First, we give an explicit description of all the mappings from the phace space of the Kepler problem to the phase space of the geodesics on the sphere, which transform the constants of motion of the Kepler problem to the angular momentum. Second, among these we describe those mappings which in addition send Kepler solutions to parametrized geodesics. Third, we describe those mappings which in addition are canonical transformations of the respective phase space. Finally we prove that among these the Ligon-Schaaf map is the unique one which maps the collison orbits to the geodesics which pass through the north pole. In this way we also give a new proof that the Ligon-Schaaf map has all the properties described above
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
peer reviewedThe paper gives an exact vectorial solution to the Kepler problem. A vectorial regulari...
First, we give an explicit description of all the mappings from the phace space of the Kepler proble...
First, we give an explicit description of all the mappings from the phace space of the Kepler proble...
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
In 1970, Moser showed that the Hamiltonian flow of the Kepler problem in R^n for a fixed negative en...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
peer reviewedThe paper gives an exact vectorial solution to the Kepler problem. A vectorial regulari...
First, we give an explicit description of all the mappings from the phace space of the Kepler proble...
First, we give an explicit description of all the mappings from the phace space of the Kepler proble...
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
The Ligon-Schaaf regularization (LS mapping) was introduced in 1976 and has been used several times....
In 1970, Moser showed that the Hamiltonian flow of the Kepler problem in R^n for a fixed negative en...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
The KS regularization connects the dynamics of the harmonic oscillator to the dynamics of bounded Ke...
peer reviewedThe paper gives an exact vectorial solution to the Kepler problem. A vectorial regulari...