This preview shows pages 1–2. Sign up to view the full content.
This preview has intentionally blurred sections. Sign up to view the full version.View Full Document
Unformatted text preview: Fyta12:1 Motion in a Central Force Field A central force F = F ( r ) e r results from a spherically symmetric potential function V ( r ), as F ( r ) =- V ( r ). The motion is restricted to a plane, and in plane-polar coordinates ( r, ) the Lagrangian is L = m 2 r 2 + m 2 r 2 2- V ( r ) (1) which gives the equations of motion (note the cyclicity of ) m r = mr 2- V ( r ) (2) d d t ( mr 2 ) = (3) = L mr 2 (4) where L is the value of the conserved angular momentum . Inserting the expression (4) for into the r equation yields m r = L 2 mr 3- V ( r ) (5) Note that the radial force as described by (5) can be seen as formally resulting from an effective potential , V eff ( r ), where a repulsive centrifugal term, L 2 / (2 mr 2 ) mr 2 2 / 2 representing the angular part of the kinetic energy, is added to V ( r ), yielding V eff ( r ) = V ( r ) + L 2 2 mr 2 (6) A first integration of eq. (5) is easily done, yielding m 2...
View Full Document
- Spring '10