 206, 33100 Udine, Italy
[email protected]
   Fabio Zanolin Department of Mathematics, Computer Science and Physics, University of Udine
Via delle Scienze 206, 33100 Udine, Italy
[email protected]
Abstract.

We provide an extension of the Hartman–Knobloch theorem for periodic solutions of vector differential systems to a general class of ϕ\phi-Laplacian differential operators. Our main tool is a variant of the Manásevich–Mawhin continuation theorem developed for this class of operator equations, together with the theory of bound sets. Our results concern the case of convex bound sets for which we show some new connections using a characterisation of sublevel sets due to Krantz and Parks. We also extend to the ϕ\phi-Laplacian vector case a classical theorem of Reissig for scalar periodically perturbed Liénard equations.

Key words and phrases:
Periodic solutions, continuation theorems, ϕ\phi-Laplacian operators, bound sets, Nagumo–Hartman condition, Liénard and Rayleigh systems.
1991 Mathematics Subject Classification:
34B15, 34C25, 47H11.

1. Introduction

In the present paper, we study the existence of periodic solutions to differential systems involving a ϕ\phi-Laplacian differential operator, with the aim of extending the classical theorem of Hartman–Knobloch for the differential system

x′′=f(t,x,x).x^{\prime\prime}=f(t,x,x^{\prime}). (1.1)

In his original work [18] (see also [19, ch. XII]), Hartman considered the two-point boundary value problem (BVP) associated with (1.1), assuming a (at most quadratic) growth condition of f(t,x,y)\|f(t,x,y)\| in yy (the so-called “Bernstein–Nagumo–Hartman condition”, cf. [9, 32]) and the hypothesis that the vector field is “repulsive” according to

f(t,x,y),x+y20,\displaystyle\langle f(t,x,y),x\rangle+\|y\|^{2}\geq 0, for every xnx\in\mathbb{R}^{n} with x=R\|x\|=R (1.2)
and yny\in\mathbb{R}^{n} such that x,y=0\langle x,y\rangle=0.

In the special case of a Newtonian force without friction f=f(t,x)f=f(t,x), condition (1.2) reads as

f(t,x),x0,for every xn with x=R.\langle f(t,x),x\rangle\geq 0,\quad\text{for every $x\in\mathbb{R}^{n}$ with $\|x\|=R$.} (1.3)

Under the above assumptions, one find that the BVP has at least one solution in the closed ball B[0,R]={xn:xR}B[0,R]=\{x\in\mathbb{R}^{n}\colon\|x\|\leq R\} with center 0 and radius RR (or in the open one B(0,R)B(0,R), if the inequalities in (1.2) or (1.3) are strict). The result was then obtained in the context of the periodic BVP by Knobloch in [22], under the same geometric conditions on the vector field.

In the Seventies, from these results a line of research initiated and received a great interest, as shown by a series of works [4, 5, 29, 49]. In particular, assumptions (1.2) and (1.3), referring to the boundary of a ball, were extended to a broader families of domains. With this respect, very general conditions were proposed by Mawhin [29] and Bebernes [4], by introducing the concept of “bounding function”, namely a Lyapunov-like function V:nV\colon\mathbb{R}^{n}\to\mathbb{R} of class 𝒞2\mathcal{C}^{2} which plays the same role as x2/2\|x\|^{2}/2, so that (1.2) can be written as

f(t,x,y),V(x)+V′′(x)y,y0,\displaystyle\langle f(t,x,y),V^{\prime}(x)\rangle+\langle V^{\prime\prime}(x)y,y\rangle\geq 0, for every xnx\in\mathbb{R}^{n} with V(x)=cV(x)=c (1.4)
and yny\in\mathbb{R}^{n} such that V(x),y=0\langle V^{\prime}(x),y\rangle=0,

where we have denoted with VV^{\prime} the gradient of VV and by V′′V^{\prime\prime} its Hessian matrix. In this case, the open ball B(0,R)B(0,R) is replaced by the sublevel set [V<c]:={xn:V(x)<c}[V<c]:=\{x\in\mathbb{R}^{n}\colon V(x)<c\}.

Assumptions of the form (1.2) or (1.4) (typically with the strict inequality) imply that there are no solutions “tangent from the interior” to the boundary of a given open bounded set GnG\subseteq\mathbb{R}^{n} (i.e., GG an open ball or a sublevel set in the above examples), namely the vector field satisfies Ważewski-type conditions at the boundary (see [20], as well as [51] and the references therein). This in turn lead to the concept of bound set introduced in [14], which has found many relevant applications to first and second order differential systems. Extensions of these methods have been obtained by several authors in various directions such as Floquet BVPs, Carathéodory conditions, non-smooth bounding functions and non-smooth boundaries, differential inclusions, extensions to Banach spaces, PDEs, integro-differential equations, differential equations with impulses, nonlocal BVPs. A constantly growing literature in this area shows the persistent influence of the bound sets and bounding functions approach; see [2, 3, 6, 7, 37, 38, 39, 44] and the references therein.

The aim of our work is to propose further applications of the bound set technique to the study of the periodic BVP associated with the second-order ϕ\phi-Laplacian differential operator

(ϕ(x))=f(t,x,x),(\phi(x^{\prime}))^{\prime}=f(t,x,x^{\prime}), (1.5)

where ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} is a homeomorphism such that ϕ(0)=0\phi(0)=0, and f:×n×nnf\colon\mathbb{R}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\to\mathbb{R}^{n} is a continuous vector field which is TT-periodic in the tt-variable. The study of nonlinear scalar differential equations with a pp-Laplacian operator, or more generally of the form

div𝒜(ξ,u,uξ)=(ξ,u,uξ),\mathrm{div}\mathcal{A}(\xi,u,u_{\xi})=\mathcal{B}(\xi,u,u_{\xi}),

for ξ\xi in a domain of N\mathbb{R}^{N}, is a classical topic in the area of PDEs, see [50] (cf. also [46] and the references therein). In the setting of ODEs differential systems, a systematic investigation of the periodic problem was initiated by Manásevich and Mawhin in [26]. It is noteworthy that the analysis of systems has an independent interest also from the point of view of the analysis of differential equations in the complex plane or in the complex space n\mathbb{C}^{n} (cf. [35]).

Our contribution pursues a line of research started by Mawhin [34] and by Mawhin and Ureña [41], dealing with the pp-Laplacian operator ϕ(s)=ϕp(s):=|s|p2s\phi(s)=\phi_{p}(s):=|s|^{p-2}s with p>1p>1, with the aim of further extending Hartman–Knobloch theorem to a broader class of nonlinear differential operators. A partial result in this direction was obtained in [10, Theorem 5.2] when the domain is a ball. Here, we extend also this result to more general domains.

The plan of the paper is as follows. In Section 2, we introduce the main theoretical tools for the solvability of the periodic BVP associated with (1.5), which are based on the Manásevich–Mawhin continuation theorems [26] in the versions stated in [10] for a general homeomorphism ϕ\phi. This leads to Theorem 2.3 and Theorem 2.4, after the introduction of the concept of bound sets and Nagumo–Hartman condition for equation (1.5). As a next step, following [14, 29, 30, 31], we introduce a family of bounding functions and obtain the corresponding Theorem 2.5 and Theorem 2.6. Section 3 is devoted to the application of these latter results. In particular, for a set G:=[V<0]G:=[V<0] and the equation

(ϕ(x))=f(t,x),(\phi(x^{\prime}))^{\prime}=f(t,x),

we find the existence of a TT-periodic solution with values in G¯\overline{G}, provided that

  • (i)(i)

    V(x)0V^{\prime}(x)\neq 0, for every x[V=0]x\in[V=0];

  • (ii)(ii)

    V′′(x)y,y0\langle V^{\prime\prime}(x)y,y\rangle\geq 0, for every xGx\in\partial G and yny\in\mathbb{R}^{n} with V(x),y=0\langle V^{\prime}(x),y\rangle=0;

  • (iii)(iii)

    V(x),f(t,x)0\langle V^{\prime}(x),f(t,x)\rangle\geq 0, for every t[0,T]t\in\mathopen{[}0,T\mathclose{]} and xGx\in\partial G.

The class of ϕ\phi-Laplacians for which the above result holds require that ϕ(ξ)=A(ξ)ξ\phi(\xi)=A(\xi)\xi, ξn\xi\in\mathbb{R}^{n}, with AA a positive scalar function. As shown in [10], maps of this form are not necessarily monotone and include all the pp-Laplacian vector differential operators, thus extending Hartman–Knobloch theorem for frictionless vector fields along the line of [34]. The case of a vector field depending on xx^{\prime} is studied in Section 3.2 extending [29, Corollary 6.3] for vector Rayleigh systems to the ϕ\phi-Laplacians. Another result for vector ϕ\phi-Laplacian Liénard systems is given in Section 3.3 extending [45, Theorem 3.3] as well as a classical theorem of Reissig [47, Theorem 3].

We observe that conditions (i)(i) and (ii)(ii) appear explicitly or implicitly in some classical results for equation (1.1), see for instance [4, 17, 29]. Indeed, consider condition (1.4) already assumed in the above quoted papers in the special case when f=f(t,x)f=f(t,x). From

V′′(x)y,yV(x),f(t,x)M,\langle V^{\prime\prime}(x)y,y\rangle\geq-\langle V^{\prime}(x),f(t,x)\rangle\geq-M, (1.6)

(with M:=sup{V(x),f(t,x):t[0,T],xG¯}M:=\sup\{\langle V^{\prime}(x),f(t,x)\rangle\colon t\in\mathopen{[}0,T\mathclose{]},x\in\overline{G}\}), we obtain that the quadratic form yV′′(x)y,yy\mapsto\langle V^{\prime\prime}(x)y,y\rangle is bounded from below and hence positive semi-definite, so that (ii)(ii) holds. Notice also that (iii)(iii) follows reading (1.4) for y=0y=0. Conditions (i)(i) and (ii)(ii) hint some kind of convexity properties for the sublevel sets of VV, however, at the best of our knowledge, there are no explicit proofs relating these conditions with the convexity of the set [V0][V\leq 0]. In general, the convexity of the sublevel set is not guaranteed by the sole conditions (i)(i) and (ii)(ii), as it could be shown by an example of a sublevel set made by the union of two disjoint balls. On the other hand, if we assume that [V0][V\leq 0] is connected, then the convexity is achieved thanks to an analysis due to Krantz and Parks in [24] (see also [23]). For the reader’s convenience, we propose a different proof of this result in Appendix A. We exploit this characterization of the convexity (see Lemma 3.1) in the proof of Corollary 3.2. Clearly, for a general ff depending on y=xy=x^{\prime}, or if we have some information on the a priori bounds on xx^{\prime} (say xK\|x^{\prime}\|_{\infty}\leq K), we are not allowed to conclude with the positive semi-definiteness of V′′(x)V^{\prime\prime}(x) from (1.6) because only the yy with yK\|y\|\leq K will be involved in (1.6). An investigation of non-convex bound sets was proposed in [1] (see also [58] for some remarks about this problem).

Throughout the paper, we denote by \|\cdot\| the Euclidean norm in n\mathbb{R}^{n} and by ,\langle\cdot,\cdot\rangle the associated standard inner product.

2. Main results

We consider the vector differential equation

(ϕ(x))=f(t,x,x),(\phi(x^{\prime}))^{\prime}=f(t,x,x^{\prime}), (2.1)

where ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} is a homeomorphism such that ϕ(0)=0\phi(0)=0, and f:×n×nnf\colon\mathbb{R}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\to\mathbb{R}^{n} is a continuous vector field which is TT-periodic in the tt-variable.

We study the problem of the existence of TT-periodic solutions for (2.1), which, equivalently, can be reduced to the search of solutions of (2.1) satisfying the boundary condition

x(0)=x(T),x(0)=x(T).x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T). (2.2)

By a solution of (2.1) we mean a continuously differentiable function x()x(\cdot) with ϕ(x())\phi(x^{\prime}(\cdot)) continuously differentiable and satisfying (2.1) for all tt. With this respect, it is useful to introduce the space 𝒞T1\mathcal{C}^{1}_{T} of the continuously differentiable functions x:[0,T]nx\colon\mathopen{[}0,T\mathclose{]}\to\mathbb{R}^{n} satisfying the boundary condition (2.2), endowed with the 𝒞1\mathcal{C}^{1}-norm

x𝒞1:=x+x,\|x\|_{\mathcal{C}^{1}}:=\|x\|_{\infty}+\|x^{\prime}\|_{\infty},

where, for a continuous function u:[0,T]nu\colon\mathopen{[}0,T\mathclose{]}\to\mathbb{R}^{n}, we denote

u:=supt[0,T]u(t)\|u\|_{\infty}:=\sup_{t\in\mathopen{[}0,T\mathclose{]}}\|u(t)\|

the classical sup\sup-norm.

Equivalently, instead of (2.1), we can consider the differential system in n×n\mathbb{R}^{n}\times\mathbb{R}^{n}

{x=ϕ1(y)y=f(t,x,ϕ1(y))\begin{cases}\,x^{\prime}=\phi^{-1}(y)\\ \,y^{\prime}=f(t,x,\phi^{-1}(y))\end{cases} (2.3)

and look for a (continuously differentiable) solution (x(),y())(x(\cdot),y(\cdot)). Every TT-periodic solution x()x(\cdot) of (2.1) corresponds to the TT-periodic solution (x(),y())(x(\cdot),y(\cdot)) of (2.3) with y()=ϕ(x())y(\cdot)=\phi(x^{\prime}(\cdot)). Note that a solution of (2.1) defined on [0,T]\mathopen{[}0,T\mathclose{]} is bounded in the 𝒞1\mathcal{C}^{1}-norm if and only if the corresponding solution of (2.3) is bounded in the uniform norm of 𝒞([0,T],2n)\mathcal{C}(\mathopen{[}0,T\mathclose{]},\mathbb{R}^{2n}).

For the existence of TT-periodic solutions of (2.1), we apply the Manásevich–Mawhin continuation theorems [26] in the versions elaborated in [10] where weaker conditions on ϕ\phi are assumed.

Theorem 2.1.

