Classical MechanicsBSc · Notes

Geometry, dynamics, and conserved quantities

The four units develop different parts of one argument. Constraints determine admissible configurations and virtual directions. Force projection then becomes an energy-based equation. Momentum and symmetry reduce the dynamics, and the central-force problem turns those reductions into a geometric orbit.

ConstraintsCoordinatesVirtual workKinetic energyD’AlembertLagrangianCentral-force symmetryHamiltonianOrbital plane & areaEffective potentialKepler lawsConics & Runge–Lenz
Course connections. Geometry feeds the energy formulation; central symmetry and the Hamiltonian reductions meet in orbital dynamics.

Connections to be able to explain

Earlier idea Later use What carries across
Independent generalized coordinates Lagrange equations One equation per independent virtual direction
Transformation derivatives Kinetic-energy matrix Geometry converts coordinate rates into physical velocity
Virtual work Generalized non-conservative force Work projection determines the force coefficient
D’Alembert principle Lagrangian inertial terms Acceleration projection is encoded by derivatives of TT
Conjugate momentum Hamiltonian construction Invertible velocity–momentum relation changes state variables
Cyclic coordinate Angular-momentum conservation A missing polar angle gives constant pθp_\theta
Time independence Energy balance The energy function is conserved only with the required force conditions
Phase-space trajectory Radial effective-potential motion Position and momentum together distinguish inward and outward motion
Angular momentum Planarity and equal areas A fixed vector determines the plane and an area rate
Fixed angular momentum Effective potential Angular kinetic energy becomes a radial barrier term
Reciprocal radius Inverse-square conic The orbit equation becomes a forced harmonic equation
Conic geometry and area law Kepler period law Orbit area divided by area rate yields the period
Runge–Lenz vector Fixed periapsis An extra constant captures orientation inside the orbital plane

One pendulum, three descriptions

Newton's tangent equation is maθ¨=−mgsin⁡θma\ddot\theta=-mg\sin\theta. The Lagrangian is L=ma2θ˙2/2−mga(1−cos⁡θ)L=ma^2\dot\theta^2/2-mga(1-\cos\theta). The Hamiltonian is H=pθ2/(2ma2)+mga(1−cos⁡θ)H=p_\theta^2/(2ma^2)+mga(1-\cos\theta), with pθ=ma2θ˙p_\theta=ma^2\dot\theta. Each gives the same exact angular equation. What changes is how the geometric restriction and inertia are organized.

One orbit, three reductions

First, zero torque fixes the orbital plane. Second, angular-momentum conservation gives θ˙=ℓ/(μr2)\dot\theta=\ell/(\mu r^2) and the radial effective potential. Third, changing the independent variable from time to angle gives Binet's equation. Inverse-square attraction then produces a conic, while the area law restores its timing. The Runge–Lenz vector packages the same conic's eccentricity and orientation into one conserved object.

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