Classical mechanics

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What is it?

Newton's second law F=mx¨F = m\ddot x turns forces into a second-order ODE for the motion. Gravity, springs, friction and collisions are all modelled this way; energy and momentum are the conserved quantities that check a simulation.

Formulas

m x¨=F(x,x˙,t),Fgrav=−G m1m2r2 r^m\,\ddot x = F(x, \dot x, t), \qquad F_{\text{grav}} = -\frac{G\,m_1m_2}{r^2}\,\hat r
E=12m∥x˙∥2+U(x),dEdt=0E = \tfrac12 m\norm{\dot x}^2 + U(x), \qquad \frac{\dd E}{\dd t} = 0
energy is conserved when the force is conservative, F=−∇UF = -\nabla U

The mathematics behind it

Where is it used?

Computing topics reachable from here, through the chain of ideas that leads to them:

What depends on it

Exercises

1Computation

A ball is thrown up at 20 m/s (g=9.8g = 9.8 m/s²). Using calculus, find the maximum height and the time to reach it.

Solution

y(t)=20t−4.9t2y(t) = 20t - 4.9t^2; y′(t)=20−9.8t=0⇒t≈2.04y'(t) = 20 - 9.8t = 0 \Rightarrow t \approx 2.04 s, y≈20.4y \approx 20.4 m.

This page has the essentials. A fuller treatment (intuition, formal definition, worked example) is on the way.

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