Let F=F(t,x,y;λ):[0,T]×n×n×[0,1]nF=F(t,x,y;\lambda)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\times\mathopen{[}0,1\mathclose{]}\to\mathbb{R}^{n} be a continuous function such that

F(t,x,y;1)=f(t,x,y),F(t,x,y;0)=f0(x,y),F(t,x,y;1)=f(t,x,y),\qquad F(t,x,y;0)=f_{0}(x,y),

where f0:n×nnf_{0}\colon\mathbb{R}^{n}\times\mathbb{R}^{n}\to\mathbb{R}^{n} is an autonomous vector field. Let Ω𝒞T1\Omega\subseteq\mathcal{C}^{1}_{T} be an open and bounded set. Suppose that

  • (h1)(\textsc{h}_{1})

    for each λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[} the problem

    {(ϕ(x))=F(t,x,x;λ),x(0)=x(T),x(0)=x(T),\begin{cases}\,(\phi(x^{\prime}))^{\prime}=F(t,x,x^{\prime};\lambda),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T),\end{cases} (Pλ)

    has no solution xΩx\in\partial\Omega;

  • (h2)(\textsc{h}_{2})

    the condition on the Brouwer degree

    dB(f0(,0),Ωn,0)0\mathrm{d}_{\mathrm{B}}(f_{0}(\cdot,0),\Omega\cap\mathbb{R}^{n},0)\neq 0

    holds.

Then, problem (2.1)-(2.2) has at least a solution in Ω¯\overline{\Omega}.

Theorem 2.1 corresponds to [26, Theorem 4.1] (see also [10, Theorem 4.6]). We recall also another version which is strictly related to the classical Mawhin continuation theorem [27, 33], in an appropriate form for the ϕ\phi-Laplacian operators given in [26, Theorem 3.1] (see also [10, Theorem 3.11]).

Theorem 2.2.

Let F=F(t,x,y):[0,T]×n×nnF=F(t,x,y)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Let Ω𝒞T1\Omega\subseteq\mathcal{C}^{1}_{T} be an open and bounded set. Suppose that

  • (h1)(\textsc{h}^{\prime}_{1})

    for each λ]0,1[\lambda\in\mathopen{]}0,1\mathclose{[} the problem

    {(ϕ(x))=λF(t,x,x),x(0)=x(T),x(0)=x(T),\begin{cases}\,(\phi(x^{\prime}))^{\prime}=\lambda F(t,x,x^{\prime}),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T),\end{cases} (Pλ)

    has no solution xΩx\in\partial\Omega;

  • (h2)(\textsc{h}^{\prime}_{2})

    the condition on the Brouwer degree

    dB(F#,Ωn,0)0\mathrm{d}_{\mathrm{B}}(F^{\#},\Omega\cap\mathbb{R}^{n},0)\neq 0

    holds, where F#(s):=1T0TF(t,s,0)dtF^{\#}(s):=\frac{1}{T}\int_{0}^{T}F(t,s,0)\,\mathrm{d}t.

Then, problem (2.1)-(2.2) has at least a solution in Ω¯\overline{\Omega}.

We propose now some applications of the above continuation theorems which are motivated by the theory of bound sets (cf. [14, 30, 31]). We shall focus our attention to the case of Theorem 2.1. Similar applications can be given starting from Theorem 2.2.

The bound set approach represents a general method to verify the abstract condition of the non-existence of solutions in Ω\partial\Omega, given in (h1)(\textsc{h}_{1}) (respectively (h1)(\textsc{h}^{\prime}_{1})), by introducing a more concrete condition of the non-existence of solutions tangent to the boundary of an open and bounded set GnG\subseteq\mathbb{R}^{n}. In this setting, we also introduce some Nagumo–Hartman conditions (cf. [18, 41]), which are classical in this framework (cf. [32]) and allow to find a priori bounds for x\|x^{\prime}\|_{\infty}.

Let GnG\subseteq\mathbb{R}^{n} be an open and bounded set. Following [29] (see also [58]), we say that the system

(ϕ(x))=F(t,x,x;λ)(\phi(x^{\prime}))^{\prime}=F(t,x,x^{\prime};\lambda) (Eλ)

is a Nagumo equation with respect to GG (with constant KK) if there exists a constant K>0K>0 such that, for every λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[} and for every solution x()x(\cdot) of problem (Pλ)(P_{\lambda}), with x(t)G¯x(t)\in\overline{G} for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}, it holds that xK\|x^{\prime}\|_{\infty}\leq K.

If the Nagumo condition is satisfied, from Theorem 2.1 we deduce the next result.

Theorem 2.3.

Let F=F(t,x,y;λ):[0,T]×n×n×[0,1]nF=F(t,x,y;\lambda)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\times\mathopen{[}0,1\mathclose{]}\to\mathbb{R}^{n} be a continuous function such that

F(t,x,y;1)=f(t,x,y),F(t,x,y;0)=f0(x,y),F(t,x,y;1)=f(t,x,y),\qquad F(t,x,y;0)=f_{0}(x,y),

where f0:n×nnf_{0}\colon\mathbb{R}^{n}\times\mathbb{R}^{n}\to\mathbb{R}^{n} is an autonomous vector field. Suppose that there exists an open bounded set GnG\subseteq\mathbb{R}^{n} such that

  • (hN)(\textsc{h}_{\mathrm{N}})

    the system (Eλ)(E_{\lambda}) is a Nagumo equation with respect to GG;

  • (hBS)(\textsc{h}_{\mathrm{BS}})

    for each λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[} there is no solution of (Pλ)(P_{\lambda}) such that x(t)G¯x(t)\in\overline{G} for all t[0,T]t\in\mathopen{[}0,T\mathclose{]} and x(t0)Gx(t_{0})\in\partial G for some t0[0,T]t_{0}\in\mathopen{[}0,T\mathclose{]};

  • (hD)(\textsc{h}_{\mathrm{D}})

    dB(f0(,0),G,0)0\mathrm{d}_{\mathrm{B}}(f_{0}(\cdot,0),G,0)\neq 0.

Then, problem (2.1)-(2.2) has at least a solution x~\tilde{x} such that x~(t)G¯\tilde{x}(t)\in\overline{G}, for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}.

In the sequel, we refer to (hBS)(\textsc{h}_{\mathrm{BS}}) as a bound set condition. As previously observed, this condition of non-tangency of the solutions at the boundary of GG replaces condition (h1)(\textsc{h}_{1}) of Theorem 2.1.

Proof.

Our argument borrows the classical scheme in [29]. We are going to apply Theorem 2.1. According to the Nagumo condition (hN)(\textsc{h}_{\mathrm{N}}), there exists a constant K>0K>0 such that all the solutions of (Pλ)(P_{\lambda}) with values in G¯\overline{G} have the derivative bounded by KK. Hence, we define the set of functions

Ω:={x𝒞T1:x(t)G for all t[0,T]x<K+1},\Omega:=\bigl{\{}x\in\mathcal{C}^{1}_{T}\colon\text{$x(t)\in G$ for all $t\in\mathopen{[}0,T\mathclose{]}$, $\|x^{\prime}\|_{\infty}<K+1$}\bigr{\}},

which is open and bounded in 𝒞T1\mathcal{C}^{1}_{T} (cf. [14, 31]). In order to check that condition (h1)(\textsc{h}_{1}) holds, observe that if (by contradiction) a solution xx of (Pλ)(P_{\lambda}) satisfies xΩx\in\partial\Omega, then xΩ¯x\in\overline{\Omega}, hence x(t)G¯x(t)\in\overline{G} for all tt. Then, by the Nagumo condition, xK<K+1\|x^{\prime}\|_{\infty}\leq K<K+1. By the definition of Ω\Omega and the assumption xΩx\in\partial\Omega, we cannot have x(t)Gx(t)\in G for all tt and therefore there exists t0[0,T]t_{0}\in\mathopen{[}0,T\mathclose{]} such that x(t0)G=G¯Gx(t_{0})\in\partial G=\overline{G}\setminus G. This situation is not possible in view of the bound set condition (hBS)(\textsc{h}_{\mathrm{BS}}).

To check (h2)(\textsc{h}_{2}) we simply observe that Ωn=G\Omega\cap\mathbb{R}^{n}=G and thus apply (hD)(\textsc{h}_{\mathrm{D}}). This concludes the proof. ∎

The concept of Nagumo equation was introduced by Mawhin in [29] and further developed in [32] as a generalization of the classical Nagumo–Hartman condition [18, 19]. This latter condition was originally expressed as a growth restriction on the vector field f(t,x,y)f(t,x,y) in order to provide an a priori bound on x(t)\|x^{\prime}(t)\| for the solutions of the second-order vector differential equation

x′′=f(t,x,x)x^{\prime\prime}=f(t,x,x^{\prime}) (2.4)

with x(t)\|x(t)\| uniformly bounded.

For the periodic boundary value problem associated with (2.4), the Nagumo–Hartman condition reads as follows: given R>0R>0,

  • (nh1)(\textsc{nh}_{1})

    there exists a continuous function η:[0,+[]0,+[\eta\colon\mathopen{[}0,+\infty\mathclose{[}\to\mathopen{]}0,+\infty\mathclose{[} such that

    +sη(s)ds=+ and f(t,x,y)η(y),t[0,T],xR,yn;\int^{+\infty}\dfrac{s}{\eta(s)}\,\mathrm{d}s=+\infty\;\text{ and }\;\|f(t,x,y)\|\leq\eta(\|y\|),\;\forall\,t\in\mathopen{[}0,T\mathclose{]},\;\|x\|\leq R,\;y\in\mathbb{R}^{n};
  • (nh2)(\textsc{nh}_{2})

    if n>1n>1, there are non-negative constants α,β\alpha,\beta such that

    f(t,x,y)2α(x,f(t,x,y)+y2)+β,t[0,T],xR,yn.\|f(t,x,y)\|\leq 2\alpha\bigl{(}\langle x,f(t,x,y)\rangle+\|y\|^{2}\bigr{)}+\beta,\quad\forall\,t\in\mathopen{[}0,T\mathclose{]},\;\|x\|\leq R,\;y\in\mathbb{R}^{n}.

Under these assumptions it holds that for every R>0R>0 there exists a constant K>0K>0 (depending on R,η,α,β,TR,\eta,\alpha,\beta,T) such that every TT-periodic solution x()x(\cdot) of (2.4) satisfying xR\|x\|_{\infty}\leq R is such that xK\|x^{\prime}\|_{\infty}\leq K (cf. [4, 22, 29]). Observe that condition (nh2)(\textsc{nh}_{2}) implies that the solution x()x(\cdot) satisfies the constraint x′′(t)αd2dt2x(t)2+β\|x^{\prime\prime}(t)\|\leq\alpha\tfrac{d^{2}}{dt^{2}}\|x(t)\|^{2}+\beta for all tt.

In the setting of Theorem 2.3, for the special case ϕ(ξ)=ξ\phi(\xi)=\xi, the condition should be applied with F(t,x,y;λ)F(t,x,y;\lambda) in place of f(t,x,y)f(t,x,y) (and uniformly with respect to λ[0,1]\lambda\in\mathopen{[}0,1\mathclose{]}).

As observed in [29, Proposition 5.2], the concept of Nagumo equation is more general as it covers some second-order differential systems for which (nh1)(\textsc{nh}_{1})-(nh2)(\textsc{nh}_{2}) are not satisfied. Extensions of the Nagumo–Hartman conditions to more general differential operators have been obtained in more recent years, see, for instance, [41] dealing with the vector pp-Laplacian, and [40] for more general scalar nonlinear differential operators. In previous works, it has been provided precise growth assumptions for the vector field ff, generalizing to the pp-Laplacian type operator the classical conditions (nh1)(\textsc{nh}_{1})-(nh2)(\textsc{nh}_{2}), for the second order linear differential operator (cf. [41, conditions (b)(b)-(c)(c)]). Typically these modified Hartman–Nagumo conditions involve a growth assumption on ff with respect to the yy-variable which is related to the exponent pp in the pp-Laplacian operator. For a general ϕ\phi-Laplacian the situation appears more complicated. Indeed, the following example shows that, for any homeomorphism ϕ\phi of the real line having a power-growth at infinity, we can determine a suitable growth-rate in xx^{\prime} such that the Hartman–Nagumo condition is not satisfied.

Example 2.1.

Let ϕ:ϕ()=\phi\colon\mathbb{R}\to\phi(\mathbb{R})=\mathbb{R} be an increasing homeomorphism such that ϕ(0)=0\phi(0)=0. Suppose also that 1+ϕ1(ξ)ξ1+γγdξ<\int_{1}^{+\infty}\phi^{-1}(\xi)\xi^{-\frac{1+\gamma}{\gamma}}\,\mathrm{d}\xi<\infty, for some γ>0\gamma>0. Then, the differential equation

(ϕ(x))=γ(ϕ(x))1+γγ,in ]0,1[,(\phi(x^{\prime}))^{\prime}=\gamma\bigl{(}\phi(x^{\prime})\bigr{)}^{\!\frac{1+\gamma}{\gamma}},\quad\text{in $\mathopen{]}0,1\mathclose{[}$,} (2.5)

has bounded solutions x()x(\cdot), with x()x^{\prime}(\cdot) as well as ϕ(x())\phi(x^{\prime}(\cdot)) unbounded. Indeed, setting u(t):=ϕ(x(t))u(t):=\phi(x^{\prime}(t)) we find that u(t)=(1t)γu(t)=(1-t)^{-\gamma} solves the equation u=γu1+γγu^{\prime}=\gamma\,u^{\frac{1+\gamma}{\gamma}} with u(0)=1u(0)=1. Next, we obtain x(t)=ϕ1((1t)γ)x^{\prime}(t)=\phi^{-1}((1-t)^{-\gamma}) and thus

x(t)=0tϕ1((1s)γ)dsx(t)=\int_{0}^{t}\phi^{-1}((1-s)^{-\gamma})\,\mathrm{d}s

is a solution of (2.5) such that x(0)=0x(0)=0, x(0)=ϕ1(1)x^{\prime}(0)=\phi^{-1}(1), with x()x(\cdot) bounded in [0,1]\mathopen{[}0,1\mathclose{]} and x(t)+x^{\prime}(t)\to+\infty for t1t\to 1^{-}. The example can be modified in order to consider the case of periodic solutions as well. Clearly, if ϕ(ξ)ξβ\phi(\xi)\sim\xi^{\beta} at ++\infty, then taking 0<γ<β0<\gamma<\beta we provide an example where there are bounded solutions with unbounded derivatives. \lhd

Due to the great generality of our differential operator ϕ\phi, we prefer to not propose a specific growth assumption, like in the above quoted papers. On the other hand, in Section 3, we provide some specific application where conditions (nh1)(\textsc{nh}_{1})-(nh2)(\textsc{nh}_{2}) can be checked by a direct inspection.

