<p>We consider time-periodic Hamiltonians of the form <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="30_2025_1024_Article_IEq1.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="91" /> </InlineMediaObject> <EquationSource Format="TEX">\(H(t, {\textbf {Q}}, {\textbf {P}}, \epsilon )\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>H</mi> <mo stretchy="false">(</mo> <mi>t</mi> <mo>,</mo> <mi mathvariant="bold">Q</mi> <mo>,</mo> <mi mathvariant="bold">P</mi> <mo>,</mo> <mi>ϵ</mi> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> where <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="30_2025_1024_Article_IEq2.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="10" /> </InlineMediaObject> <EquationSource Format="TEX">\(\epsilon \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>ϵ</mi> </math></EquationSource> </InlineEquation> is a small parameter: The unperturbed function <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="30_2025_1024_Article_IEq3.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="181" /> </InlineMediaObject> <EquationSource Format="TEX">\(H_0({\textbf {Q}}, {\textbf {P}})=H(t,{\textbf {Q}}, {\textbf {P}}, 0)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>H</mi> <mn>0</mn> </msub> <mrow> <mo stretchy="false">(</mo> <mi mathvariant="bold">Q</mi> <mo>,</mo> <mi mathvariant="bold">P</mi> <mo stretchy="false">)</mo> </mrow> <mo>=</mo> <mi>H</mi> <mrow> <mo stretchy="false">(</mo> <mi>t</mi> <mo>,</mo> <mi mathvariant="bold">Q</mi> <mo>,</mo> <mi mathvariant="bold">P</mi> <mo>,</mo> <mn>0</mn> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation> is autonomous, integrable and has periodic solutions. It is assumed that these Hamiltonian functions can be written in convenient symplectic coordinates in the form <Equation ID="Equ109"> <MediaObject> <ImageObject Color="BlackWhite" FileRef="30_2025_1024_Article_Equ109.gif" Format="GIF" Height="22" Rendition="HTML" Resolution="72" Type="Linedraw" Width="465" /> </MediaObject> <EquationSource Format="TEX">\(\begin{aligned} H(t,\theta , \phi ,{\textbf {q}}, I, J, {\textbf {p}},\epsilon )=H_0(I,J)+\epsilon H_1(t,\theta , \phi ,{\textbf {q}}, I, J,{\textbf {p}})+\mathcal {O}(\epsilon ^2), \end{aligned}\)</EquationSource> <EquationSource Format="MATHML"><math display="block"> <mrow> <mtable> <mtr> <mtd columnalign="right"> <mrow> <mi>H</mi> <mrow> <mo stretchy="false">(</mo> <mi>t</mi> <mo>,</mo> <mi>θ</mi> <mo>,</mo> <mi>ϕ</mi> <mo>,</mo> <mi mathvariant="bold">q</mi> <mo>,</mo> <mi>I</mi> <mo>,</mo> <mi>J</mi> <mo>,</mo> <mi mathvariant="bold">p</mi> <mo>,</mo> <mi>ϵ</mi> <mo stretchy="false">)</mo> </mrow> <mo>=</mo> <msub> <mi>H</mi> <mn>0</mn> </msub> <mrow> <mo stretchy="false">(</mo> <mi>I</mi> <mo>,</mo> <mi>J</mi> <mo stretchy="false">)</mo> </mrow> <mo>+</mo> <mi>ϵ</mi> <msub> <mi>H</mi> <mn>1</mn> </msub> <mrow> <mo stretchy="false">(</mo> <mi>t</mi> <mo>,</mo> <mi>θ</mi> <mo>,</mo> <mi>ϕ</mi> <mo>,</mo> <mi mathvariant="bold">q</mi> <mo>,</mo> <mi>I</mi> <mo>,</mo> <mi>J</mi> <mo>,</mo> <mi mathvariant="bold">p</mi> <mo stretchy="false">)</mo> </mrow> <mo>+</mo> <mi mathvariant="script">O</mi> <mrow> <mo stretchy="false">(</mo> <msup> <mi>ϵ</mi> <mn>2</mn> </msup> <mo stretchy="false">)</mo> </mrow> <mo>,</mo> </mrow> </mtd> </mtr> </mtable> </mrow> </math></EquationSource> </Equation>where <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="30_2025_1024_Article_IEq4.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="59" /> </InlineMediaObject> <EquationSource Format="TEX">\(\theta ,\phi \in \mathbb {T}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>θ</mi> <mo>,</mo> <mi>ϕ</mi> <mo>∈</mo> <mi mathvariant="double-struck">T</mi> </mrow> </math></EquationSource> </InlineEquation>, <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="30_2025_1024_Article_IEq5.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="60" /> </InlineMediaObject> <EquationSource Format="TEX">\(I,J\in \mathbb {R}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>I</mi> <mo>,</mo> <mi>J</mi> <mo>∈</mo> <mi mathvariant="double-struck">R</mi> </mrow> </math></EquationSource> </InlineEquation>, <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="30_2025_1024_Article_IEq6.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="69" /> </InlineMediaObject> <EquationSource Format="TEX">\({\textbf {q}}, {\textbf {p}}\in \mathbb {R}^n\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi mathvariant="bold">q</mi> <mo>,</mo> <mi mathvariant="bold">p</mi> <mo>∈</mo> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mi>n</mi> </msup> </mrow> </math></EquationSource> </InlineEquation>. The aim of this paper is to show the existence of periodic solutions of the previous family of time-dependent <InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="30_2025_1024_Article_IEq7.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="21" /> </InlineMediaObject> <EquationSource Format="TEX">\(2\pi \)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mn>2</mn> <mi>π</mi> </mrow> </math></EquationSource> </InlineEquation>-periodically perturbed Hamiltonian systems under different approaches.</p>

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Periodic solutions of time-dependent perturbed Hamiltonian systems

  • Angelo Alberti,
  • Claudio Vidal

摘要

We consider time-periodic Hamiltonians of the form \(H(t, {\textbf {Q}}, {\textbf {P}}, \epsilon )\) H ( t , Q , P , ϵ ) where \(\epsilon \) ϵ is a small parameter: The unperturbed function \(H_0({\textbf {Q}}, {\textbf {P}})=H(t,{\textbf {Q}}, {\textbf {P}}, 0)\) H 0 ( Q , P ) = H ( t , Q , P , 0 ) is autonomous, integrable and has periodic solutions. It is assumed that these Hamiltonian functions can be written in convenient symplectic coordinates in the form \(\begin{aligned} H(t,\theta , \phi ,{\textbf {q}}, I, J, {\textbf {p}},\epsilon )=H_0(I,J)+\epsilon H_1(t,\theta , \phi ,{\textbf {q}}, I, J,{\textbf {p}})+\mathcal {O}(\epsilon ^2), \end{aligned}\) H ( t , θ , ϕ , q , I , J , p , ϵ ) = H 0 ( I , J ) + ϵ H 1 ( t , θ , ϕ , q , I , J , p ) + O ( ϵ 2 ) , where \(\theta ,\phi \in \mathbb {T}\) θ , ϕ T , \(I,J\in \mathbb {R}\) I , J R , \({\textbf {q}}, {\textbf {p}}\in \mathbb {R}^n\) q , p R n . The aim of this paper is to show the existence of periodic solutions of the previous family of time-dependent \(2\pi \) 2 π -periodically perturbed Hamiltonian systems under different approaches.