Conservation of momentum
m1v1+m2v2=(m1+m2)vf
Kinetic Energy
1/2mv^2
Kinematic Equations
The Four Kinematic Equations:
1. Final Velocity:
v = v₀ + at
Newtons Law of Universal Gravitation
F = G [(M1m2)/r^2]
Impulse
Impulse is the change of momentum
Delta p = F\Delta t
Delta p = Change in momentum
F = applied force
Delta t = elapsed time
Force
F = m*a
Half Life
N(t)=N(0)e^(lamda*t)
T1/2 = ln(2) / lambda
Poisson Standard Deviation
square root of the total number of events or samples. (N^1/2)
Poisson Relative Standard Deviation
Standard deviation divided by the number of events or samples. (N^1/2)/N