A slightly variant of Theorem 2.3 can be obtained using Theorem 2.2 and referring the concept of Nagumo equation to the system

(ϕ(x))=λF(t,x,x).(\phi(x^{\prime}))^{\prime}=\lambda F(t,x,x^{\prime}). (Eλ)
Theorem 2.4.

Let F=F(t,x,y):[0,T]×n×nnF=F(t,x,y)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Suppose that there exists an open bounded set GnG\subseteq\mathbb{R}^{n} such that

  • (hN)(\textsc{h}^{\prime}_{\mathrm{N}})

    the system (Eλ)(E^{\prime}_{\lambda}) is a Nagumo equation with respect to GG;

  • (hBS)(\textsc{h}^{\prime}_{\mathrm{BS}})

    for each λ]0,1[\lambda\in\mathopen{]}0,1\mathclose{[} there is no solution of (Pλ)(P^{\prime}_{\lambda}) such that x(t)G¯x(t)\in\overline{G} for all t[0,T]t\in\mathopen{[}0,T\mathclose{]} and x(t0)Gx(t_{0})\in\partial G for some t0[0,T]t_{0}\in\mathopen{[}0,T\mathclose{]};

  • (hD)(\textsc{h}^{\prime}_{\mathrm{D}})

    dB(F#,G,0)0\mathrm{d}_{\mathrm{B}}(F^{\#},G,0)\neq 0.

Then, problem (2.1)-(2.2) has at least a solution x~\tilde{x} such that x~(t)G¯\tilde{x}(t)\in\overline{G}, for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}.

In the sequel, the following lemma will be used as a technical step to provide the desired bounds on x\|x^{\prime}\|_{\infty} in the context of condition (hN)(\textsc{h}_{N}). We denote by 𝕊n1:=B(0,1)\mathbb{S}^{n-1}:=\partial B(0,1) the unit sphere in n\mathbb{R}^{n}.

Lemma 2.1.

Let \mathcal{F} be a family of absolutely continuous and TT-periodic functions such that

  • there exists M00M_{0}\geq 0 such that for all ω𝕊n1\omega\in\mathbb{S}^{n-1} and zz\in\mathcal{F} there exists t0[0,T]t_{0}\in\mathopen{[}0,T\mathclose{]} such that |z(t0),ω|M0|\langle z(t_{0}),\omega\rangle|\leq M_{0};

  • there exist M1>0M_{1}>0 and p[1,+]p\in\mathopen{[}1,+\infty\mathclose{]} such that zLpM1\|z^{\prime}\|_{L^{p}}\leq M_{1} for every zz\in\mathcal{F}.

Then, there exists K=K(M0,M1)>0K=K(M_{0},M_{1})>0 such that zK\|z\|_{\infty}\leq K for every zz\in\mathcal{F}.

Proof.

Let zz\in\mathcal{F} with z0z\not\equiv 0. Let t^[0,T]\hat{t}\in\mathopen{[}0,T\mathclose{]} be such that z(t^)=z0\|z(\hat{t})\|=\|z\|_{\infty}\neq 0. We set ω=z(t^)/z(t^)\omega=z(\hat{t})/\|z(\hat{t})\| and t0=t0(ω,z)t_{0}=t_{0}(\omega,z) as in the first hypothesis. Therefore, we have

z=z(t^)=|z(t^),ω|\displaystyle\|z\|_{\infty}=\|z(\hat{t})\|=\bigl{|}\langle z(\hat{t}),\omega\rangle\bigr{|} =|z(t0),ω+t0t^z(s),ωds|\displaystyle=\biggl{|}\langle z(t_{0}),\omega\rangle+\int_{t_{0}}^{\hat{t}}\langle z^{\prime}(s),\omega\rangle\,\mathrm{d}s\biggr{|}
M0+zL1M0+Tp1pzLpM0+Tp1pM1.\displaystyle\leq M_{0}+\|z^{\prime}\|_{L^{1}}\leq M_{0}+T^{\frac{p-1}{p}}\|z^{\prime}\|_{L^{p}}\leq M_{0}+T^{\frac{p-1}{p}}M_{1}.

Setting K:=M0+Tp1pM1K:=M_{0}+T^{\frac{p-1}{p}}M_{1} (which does not depend on zz), the conclusion holds. ∎

We discuss now a technique introduced and developed in [14, 29, 30, 31] to verify the bound set condition. It consists in controlling locally the solutions of (Eλ)(E_{\lambda}) at the boundary of GG, by means of suitable Lyapunov-like functionals which are usually called bounding functions (see also [30] for an introduction to this topic). To this end we give the following definition (see also [11, 57, 58]).

Definition 2.1.

Let GnG\subseteq\mathbb{R}^{n} be an open and bounded set. Assume that for each uGu\in\partial G, there exist an open ball B(u,ru)B(u,r_{u}) of center uu and radius ru>0r_{u}>0 and a function Vu:B(u,ru)V_{u}\colon B(u,r_{u})\to\mathbb{R} such that Vu(u)=0V_{u}(u)=0 and

G¯B(u,ru){xB(u,ru):Vu(x)0}.\overline{G}\cap B(u,r_{u})\subseteq\bigl{\{}x\in B(u,r_{u})\colon V_{u}(x)\leq 0\bigr{\}}.

In this case, the family (Vu)uG(V_{u})_{u\in\partial G} is called a set of bounding functions for GG.

We are in position to present an application of the method of bounding functions to the periodic problem associated with (2.1) for a homeomorphism ϕ\phi having the following form

ϕ(ξ)=A(ξ)ξ,for every ξn{0},ϕ(0)=0,\phi(\xi)=A(\xi)\xi,\quad\text{for every $\xi\in\mathbb{R}^{n}\setminus\{0\}$,}\qquad\phi(0)=0, (2.6)

where A:n{0}]0,+[A\colon\mathbb{R}^{n}\setminus\{0\}\to\mathopen{]}0,+\infty\mathclose{[} is a continuous function. As shown in [10] this case includes most nonlinear differential operators considered in the literature, in particular the vector pp-Laplacians. Moreover, observe also that (2.6) does not imply that the operator ϕ\phi is monotone (cf. [10, Section 5]).

The following result holds.

Lemma 2.2.

Let ϕ\phi be a homeomorphism of n\mathbb{R}^{n} of the form (2.6). Let F=F(t,x,y;λ):[0,T]×n×n×[0,1]nF=\break F(t,x,y;\lambda)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\times\mathopen{[}0,1\mathclose{]}\to\mathbb{R}^{n} be a continuous function and let (Vu)uG(V_{u})_{u\in\partial G} be a family of bounding functions of class 𝒞2\mathcal{C}^{2} for an open bounded set GnG\subseteq\mathbb{R}^{n}. Suppose that

  • (hV)(\textsc{h}_{V})

    for every uGu\in\partial G, t[0,T]t\in\mathopen{[}0,T\mathclose{]} and λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[}

    Vu′′(u)y,ϕ(y)+Vu(u),F(t,u,y;λ)>0,yn:Vu(u),y=0.\langle V^{\prime\prime}_{u}(u)y,\phi(y)\rangle+\langle V^{\prime}_{u}(u),F(t,u,y;\lambda)\rangle>0,\quad\forall\,y\in\mathbb{R}^{n}\colon\langle V^{\prime}_{u}(u),y\rangle=0.

Then, the bound set condition (hBS)(\textsc{h}_{\mathrm{BS}}) holds with respect to problem (Pλ)(P_{\lambda}).

Proof.

By contradiction, let us suppose that (hBS)(\textsc{h}_{\mathrm{BS}}) is not valid. Therefore, for some λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[} there exists a solution x()x(\cdot) of (Pλ)(P_{\lambda}) such that x(t)G¯x(t)\in\overline{G} for all t[0,T]t\in\mathopen{[}0,T\mathclose{]} and x(t0)Gx(t_{0})\in\partial G for some t0[0,T]t_{0}\in\mathopen{[}0,T\mathclose{]}. Due to the boundary condition x(0)=x(T)x(0)=x(T), without loss of generality, we can suppose 0t0<T0\leq t_{0}<T. We consider the point u:=x(t0)Gu:=x(t_{0})\in\partial G, the ball B(u,ru)B(u,r_{u}) and the function VuV_{u} according to Definition 2.1. Thus, there exists an open neighborhood UU of t0t_{0} such that Vu(x(t))0V_{u}(x(t))\leq 0 for all tU[0,T]t\in U\cap\mathopen{[}0,T\mathclose{]} and Vu(x(t0))=0V_{u}(x(t_{0}))=0, so that t0t_{0} is a point of maximum for the function v:U[0,T]v\colon U\cap\mathopen{[}0,T\mathclose{]}\to\mathbb{R}, v(t):=Vu(x(t))v(t):=V_{u}(x(t)). By the chain rule, we have v(t)=Vu(x(t)),x(t)v^{\prime}(t)=\langle V_{u}^{\prime}(x(t)),x^{\prime}(t)\rangle for all tU[0,T]t\in U\cap\mathopen{[}0,T\mathclose{]}. If 0<t0<T0<t_{0}<T, then v(t0)=0v^{\prime}(t_{0})=0 and therefore

Vu(u),y=0,for y=x(t0).\langle V_{u}^{\prime}(u),y\rangle=0,\quad\text{for $y=x^{\prime}(t_{0})$.} (2.7)

On the other hand, if t0=0t_{0}=0 then both 0 and TT are maximum points for the differentiable function v()v(\cdot) which now is defined on a neighborhood of both points. Since v(0)=v(T)=0v(0)=v(T)=0 and v(t)0v(t)\leq 0 for tt in a right neighborhood of 0 and in a left neighborhood of TT, then v(0)=v(0+)0v(T)=v(T)v^{\prime}(0)=v^{\prime}(0^{+})\leq 0\leq v^{\prime}(T^{-})=v^{\prime}(T) and, using the boundary condition x(0)=x(T)x^{\prime}(0)=x^{\prime}(T), we obtain again (2.7).

As a next step, we introduce the auxiliary function

w(t):=ϕ(x(t)),Vu(x(t)).w(t):=\langle\phi(x^{\prime}(t)),V_{u}^{\prime}(x(t))\rangle.

Observe that w(t0)=0w(t_{0})=0. This is trivial if x(t0)=0x^{\prime}(t_{0})=0, because ϕ(0)=0\phi(0)=0. If x(t0)0x^{\prime}(t_{0})\neq 0, then w(t0)=A(x(t0))x(t0),Vu(x(t0))=0w(t_{0})=A(x^{\prime}(t_{0}))\langle x^{\prime}(t_{0}),V_{u}^{\prime}(x(t_{0}))\rangle=0, by (2.7). By differentiating w()w(\cdot) in a neighborhood of t0t_{0} we obtain

w(t)\displaystyle w^{\prime}(t) =ddtϕ(x(t)),Vu(x(t))\displaystyle=\dfrac{\mathrm{d}}{\mathrm{d}t}\langle\phi(x^{\prime}(t)),V_{u}^{\prime}(x(t))\rangle
=(ϕ(x(t))),Vu(x(t))+ϕ(x(t)),Vu′′(x(t))x(t)\displaystyle=\langle(\phi(x^{\prime}(t)))^{\prime},V_{u}^{\prime}(x(t))\rangle+\langle\phi(x^{\prime}(t)),V_{u}^{\prime\prime}(x(t))x^{\prime}(t)\rangle
=F(t,x(t),x(t);λ),Vu(x(t))+Vu′′(x(t))x(t),ϕ(x(t)).\displaystyle=\langle F(t,x(t),x^{\prime}(t);\lambda),V_{u}^{\prime}(x(t))\rangle+\langle V_{u}^{\prime\prime}(x(t))x^{\prime}(t),\phi(x^{\prime}(t))\rangle.

Hence, from (hV)(\textsc{h}_{V}) and (2.7) we find that w(t0)>0w^{\prime}(t_{0})>0. This implies that there exists an interval [t0,t0+ε[U[0,T]\mathopen{[}t_{0},t_{0}+\varepsilon\mathclose{[}\subseteq U\cap\mathopen{[}0,T\mathclose{]} such that w(t)>0w(t)>0 for all t]t0,t0+ε[t\in\mathopen{]}t_{0},t_{0}+\varepsilon\mathclose{[}. From the definition of w()w(\cdot) and ϕ(0)=0\phi(0)=0, we must have x(t)0x^{\prime}(t)\neq 0 for all t]t0,t0+ε[t\in\mathopen{]}t_{0},t_{0}+\varepsilon\mathclose{[} and hence

w(t)=A(x(t))x(t),Vu(x(t))>0,for all t]t0,t0+ε[.w(t)=A(x^{\prime}(t))\langle x^{\prime}(t),V^{\prime}_{u}(x(t))\rangle>0,\quad\text{for all $t\in\mathopen{]}t_{0},t_{0}+\varepsilon\mathclose{[}$.}

Using the fact that A(ξ)>0A(\xi)>0 for all ξ0\xi\neq 0, we obtain that the map

tx(t),Vu(x(t))=ddtVu(x(t))=v(t)t\mapsto\langle x^{\prime}(t),V^{\prime}_{u}(x(t))\rangle=\dfrac{\mathrm{d}}{\mathrm{d}t}V_{u}(x(t))=v^{\prime}(t)

is strictly positive on ]t0,t0+ε[\mathopen{]}t_{0},t_{0}+\varepsilon\mathclose{[}. We conclude that v()v(\cdot) is strictly increasing on a right neighborhood of t0t_{0} and thus v(t)>v(t0)v(t)>v(t_{0}) for all t]t0,t0+ε[t\in\mathopen{]}t_{0},t_{0}+\varepsilon\mathclose{[}. This contradicts the fact that t0t_{0} is a maximum point for v()v(\cdot). The proof is thus complete. ∎

At last, by combining Theorem 2.3 with Lemma 2.2, we are in position to state our main result which combines the abstract continuation theorem with the bounding function technique.

Theorem 2.5.

