Newton's Laws with Calculus
Newton's Second Law
Vector form:
Fnet=ma=mdtdv=mdt2d2r
Component form:
Fx=mdtdvx,Fy=mdtdvy,Fz=mdtdvz
Impulse-Momentum Theorem
From Newton's second law:
F=dtdp
where momentum p=mv.
Integrating both sides:
∫t1t2Fdt=∫t1t2dtdpdt=p2−p1=Δp
Impulse:
J=∫t1t2Fdt=Δp
Variable Force Example
If F(t)=F0cos(ωt) for time 0 to T=π/(2ω):
J=∫0TF0cos(ωt)dt=ωF0sin(ωt)0T=ωF0
Variable Mass Systems
For systems where mass changes with time (rockets):
Fext=dtdp=dtd(mv)=mdtdv+vdtdm
Rocket equation:
mdtdv=−vreldtdm+Fext
where vrel is exhaust velocity relative to rocket.
For no external forces and integrating:
Δv=vrellnmfm0
(Tsiolkovsky rocket equation)
Drag Forces
Linear drag: Fd=−bv
mdtdv=−bv
Solution: v(t)=v0e−bt/m
Quadratic drag: Fd=−cv2
mdtdv=−cv2
Separating variables:
∫v0vv′2dv′=−mc∫0tdt′
v(t)=1+mcv0tv0
Falling with Air Resistance
Equation of motion:
mdtdv=mg−bv
Terminal velocity: vt=bmg
Rewrite as:
dtdv=g−mbv=mb(vt−v)
Solution:
v(t)=vt(1−e−bt/m)
Forces in Polar Coordinates
Newton's second law in polar coordinates:
Radial direction:
Fr=m(r¨−rθ˙2)
Tangential direction:
Fθ=m(rθ¨+2r˙θ˙)
Example: Central Force
For motion under central force (depends only on r):
Fθ=0, so:
rθ¨+2r˙θ˙=0
dtd(r2θ˙)=0
This means r2θ˙=L/m is constant (angular momentum conservation).