1.1 Force and Newton’s three laws

Mechanics is the science of motion under force. Its entire classical content rests on three laws stated by Newton in 1687, from which every problem — a thrown ball, an orbiting planet, a vibrating string, a slab of fluid — is assembled by applying the second law to the right body.

The three laws

In an inertial frame:

  1. A body free of external force moves with constant velocity.
  2. The rate of change of momentum equals the applied force, F  =  dpdt,p  =  mv.\mathbf{F} \;=\; \frac{d\mathbf{p}}{dt}, \qquad \mathbf{p} \;=\; m\mathbf{v}.
  3. Forces between two bodies are equal and opposite: F12=F21\mathbf{F}_{12} = -\mathbf{F}_{21}.

The first law fixes what counts as an inertial frame: one in which the second law holds in the simple form above, without phantom forces. The second law is the operative one — every problem in classical mechanics is the assembly of F=dp/dt\mathbf F = d\mathbf p/dt for the right body or element. The third law is what closes the books: pairing every “force on A from B” with its reaction “force on B from A” is what lets internal forces cancel when a system is summed over.

For a body of constant mass mm, the second law reduces to the familiar F=ma\mathbf F = m\mathbf a. The momentum form F=dp/dt\mathbf F = d\mathbf p/dt is the more fundamental one, holding also when the mass changes (a rocket shedding fuel) or when momentum is the natural variable (a stream of molecules striking a wall).

Systems of particles and the centre of mass

Sum the second law over all the particles of a system. By the third law the internal forces cancel in pairs, leaving only the external forces:

dPtotdt  =  Fext,Ptot=imivi=Mvcm.\frac{d\mathbf{P}_\text{tot}}{dt} \;=\; \mathbf{F}_\text{ext}, \qquad \mathbf{P}_\text{tot} = \sum_i m_i\mathbf v_i = M\mathbf{v}_\text{cm}.

The total momentum moves as though the whole mass MM were concentrated at the centre of mass and the external force applied there. Internal forces — however violent — never accelerate the centre of mass. When Fext=0\mathbf F_\text{ext} = 0 the total momentum is conserved; this is the formal basis for the collision analysis of the next lesson.

Free-body diagrams as a discipline

Turning a physical situation into equations is a procedure, not an inspiration. A free-body diagram isolates one body — or one differential element of a continuum — draws every external force acting on it, and sets the vector sum equal to mam\mathbf a. Choose the body, choose the frame, list every contact and field force, and only then write equations. The discipline keeps two errors at bay: double-counting an internal force, and forgetting a constraint reaction (the normal force of a surface, the tension of a string). Every derivation in continuum mechanics — the force balance on a slab of fluid, on a segment of string, on an element of solid — is a free-body diagram drawn on an infinitesimal piece.