Let F=F(t,x,y;λ):[0,T]×n×n×[0,1]nF=F(t,x,y;\lambda)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\times\mathopen{[}0,1\mathclose{]}\to\mathbb{R}^{n} be a continuous function such that

F(t,x,y;1)=f(t,x,y),F(t,x,y;0)=f0(x,y),F(t,x,y;1)=f(t,x,y),\qquad F(t,x,y;0)=f_{0}(x,y),

where f0:n×nnf_{0}\colon\mathbb{R}^{n}\times\mathbb{R}^{n}\to\mathbb{R}^{n} is an autonomous vector field. Suppose that there exists an open bounded set GnG\subseteq\mathbb{R}^{n} satisfying condition (hN)(\textsc{h}_{\mathrm{N}}). Assume that GG admits a family (Vu)uG(V_{u})_{u\in\partial G} of bounding functions of class 𝒞2\mathcal{C}^{2} satisfying (hV)(\textsc{h}_{V}). Assume also (hD)(\textsc{h}_{D}). Then, problem (2.1)-(2.2) has at least a solution x~\tilde{x} such that x~(t)G¯\tilde{x}(t)\in\overline{G}, for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}.

Using the continuation Theorem 2.2 we can provide a variant of Theorem 2.5 which reads as follows. Clearly the next result is strongly connected with the classical one in [29] for ϕ(ξ)=ξ\phi(\xi)=\xi.

Theorem 2.6.

Let F=F(t,x,y):[0,T]×n×nnF=F(t,x,y)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Suppose that there exists an open bounded set GnG\subseteq\mathbb{R}^{n} satisfying condition (hN)(\textsc{h}^{\prime}_{\mathrm{N}}). Assume that GG admits a family (Vu)uG(V_{u})_{u\in\partial G} of bounding functions of class 𝒞2\mathcal{C}^{2} satisfying

  • (hV)(\textsc{h}^{\prime}_{V})

    for every uGu\in\partial G, t[0,T]t\in\mathopen{[}0,T\mathclose{]} and λ]0,1[\lambda\in\mathopen{]}0,1\mathclose{[}

    Vu′′(u)y,ϕ(y)+λVu(u),F(t,u,y)>0,yn:Vu(u),y=0.\langle V^{\prime\prime}_{u}(u)y,\phi(y)\rangle+\lambda\langle V^{\prime}_{u}(u),F(t,u,y)\rangle>0,\quad\forall\,y\in\mathbb{R}^{n}\colon\langle V^{\prime}_{u}(u),y\rangle=0.

Assume also (hD)(\textsc{h}^{\prime}_{\mathrm{D}}). Then, problem (2.1)-(2.2) has at least a solution x~\tilde{x} such that x~(t)G¯\tilde{x}(t)\in\overline{G}, for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}.

Variants of the results presented in this section could be provided for the more general case of a vector field satisfying the Carathéodory conditions. For the linear differential operator ϕ(ξ)=ξ\phi(\xi)=\xi, this approach has been already considered in [40] (see also [2, 3, 52, 53]). In the Carathéodory case, pointwise estimates must be replaced by suitable control of the solutions in a neighborhood of the boundary of the set GG. For simplicity in the exposition, we will not investigate this framework.

3. Applications

In this section, we present some applications of our main results contained in Section 2. In Section 3.1 we consider frictionless vector fields f=f(t,x)f=f(t,x), while in Section 3.2 and Section 3.3 we analyse more general situations: a ϕ\phi-Laplacian Rayleigh-type equation and a ϕ\phi-Laplacian Liénard equation, respectively.

3.1. The case f=f(t,x)f=f(t,x)

We start with the simplest case f=f(t,x)f=f(t,x), namely, we consider the periodic boundary value problem

{(ϕ(x))=f(t,x),x(0)=x(T),x(0)=x(T),\begin{cases}\,(\phi(x^{\prime}))^{\prime}=f(t,x),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T),\end{cases} (3.1)

where ϕ\phi is an homeomorphism of the form (2.6) (considered in the previous section) and f=f(t,x):[0,T]×nnf=f(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} is a continuous function.

In our first result, we apply the concept of field of outer normals at the boundary of a convex body. The use of outer normals in the theory of bound sets is classical and dates back to the Seventies (cf. [4, 16]). We refer to [37, 38, 39] for a recent renewal of considerations of this technique for boundary value problems of non-local type and also for the rich bibliography.

Recall that if DnD\subseteq\mathbb{R}^{n} is a convex body (i.e. the closure of an open bounded convex set of n\mathbb{R}^{n}) then for each uDu\in\partial D there exists a normal cone 𝒩u\mathcal{N}_{u} such that for each ν𝒩u{0}\nu\in\mathcal{N}_{u}\setminus\{0\} we have that

D{xn:xu,ν0}.D\subseteq\bigl{\{}x\in\mathbb{R}^{n}\colon\langle x-u,\nu\rangle\leq 0\bigr{\}}.

A family of vectors 𝒱=(νu)uD\mathcal{V}=(\nu_{u})_{u\in\partial D} is called a field of outer normals for DD if νu𝒩u{0}\nu_{u}\in\mathcal{N}_{u}\setminus\{0\} for each uDu\in\partial D (cf. [12]). We notice that if 0intD0\in\mathrm{int}D then we also have u,νu>0\langle u,\nu_{u}\rangle>0 for all uDu\in\partial D with νu𝒩u{0}\nu_{u}\in\mathcal{N}_{u}\setminus\{0\}.

The following result holds.

Corollary 3.1.

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism of the form (2.6) and f=f(t,x):[0,T]×nnf=f(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Suppose that there exists a field of outer normals 𝒱=(νu)uG{\mathcal{V}}=(\nu_{u})_{u\in\partial G}, for an open convex bounded set GnG\subseteq\mathbb{R}^{n} such that

f(t,u),νu0,for all t[0,T].\langle f(t,u),\nu_{u}\rangle\geq 0,\quad\text{for all $t\in\mathopen{[}0,T\mathclose{]}$.}

Then, problem (3.1) has at least a solution with values in G¯\overline{G}.

Proof.

We fix a point PGP\in G and observe that from basic properties of convex sets (cf. [11, p. 107] and [25]) we have uP,νu>0\langle u-P,\nu_{u}\rangle>0 for all uGu\in\partial G. Thus, we define

F(t,x,y;λ):=λf(t,x)+(1λ)(xP),F(t,x,y;\lambda):=\lambda f(t,x)+(1-\lambda)(x-P),

so that F(t,x,y;1)=f(t,x)F(t,x,y;1)=f(t,x) and F(t,x,y;0)=f0(x)=xPF(t,x,y;0)=f_{0}(x)=x-P. In this manner, (hD)(\textsc{h}_{\mathrm{D}}) is clearly satisfied as

dB(IdnP,G,0)=dB(Idn,G,P)=1.\mathrm{d}_{\mathrm{B}}(\mathrm{Id}_{\mathbb{R}^{n}}-P,G,0)=\mathrm{d}_{\mathrm{B}}(\mathrm{Id}_{\mathbb{R}^{n}},G,P)=1.

To prove condition (hV)(\textsc{h}_{\mathrm{V}}) we define Vu(x):=xu,νuV_{u}(x):=\langle x-u,\nu_{u}\rangle and observe that Vu(u)=νuV^{\prime}_{u}(u)=\nu_{u} and Vu′′(u)=0V^{\prime\prime}_{u}(u)=0. Hence

Vu(u),F(t,u,y;λ)=λf(t,u),νu+(1λ)uP,νu(1λ)uP,νu>0,\langle V_{u}(u),F(t,u,y;\lambda)\rangle=\lambda\langle f(t,u),\nu_{u}\rangle+(1-\lambda)\langle u-P,\nu_{u}\rangle\geq(1-\lambda)\langle u-P,\nu_{u}\rangle>0,

for every λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[}, t[0,T]t\in\mathopen{[}0,T\mathclose{]} and uGu\in\partial G; then (hV)(\textsc{h}_{V}) holds.

To conclude the proof we have still to check (hN)(\textsc{h}_{N}), that is (3.1) is a Nagumo equation with respect to GG. To this end, let λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[} and x()x(\cdot) be a solution of (Pλ)(P_{\lambda}) with values in the bounded set GG. Then, x()x(\cdot) is uniformly bounded and consequently f(,x())f(\cdot,x(\cdot)) is bounded as well. Hence, there are two positive constants R1,R2R_{1},R_{2} such that every solution of (Pλ)(P_{\lambda}) satisfies

xR1,(ϕ(x))R2.\|x\|_{\infty}\leq R_{1},\quad\|(\phi(x^{\prime}))^{\prime}\|_{\infty}\leq R_{2}.

Let ω𝕊n1\omega\in\mathbb{S}^{n-1}, and consider the auxiliary function ψx,ω(t):=x(t),ω\psi_{x,\omega}(t):=\langle x(t),\omega\rangle, t[0,T]t\in\mathopen{[}0,T\mathclose{]}. By Rolle’s theorem there exists t0=t0(x,ω)[0,T]t_{0}=t_{0}(x,\omega)\in\mathopen{[}0,T\mathclose{]} such that ψx,ω(t0)=x(t0),ω=0\psi_{x,\omega}^{\prime}(t_{0})=\langle x^{\prime}(t_{0}),\omega\rangle=0. Therefore, for z(t):=ϕ(x(t))=A(x(t))x(t)z(t):=\phi(x^{\prime}(t))=A(x^{\prime}(t))x^{\prime}(t) the conditions in Lemma 2.1 are satisfied with M0:=0M_{0}:=0, p=p=\infty, M1:=R2M_{1}:=R_{2}. We conclude hat there exists a constant K:=TR2K:=TR_{2} such that

ϕ(x(t))K,for every t[0,T],\|\phi(x^{\prime}(t))\|\leq K,\quad\text{for every $t\in\mathopen{[}0,T\mathclose{]}$,}

holds for every possible solution x()x(\cdot) of (Pλ)(P_{\lambda}). As a consequence of the above inequality, we get that ϕ(x())\phi(x^{\prime}(\cdot)), and so x()x^{\prime}(\cdot), is uniformly bounded. This proves (hN).(\textsc{h}_{N}). Finally, we conclude with an application of Theorem 2.5. ∎

In the next result the domain GG is the sublevel set of a functional. Preliminarily, we make some remarks.

For given function V:nV\colon\mathbb{R}^{n}\to\mathbb{R} and cc\in\mathbb{R}, we denote by [Vc][V\leq c] the sublevel set {xn:V(x)c}\{x\in\mathbb{R}^{n}\colon V(x)\leq c\} and similarly [V=c]:={xn:V(x)=c}[V=c]:=\{x\in\mathbb{R}^{n}\colon V(x)=c\} and [V<c]:={xn:V(x)<c}[V<c]:=\{x\in\mathbb{R}^{n}\colon V(x)<c\}. Assume that VV is of class 𝒞1\mathcal{C}^{1} and that, for some cc\in\mathbb{R}, the set D:=[Vc]D:=[V\leq c] is nonempty and, moreover,

V(u)0,for all u[V=c].V^{\prime}(u)\neq 0,\quad\text{for all $u\in[V=c]$.} (3.2)

In this case, it turns out that DD is a regularly closed set, namely for G:=intD=DDG:=\mathrm{int}D=D\setminus\partial D we have G¯=D\overline{G}=D and, moreover, G=D=[V=c]\partial G=\partial D=[V=c] as well as G=[V<c]G=[V<c].

To prove this claim, we observe that in any case, we have [V<c]G,[V<c]\subseteq G, G¯D\overline{G}\subseteq D and GD[V=c]\partial G\subseteq\partial D\subseteq[V=c]. On the other hand, if for every uDu\in\partial D we consider the scalar function w(ϑ):=V(u+ϑV(u)),w(\vartheta):=V(u+\vartheta V^{\prime}(u)), we find that w(0)=cw(0)=c and w(0)>0,w^{\prime}(0)>0, so that in any neighborhood of uu there are points of G,G, from which we obtain that DG¯\partial D\subseteq\overline{G}. Finally, from G=D\partial G=\partial D we also conclude that G¯=GG=intDD=D\overline{G}=G\cup\partial G=\mathrm{int}D\cup\partial D=D and thus the claim is proved.

Generally speaking, the condition V(u)0V^{\prime}(u)\neq 0, for all uDu\in\partial D, is not enough to guarantee the same property, as shown by the example V:V\colon\mathbb{R}\to\mathbb{R}, V(x):=x4x2V(x):=x^{4}-x^{2}, and c=0c=0. In this case, D={1,1}{1,0,1}=[V=0]\partial D=\{-1,1\}\subsetneq\{-1,0,1\}=[V=0].

The next lemma, which is borrowed and adapted from [24] (see also the survey [23]), is useful in this context as it allows to study the case of sublevel domains with a minimal set of assumptions.

Lemma 3.1.

Let V:nV\colon\mathbb{R}^{n}\to\mathbb{R} be a 𝒞2\mathcal{C}^{2}-function satisfying (3.2) for some cc\in\mathbb{R} with D:=[Vc]D:=[V\leq c] nonempty, bounded and connected. Then, DD (as well as intD\mathrm{int}D) is convex if and only if

  • (C)(C)

    for all uDu\in\partial D, V′′(u)y,y0\langle V^{\prime\prime}(u)y,y\rangle\geq 0, for all yny\in\mathbb{R}^{n} with V(u),y=0\langle V^{\prime}(u),y\rangle=0.

Lemma 3.1 can be proved by combining the results in [24, ch. 6, pp. 195–196] or [23]. In Appendix A we provide a sketch of the proof. Clearly it is not restrictive to consider the case c=0c=0, as done in the sequel.

The following result provides a variant of Corollary 3.1 for convex sets with smooth boundary, observing that the involved domain is a sublevel set (see [4, 29] for classical results in this direction for the linear differential operator).

Corollary 3.2.

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism of the form (2.6) and f=f(t,x):[0,T]×nnf=f(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Let V:nV\colon\mathbb{R}^{n}\to\mathbb{R} be a 𝒞2\mathcal{C}^{2}-function such that V(u)0V^{\prime}(u)\neq 0 for all u[V=0]u\in[V=0]. Let D:=[V0]D:=[V\leq 0] be nonempty and bounded. Suppose that for every t[0,T]t\in\mathopen{[}0,T\mathclose{]} and uDu\in\partial D

  • V(u),f(t,u)0\langle V^{\prime}(u),f(t,u)\rangle\geq 0;

  • V′′(u)y,y0\langle V^{\prime\prime}(u)y,y\rangle\geq 0, for all yny\in\mathbb{R}^{n} with V(u),y=0\langle V^{\prime}(u),y\rangle=0.

