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.
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Abstract. Posing Kepler’s problem of motion around a fixed “sun ” requires the geometric mechanician...
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 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...
Abstract: Kepler’s equations are considered as central to Celestial Mechanics since their solutions ...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Abstract. Posing Kepler’s problem of motion around a fixed “sun ” requires the geometric mechanician...
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 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...
Abstract: Kepler’s equations are considered as central to Celestial Mechanics since their solutions ...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Summary: The canonical map τ of the field of quaternions ℍ to SO(E) yields a logarithmic scale on th...
Abstract. Posing Kepler’s problem of motion around a fixed “sun ” requires the geometric mechanician...