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The Three-Body Problem and the Equations of Dynamics
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The Three-Body Problem and the Equations of Dynamics

In an effort to understand the stability of orbits in the solar system, Poincaré applied a Hamiltonian formulation to the equations of planetary motion and studied these differential equations in the limited case of three bodies to arrive at properties of the equations’ solutions, such as orbital resonances and horseshoe orbits.
Undertitel
Poincaré’s Foundational Work on Dynamical Systems Theory
Författare
Henri Poincaré
Översättare
Bruce D Popp
Upplaga
1st ed. 2017
ISBN
9783319528984
Språk
Engelska
Vikt
446 gram
Utgivningsdatum
2017-05-22
Sidor
248