Then, problem (3.1) has at least a solution with values in DD.

Proof.

We define G:=intD=DDG:={\rm int}D=D\setminus\partial D and therefore G=[V<0]G=[V<0]. By the preliminary observation we also have G¯=D\overline{G}=D and G=D=[V=0]\partial G=\partial D=[V=0]. Let G0G_{0} be a connected component of GG. Setting Vu=VV_{u}=V for all uG0u\in\partial G_{0}, we have that (Vu)uG0(V_{u})_{u\in\partial G_{0}} is a family of bounding functions for G0G_{0}. Next, we consider the homotopy

F(t,x,y;λ):=λf(t,x)+(1λ)V(x)F(t,x,y;\lambda):=\lambda f(t,x)+(1-\lambda)V^{\prime}(x)

and observe that

V′′(u)y,ϕ(y)+V(u),F(t,u,y;λ)=\displaystyle\langle V^{\prime\prime}(u)y,\phi(y)\rangle+\langle V^{\prime}(u),F(t,u,y;\lambda)\rangle=
=A(y)V′′(u)y,y+λV(u),f(t,u)+(1λ)V(u)>0,\displaystyle=A(y)\langle V^{\prime\prime}(u)y,y\rangle+\lambda\langle V^{\prime}(u),f(t,u)\rangle+(1-\lambda)\|V^{\prime}(u)\|>0,

for every λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[}, t[0,T]t\in\mathopen{[}0,T\mathclose{]}, uG0u\in\partial G_{0}, and yny\in\mathbb{R}^{n} such that V(u),y=0\langle V^{\prime}(u),y\rangle=0. Therefore, condition (hV)(\textsc{h}_{V}) holds. Next, from Lemma 3.1 we observe that G0G_{0} is convex and therefore

dB(V,G0,0)=1.\mathrm{d}_{\mathrm{B}}(V^{\prime},G_{0},0)=1. (3.3)

To prove the above formula, let us fix a point P0G0P_{0}\in G_{0}. We claim that

V(u),uP00,for all uG0.\langle V^{\prime}(u),u-P_{0}\rangle\geq 0,\quad\text{for all $u\in\partial G_{0}$.} (3.4)

Indeed, setting v(ϑ):=V(P0+ϑ(uP0))v(\vartheta):=V(P_{0}+\vartheta(u-P_{0})) for ϑ[0,1]\vartheta\in\mathopen{[}0,1\mathclose{]}, we have that v(1)=0v(1)=0 and v(ϑ)<0v(\vartheta)<0 for all ϑ[0,1[\vartheta\in\mathopen{[}0,1\mathclose{[}. Hence, V(u),uP0=v(1)0\langle V^{\prime}(u),u-P_{0}\rangle=v^{\prime}(1)\geq 0. From (3.4), via the convex homotopy (1λ)V(x)+λ(xP0)(1-\lambda)V^{\prime}(x)+\lambda(x-P_{0}) we find that

dB(V,G0,0)=dB(IdnP0,G0,0)=dB(Idn,G0,P0)=1.\mathrm{d}_{\mathrm{B}}(V^{\prime},G_{0},0)=\mathrm{d}_{\mathrm{B}}(\mathrm{Id}_{\mathbb{R}^{n}}-P_{0},G_{0},0)=\mathrm{d}_{\mathrm{B}}(\mathrm{Id}_{\mathbb{R}^{n}},G_{0},P_{0})=1.

An alternative manner to prove (3.3) is to apply [12, Theorem 3] to the vector field V(x)-V^{\prime}(x) on the convex set G0G_{0}.

Finally, we conclude with an application of Theorem 2.5 which implies the existence of a solution in G0¯\overline{G_{0}} and hence in DD. ∎

We can reestablish the following version of the Hartman–Knobloch theorem (see [10, 34]).

Theorem 3.1 (Hartman–Knobloch).

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism of the form (2.6) and f=f(t,x):[0,T]×nnf=f(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. If there exists R>0R>0 such that Hartman’s condition

f(t,x),x0,for every t[0,T] and xn with x=R,\langle f(t,x),x\rangle\geq 0,\quad\text{for every $t\in\mathopen{[}0,T\mathclose{]}$ and $x\in\mathbb{R}^{n}$ with $\|x\|=R$,}

holds, then there exists a solution xx of (3.1) such that x(t)R\|x(t)\|\leq R for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}.

Proof.

We can propose two different proofs. The first one is based on Corollary 3.1. We consider the set G={xn:x<R}G=\{x\in\mathbb{R}^{n}\colon\|x\|<R\} and observe that νx=x\nu_{x}=x for all xGx\in\partial G. Therefore, Hartman’s condition corresponds to the assumption in Corollary 3.1 and thus Theorem 3.1 follows.

The second proof is based on Corollary 3.2. We deal with the 𝒞\mathcal{C}^{\infty}-function V(x)=(x2R2)/2V(x)=(\|x\|^{2}-R^{2})/2 and notice that V(x)=xV^{\prime}(x)=x and V′′V^{\prime\prime} is the identity matrix. The conclusion is reached as a direct application of Corollary 3.2. ∎

We can further state another straightforward consequence of Corollary 3.1.

Theorem 3.2 (Poincaré–Miranda).

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism of the form (2.6) and let f=f(t,x):[0,T]×nnf=f(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Assume that there exists a nn-dimensional rectangle :=i=1n[ai,bi]\mathcal{R}:=\prod_{i=1}^{n}\mathopen{[}a_{i},b_{i}\mathclose{]} such that for each i{1,,n}i\in\{1,\ldots,n\} it holds that

{fi(t,x)0,for all x with xi=ai,fi(t,x)0,for all x with xi=bi.\begin{cases}\,f_{i}(t,x)\leq 0,&\text{for all $x\in\partial\mathcal{R}$ with $x_{i}=a_{i}$,}\\ \,f_{i}(t,x)\geq 0,&\text{for all $x\in\partial\mathcal{R}$ with $x_{i}=b_{i}$.}\end{cases} (3.5)

Then, there exists a solution xx of (3.1) with x(t)x(t)\in\mathcal{R} for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}.

As is well known, the inequalities in (3.5) can be reversed for first order systems; on the other hand, for second-order systems (as in our case) reversing the inequalities is not possible unless further growth (non-resonance) assumptions on the vector field are imposed, as one can see from the trivial example x′′=x+εsin(t)x^{\prime\prime}=-x+\varepsilon\sin(t) (see, for instance, [28] for a result in this direction).

It is worth noticing that Theorem 3.2 is related to the theory of (well ordered) lower and upper solutions for a differential system in n\mathbb{R}^{n}, as it represents the case of vector valued lower solution α\alpha and vector valued upper solution β\beta with αiai\alpha_{i}\equiv a_{i} and βi=bi\beta_{i}=b_{i}. In order to deal with non-constant lower and upper solutions in n\mathbb{R}^{n}, one could adapt to our case the technique of “curvature bound sets” in [13, 14] or “non autonomous bounding Lyapunov functions” in [4]; see also [17] for a similar approach.

3.2. A ϕ\phi-Laplacian Rayleigh-type equation

Up to now we have considered only a trivial case of the Nagumo–Hartman condition, namely when the vector field does not depend on xx^{\prime}. In the next example, inspired by a case studied in [29], we treat a more general situation.

Let us consider the following TT-periodic boundary value problem associated with a ϕ\phi-Laplacian Rayleigh-type equation

{(ϕ(x))=g(x)+h(t,x),x(0)=x(T),x(0)=x(T),\begin{cases}\,(\phi(x^{\prime}))^{\prime}=g(x^{\prime})+h(t,x),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T),\end{cases} (3.6)

which is a natural generalisation of the system x′′=g(x)+h(t,x)x^{\prime\prime}=g(x^{\prime})+h(t,x) considered in [29]. In this framework, we state the following result, which is in the spirit of Corollary 3.2. It can be seen as an extension of [29, Corollary 6.3] (for V(x)=(x2R2)/2V(x)=(\|x\|^{2}-R^{2})/2).

Theorem 3.3.

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism of the form (2.6) and let h=h(t,x):[0,T]×nnh=h(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Let g:nng\colon\mathbb{R}^{n}\to\mathbb{R}^{n} be continuous and such that g(y)g(y) has either the same or the opposite direction of yy. Assume also that there exists 𝒢:n\mathcal{G}\colon\mathbb{R}^{n}\to\mathbb{R} of class 𝒞1\mathcal{C}^{1} such that

  • g(y)𝒢(ϕ(y))g(y)-\nabla\mathcal{G}(\phi(y)) is bounded.

Let V:nV\colon\mathbb{R}^{n}\to\mathbb{R} be a 𝒞2\mathcal{C}^{2}-function such that V(u)0V^{\prime}(u)\neq 0 for all u[V=0]u\in[V=0]. Let D:=[V0]D:=[V\leq 0] be nonempty and bounded. Suppose that for every t[0,T]t\in\mathopen{[}0,T\mathclose{]} and uDu\in\partial D

  • V(u),h(t,u)0\langle V^{\prime}(u),h(t,u)\rangle\geq 0;

  • V′′(u)y,y0\langle V^{\prime\prime}(u)y,y\rangle\geq 0, for all yny\in\mathbb{R}^{n} with V(u),y=0\langle V^{\prime}(u),y\rangle=0.

Then, problem (3.6) has at least a solution with values in DD.

Proof.

The proof follows the same steps of Corollary 3.2. Accordingly we just point out the main modifications which are needed. Having defined G:=intD=[V<0]G:={\rm int}D=[V<0] and G0G_{0} as above, we consider the homotopy

F(t,x,y;λ):=g(y)+λh(t,x)+(1λ)V(x).F(t,x,y;\lambda):=g(y)+\lambda h(t,x)+(1-\lambda)V^{\prime}(x).

For every λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[}, t[0,T]t\in\mathopen{[}0,T\mathclose{]}, uG0u\in\partial G_{0}, and yny\in\mathbb{R}^{n} such that Vu(u),y=0\langle V^{\prime}_{u}(u),y\rangle=0, it holds that

V′′(u)y,ϕ(y)+V(u),F(t,u,y;λ)=\displaystyle\langle V^{\prime\prime}(u)y,\phi(y)\rangle+\langle V^{\prime}(u),F(t,u,y;\lambda)\rangle=
=A(y)V′′(u)y,y+V(u),g(y)+λV(u),h(t,u)+(1λ)V(u)\displaystyle=A(y)\langle V^{\prime\prime}(u)y,y\rangle+\langle V^{\prime}(u),g(y)\rangle+\lambda\langle V^{\prime}(u),h(t,u)\rangle+(1-\lambda)\|V^{\prime}(u)\|
=A(y)V′′(u)y,y+λV(u),h(t,u)+(1λ)V(u)>0,\displaystyle=A(y)\langle V^{\prime\prime}(u)y,y\rangle+\lambda\langle V^{\prime}(u),h(t,u)\rangle+(1-\lambda)\|V^{\prime}(u)\|>0,

where we have used the fact that g(y)g(y) is parallel to yy. Therefore, condition (hV)(\textsc{h}_{V}) holds. The verification of the degree conditions is the same as in the proof of Corollary 3.2 using the convexity of G0G_{0}.

In order to conclude the proof, we need only to check that the Nagumo condition (hN)(\textsc{h}_{N}) is satisfied with respect to the set G0G_{0}. To this end, let λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[} and x()x(\cdot) be a solution of (Pλ)(P_{\lambda}) with values in the bounded set G0G_{0}. Then, x()x(\cdot) is uniformly bounded and consequently

w(t):=λh(t,x(t))+(1λ)V(x(t))w(t):=\lambda h(t,x(t))+(1-\lambda)V^{\prime}(x(t))

is uniformly bounded too, by a constant R0R_{0}. Consider now the system

{(ϕ(x))=g(x)+w(t),x(0)=x(T),x(0)=x(T).\begin{cases}\,(\phi(x^{\prime}))^{\prime}=g(x^{\prime})+w(t),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T).\end{cases}

From this we have

(ϕ(x(t)))2\displaystyle\|(\phi(x^{\prime}(t)))^{\prime}\|^{2} =g(x(t))𝒢(ϕ(x(t))),(ϕ(x(t)))\displaystyle=\langle g(x^{\prime}(t))-\nabla\mathcal{G}(\phi(x^{\prime}(t))),(\phi(x^{\prime}(t)))^{\prime}\rangle
+𝒢(ϕ(x(t))),(ϕ(x(t)))+w(t),(ϕ(x(t)))\displaystyle\quad+\langle\nabla\mathcal{G}(\phi(x^{\prime}(t))),(\phi(x^{\prime}(t)))^{\prime}\rangle+\langle w(t),(\phi(x^{\prime}(t)))^{\prime}\rangle
L(ϕ(x(t)))+R0(ϕ(x(t)))+ddt𝒢(ϕ(x(t))),\displaystyle\leq L\|(\phi(x^{\prime}(t)))^{\prime}\|+R_{0}\|(\phi(x^{\prime}(t)))^{\prime}\|+\dfrac{\mathrm{d}}{\mathrm{d}t}\mathcal{G}(\phi(x^{\prime}(t))),

where L>0L>0 is a constant which bounds g(y)𝒢(ϕ(y))g(y)-\nabla\mathcal{G}(\phi(y)). An integration on [0,T]\mathopen{[}0,T\mathclose{]} yields to

(ϕ(x))L22(L+R0)T(ϕ(x))L2\|(\phi(x^{\prime}))^{\prime}\|_{L^{2}}^{2}\leq(L+R_{0})\sqrt{T}\,\|(\phi(x^{\prime}))^{\prime}\|_{L^{2}}

and thus a bound for (ϕ(x()))(\phi(x^{\prime}(\cdot)))^{\prime} in L2L^{2} is achieved. An application of Lemma 2.1 for p=2p=2, arguing as in the proof of Corollary 3.1, ensures an a priori bound for x\|x^{\prime}\|_{\infty}. Finally, Theorem 2.5 implies the existence of a solution in G0¯\overline{G_{0}} and hence in DD. ∎

As in Section 3.1 we have the following straightforward corollaries.

Corollary 3.3 (Hartman–Knobloch).

