Essential Physics Formulas

1. Classical Mechanics

Kinematics

  • xx — position
  • x0x_0​ — initial position
  • vv — velocity
  • v0v_0 — initial velocity
  • aa — acceleration
  • tt — time

Kinematics (uniform acceleration only)

v=dxdta=dvdtv = \frac{dx}{dt} \quad a = \frac{dv}{dt} x=x0+v0t+12at2v2=v02+2a(xx0)x = x_0 + v_0 t + \frac{1}{2}at^2 \quad v^2 = v_0^2 + 2a(x-x_0)


Dynamics

F=ma(constant mass)\vec{F} = m\vec{a} \quad\text{(constant mass)} F=dpdtp=mv\vec{F} = \frac{d\vec{p}}{dt} \quad \vec{p} = m\vec{v}

Gravitation (point masses / spherical symmetry):F=Gm1m2r2F = G\frac{m_1 m_2}{r^2}​​


Work, Energy, Power

W=FdrW = \int \vec{F}\cdot d\vec{r} K=12mv2Ug=mgh  (near Earth, constant g)K = \frac{1}{2}mv^2 \quad U_g = mgh \;\text{(near Earth, constant \(g\))} Us=12kx2  (Hookean regime)U_s = \frac{1}{2}kx^2 \;\text{(Hookean regime)}E=K+UP=FvE = K + U \quad P = \vec{F}\cdot\vec{v}


Rotation

L=r×pτ=dLdt\vec{L} = \vec{r}\times\vec{p} \quad \vec{\tau} = \frac{d\vec{L}}{dt}I=mr2  (discrete)Krot=12Iω2I = \sum mr^2 \;(\text{discrete}) \quad K_{rot} = \frac{1}{2}I\omega^2


x3x^3
y4y^4
F=maF = m*a

Oscillations (simple harmonic motion)

F=kxω=kmF = -kx \quad \omega = \sqrt{\frac{k}{m}} x(t)=Acos(ωt+ϕ)x(t) = A\cos(\omega t + \phi)