Recall

Work = W = Fs cosq

Power

Power is defined as work divided by the time in which the work is accomplished, P = W/Dt. Power is measured in watts, W. For engines and motors, it is still traditional to specify power in the unit horsepower, 1hp = 746W. Note that if we use W=FDs, then P=FDs/ Dt = Fv. This last form is an easy way to calculate the instantaneous power of an object that is being accelerated, like a car.
Example: P5.46
A 650kg elevator starts from rest. It moves upward for 3.00s with constant acceleration until it reaches its cruising speed of 1.75m/s. (a) What is the average power delivered by the elevator motor during the acceleration? (b) What is the instantaneous power at t=3.00s?

The acceleration is a=v/t=(1.75m/s)/(3.00s) = 0.583m/s2. The net force on the elevator must be Fnet=ma = (650kg)(0.583) = 379N. The net force is the force from the motor minus the force of gravity, so Fmotor = Fnet + mg = 379N + (650kg)(9.8) = 6750N. In 3s the elevator moves a distance x=1/2 at2 = (.583)(3.00s)2/2 = 2.62m. The work done by the motor is then Wmotor= Fmotorx = (6750N)(2.62m) = 17,700J. The average power of the motor is P=W/t = 17700J/3.00s = 5900W

At t=3.00s, the instantaneous power is P=Fv = (6750N)(1.75m/s) = 11,800 W.

Chapter 6: Momentum and Collisions

Momentum

The linear momentum of an object is defined as the product of its mass times its velocity, p=mv, a vector relationship. There is no special unit for momentum, its units are simply kg m/s.

The component equations for momentum are: px = mvx and py = mvy.

Newton actually expressed his second law not as F=ma, but as F = Dp/Dt. Written this way, the second law basically says that the time rate of change of momentum of an object is equal to the net force acting on it.

Rewriting the above expression we get the impulse-momentum theorem: FDt = Dp = mvf - mvi.

The quantity FDt is called the impulse. The above expression says that the impulse acting on an object equals the change in momentum of the object. It is often not possible to know exactly what force is acting on an object. For instance, when a ball bounces off the floor, the force changes rapidly with time, from nearly zero when the ball first touches the floor to a large value as the velocity of the ball comes to zero, and reverses, then back to a small value as the ball begins to move up from the floor. But by using the impulse, we don't need to know exactly how the force varies of this short time, we can use the average force exerted on the ball during the time it is in contact with the floor.

Example: like P6.13
A 1.3kg basketball bounced off the floor with a speed of 10.0m/s rebounds with a velocity of 9.8m/s. (a) What is the impulse delivered to the ball? (b) What is the average force on the ball if it is in contact with the floor for 2.6x10-3s?

(a) Impulse = FDt = pf-pi = mvf - mvi = (1.3kg)(-10.0 - 9.8m/s) = 26kg m/s.

(b) Favg = FDt/Dt = (26kg m/s)/(2.6x10-3s) = 104N.

Conservation of Momentum

Conservation of momentum is as fundamental in physics as conservation of energy, but better. Momentum is conserved in all isolated systems. A system is isolated if there is no outside influence (forces) acting on it. Examples of isolated systems are:

You should notice the repeated use of the word collision. The interaction of two objects is generally treated as a collision.

Consider a collision between two objects, 1 and 2. (Drawing of 2 objects before and after collision, indicating masses and velocities.) The impulse on object 1 is F1Dt = m1v1f - m1v1i. Likewise for object 2, F2Dt = m2v2f - m2v2i.

Recall Newton's third law: F2 on 1 = -F1 on 2. In terms of the forces given above this means that F1 = -F2. (Although the impulse equation involves an average force, since F1 equals -F2 at every instant in time, then the same result holds for the averages.) Therefore, F1Dt = -F2Dt, or

m1v1f - m1v1i = -(m2v2f - m2v2i)

Putting the initial quantities on the left and the final quantities on the right yields:

m1v1i + m2v2i = m1v1f + m2v2f

This result is called conservation of momentum. It says that the initial momentum equals the final momentum. The key to this result is Newton's third law, and the fact that there are no other forces acting on the system. In this derivation, we used a system with two objects, but the result holds for systems with any number of objects.

