<p>We prove the integrability of magnetic geodesic flows of <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq2.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="49" /> </InlineMediaObject> <EquationSource Format="TEX">\(SO(n)\)</EquationSource> </InlineEquation>-invariant Riemannian metrics on the rank two Stefel variety <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq1.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="28" /> </InlineMediaObject> <EquationSource Format="TEX">\(V_{n,2}\)</EquationSource> </InlineEquation> with respect to the magnetic field <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq4.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="33" /> </InlineMediaObject> <EquationSource Format="TEX">\(\eta d\alpha\)</EquationSource> </InlineEquation>, where <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq5.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="14" /> </InlineMediaObject> <EquationSource Format="TEX">\(\alpha\)</EquationSource> </InlineEquation> is the standard contact form on <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq1.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="28" /> </InlineMediaObject> <EquationSource Format="TEX">\(V_{n,2}\)</EquationSource> </InlineEquation> and <InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq7.gif" Format="GIF" Height="12" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\(\eta\)</EquationSource> </InlineEquation> is a real parameter.Also, we prove the integrability of magnetic sub-Riemannian geodesic flows for <InlineEquation ID="IEq8"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq2.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="49" /> </InlineMediaObject> <EquationSource Format="TEX">\(SO(n)\)</EquationSource> </InlineEquation>-invariant sub-Riemannian structures on <InlineEquation ID="IEq9"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq1.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="28" /> </InlineMediaObject> <EquationSource Format="TEX">\(V_{n,2}\)</EquationSource> </InlineEquation>. All statements in the limit <InlineEquation ID="IEq10"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq10.gif" Format="GIF" Height="16" Rendition="HTML" Resolution="72" Type="Linedraw" Width="42" /> </InlineMediaObject> <EquationSource Format="TEX">\(\eta=0\)</EquationSource> </InlineEquation> imply the integrability of the problems without the influence of the magnetic field. We also consider integrable pendulum-type natural mechanical systems with the kinetic energy defined by <InlineEquation ID="IEq11"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq11.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="115" /> </InlineMediaObject> <EquationSource Format="TEX">\(SO(n)\times SO(2)\)</EquationSource> </InlineEquation>-invariant Riemannian metrics. For <InlineEquation ID="IEq12"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq12.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="42" /> </InlineMediaObject> <EquationSource Format="TEX">\(n=3\)</EquationSource> </InlineEquation>, using the isomorphism <InlineEquation ID="IEq13"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11819_2025_7273_Article_IEq13.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="95" /> </InlineMediaObject> <EquationSource Format="TEX">\(V_{3,2}\cong SO(3)\)</EquationSource> </InlineEquation>, the obtained integrable magnetic models reduce tointegrable cases of the motion of a heavy rigid body with a gyrostat around a fixed point:the Zhukovskiy – Volterra gyrostat, the Lagrange top with a gyrostat, and the Kowalevskitop with a gyrostat. As a by-product we obtain the Lax presentations for the Lagrangegyrostat and the Kowalevski gyrostat in the fixed reference frame (dual Lax representations).</p>

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Contact Magnetic Geodesic and Sub-Riemannian Flows on \(V_{n,2}\) and Integrable Cases of a Heavy Rigid Body with a Gyrostat

  • Božidar Jovanović

摘要

We prove the integrability of magnetic geodesic flows of \(SO(n)\) -invariant Riemannian metrics on the rank two Stefel variety \(V_{n,2}\) with respect to the magnetic field \(\eta d\alpha\) , where \(\alpha\) is the standard contact form on \(V_{n,2}\) and \(\eta\) is a real parameter.Also, we prove the integrability of magnetic sub-Riemannian geodesic flows for \(SO(n)\) -invariant sub-Riemannian structures on \(V_{n,2}\) . All statements in the limit \(\eta=0\) imply the integrability of the problems without the influence of the magnetic field. We also consider integrable pendulum-type natural mechanical systems with the kinetic energy defined by \(SO(n)\times SO(2)\) -invariant Riemannian metrics. For \(n=3\) , using the isomorphism \(V_{3,2}\cong SO(3)\) , the obtained integrable magnetic models reduce tointegrable cases of the motion of a heavy rigid body with a gyrostat around a fixed point:the Zhukovskiy – Volterra gyrostat, the Lagrange top with a gyrostat, and the Kowalevskitop with a gyrostat. As a by-product we obtain the Lax presentations for the Lagrangegyrostat and the Kowalevski gyrostat in the fixed reference frame (dual Lax representations).