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By Professor Dr. Josef Honerkamp, Professor Dr. Hartmann Römer (auth.)

This advent to classical theoretical physics emerged from a direction for college students within the 3rd and fourth semester, which the authors have given numerous instances on the college of Freiburg (Germany). The aim of the path is to offer the scholar a complete and coherent assessment of the relevant parts of classical theoretical physics. according to this target, the content material, the terminology, and the mathematical ideas of theoret­ ical physics are all offered besides functions, to function a fantastic starting place for extra classes within the simple parts of experimental and theoretical physics. In conceiving the path, the authors had 4 interdependent targets in brain: • the presentation of a constant assessment, even at this straightforward point • the institution of a well-balanced interactive dating among phys­ ical content material and mathematical equipment • an illustration of the real purposes of physics, and • an acquisition of an important mathematical strategies had to resolve particular difficulties. when it comes to the 1st element, it used to be essential to restrict the quantity of fabric handled. This introductory path was once now not meant to preempt a later, totally on the opposite hand, we aimed for a undeniable completeness in theoretical, course.

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Iv) Considering Ueff(r) as a function of r, we can qualitatively describe the progress of the trajectory. The procedure is exactly analogous to one-dimensional motion. From the graph of the function Ueff , we can immediately read off the allowed values of the variable r corresponding to given values of Ere) and I. Minima and maxima of Ueff now correspond to stable and unstable circular orbits. It is interesting to examine the following cases in some detail: a) Assume that the graph of the effective potential looks like Fig.

1). 5) dA = tlrx;'ldt , since this area is a triangle with two sides formed by the vectors a = r(t) and h = r(t)dt. 1. The area dA swept out by the relative position vector r(t) in the time interval [t,t + dt] 46 2. Newtonian Mechanics and since ILrell is constant, it follows that: The areas swept out by the radius vector during equal amounts of time are equal. We recognize this statement as Kepler's second law of planetary motion, which we have derived as a direct consequence of the conservation of angular momentum.

Let Ere) = Eo be given: Since then for every point on the trajectory we must have Ueff(r) ::; Eo. 27) 0 is the kinetic energy of the "radial" motion. At r = rmin and r = r max , we have Ueff(r) = Eo and thus f = O. However, since 1 =t= 0, and thus

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