Example: P6.15

A 730N man stands in the middle of a frozen pond of radius 5.0m. He is unable to get to the side because of a lack of friction between his shoes and the ice. To overcome this difficulty (since he just learned about conservation of momentum) he throws his 1.2kg physics textbook horizontally toward the north shore, at a speed of 5.0m/s. How long does it take him to reach the south shore?

Apply conservation of momentum. When he throws the textbook, he will get a push from the reaction force of the textbook on him.

mbvb = -mmvm

vm = -mbvb/mm = -(1.2kg)(5.0m/s)/((730N)/(9.8m/s2)) = -0.081m/s. (minus sign means the directions are opposite, I'll ignore it from here.) The time to move to the edge is t=(5.0m)/(0.081m/s) = 62s.

Collisions

Interactions between two objects often fall into the category of collisions -- even many things that don't seem to be related to collisions at all, for example, air pressure or glaucoma testing (see text). While momentum is strictly conserved in collisions (emphasizing again that there are no external forces), energy need not be conserved. Quick example: When a ball is dropped and bounces off the floor, it doesn't return to the same height it was dropped from. Energy is lost in the collision. Momentum is conserved, but you must consider the system of the ball and the Earth!

We call a collision where momentum is conserved but energy is not an inelastic collision. When the two objects stick together, like two train cars that hit and couple together, we say that the collision is perfectly inelastic.

When both momentum and energy are conserved, we say that the collision is elastic. Examples of truly elastic collisions are collisions between subatomic particles, or "collisions" between stellar objects. In the latter, the objects should not make physical contact, but we can treat their gravitational interaction as a collision.

Example: Inelastic Collision P6.25
A 0.030kg bullet is fired vertically at 200m/s into a 0.15kg baseball that is initially at rest. How high does the combination rise after the collision, assuming the bullet embeds in the ball.

Since the bullet embeds (sticks) in the ball, this is a perfectly inelastic collision. Initially we have 2 objects, and afterward we have one object with a mass that is the sum of the original masses.

(Drawing) m1v1+m2v2 = (m1+m2)vf.

Thus vf = (m1v1+m2v2) / (m1+m2) = (0.030kg)(200m/s)/(0.030kg+0.15kg) = 33.3m/s.

So the ball will rise to a height y = v2/2g = (33.3m/s)2/2(9.8m/s2) = 57m.

Example: Elastic Collision P6.30
A 10.0g object moving to the right at 20.0cm/s makes an elastic head-on collision with a 15.0g object moving in the opposite direction at 30.0cm/s. Find the velocity of each object after the collision.

Since this is an elastic collision, momentum and energy are conserved, so we have 2 equations:

m1v1i + m2v2i = m1v1f + m2v2f, and

1/2 m1v1i2 + 1/2 m2v2i2 = 1/2 m1v1f2 + 1/2 m2v2f2

From the statement of the problem we know m1 = 0.0100kg, m2 = 0.0150kg, v1i = 0.200m/s, and v2i = -0.300m/s. We are left to find v1f, v2f. We have 2 equations and 2 unknowns. m1v1i + m2v2i = 0.00650 kg m/s. 1/2 m1v1i2 + 1/2 m2v2i2 = 0.000875J. Begin by eliminating v2f = (m1v1i + m2v2i - m1v1f) / m2 = 0.433 - 0.667 v1f from the energy equation.

0.000875J = 1/2 m1v1f2 + 1/2 m2(0.433 - 0.667 v1f)2 = 0.00500 v1f2 + 0.00141 - 0.0100 v1f + 0.00334 v1f2

This results in a quadratic equation:

0.00834 v1f2 - 0.0100 v1f + 0.000535 = 0

The solutions are