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Physics Formulas

Meanings of the symbols a\,: acceleration
A\,: area or amplitude
E\,: energy
F\,: force
\sum F: net force
f_k\,: kinetic friction force
f_s\,: static friction force
g\,: acceleration due to gravity
J\,: Impulse
KE\,: kinetic energy
m\,: mass
\mu_k\,: coefficient of kinetic friction
\mu_s\,: coefficient of static friction
N\,: Normal force to a surface
\nu \,: Frequency
\vec{p}: Momentum
P\,: Power
Q\,: heat or flowrate
r\,: radius
\vec{s}\,: Distance traveled
T\,: Period, Temperature
t\,: time
\theta\,: Angle (see annotations next to each individual formula for details)
U_g\,: gravitational potential energy
V\,: volume
V_{df}\,: volume of displaced fluid
v_f\,: initial velocity
Vo: final velocity
x_f\,: final position
x_i\,: initial position

Dynamics

Like kinematics, dynamics deal with motion, but take into consideration force and mass.
{\sum F} = ma\,\ -- Newton's second law
N = mg\cos \theta\, (\theta\, is the angle between the supporting surface and the vertical)
f_k = {\mu_k}N\,\ (object moving relative to surface)
f_s = {\mu_s}N\,\ (object not moving relative to surface)

Work, energy and power

Work, energy, and power describes an objects ability to affect nature.
 W = \int \vec{F} \cdot d\vec{s} -- definition of mechanical work
 W = \Delta {KE}\,\!
 W = -\Delta {U}\,\!
 U_g = mgh \,\!
 E = KE + U \,\!
 KE = \frac{1}{2}{mv^2}\,\!
 P = \frac{dE}{dt} = \int \vec{F}\cdot \vec{v} \,\!
 P_{avg} = \frac{\Delta E}{\Delta t}\,\!

Simple Harmonic Motion

These are mechanics formulae that deal with simple harmonic motion.
 F = -kx\,\! (k\, is the spring constant) -- Hooke's law
 T_{spring} = (1/2\pi)\sqrt{\frac{m}{k}}\,\!
 \nu = \frac{1}{T}\,\!
 U_s = \frac{1}{2}kx^2\,\! (k\, is the spring constant)
 v_{maxspring} = x\sqrt{\frac{k}{m}}\,\!
 T_{pendulum} = 2\pi\sqrt{\frac{L}{g}}\,\! (for a simple pendulum)

Momentum

Momentum is the amount of mass moving, in classical mechanics.
 \vec{p} = m\vec{v} \,\! -- definition of momentum
 J = \int F \,dt -- definition of impulse
 J = \Delta p \,\!
 m_1\vec{v_1} + m_2\vec{v_2} = m_1\vec{v_1'} + m_2\vec{v_2'} \,\! -- conservation of momentum
 \frac{1}{2}m_1v_1^2 + \frac{1}{2}m_2v_2^2 = \frac{1}{2}m_1v_1'^2 + \frac{1}{2}m_2v_2'^2 \,\! (Note: this is only true for elastic collisions)

Uniform circular Motion and Gravitation

An object moving along a circular path at constant speed is in uniform circular motion. In this section, ac, Fc, et cetera, stand for centripetal acceleration and force, respectively.
 a_c = \frac{v^2}{r} = \frac{4\pi^2r}{t^2}\,\!
 F_c = \frac{mv^2}{r}\,\!
 F_g = G\frac{m_1m_2}{r^2}\,\!
 a_{gravity} = G\frac{m_{planet}}{r^2}\,\!
 v_{satellite} = \sqrt{\frac{Gm_{planet}}{R}}
 U_{gravitational} = G\frac{m_1m_2}{r}
 KE_{satellite} = G\frac{m_sm_{planet}}{2R}
 E_{satellite} = -G\frac{m_sm_{planet}}{2R}
 \frac{T_1^2}{a_1^3} = \frac{T_2^2}{a_2^3}

Thermodynamics

Thermodynamics deal with the energy, motion, and entropy of microscopic particles.
 Q = mc \Delta T \,\!
 \Delta L = L_i \alpha \Delta T \,\!
 \Delta V = V_i \beta \Delta T \,\!
 PV = nRT \,\!
 \frac{P_iV_i}{T_i} = \frac{P_fV_f}{T_f} \,\!
 \Delta U = \Delta Q + \Delta T \,\!
 e = 1-\frac{\Delta Q_{out}}{\Delta Q_{in}}   \,\!

Rotational Motion

\boldsymbol \tau=rF \sin \theta

Fluids

 F_{buoyancy} = \rho g V_{df}\,
 p = p_{atmospheric} + \rho g h\,
 p = \frac{F}{a}\,\!
 Q = Av\,\!
 P + \rho gh + \frac{1}{2} \rho v^2 = k
pV = k
 \frac{P}{T}=k