Ph · Physics

What Differential Equation Describes Newtonian Motion?

Published By the 9to5Science editorial team

At a glance

  1. 1. State Newton’s law

    In an inertial frame, set mass times acceleration equal to the net force.

  2. 2. Specify the force

    Write the force in terms of position, velocity, and time, as appropriate.

  3. 3. Give initial conditions

    For a second-order equation, provide the starting position and velocity.

  4. 4. Solve for motion

    Find the trajectory analytically when possible, or use a numerical method.

Newtonian mechanics describes motion through differential equations: acceleration is related to the net force acting on a body. The law alone does not give a specific trajectory, however. You must also specify how the force depends on the body’s position, velocity, and time, and give its initial position and velocity.

Newton’s law as a differential equation

For a particle of constant mass mm moving in an inertial reference frame, Newton’s second law is

mr¨(t)=F(r(t),r˙(t),t),m\ddot{\mathbf r}(t)=\mathbf F(\mathbf r(t),\dot{\mathbf r}(t),t),

where r(t)\mathbf r(t) is the position, r˙(t)\dot{\mathbf r}(t) is the velocity, r¨(t)\ddot{\mathbf r}(t) is the acceleration, and F\mathbf F is the net force. The dots mean derivatives with respect to time. Because position is differentiated twice, this is a second-order ordinary differential equation.

In one dimension, the same law is

md2xdt2=F(x,x˙,t).m\frac{d^2x}{dt^2}=F(x,\dot{x},t).

The right-hand side is a force law. For example, a spring obeying Hooke’s law has F=−kxF=-kx, while gravity near Earth’s surface is approximately F=−mgF=-mg if upward is chosen as the positive direction.

For a system of NN particles, write one vector equation for each particle:

mir¨i=Fi.m_i\ddot{\mathbf r}_i=\mathbf F_i.

The force on each particle may depend on the positions and velocities of several particles. Constraints, such as motion along a track, can also restrict the allowed positions and require additional equations or constraint forces.

Why initial conditions are needed

A second-order equation generally needs two initial conditions for each independent coordinate. For one-dimensional motion, these are usually the initial position and velocity:

x(0)=x0,x˙(0)=v0.x(0)=x_0,\qquad \dot{x}(0)=v_0.

Together, the force law and these initial values select a particular solution from the family of possible trajectories. Under the usual smoothness conditions on the force, that solution is locally unique. Without a force law, Newton’s law says how acceleration relates to force but does not predict what the motion will be.

You can also rewrite the second-order equation as two first-order equations by introducing velocity v=x˙v=\dot{x}:

x˙=v,v˙=1mF(x,v,t).\dot{x}=v,\qquad \dot{v}=\frac{1}{m}F(x,v,t).

This form is especially useful in numerical simulations and in the phase-space description of mechanics, where the state is specified by position and velocity.

Worked example: a mass on a spring

Consider a mass mm attached to an ideal spring with spring constant kk, moving without friction along a horizontal line. If x=0x=0 is the spring’s equilibrium position, Hooke’s law gives F=−kxF=-kx. Newton’s law therefore becomes

mx¨=−kx,m\ddot{x}=-kx,

or

x¨+ω2x=0,ω=km.\ddot{x}+\omega^2x=0,\qquad \omega=\sqrt{\frac{k}{m}}.

The general solution is

x(t)=Acos⁡(ωt)+Bsin⁡(ωt),x(t)=A\cos(\omega t)+B\sin(\omega t),

where AA and BB are constants set by the initial conditions. Suppose the mass starts at x(0)=0.10 mx(0)=0.10\,\mathrm{m} with velocity x˙(0)=0\dot{x}(0)=0, and let m=0.50 kgm=0.50\,\mathrm{kg} and k=8.0 N/mk=8.0\,\mathrm{N/m}. Then

ω=8.00.50=4.0 s−1.\omega=\sqrt{\frac{8.0}{0.50}}=4.0\,\mathrm{s}^{-1}.

From x(0)=Ax(0)=A, we get A=0.10 mA=0.10\,\mathrm{m}. Differentiating the solution gives x˙(t)=−Aωsin⁡(ωt)+Bωcos⁡(ωt)\dot{x}(t)=-A\omega\sin(\omega t)+B\omega\cos(\omega t). Thus x˙(0)=Bω=0\dot{x}(0)=B\omega=0, so B=0B=0. The motion is

x(t)=0.10cos⁡(4.0t) m,x(t)=0.10\cos(4.0t)\,\mathrm{m},

with time measured in seconds. The force law produced the differential equation; the initial position and velocity determined which solution describes this particular motion.

Common mistakes

  • Leaving out the force law: mx¨=Fm\ddot{x}=F is not a complete solvable model until FF is specified or otherwise known.
  • Providing only a starting position: A second-order equation normally needs both position and velocity at the initial time.
  • Using a force with the wrong sign: Signs depend on the chosen coordinate direction. For a spring, the force points toward equilibrium; for gravity, it points downward.
  • Applying the law outside its assumptions: The usual equation assumes an inertial frame and constant mass. Accelerating frames require additional inertial forces, and variable-mass systems need a careful momentum balance.
  • Assuming every solution has a simple formula: Many force laws do not yield elementary closed-form solutions. Numerical integration can still approximate the motion if the model and initial data are specified.

References

  1. Classical Mechanics, John R. Taylor
  2. An Introduction to Mechanics, Daniel Kleppner and Robert J. Kolenkow

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