Perturbation Theory in Celestial Mechanics
نویسنده
چکیده
4 Classical perturbation theory 4 4.1 The classical theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4 4.2 The precession of the perihelion of Mercury . . . . . . . . . . . . . . . . . . . . 6 4.2.1 Delaunay action–angle variables . . . . . . . . . . . . . . . . . . . . . . 6 4.2.2 The restricted, planar, circular, three–body problem . . . . . . . . . . . 7 4.2.3 Expansion of the perturbing function . . . . . . . . . . . . . . . . . . . . 7 4.2.4 Computation of the precession of the perihelion . . . . . . . . . . . . . . 8
منابع مشابه
On the status of perturbation theory
Perturbation theory has always been an important part of natural sciences. From celestial mechanics to quantum theory of fields it has always played a central role that this little note would like to analyze briefly. We will show in particular how its epistemological situation has changed, from being a ”tool” to being the basis of definition of objects in quantum field theory.
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تاریخ انتشار 2009