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism of the form (2.6) and let h=h(t,x):[0,T]×nnh=h(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Let g:nng\colon\mathbb{R}^{n}\to\mathbb{R}^{n} be continuous and such that g(y)g(y) has either the same or the opposite direction of yy. If there exists R>0R>0 such that Hartman’s condition

h(t,x),x0,for every t[0,T] and xn with x=R,\langle h(t,x),x\rangle\geq 0,\quad\text{for every $t\in\mathopen{[}0,T\mathclose{]}$ and $x\in\mathbb{R}^{n}$ with $\|x\|=R$,}

holds, then there exists a solution xx of (3.1) such that x(t)R\|x(t)\|\leq R for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}.

Corollary 3.4 (Poincaré–Miranda).

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism of the form (2.6) and let h=h(t,x):[0,T]×nnh=h(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function. Assume that there exists a nn-dimensional rectangle :=i=1n[ai,bi]\mathcal{R}:=\prod_{i=1}^{n}\mathopen{[}a_{i},b_{i}\mathclose{]} such that for each i{1,,n}i\in\{1,\ldots,n\} it holds that

{hi(t,x)0,for all x with xi=ai,hi(t,x)0,for all x with xi=bi.\begin{cases}\,h_{i}(t,x)\leq 0,&\text{for all $x\in\partial\mathcal{R}$ with $x_{i}=a_{i}$,}\\ \,h_{i}(t,x)\geq 0,&\text{for all $x\in\partial\mathcal{R}$ with $x_{i}=b_{i}$.}\end{cases}

Then, there exists a solution xx of (3.1) with x(t)x(t)\in\mathcal{R} for all t[0,T]t\in\mathopen{[}0,T\mathclose{]}.

3.3. A ϕ\phi-Laplacian Liénard equation

All the preceding examined examples depend on the fact that first we find a set GnG\subseteq\mathbb{R}^{n} with no solutions tangent to the boundary from the interior, and next we provide some a priori bound on x(t)\|x^{\prime}(t)\| using Nagumo-type conditions. There are however some situations in which the particular form of the equations allows to find a priori bounds on xLp\|x^{\prime}\|_{L^{p}} (for some pp) independently on xx. In such cases, the set GG can be found using some “sign-conditions” on the nonlinearity. As a possible example in this direction and our third application, we deal with the following TT-periodic boundary value problem associated with a ϕ\phi-Laplacian Liénard equation

{(ϕ(x))=ddt𝒢(x)+h(t,x),x(0)=x(T),x(0)=x(T).\begin{cases}\,(\phi(x^{\prime}))^{\prime}=\dfrac{\mathrm{d}}{\mathrm{d}t}\nabla\mathcal{G}(x)+h(t,x),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T).\end{cases} (3.7)

In this setting, we can state the following.

Theorem 3.4.

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism such that

  • (hϕ)(\textsc{h}_{\phi})

    ϕ(ξ),ξ>0\langle\phi(\xi),\xi\rangle>0 for every ξn{0}\xi\in\mathbb{R}^{n}\setminus\{0\}, and for every η>0\eta>0 there exists Mη>0M_{\eta}>0 such that ϕ(ξ),ξηξMη\langle\phi(\xi),\xi\rangle\geq\eta\|\xi\|-M_{\eta}, for all ξn\xi\in\mathbb{R}^{n}.

Let 𝒢:nn\mathcal{G}\colon\mathbb{R}^{n}\to\mathbb{R}^{n} be a 𝒞2\mathcal{C}^{2}-function. Let h=h(t,x):[0,T]×nnh=h(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function such that

  • (hh)(\textsc{h}_{\textsc{h}})

    there exists R>0R>0 such that h(t,x),x0\langle h(t,x),x\rangle\geq 0, for every t[0,T]t\in\mathopen{[}0,T\mathclose{]} and xnx\in\mathbb{R}^{n} with xR\|x\|\geq R.

Then, problem (3.7) has at least a solution.

Proof.

We aim to apply Theorem 2.1. Accordingly, we introduce the parameter-dependent problem

{(ϕ(x))=λddt𝒢(x)+hλ(t,x),x(0)=x(T),x(0)=x(T),\begin{cases}\,(\phi(x^{\prime}))^{\prime}=\lambda\dfrac{\mathrm{d}}{\mathrm{d}t}\nabla\mathcal{G}(x)+h_{\lambda}(t,x),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T),\end{cases} (3.8)

where

hλ(t,x):=λh(t,x)+(1λ)x,λ[0,1].h_{\lambda}(t,x):=\lambda h(t,x)+(1-\lambda)x,\quad\lambda\in\mathopen{[}0,1\mathclose{]}. (3.9)

We divide the proof in some steps.

Step 1. A priori bound of xL1\|x^{\prime}\|_{L^{1}}. Let x()x(\cdot) be a solution of problem (3.12). By integrating the scalar product between x()x(\cdot) and the equation in (3.8), we have

0Tϕ(x(t)),x(t)dt+0Thλ(t,x(t)),x(t)dt=0.\int_{0}^{T}\langle\phi(x^{\prime}(t)),x^{\prime}(t)\rangle\,\mathrm{d}t+\int_{0}^{T}\langle h_{\lambda}(t,x(t)),x(t)\rangle\,\mathrm{d}t=0. (3.10)

Next, we observe that condition (hh)(\textsc{h}_{\textsc{h}}) implies the existence of K0>0K_{0}>0 such that h(t,x),xK0\langle h(t,x),x\rangle\geq-K_{0}, for every t[0,T]t\in\mathopen{[}0,T\mathclose{]} and xnx\in\mathbb{R}^{n}. Therefore, from (3.10), we deduce that

0Tϕ(x(t)),x(t)dtTK0.\int_{0}^{T}\langle\phi(x^{\prime}(t)),x^{\prime}(t)\rangle\,\mathrm{d}t\leq TK_{0}.

We fix η=1\eta=1 and, by hypothesis (hϕ)(\textsc{h}_{\phi}), we obtain that

xL1=0Tx(t)dtT(K0+M1)=:K1,\|x^{\prime}\|_{L^{1}}=\int_{0}^{T}\|x^{\prime}(t)\|\,\mathrm{d}t\leq T(K_{0}+M_{1})=:K_{1},

which is the desired bound.

Step 2. A priori bound of x\|x\|_{\infty}. Let x()x(\cdot) be a solution of problem (3.12). First, we prove that there exists t~[0,T]\tilde{t}\in\mathopen{[}0,T\mathclose{]} such that x(t~)<R\|x(\tilde{t})\|<R. Indeed, if it is not true, x(t)R\|x(t)\|\geq R for all t[0,T]t\in\mathopen{[}0,T\mathclose{]} and from (3.10) (and since λ[0,1[\lambda\in\mathopen{[}0,1\mathclose{[}), we deduce that

0=0Tϕ(x(t)),x(t)dt+λ0Th(t,x(t)),x(t)dt+(1λ)0Tx(t)2dt>0,0=\int_{0}^{T}\langle\phi(x^{\prime}(t)),x^{\prime}(t)\rangle\,\mathrm{d}t+\lambda\int_{0}^{T}\langle h(t,x(t)),x(t)\rangle\,\mathrm{d}t+(1-\lambda)\int_{0}^{T}\|x(t)\|^{2}\,\mathrm{d}t>0,

a contradiction. Consequently, for every t[0,T]t\in\mathopen{[}0,T\mathclose{]}, we immediately obtain

x(t)=x(t~)+t~tx(s)dsx(t~)+0Tx(s)ds<R+K1T=:R,\|x(t)\|=\biggl{\|}x(\tilde{t})+\int_{\tilde{t}}^{t}x^{\prime}(s)\,\mathrm{d}s\biggr{\|}\leq\|x(\tilde{t})\|+\int_{0}^{T}\|x^{\prime}(s)\|\,\mathrm{d}s<R+K_{1}T=:R^{*},

and thus x<R\|x\|_{\infty}<R^{*}, as desired. As a consequence, the open ball G=B(0,R)G=B(0,R^{*}) is (trivially) a bound set for system (3.8).

Step 3. Conclusion. From

(ϕ(x))L1=0T(ϕ(x(t)))dtHess𝒢(x)xL1+Thλ(,x),\|(\phi(x^{\prime}))^{\prime}\|_{L^{1}}=\int_{0}^{T}\|(\phi(x^{\prime}(t)))^{\prime}\|\,\mathrm{d}t\leq\|\mathrm{Hess}\,\mathcal{G}(x)\|_{\infty}\|x^{\prime}\|_{L^{1}}+T\|h_{\lambda}(\cdot,x)\|_{\infty},

we have that (ϕ(x()))(\phi(x^{\prime}(\cdot)))^{\prime} is bounded in L1L^{1}. Therefore, an application of Lemma 2.1 for p=1p=1, arguing as in the proof of Corollary 3.1, ensures an a priori bound for x\|x^{\prime}\|_{\infty}.

For λ=0\lambda=0, we have dB(Idn,G,0)=10\mathrm{d}_{\mathrm{B}}(\mathrm{Id}_{\mathbb{R}^{n}},G,0)=1\neq 0. Therefore, the thesis follows from Theorem 2.3. ∎

Remark 3.1.

If ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} is a homeomorphism of the form (2.6), then ϕ\phi satisfies hypothesis (hϕ)(\textsc{h}_{\phi}) of Theorem 3.4. Indeed, for ξ0\xi\neq 0, we have

ϕ(ξ),ξξ=A(ξ)ξ2ξ=A(ξ)ξ=ϕ(ξ)+,as ξ+.\dfrac{\langle\phi(\xi),\xi\rangle}{\|\xi\|}=\dfrac{A(\xi)\|\xi\|^{2}}{\|\xi\|}=\|A(\xi)\xi\|=\|\phi(\xi)\|\to+\infty,\quad\text{as $\|\xi\|\to+\infty$.}

Hence, (hϕ)(\textsc{h}_{\phi}) follows. \lhd

Our result is related to a classical theorem by Reissig [47, Theorem 3] for the classical scalar generalized Liénard equation with a periodic forcing term

x′′+(x)x+𝒢(x)=p(t)p(t+T),x^{\prime\prime}+\mathscr{F}(x)x^{\prime}+\mathscr{G}(x)=p(t)\equiv p(t+T),

where the existence of a TT-periodic solution is proved by assuming 𝒢(x)x0\mathscr{G}(x)x\leq 0 for every xx\in\mathbb{R} with |x|d>0|x|\geq d>0 and 0Tp(t)dt=0\int_{0}^{T}p(t)\,\mathrm{d}t=0. No special assumption besides continuity on \mathscr{F} is considered. Extensions of this and other related results for a ϕ\phi-Laplacian differential operator with or without singularity (including the Minkowski operator for the relativistic acceleration) have been obtained in [8, 36] in the scalar case. We show now how the proof of Theorem 3.4 can be easily adapted to treat the case of a periodic forcing term with zero mean value, namely we deal with

{(ϕ(x))=ddt𝒢(x)+h(t,x)+p(t),x(0)=x(T),x(0)=x(T).\begin{cases}\,(\phi(x^{\prime}))^{\prime}=\dfrac{\mathrm{d}}{\mathrm{d}t}\nabla\mathcal{G}(x)+h(t,x)+p(t),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T).\end{cases} (3.11)
Theorem 3.5.

Let ϕ:nϕ(n)=n\phi\colon\mathbb{R}^{n}\to\phi(\mathbb{R}^{n})=\mathbb{R}^{n} be a homeomorphism satisfying (hϕ)(\textsc{h}_{\phi}). Let 𝒢:nn\mathcal{G}\colon\mathbb{R}^{n}\to\mathbb{R}^{n} be a 𝒞2\mathcal{C}^{2}-function. Let p:[0,T]np\colon\mathopen{[}0,T\mathclose{]}\to\mathbb{R}^{n} be a continuous function with 0Tp(t)dt=0\int_{0}^{T}p(t)\,\mathrm{d}t=0. Let h=h(t,x):[0,T]×nnh=h(t,x)\colon\mathopen{[}0,T\mathclose{]}\times\mathbb{R}^{n}\to\mathbb{R}^{n} be a continuous function such that

  • (hh+)(\textsc{h}_{\textsc{h}}^{+})

    there exists K0>0K_{0}>0 such that h(t,x),xK0\langle h(t,x),x\rangle\geq-K_{0}, for all xnx\in\mathbb{R}^{n}.

Moreover, suppose that at least one of the following three condition holds:

  • (i)(i)

    h(t,x),x+\langle h(t,x),x\rangle\to+\infty as x+\|x\|\to+\infty uniformly in tt;

  • (ii)(ii)

    for every ρ>0\rho>0 there exists Rρ>0R_{\rho}>0 such that h(x+y),x0\langle h(x+y),x\rangle\geq 0, for all (x,y)2n(x,y)\in\mathbb{R}^{2n} with x>Rρ\|x\|>R_{\rho} and yρ\|y\|\leq\rho;

  • (iii)(iii)

    there exists d>0d>0 such that, for every i=1,,ni=1,\ldots,n, hi(t,x)xi0h_{i}(t,x)x_{i}\geq 0, for every x=(x1,,xn)nx=(x_{1},\ldots,x_{n})\in\mathbb{R}^{n} with |xi|>d|x_{i}|>d.

Then, problem (3.11) has at least a solution.

Proof.

The proof is similar to the one of Theorem 3.4 and thus we only focus on the main modifications requested. We introduce the parameter-dependent problem

{(ϕ(x))=λddt𝒢(x)+hλ(t,x)+λp(t),x(0)=x(T),x(0)=x(T),\begin{cases}\,(\phi(x^{\prime}))^{\prime}=\lambda\dfrac{\mathrm{d}}{\mathrm{d}t}\nabla\mathcal{G}(x)+h_{\lambda}(t,x)+\lambda p(t),\\ \,x(0)=x(T),\quad x^{\prime}(0)=x^{\prime}(T),\end{cases} (3.12)

where hλ(t,x)h_{\lambda}(t,x) is defined as in (3.9). Since 0Tp(t)dt=0\int_{0}^{T}p(t)\,\mathrm{d}t=0, it is convenient to fix a TT-periodic continuously differentiable function P:NP\colon\mathbb{R}\to\mathbb{R}^{N} such that P(t)=p(t)P^{\prime}(t)=p(t). We divide the proof in some steps.

