Linear Momentum

Linear momentum is the product of the mass and velocity of an object, it is conserved in elastic and inelastic collisions.

In classical mechanics, linear momentum, or simply momentum (SI unit kg m/s, or equivalently N s), is the product of the mass and velocity of an object. Mathematically it is stated as:

[latex]\mathbf{\text{p}} = \text{m} \mathbf{\text{v}}[/latex].

(Note here that p and v are vectors. ) Like velocity, linear momentum is a vector quantity, possessing a direction as well as a magnitude. Linear momentum is particularly important because it is a conserved quantity, meaning that in a closed system (without any external forces ) its total linear momentum cannot change.

Because momentum has a direction, it can be used to predict the resulting direction of objects after they collide, as well as their speeds. Momentum is conserved in both inelastic and elastic collisions. (Kinetic energy is not conserved in inelastic collisions but is conserved in elastic collisions. ) It important to note that if the collision takes place on a surface with friction, or if there is air resistance, we would need to account for the momentum of the bodies that would be transferred to the surface and/or air.

Let’s take a look at a simple, one-dimensional example: The momentum of a system of two particles is the sum of their momenta. If two particles have masses m₁ and m₂, and velocities v₁ and v₂, the total momentum is:

[latex]\text{p} = \text{p}_1 + \text{p}_2 = \text{m}_1 \text{v}_1 + \text{m}_2 \text{v}_2\,[/latex].

Keep in mind that momentum and velocity are vectors. Therefore, in 1D, if two particles are moving in the same direction, v1 and v2 have the same sign. If the particles are moving in opposite directions they will have opposite signs.

If two particles were moving on a plane we would choose our xy-plane to be on the plane of motion. We can then write the x and y component of the total momentum as:

[latex]\text{p}_\text{x} = \text{p}_{1\text{x}} + \text{p}_{2\text{x}} = \text{m}_1 \text{v}_{1\text{x}} + \text{m}_2 \text{v}_{2\text{x}}\, \\ \text{p}_\text{y} = \text{p}_{1\text{y}} + \text{p}_{2\text{y}} = \text{m}_1 \text{v}_{1\text{y}} + \text{m}_2 \text{v}_{2\text{y}}.[/latex]

If the 2D momentum vector is decomposed into two components, the equations for each component are reduced to its 1D equivalents.

Momentum, like energy, is important because it is conserved. “Newton’s cradle” shown in is an example of conservation of momentum. As we will discuss in the next concept (on Momentum, Force, and Newton’s Second Law ), in classical mechanics, conservation of linear momentum is implied by Newton’s laws. Only a few physical quantities are conserved in nature. Studying these quantities yields fundamental insight into how nature works.

Momentum, Force, and Newton’s Second Law

In the most general form, Newton’s 2^nd law can be written as [latex]\text{F} = \frac{\text{dp}}{\text{dt}}[/latex].

In a closed system (one that does not exchange any matter with the outside and is not acted on by outside forces), the total momentum is constant. This fact, known as the law of conservation of momentum, is implied by Newton’s laws of motion. Suppose, for example, that two particles interact. Because of the third law, the forces between them are equal and opposite. If the particles are numbered 1 and 2, the second law states that

[latex]\frac{\text{d} \text{p}_1}{\text{d} \text{t}} = - \frac{\text{d} \text{p}_2}{\text{d} \text{t}}[/latex]

or

[latex]\frac{\text{d}}{\text{d} \text{t}} \left(\text{p}_1+ \text{p}_2\right)= 0[/latex]

Therefore, total momentum (p₁+p₂) is constant. If the velocities of the particles are u₁ and u₂ before the interaction, and afterwards they are v₁ and v₂, then

[latex]\text{m}_1 \text{u}_{1} + \text{m}_2 \text{u}_{2} = \text{m}_1 \text{v}_{1} + \text{m}_2 \text{v}_{2}[/latex]

This law holds regardless of the nature of the interparticle (or internal) force, no matter how complicated the force is between particles. Similarly, if there are several particles, the momentum exchanged between each pair of particles adds up to zero, so the total change in momentum is zero.

Newton’s Second Law

Newton actually stated his second law of motion in terms of momentum: The net external force equals the change in momentum of a system divided by the time over which it changes. Using symbols, this law is

[latex]\text{F}_{\text{net}} = \frac{\Delta \text{p}}{\Delta \text{t}}[/latex],

where [latex]\text{F}_{\text{net}}[/latex] is the net external force, Δp is the change in momentum, and Δt is the change in time.

This statement of Newton’s second law of motion includes the more familiar [latex]\text{F}_{\text{net}} = \text{ma}[/latex] as a special case. We can derive this form as follows. First, note that the change in momentum Δp is given by Δp=Δ(mv). If the mass of the system is constant, then Δ(mv)=mΔv. So for constant mass, Newton’s second law of motion becomes

[latex]\text{F}_{\text{net}} = \frac{\Delta \text{p}}{\Delta \text{t}} = \frac{\text{m}\Delta \text{v}}{\Delta \text{t}}[/latex].

Because Δv/Δt=a, we get the familiar equation [latex]\text{F}_{\text{net}} = \text{ma}[/latex] when the mass of the system is constant. Newton’s second law of motion stated in terms of momentum is more generally applicable because it can be applied to systems where the mass is changing, such as rockets, as well as to systems of constant mass.

Impulse

Impulse, or change in momentum, equals the average net external force multiplied by the time this force acts.

Impulse

Forces produce either acceleration or deceleration on moving bodies, and the greater the force acting on an object, the greater its change in velocity and, hence, the greater its change in momentum. However, changing momentum is also related to how long a time the force acts. If a brief force is applied to a stalled automobile, a change in its momentum is produced. The same force applied over an extended period of time produces a greater change in the automobile’s momentum. The quantity of impulse is force × time interval, or in shorthand notation:

[latex]\text{Impulse} = \text{F} \Delta \text{t}[/latex],

where F is the net force on the system, and Δt is the duration of the force.

From Newton’s 2nd law:

[latex]\text{F} = \frac {\Delta \text{p}}{\Delta \text{t}}[/latex] (Δp: change in momentum),

change in momentum equals the average net external force multiplied by the time this force acts.

[latex]\Delta \text{p} = \text{F} \Delta \text{t}[/latex].

Therefore, impulse as defined in the previous paragraph is simply equivalent to p.

A force sustained over a long time produces more change in momentum than does the same force applied briefly. A small force applied for a long time can produce the same momentum change as a large force applied briefly because it is the product of the force and the time for which it is applied that is important. Impulse is always equal to change in momentum and is measured in Ns (Newton seconds), as both force and the time interval are important in changing momentum.

Our definition of impulse includes an assumption that the force is constant over the time interval Δt. Forces are usually not constant. Forces vary considerably even during the brief time intervals considered. It is, however, possible to find an average effective force Feff that produces the same result as the corresponding time-varying force. shows a graph of what an actual force looks like as a function of time for a ball bouncing off the floor. The area under the curve has units of momentum and is equal to the impulse or change in momentum between times t1 and t2. That area is equal to the area inside the rectangle bounded by Feff, t1, and t2. Thus, the impulses and their effects are the same for both the actual and effective forces. Equivalently, we can simple find the area under the curve F(t) between t1 and t2 to compute the impulse in mathematical form:

[latex]\text{Impulse} = \int_{\text{t}_1}^{\text{t}_2} \text{F}(\text{t}) \text{dt}[/latex].