2.1.6Analytical Mechanics

Applying E-L equations to various systems

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The recipe (what you actually do)

WHY this is true (sketch of the derivation): Hamilton's principle says the real path makes the action S=LdtS=\int L\,dt stationary (δS=0\delta S = 0). Demanding that the first variation vanish for arbitrary wiggles δqi(t)\delta q_i(t) that vanish at the endpoints, and integrating the q˙\dot q-term by parts, gives exactly the equation above. (Full derivation lives in 2.1.05-Deriving-the-Euler-Lagrange-equation.)

HOW to apply it — the universal 5-step procedure:

  1. Count DOF → pick that many independent generalized coordinates qiq_i.
  2. Write TT in terms of qi,q˙iq_i,\dot q_i (express every Cartesian velocity through your coords).
  3. Write VV in terms of qiq_i.
  4. Form L=TVL=T-V, compute Lqi\dfrac{\partial L}{\partial q_i} and Lq˙i\dfrac{\partial L}{\partial \dot q_i}.
  5. Plug into E–L, take the time derivative, simplify → equation of motion.

Figure — Applying E-L equations to various systems

Example 1 — Simple Pendulum (1 DOF)


Example 2 — Bead on a Rotating Wire / Atwood Machine (2 systems, 1 DOF each)


Example 3 — Block on Frictionless Incline (1 DOF, tilted coordinate)


Example 4 — 2D Central Force (2 DOF, plane polar)


Common mistakes (steel-manned)


Active recall

Recall Quick self-test (cover the answers!)
  • What is LL? → TVT-V.
  • How many coordinates do you need? → one per DOF.
  • What does a cyclic coordinate give you? → a conserved generalized momentum.
  • Why don't tension/normal force appear? → ideal constraints do no work; coordinates absorb them.
  • Pendulum EOM? → θ¨=(g/)sinθ\ddot\theta=-(g/\ell)\sin\theta.
Recall Feynman: explain to a 12-year-old

Imagine you want to predict how a swing moves. The hard way: track every push and pull, including the rope's tug. The easy way: just keep a "score" — how much moving energy it has minus how much height energy it has. Nature is lazy and always picks the path that keeps this score "balanced" over time. We wrote down a magic rule (the E–L equation) that, given the energy score in whatever measuring stick you like (angle, distance, whatever), automatically spits out exactly how the thing moves — and you never had to think about the rope at all.


The Lagrangian LL equals
TVT - V (kinetic minus potential energy)
Number of generalized coordinates required
one per degree of freedom
Euler–Lagrange equation for coordinate qiq_i
ddtLq˙iLqi=0\frac{d}{dt}\frac{\partial L}{\partial\dot q_i}-\frac{\partial L}{\partial q_i}=0
Why constraint forces (tension, normal) don't appear in E–L
they do no work and are absorbed by the choice of independent coordinates
Kinetic energy in plane polar coordinates
T=12m(r˙2+r2θ˙2)T=\tfrac12 m(\dot r^2 + r^2\dot\theta^2)
A cyclic (ignorable) coordinate (absent from LL) implies
its conjugate momentum L/q˙\partial L/\partial\dot q is conserved
EOM of a simple pendulum
θ¨=(g/)sinθ\ddot\theta = -(g/\ell)\sin\theta
Atwood machine acceleration
x¨=(m1m2)g/(m1+m2)\ddot x = (m_1-m_2)g/(m_1+m_2)
Block on frictionless incline acceleration along slope
gsinαg\sin\alpha
Conserved quantity for central force motion
angular momentum Lz=mr2θ˙L_z=mr^2\dot\theta
First step of the E–L recipe
count degrees of freedom and pick that many coordinates
Inside the partial derivatives of LL, how are qq and q˙\dot q treated
as independent variables

Connections

  • 2.1.05-Deriving-the-Euler-Lagrange-equation — where the recipe comes from.
  • 2.1.07-Cyclic-coordinates-and-conservation-laws — exploiting ignorable coordinates.
  • 2.1.08-Generalized-momenta-and-the-Hamiltonian — next step after E–L.
  • Constraints-and-degrees-of-freedom — choosing good coordinates.
  • Noethers-theorem — symmetry ↔ conservation, generalizing Example 4.

Concept Map

derived from

determines number of

express

express

combine

combine

plug into

yields

systematizes

applied to

small angle

Hamilton's Principle deltaS=0

Euler-Lagrange Equation

Lagrangian L = T - V

Kinetic Energy T

Potential Energy V

Generalized Coordinates q_i

Degrees of Freedom

5-Step Recipe C-T-V-L-E

Equations of Motion

Simple Pendulum Example

SHM omega=sqrt g over l

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, Newton ke method mein har jagah forces, directions aur constraint forces (tension, normal reaction) ka hisaab rakhna padta hai — kaafi headache. Euler–Lagrange (E–L) method bolta hai: bhai, sirf energy sambhal. Tum bas kinetic energy TT aur potential energy VV likho, L=TVL=T-V banao, aur ek fix formula mein daal do. Bas, equation of motion nikal aati hai. Sabse pyaari baat — tension aur normal force kabhi aate hi nahi, kyunki acche coordinates choose karne se woh apne aap "absorb" ho jaate hain (kyunki woh koi work nahi karte).

Recipe yaad rakho — C-T-V-L-E: pehle Count degrees of freedom (utne hi coordinates lo), phir TT likho, phir VV, phir L=TVL=T-V, phir E–L equation ddtLq˙Lq=0\frac{d}{dt}\frac{\partial L}{\partial \dot q}-\frac{\partial L}{\partial q}=0 apply karo. Pendulum mein θ\theta lo, Atwood mein ek xx, incline pe slope ke along ss, aur central force mein polar (r,θ)(r,\theta). Polar mein dhyan rakho — T=12m(r˙2+r2θ˙2)T=\frac12 m(\dot r^2 + r^2\dot\theta^2), sirf r˙2\dot r^2 likhna bada common mistake hai.

Ek aur jhakaas cheez: agar kisi coordinate (jaise θ\theta central force mein) LL mein explicitly aata hi nahi, toh uska momentum conserve ho jaata hai — angular momentum free mein mil gaya! Isko cyclic coordinate kehte hain. Yeh method itna systematic hai ki ek baar coordinates set kar liye, baaki sab mechanical calculation hai — isliye exam mein speed aur accuracy dono milti hai. Practice karo 3-4 systems, pattern haath mein aa jaayega.

Go deeper — visual, from zero

Test yourself — Analytical Mechanics

Connections