Step 1. A priori bound of xL1\|x^{\prime}\|_{L^{1}}. Let x()x(\cdot) be a solution of problem (3.12). By integrating the scalar product between x()x(\cdot) and the equation in (3.12), we have

0Tϕ(x(t)),x(t)dt\displaystyle\int_{0}^{T}\langle\phi(x^{\prime}(t)),x^{\prime}(t)\rangle\,\mathrm{d}t =0Thλ(x(t)),x(t)dtλ0Tp(t),x(t)dt.\displaystyle=-\int_{0}^{T}\langle h_{\lambda}(x(t)),x(t)\rangle\,\mathrm{d}t-\lambda\int_{0}^{T}\langle p(t),x(t)\rangle\,\mathrm{d}t. (3.13)
=0Thλ(x(t)),x(t)dt+λ0TP(t),x(t)dt.\displaystyle=-\int_{0}^{T}\langle h_{\lambda}(x(t)),x(t)\rangle\,\mathrm{d}t+\lambda\int_{0}^{T}\langle P(t),x^{\prime}(t)\rangle\,\mathrm{d}t.

Next, from hypothesis (hh+)(\textsc{h}_{\textsc{h}}^{+}) and the fact that λ[0,1]\lambda\in\mathopen{[}0,1\mathclose{]}, we deduce that

0Tϕ(x(t)),x(t)dtTK0+P0Tx(t)dt.\int_{0}^{T}\langle\phi(x^{\prime}(t)),x^{\prime}(t)\rangle\,\mathrm{d}t\leq TK_{0}+\|P\|_{\infty}\int_{0}^{T}\|x^{\prime}(t)\|\,\mathrm{d}t.

We fix η>P\eta>\|P\|_{\infty} and, by hypothesis (hϕ)(\textsc{h}_{\phi}), we obtain that

(ηP)0Tx(t)dtT(K0+M),(\eta-\|P\|_{\infty})\int_{0}^{T}\|x^{\prime}(t)\|\,\mathrm{d}t\leq T(K_{0}+M),

and so

xL1T(K0+M)ηP=:K1,\|x^{\prime}\|_{L^{1}}\leq\dfrac{T(K_{0}+M)}{\eta-\|P\|_{\infty}}=:K_{1},

which is the desired bound.

Step 2. A priori bound of x\|x\|_{\infty}. Without loss of generality, we can consider λ]0,1[\lambda\in\mathopen{]}0,1\mathclose{[}; indeed, an easy computation shows that for λ=0\lambda=0 the only TT-periodic solution is the trivial one. Let x()x(\cdot) be a solution of problem (3.12).

Assume condition (i)(i). From (3.13) we have

λ0Th(t,x(t)),x(t)dt+(1λ)0Tx(t)dtλPK1,\lambda\int_{0}^{T}\langle h(t,x(t)),x(t)\rangle\,\mathrm{d}t+(1-\lambda)\int_{0}^{T}\|x(t)\|\mathrm{d}t\leq\lambda\|P\|_{\infty}K_{1},

and so, dividing by λ>0\lambda>0,

0Th(t,x(t)),x(t)dtPK1.\int_{0}^{T}\langle h(t,x(t)),x(t)\rangle\,\mathrm{d}t\leq\|P\|_{\infty}K_{1}.

Let γ>PK1/T\gamma>\|P\|_{\infty}K_{1}/T. By (i)(i) there exists Rγ>0R_{\gamma}>0 such that h(t,x(t)),x(t)>γ\langle h(t,x(t)),x(t)\rangle>\gamma for all t[0,T]t\in\mathopen{[}0,T\mathclose{]} such that x(t)Rγ\|x(t)\|\geq R_{\gamma}. We immediately conclude that there exists t~[0,T]\tilde{t}\in\mathopen{[}0,T\mathclose{]} such that x(t~)<Rγ\|x(\tilde{t})\|<R_{\gamma}, otherwise a contradiction can be easily obtained. Then, arguing as in the proof of Theorem 3.4, we have that x<Rγ+K1T:=R\|x\|_{\infty}<R_{\gamma}+K_{1}T:=R^{*}.

Assume now condition (ii)(ii) or condition (iii)(iii). Let us also denote by x¯\bar{x} the mean value of x()x(\cdot). Let ν𝕊n1\nu\in\mathbb{S}^{n-1} (arbitrary). An integration of the scalar product between ν\nu and the equation in (3.12) gives

0Thλ(t,x(t)),νdt=λ0Tp(t),νdt=λ0Tp(t)dt,ν=0,\int_{0}^{T}\langle h_{\lambda}(t,x(t)),\nu\rangle\,\mathrm{d}t=\lambda\int_{0}^{T}\langle p(t),\nu\rangle\,\mathrm{d}t=\lambda\langle\int_{0}^{T}p(t)\mathrm{d}t,\nu\rangle=0,

which equivalently reads as

λ1T0Th(t,x(t)),νdt+(1λ)x¯,ν=0.\lambda\dfrac{1}{T}\int_{0}^{T}\langle h(t,x(t)),\nu\rangle\,\mathrm{d}t+(1-\lambda)\langle\bar{x},\nu\rangle=0. (3.14)

Let (ii)(ii) hold. If x¯0\bar{x}\neq 0, we set ν:=x¯/x¯\nu:=\bar{x}/\|\bar{x}\| and so 0Th(t,x(t)),x¯dt<0\int_{0}^{T}\langle h(t,x(t)),\bar{x}\rangle\,\mathrm{d}t<0. Then, there exists t~x¯[0,T]\tilde{t}_{\bar{x}}\in\mathopen{[}0,T\mathclose{]} such that h(t~x¯,x(t~x¯)),x¯<0\langle h(\tilde{t}_{\bar{x}},x(\tilde{t}_{\bar{x}})),\bar{x}\rangle<0. On the other hand, we have that x(t~x¯)x¯\|x(\tilde{t}_{\bar{x}})-\bar{x}\| is bounded. Indeed, let t^i[0,T]\hat{t}_{i}\in\mathopen{[}0,T\mathclose{]} be such that xi(t^i)=x¯ix_{i}(\hat{t}_{i})=\bar{x}_{i}, thus

|xi(t~x¯)x¯i|=|t~x¯t^ixi(s)ds|0T|xi(s)|ds0Tx(s)ds=xL1K1,|x_{i}(\tilde{t}_{\bar{x}})-\bar{x}_{i}|=\biggl{|}\int_{\tilde{t}_{\bar{x}}}^{\hat{t}_{i}}x_{i}^{\prime}(s)\,\mathrm{d}s\biggr{|}\leq\int_{0}^{T}|x_{i}^{\prime}(s)|\,\mathrm{d}s\leq\int_{0}^{T}\|x^{\prime}(s)\|\,\mathrm{d}s=\|x^{\prime}\|_{L^{1}}\leq K_{1},

and so x(t~x¯)x¯nK1\|x(\tilde{t}_{\bar{x}})-\bar{x}\|\leq\sqrt{n}\,K_{1}. Therefore, from x(t~x¯)=x¯+(x(t~x¯)x¯)x(\tilde{t}_{\bar{x}})=\bar{x}+(x(\tilde{t}_{\bar{x}})-\bar{x}) and (ii)(ii), we have that there exists R^>0\hat{R}>0 such that x¯<R^\|\bar{x}\|<\hat{R}. Clearly, the same inequality holds if x¯=0\bar{x}=0. Next, it is easy to prove that

|xi(t)||x¯i|+|xi(t)x¯i|x¯+xL1<R^+K1|x_{i}(t)|\leq|\bar{x}_{i}|+|x_{i}(t)-\bar{x}_{i}|\leq\|\bar{x}\|+\|x^{\prime}\|_{L^{1}}<\hat{R}+K_{1}

and thus x<n(R^+K1)=:R\|x\|_{\infty}<\sqrt{n}(\hat{R}+K_{1})=:R^{*}. Let (iii)(iii) hold. We prove that for every i=1,,ni=1,\ldots,n there exists t~i[0,T]\tilde{t}_{i}\in\mathopen{[}0,T\mathclose{]} such that xi(t~i)<d\|x_{i}(\tilde{t}_{i})\|<d. Indeed, let ν:=ei\nu:=e_{i}. From (3.14), we have

λ0Thi(t,x(t))dt+(1λ)0Txi(t)dt=0\lambda\int_{0}^{T}h_{i}(t,x(t))\,\mathrm{d}t+(1-\lambda)\int_{0}^{T}x_{i}(t)\,\mathrm{d}t=0

and, proceeding by contradiction, we easily reach the claim. Then, arguing as above, we have that x<n(d+K1)=:R\|x\|_{\infty}<\sqrt{n}(d+K_{1})=:R^{*}.

As a consequence, the open ball G=B(0,R)G=B(0,R^{*}) is (trivially) a bound set for system (3.8).

Step 3. Conclusion. From

(ϕ(x))L1Hess𝒢(x)xL1+Thλ(,x)+pL1,\|(\phi(x^{\prime}))^{\prime}\|_{L^{1}}\leq\|\mathrm{Hess}\,\mathcal{G}(x)\|_{\infty}\|x^{\prime}\|_{L^{1}}+T\|h_{\lambda}(\cdot,x)\|_{\infty}+\|p\|_{L^{1}},

we have that (ϕ(x()))(\phi(x^{\prime}(\cdot)))^{\prime} is bounded in L1L^{1} and we conclude as above. ∎

Remark 3.2.

Theorem 3.5 in the variant (i)(i) provides an extension of [45, Theorem 3.3], where the result has been proved for ϕ=ϕp\phi=\phi_{p} and h(t,x)=h(x)h(t,x)=h(x) a conservative vector field satisfying the more restrictive condition h(x),xbxαc\langle h(x),x\rangle\geq b\|x\|^{\alpha}-c for every xnx\in\mathbb{R}^{n}, with b>0b>0, c0c\geq 0 and α>1\alpha>1.

Conditions (ii)(ii) and (iii)(iii) are classical ones in this context for vector second-order systems of Liénard-type (cf. [15, 28, 43, 56]). Observe that both conditions are satisfied in the one-dimensional case if we assume the sign-condition h(t,x)x0h(t,x)x\geq 0 for every tt and xx with |x|>d>0|x|>d>0. Thus, Theorem 3.5 extends to a large class of ϕ\phi-Laplacian differential systems the classical theorem of Reissig mentioned above. \lhd

Remark 3.3.

Some comments on the hypotheses of Theorem 3.5 are in order. First of all, we notice that, in dimension n=1n=1, condition (i)(i) implies the validity of (ii)(ii) and (iii)(iii), which are equivalent each other. On the other hand, the function

q(x)=xe|x|,x,q(x)=xe^{-|x|},\quad x\in\mathbb{R}, (3.15)

satisfies (ii)(ii) and (iii)(iii), but not (i)(i). In this case, q(x)x0q(x)x\geq 0 for every xx\in\mathbb{R} and thus (hh+)(\textsc{h}_{\textsc{h}}^{+}) follows.

We focus on the case n2n\geq 2. In order to show that (i)(i), (ii)(ii), (iii)(iii) are independent, we are going to present three examples for which exactly one of the hypotheses is valid. Every example is given for n=2n=2, however it can be easily generalized to treat the nn-dimensional case for a general n2n\geq 2. Moreover, in each example condition (hh+)(\textsc{h}_{\textsc{h}}^{+}) can be straightforwardly checked.

Example 1. Let ε]0,π1[\varepsilon\in\mathopen{]}0,\pi^{-1}\mathclose{[}. Let us consider the function

h(x1,x2)=(x12x2+εarctanx1,x2+εarctanx2),x=(x1,x2)2.h(x_{1},x_{2})=\bigl{(}x_{1}-2x_{2}+\varepsilon\arctan x_{1},x_{2}+\varepsilon\arctan x_{2}\bigr{)},\quad x=(x_{1},x_{2})\in\mathbb{R}^{2}.

We observe that

h(x),x=(x1x2)2+x1εarctanx1+x2εarctanx2ε(x1arctanx1+x2arctanx2),\langle h(x),x\rangle=(x_{1}-x_{2})^{2}+x_{1}\varepsilon\arctan x_{1}+x_{2}\varepsilon\arctan x_{2}\geq\varepsilon(x_{1}\arctan x_{1}+x_{2}\arctan x_{2}),

which tends to ++\infty as x+\|x\|\to+\infty. Therefore, (i)(i) holds. Moreover, we have

h(x+y),x=(x1x2)2+x1εarctan(x1+y1)+x2εarctan(x2+y2)+x1y1+y2(x22x1).\langle h(x+y),x\rangle=(x_{1}-x_{2})^{2}+x_{1}\varepsilon\arctan(x_{1}+y_{1})+x_{2}\varepsilon\arctan(x_{2}+y_{2})+x_{1}y_{1}+y_{2}(x_{2}-2x_{1}).

Let x=(s,s)x=(s,s), s>0s>0, and y=(1,0)y=(-1,0). Therefore,

h(x+y),x=εs(arctan(s1)+arctans)ss(επ1)<0.\langle h(x+y),x\rangle=\varepsilon s(\arctan(s-1)+\arctan s)-s\leq s(\varepsilon\pi-1)<0.

Hence, (ii)(ii) does not hold. Let again x=(s,s)x=(s,s), s>0s>0, then h1(x)x1=s2+εsarctans<0h_{1}(x)x_{1}=-s^{2}+\varepsilon s\arctan s<0 for ss sufficiently large. Therefore, (iii)(iii) does not hold.

Example 2. Let us consider the function

h(x1,x2)=((x1x2)q(x),x2q(x)),x=(x1,x2)2,h(x_{1},x_{2})=\bigl{(}(x_{1}-x_{2})q(\|x\|),x_{2}q(\|x\|)\bigr{)},\quad x=(x_{1},x_{2})\in\mathbb{R}^{2},

where qq is defined as in (3.15). We observe that

h(x),x=(x12x1x2+x22)q(x)32x2q(x),\langle h(x),x\rangle=(x_{1}^{2}-x_{1}x_{2}+x_{2}^{2})q(\|x\|)\leq\dfrac{3}{2}\|x\|^{2}q(\|x\|),

which tends to 0 as x+\|x\|\to+\infty. Therefore, (i)(i) does not hold. Moreover,

h(x+y),x\displaystyle\langle h(x+y),x\rangle =(x12x1x2+x22+x1y1x1y2+x2y2)q(x+y)\displaystyle=(x_{1}^{2}-x_{1}x_{2}+x_{2}^{2}+x_{1}y_{1}-x_{1}y_{2}+x_{2}y_{2})q(\|x+y\|)
(12x23xy)q(x+y)0\displaystyle\geq\biggl{(}\dfrac{1}{2}\|x\|^{2}-3\|x\|\|y\|\biggr{)}q(\|x+y\|)\geq 0

whenever x6y\|x\|\geq 6\|y\| and y\|y\| is bounded. Therefore, (ii)(ii) holds.

