Abstract <p>The version of the three-dimensional Inverse Problem of Newtonian dynamics considered here is the following: given a family of spatial curves in the form <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(f(x,y,z)=k_{1}\)</EquationSource> <!--LobJMat2560926Kotoulas-m1--> </InlineEquation>, <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(g(x,y,z)=k_{2}\)</EquationSource> <!--LobJMat2560926Kotoulas-m2--> </InlineEquation> (<InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(k_{1}\)</EquationSource> <!--LobJMat2560926Kotoulas-m3--> </InlineEquation>, <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(k_{2}=\text{const}\)</EquationSource> <!--LobJMat2560926Kotoulas-m4--> </InlineEquation>), find all the potentials <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(V=F(u,w)\)</EquationSource> <!--LobJMat2560926Kotoulas-m5--> </InlineEquation>, where <InlineEquation ID="IEq6"> <EquationSource Format="TEX">\(u=u(x,y,z)\)</EquationSource> <!--LobJMat2560926Kotoulas-m6--> </InlineEquation>, <InlineEquation ID="IEq7"> <EquationSource Format="TEX">\(w=w(x,y,z)\)</EquationSource> <!--LobJMat2560926Kotoulas-m7--> </InlineEquation>, which give rise to this two-parametric family of orbits. Each family of orbits is represented uniquely by a pair of ‘‘<i>slope functions</i>’’ <InlineEquation ID="IEq8"> <EquationSource Format="TEX">\(\alpha=\alpha(x,y,z)\)</EquationSource> <!--LobJMat2560926Kotoulas-m8--> </InlineEquation> and <InlineEquation ID="IEq9"> <EquationSource Format="TEX">\(\beta=\beta(x,y,z)\)</EquationSource> <!--LobJMat2560926Kotoulas-m9--> </InlineEquation>. The solution of this problem is based on two linear partial differential equations (PDEs) in the unknown potential function <InlineEquation ID="IEq10"> <EquationSource Format="TEX">\(V=V(x,y,z)\)</EquationSource> <!--LobJMat2560926Kotoulas-m10--> </InlineEquation>. In the present work, we establish three differential conditions for the slope functions (<InlineEquation ID="IEq11"> <EquationSource Format="TEX">\(\alpha,\;\beta\)</EquationSource> <!--LobJMat2560926Kotoulas-m11--> </InlineEquation>). If these are satisfied, then they guarantee the existence of such a potential and it is found by quadratures. Pertinent examples are given and the families of straight lines are studied separately.</p>

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On Analytical Solutions of the 3D Inverse Problem of Newtonian Dynamics

  • Th. Kotoulas

摘要

Abstract

The version of the three-dimensional Inverse Problem of Newtonian dynamics considered here is the following: given a family of spatial curves in the form \(f(x,y,z)=k_{1}\) , \(g(x,y,z)=k_{2}\) ( \(k_{1}\) , \(k_{2}=\text{const}\) ), find all the potentials \(V=F(u,w)\) , where \(u=u(x,y,z)\) , \(w=w(x,y,z)\) , which give rise to this two-parametric family of orbits. Each family of orbits is represented uniquely by a pair of ‘‘slope functions’’ \(\alpha=\alpha(x,y,z)\) and \(\beta=\beta(x,y,z)\) . The solution of this problem is based on two linear partial differential equations (PDEs) in the unknown potential function \(V=V(x,y,z)\) . In the present work, we establish three differential conditions for the slope functions ( \(\alpha,\;\beta\) ). If these are satisfied, then they guarantee the existence of such a potential and it is found by quadratures. Pertinent examples are given and the families of straight lines are studied separately.