Central Force Problem: Orbits, Virial Theorem, and Kepler's Problem, Summaries of Physics

An overview of the central force problem, covering topics such as the classification of orbits, the virial theorem, the differential equation of orbits and integrable power-law potentials, the conditions for closed orbits (bertrand's theorem), kepler's problem with the inverse-square law of forces, the motion in time in kepler's problem, the laplace-runge-lenz vector, scattering in a central force field, and the transformation of scattering problems to laboratory coordinates. The document also includes a homework assignment and a preview of the topics to be covered in the next class. This comprehensive coverage of the central force problem would be valuable for students studying classical mechanics, orbital mechanics, or related fields in physics and engineering.

Typology: Summaries

2023/2024

Uploaded on 06/10/2024

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3. Central Force Problem
3.1 Classification of orbits,
The Equations of Motion and First Integrals
The Equivalent One-Dimensional Problem, and
Classification of Orbits
3.2 The virial theorem,
3.3 The differential equation of orbit and integrable power-law
potentials,
3.4 Conditions for closed orbits (Bertand’s theorem),
3.5 Kepler’s problem: Inverse-square law of forces,
3.6 The motion in time in the Kepler’s problem,
3.7 The Laplace-Runge-Lenz vector,
3.8 Scattering in a central force field
3.9 Transformation of the scattering problems to laboratory
coordinates.
RK; CM class on 20200820
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3. Central Force Problem

3.1 Classification of orbits, The Equations of Motion and First Integrals The Equivalent One-Dimensional Problem, and Classification of Orbits 3.2 The virial theorem, 3.3 The differential equation of orbit and integrable power-law potentials, 3.4 Conditions for closed orbits ( Bertand’s theorem), 3.5 Kepler’s problem: Inverse-square law of forces, 3.6 The motion in time in the Kepler’s problem, 3.7 The Laplace-Runge-Lenz vector, 3.8 Scattering in a central force field 3.9 Transformation of the scattering problems to laboratory coordinates. RK; CM class on 20200820

Can we say anything about their motion without integrating the equations of motion?! Let us now consider motion of particles having different energies (e.g., E 1 , E 2 , E 3 , E 4 , etc.).

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  1. The Central Force Problem: 3.1 Classification of orbits, 3.2 The virial theorem, 3.3 The differential equation of orbit and integrable power-law potentials, 3.4 Conditions for closed orbits (Bertand’s theorem), 3.5 Kepler’s problem: Inverse-square law of forces, 3.6 The motion in time in the Kepler’s problem, 3.7 The Laplace-Runge-Lenz vector, 3.8 Scattering in a central force field 3.9 Transformation of the scattering problems to laboratory coordinates.