Add to ORKGThis Demonstration shows the geodesic motion of a particle with mass in the meridian plane for a metric corresponding to two extreme Reissner–Nordström black holes, where the Coulomb repulsion between them balances the Newtonian attraction. The solution obtained by Majumdar and Papapetrou is expressed here in prolate spheroidal coordinates. This is a version of the three-body problem in general relativityEducação Superior::Ciências Exatas e da Terra::Matemátic
We consider the Deser–Sarioglu–Tekin (DST) black hole as a background, and we study the motion of ma...
A generalized Newtonian potential is derived from the geodesic motion of test particles in Schwarzsc...
We study relative equilibria of a particle in vicinity of a rigid body, assuming the body motion abo...
Educação Superior::Ciências Exatas e da Terra::AstronomiaEsta demonstração mostra o movimento geodés...
Educação Superior::Ciências Exatas e da Terra::AstronomiaEsta demonstração mostra o movimento geodés...
In Newtonian physics, a system of extremally charged particles (electric charge equal to gravitation...
In Newtonian physics, a system of extremally charged particles (electric charge equal to gravitation...
A special case of the Majumdar-Papapetrou solution of the Einstein-Maxwell equations is the static p...
We study dynamics of an extremally charged black hole on the background of two stationary, mutually ...
We present a novel method to study interacting orbits in a fixed mean gravitational field associated...
The two-body problem consists of determining the motion of two gravitationally interacting bodies wi...
The two-body problem consists of determining the motion of two gravitationally interacting bodies wi...
The two-body problem consists of determining the motion of two gravitationally interacting bodies wi...
Explore the restricted three-body problem in three dimensions-a classic problem in celestial mechani...
Explore the restricted three-body problem in three dimensions-a classic problem in celestial mechani...
We consider the Deser–Sarioglu–Tekin (DST) black hole as a background, and we study the motion of ma...
A generalized Newtonian potential is derived from the geodesic motion of test particles in Schwarzsc...
We study relative equilibria of a particle in vicinity of a rigid body, assuming the body motion abo...
Educação Superior::Ciências Exatas e da Terra::AstronomiaEsta demonstração mostra o movimento geodés...
Educação Superior::Ciências Exatas e da Terra::AstronomiaEsta demonstração mostra o movimento geodés...
In Newtonian physics, a system of extremally charged particles (electric charge equal to gravitation...
In Newtonian physics, a system of extremally charged particles (electric charge equal to gravitation...
A special case of the Majumdar-Papapetrou solution of the Einstein-Maxwell equations is the static p...
We study dynamics of an extremally charged black hole on the background of two stationary, mutually ...
We present a novel method to study interacting orbits in a fixed mean gravitational field associated...
The two-body problem consists of determining the motion of two gravitationally interacting bodies wi...
The two-body problem consists of determining the motion of two gravitationally interacting bodies wi...
The two-body problem consists of determining the motion of two gravitationally interacting bodies wi...
Explore the restricted three-body problem in three dimensions-a classic problem in celestial mechani...
Explore the restricted three-body problem in three dimensions-a classic problem in celestial mechani...
We consider the Deser–Sarioglu–Tekin (DST) black hole as a background, and we study the motion of ma...
A generalized Newtonian potential is derived from the geodesic motion of test particles in Schwarzsc...
We study relative equilibria of a particle in vicinity of a rigid body, assuming the body motion abo...