Summary of classical mechanics formulae (ch. 1–8, 4b). Derivations and limits of validity are in the respective chapters.

Uniformly accelerated motion v=v0+atv = v_0 + at Δs=v0t+12at2\Delta s = v_0 t + \tfrac12 a t^2 v2=v02+2aΔsv^2 = v_0^2 + 2a\,\Delta s

Dynamics (Newton’s second law) F=ma\pq{F} = m\pq{a}

Work and energy L=FsEk=12mv2Ep=mghL = \pq{F}\cdot\pq{s} \qquad E_k = \tfrac12 m v^2 \qquad E_p = mgh

Conservation of mechanical energy

In the presence of only conservative forces: Ek+Ep=costE_k + E_p = \text{cost}.

Momentum p=mvΔp=FΔt\pq{p} = m\pq{v} \qquad \Delta\pq{p} = \pq{F}\,\Delta t

Oscillations T=2πm/K(molla)T=2π/g(pendolo)T = 2\pi\sqrt{m/K} \quad\text{(molla)} \qquad T = 2\pi\sqrt{\ell/g}\quad\text{(pendolo)}

Gravitation F=Gm1m2r2T2r3=cost(III legge di Keplero)F = G\,\frac{m_1 m_2}{r^2} \qquad \frac{T^2}{r^3} = \text{cost}\quad\text{(III legge di Keplero)}

Topics: Kinematics · Dynamics · Work and energy · Gravitation

Related exercises: Conducting bar in a magnetic field: induction, dynamics and energy · Crate with piecewise force · Carlo’s journey