For x=(s,2s)x=(s,2s), s>0s>0, we have h1(x)x1=s2q(|s|)<0h_{1}(x)x_{1}=-s^{2}q(|s|)<0. Hence, (iii)(iii) does not hold.

Example 3. Let us consider the function

h(x1,x2)=((x133x1)q(|x1|),(x233x2)q(|x2|)),x=(x1,x2)2.h(x_{1},x_{2})=\bigl{(}(x_{1}^{3}-3x_{1})q(|x_{1}|),(x_{2}^{3}-3x_{2})q(|x_{2}|)\bigr{)},\quad x=(x_{1},x_{2})\in\mathbb{R}^{2}.

Let x=(s,1)x=(s,1), s>0s>0. The quantity

h(x),x=x12(x123)q(|x1|)+x22(x223)q(|x2|)=s2(s23)q(|s|)2q(1)\langle h(x),x\rangle=x_{1}^{2}(x_{1}^{2}-3)q(|x_{1}|)+x_{2}^{2}(x_{2}^{2}-3)q(|x_{2}|)=s^{2}(s^{2}-3)q(|s|)-2q(1)

tends to 2e1<0-2e^{-1}<0 as s+s\to+\infty. Therefore, (i)(i) and (ii)(ii) (with y=0y=0) do not hold. For every i{1,2}i\in\{1,2\}, we notice that

hi(x)xi=xi2(xi23)q(|xi|)0,h_{i}(x)x_{i}=x_{i}^{2}(x_{i}^{2}-3)q(|x_{i}|)\geq 0,

for every x2x\in\mathbb{R}^{2} with |xi|>3|x_{i}|>\sqrt{3}. Therefore, (iii)(iii) holds. \lhd

Remark 3.4.

We observe that one could add to the list of hypotheses (i)(i)(iii)(iii) in Theorem 3.5 another classical condition, that is the generalized Villari condition (cf. [26, p. 381]), which, in our context, reads as follows:

  • there exists d>0d>0 such that 0Thi(t,x(t))dt0\int_{0}^{T}h_{i}(t,x(t))\,\mathrm{d}t\neq 0 for some i=1,,ni=1,\ldots,n, for every x=(x1,,xn)x=(x_{1},\ldots,x_{n})\in\mathbb{R} with |xj|>d|x_{j}|>d for some j=1,,nj=1,\ldots,n.

It is worth noticing that condition (iii)(iii) with the strict inequalities is a special case of the generalized Villari condition. On the other hand, in Example 2 and Example 3 of Remark 3.3, if we consider the maps h(t,x)h(t,x) multiplied by a scalar function ρ(x)\rho(\|x\|) which vanishes outside a large open ball, the examples continue to satisfy (ii)(ii) and, respectively, (iii)(iii), but the generalized Villari condition does not hold. \lhd

Appendix A Remarks on the convexity of a sublevel set

In this appendix, we propose an alternative proof of Lemma 3.1 based on a classical result about convex sets, namely the Tietze–Nakajima theorem [42, 54], that we recall for reader’s convenience (see also [21, 48] for more general versions of the result). A set DnD\subseteq\mathbb{R}^{n} is locally convex if each point of DD has a neighborhood whose intersection with DD is convex (cf. [25, Section 17]). Then, the following result holds (cf. [25, 55] for the proof).

Theorem A.1 (Tietze–Nakajima).

A closed connected locally convex set in a Euclidean space is convex.

We now give the proof of Lemma 3.1.

Proof of Lemma 3.1.

Let V:nV\colon\mathbb{R}^{n}\to\mathbb{R} be a 𝒞2\mathcal{C}^{2}-function satisfying (3.2) for some cc\in\mathbb{R} with D=[Vc]D=[V\leq c] nonempty, bounded and connected. Let us assume that

  • (C)(C)

    for all uDu\in\partial D, V′′(u)y,y0\langle V^{\prime\prime}(u)y,y\rangle\geq 0, for all yny\in\mathbb{R}^{n} with V(u),y=0\langle V^{\prime}(u),y\rangle=0.

holds and we will prove that DD is convex. By Tietze–Nakajima theorem it is sufficient to verify that DD is locally convex. Accordingly, let u0u_{0} be an arbitrary but fixed point in D\partial D and we aim to prove that there exists a neighborhood UU of u0u_{0} such that DUD\cap U is convex. Recalling that V(u0)0V^{\prime}(u_{0})\neq 0 by assumption (3.2), we define the vector w:=V(u0)/V(u0)w:=V^{\prime}(u_{0})/\|V^{\prime}(u_{0})\|. Let W:={zn:z,w=0}W:=\{z\in\mathbb{R}^{n}\colon\langle z,w\rangle=0\}, that is the subspace (of dimension n1n-1) of n\mathbb{R}^{n} orthogonal to the vector ww. Since every xnx\in\mathbb{R}^{n} can be uniquely written as x=u0+αw+zx=u_{0}+\alpha w+z for (α,z)×W(\alpha,z)\in\mathbb{R}\times W, we can equivalently consider the function

𝒱(α,z):=V(u0+αw+z).\mathcal{V}(\alpha,z):=V(u_{0}+\alpha w+z).

Thus, our goal reduces to prove that there exists a neighborhood 𝒰\mathcal{U} of (0,0)(0,0) in the (α,z)(\alpha,z)-space ×W\mathbb{R}\times W such that 𝒟𝒰\mathcal{D}\cap\mathcal{U} is convex, where

𝒟:={(α,z)×W:V(u0+αw+z)c}.\mathcal{D}:=\bigl{\{}(\alpha,z)\in\mathbb{R}\times W\colon V(u_{0}+\alpha w+z)\leq c\bigr{\}}.

We observe that α𝒱(0,0)=V(u0),w=V(u0)>0\partial_{\alpha}\mathcal{V}(0,0)=\langle V^{\prime}(u_{0}),w\rangle=\|V^{\prime}(u_{0})\|>0 and thus, by the implicit function theorem, there exist a neighborhood of (0,0)(0,0) of the form ]ε,ε[×B(0,ε)\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}\times B(0,\varepsilon) and a continuously differentiable map φ:B(0,ε)]ε,ε[\varphi\colon B(0,\varepsilon)\to\mathopen{]}-\varepsilon,\varepsilon\mathclose{[} such that

V(u0+αw+z)=cif and only ifα=φ(z),V(u_{0}+\alpha w+z)=c\quad\text{if and only if}\quad\alpha=\varphi(z), (A.1)

for every (α,z)]ε,ε[×B(0,ε)(\alpha,z)\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}\times B(0,\varepsilon). Here, B(0,ε)B(0,\varepsilon) is an open neighborhood of the origin in Wn1W\cong\mathbb{R}^{n-1}. Without loss of generality, we assume also that V(ξ),w>0\langle V^{\prime}(\xi),w\rangle>0 for all ξ]ε,ε[×B(0,ε)\xi\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}\times B(0,\varepsilon). Hence, it will be sufficient to verify that the set

𝒟𝒰={(α,z)]ε,ε[×B(0,ε):αφ(z)}\mathcal{D}\cap\mathcal{U}=\bigl{\{}(\alpha,z)\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}\times B(0,\varepsilon)\colon\alpha\leq\varphi(z)\bigr{\}}

is convex. Let (α1,z1),(α2,z2)𝒟𝒰(\alpha_{1},z_{1}),(\alpha_{2},z_{2})\in\mathcal{D}\cap\mathcal{U} and set v:=(z2z1)/z2z1v:=(z_{2}-z_{1})/\|z_{2}-z_{1}\| if z1z2z_{1}\neq z_{2} and vv arbitrary with v=1\|v\|=1 otherwise. Then, to check the (local) convexity we can restrict ourselves to the intersection of 𝒟𝒰\mathcal{D}\cap\mathcal{U} with the 22-dimensional subspace Σ\Sigma of n\mathbb{R}^{n} spanned by vv and ww. We set

(β):=V(u0+φ(βv)w+βv)=c,ϑ(β):=φ(βv),for every β]ε,ε[.\ell(\beta):=V(u_{0}+\varphi(\beta v)w+\beta v)=c,\quad\vartheta(\beta):=\varphi(\beta v),\quad\text{for every $\beta\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}$.}

Then, for every β]ε,ε[\beta\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}, we have

(β)=V(u0+ϑ(β)w+βv),ϑ(β)w+v=V(u),y=0,\ell^{\prime}(\beta)=\langle V^{\prime}(u_{0}+\vartheta(\beta)w+\beta v),\vartheta^{\prime}(\beta)w+v\rangle=\langle V^{\prime}(u),y\rangle=0,

where we have set

u:=u0+ϑ(β)w+βv,y:=ϑ(β)w+v.u:=u_{0}+\vartheta(\beta)w+\beta v,\quad y:=\vartheta^{\prime}(\beta)w+v.

Moreover, for every β]ε,ε[\beta\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}, it holds that

′′(β)\displaystyle\ell^{\prime\prime}(\beta) =V′′(u0+ϑ(β)w+βv)(ϑ(β)w+v),ϑ(β)w+v\displaystyle=\langle V^{\prime\prime}(u_{0}+\vartheta(\beta)w+\beta v)(\vartheta^{\prime}(\beta)w+v),\vartheta^{\prime}(\beta)w+v\rangle
+V(u0+ϑ(β)w+βv),ϑ′′(β)w\displaystyle\quad+\langle V^{\prime}(u_{0}+\vartheta(\beta)w+\beta v),\vartheta^{\prime\prime}(\beta)w\rangle
=V′′(u)y,y+ϑ′′(β)V(u),w=0.\displaystyle=\langle V^{\prime\prime}(u)y,y\rangle+\vartheta^{\prime\prime}(\beta)\langle V^{\prime}(u),w\rangle=0.

By hypothesis (C)(C) we conclude that ϑ′′(β)0\vartheta^{\prime\prime}(\beta)\leq 0 for all β]ε,ε[\beta\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}, which implies that the subgraph of φ\varphi restricted to 𝒟𝒰Σ\mathcal{D}\cap\mathcal{U}\cap\Sigma is convex.

Conversely, assume that DD is convex. If condition (C)(C) is not satisfied there exists u0Du_{0}\in\partial D such that V′′(u0)v1,v1<0\langle V^{\prime\prime}(u_{0})v_{1},v_{1}\rangle<0 for some vector v1nv_{1}\in\mathbb{R}^{n} with v1=1\|v_{1}\|=1 and V(u0),v1=0\langle V^{\prime}(u_{0}),v_{1}\rangle=0. Arguing as in the previous part of the proof, we introduce the vector w:=V(u0)/V(u0)w:=V^{\prime}(u_{0})/\|V^{\prime}(u_{0})\| and, using the implicit function theorem we find a neighborhood of (0,0)(0,0) of the form ]ε,ε[×B(0,ε)\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}\times B(0,\varepsilon) and a continuously differentiable map φ:B(0,ε)]ε,ε[\varphi\colon B(0,\varepsilon)\to\mathopen{]}-\varepsilon,\varepsilon\mathclose{[} such that (A.1) holds for every (α,z)]ε,ε[×B(0,ε)(\alpha,z)\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}\times B(0,\varepsilon). As a next step, we consider the intersection of 𝒟𝒰\mathcal{D}\cap\mathcal{U} with the 22-dimensional subspace Σ\Sigma of n\mathbb{R}^{n} spanned by v1v_{1} and ww. By the convexity of DD it follows that the set

𝒜:={(α,β)]ε,ε[×]ε,ε[:αφ(βv1)}\mathcal{A}:=\bigl{\{}(\alpha,\beta)\in\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}\times\mathopen{]}-\varepsilon,\varepsilon\mathclose{[}\colon\alpha\leq\varphi(\beta v_{1})\bigr{\}}

is convex. On the other hand, setting as above (β):=V(u0+φ(βv1)w+βv1)\ell(\beta):=V(u_{0}+\varphi(\beta v_{1})w+\beta v_{1}) and ϑ(β):=φ(βv1)\vartheta(\beta):=\varphi(\beta v_{1}), we obtain

0\displaystyle 0 =(β)=V(u0+ϑ(β)w+βv1),ϑ(β)w+v1\displaystyle=\ell^{\prime}(\beta)=\langle V^{\prime}(u_{0}+\vartheta(\beta)w+\beta v_{1}),\vartheta^{\prime}(\beta)w+v_{1}\rangle
0\displaystyle 0 =′′(β)=V′′(u0+ϑ(β)w+βv1)(ϑ(β)w+v1),ϑ(β)w+v1\displaystyle=\ell^{\prime\prime}(\beta)=\langle V^{\prime\prime}(u_{0}+\vartheta(\beta)w+\beta v_{1})(\vartheta^{\prime}(\beta)w+v_{1}),\vartheta^{\prime}(\beta)w+v_{1}\rangle
+V(u0+ϑ(β)w+βv1),ϑ′′(β)w.\displaystyle\qquad\qquad\quad+\langle V^{\prime}(u_{0}+\vartheta(\beta)w+\beta v_{1}),\vartheta^{\prime\prime}(\beta)w\rangle.

Hence, for β=0\beta=0, we have that ϑ(0)V(u0)=V(u0),v1=0\vartheta^{\prime}(0)\|V^{\prime}(u_{0})\|=-\langle V^{\prime}(u_{0}),v_{1}\rangle=0, which implies ϑ(0)=0\vartheta^{\prime}(0)=0, and that ϑ′′(0)V(u0)=V′′(u0)v1,v1>0\vartheta^{\prime\prime}(0)\|V^{\prime}(u_{0})\|=-\langle V^{\prime\prime}(u_{0})v_{1},v_{1}\rangle>0, which implies ϑ′′(0)>0\vartheta^{\prime\prime}(0)>0. Therefore, the map βφ(βv1)\beta\mapsto\varphi(\beta v_{1}) is strictly convex in a neighborhood ]δ,δ[\mathopen{]}-\delta,\delta\mathclose{[} of the origin for a suitable δ]0,ε]\delta\in\mathopen{]}0,\varepsilon\mathclose{]}. This clearly contradicts the convexity of the set 𝒜\mathcal{A}. The proof is completed. ∎

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