Calculus-Based Physics by Jeffrey W. Schnick - HTML preview

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Chapter 26 Impulse and Momentum

F ∆t = ∆p

21

1

Replacing F with − F we obtain

21

12

− F ∆t = ∆p (26-4)

12

1

Now add equation 26-3 ( F ∆t = ∆p ) and equation 26-4 together. The result is:

12

2

F ∆t − F ∆t = ∆p + ∆p

12

12

1

2

0 = ∆p + ∆p

1

2

On the right is the total change in momentum for the pair of particles p

= p

∆ + ∆p so

TOTAL

1

2

what we have found is that

0 = ∆p

TOTAL

which can be written as

∆p

= 0 (26-5)

TOTAL

Recapping: If the net external force acting on a pair of particles is zero, the total momentum of

the pair of particles does not change. Add a third particle to the mix and any momentum change

that it might experience because of forces exerted on it by the original two particles would be

canceled by the momentum changes experienced by the other two particles as a result of the

interaction forces exerted on them by the third particle. We can extend this to any number of

particles, and since objects are made of particles, the concept applies to objects. That is, if,

during some time interval, the net external force exerted on a system of objects is zero, then the

momentum of that system of objects will not change.

As you should recall from Chapter 4, the concept is referred to as conservation of momentum for

the special case in which there is no net transfer of momentum to the system from the

surroundings, and you apply it in the case of some physical process such as a collision, by

picking a before instant and an after instant, drawing a sketch of the situation at each instant, and

writing the fact that, the momentum in the before picture has to be equal to the momentum in the

after picture, in equation form: p = p′ . When you read this chapter, you should again consider

yourself responsible for solving any of the problems, and answering any of the questions, that

you were responsible for back in Chapter 4.

1

84

Chapter 27 Oscillations: Introduction, Mass on a Spring

27 Oscillations: Introduction, Mass on a Spring

If a simple harmonic oscillation problem does not involve the time, you should

probably be using conservation of energy to solve it. A common “tactical error”

in problems involving oscillations is to manipulate the equations giving the

position and velocity as a function of time, x = x

2

cos(

f

π )t and

max

v = v

2

sin( f

π )t rather than applying the principle of conservation of energy.

max

This turns an easy five-minute problem into a difficult fifteen-minute problem.

When something goes back and forth we say it vibrates or oscillates. In many cases oscillations

involve an object whose position as a function of time is well characterized by the sine or cosine

function of the product of a constant and elapsed time. Such motion is referred to as sinusoidal

oscillation. It is also referred to as simple harmonic motion.

Math Aside: The Cosine Function

By now, you have had a great deal of experience with the cosine function of an angle as the ratio

of the adjacent to the hypotenuse of a right triangle. This definition covers angles from 0 radians

π

to

radians (0° to 90°). In applying the cosine function to simple harmonic motion, we use the

2

extended definition which covers all angles. The extended definition of the cosine of the angle θ

is that the cosine of an angle is the x component of a unit vector, the tail of which is on the origin

of an x-y coordinate system; a unit vector that originally pointed in the +x direction but has since

been rotated counterclockwise from our viewpoint, through the angle θ , about the origin.

Here we show that the extended definition is consistent with the “adjacent over hypotenuse”

π

definition, for angles between 0 radians and

radians.

2

For such angles, we have:

y

u

u

θ

y

u

x

x

in which, u, being the magnitude of a unit vector, is of course equal to 1, the pure number 1 with

no units. Now, according to the ordinary definition of the cosine of θ as the adjacent over the

hypotenuse:

1

85

Chapter 27 Oscillations: Introduction, Mass on a Spring

ux

cosθ =

u

Solving this for u we see that

x

u = u cosθ

x

Recalling that u = 1, this means that

u = cosθ

x

Recalling that our extended definition of cosθ is, that it is the x component of the unit vector uˆ

when uˆ makes an angle θ with the x-axis, this last equation is just saying that, for the case at

π

hand (θ between 0 and

radians) our extended definition of cosθ is equivalent to our ordinary

2

definition.

π

At angles between

and

radians (90° and 270°) we see that u takes on negative values

2

2

x

(when the x component vector is pointing in the negative x direction, the x component value is,

by definition, negative). According to our extended definition, cosθ takes on negative values at

such angles as well.

y

u

u

y

θ

u

x

x

1

86

Chapter 27 Oscillations: Introduction, Mass on a Spring

With our extended definition, valid for any angle θ, a graph of the cosθ vs. θ appears as:

cos θ

1

0

π

π

2

π

3

π

4

θ [radians]

-1

Some Calculus Relations Involving the Cosine

The derivative of the cosine of θ, with respect to θ :

d cosθ = −sinθ

The derivative of the sine of θ, with respect to θ :

d sinθ = cosθ

Some Jargon Involving The Sine And Cosine Functions

When you express, define, or evaluate the function of something, that something is called the

argument of the function. For instance, suppose the function is the square root function and the

expression in question is 3x . The expression is the square root of 3x, so, in that expression, 3x

is the argument of the square root function. Now when you take the cosine of something, that

something is called the argument of the cosine, but in the case of the sine and cosine functions,

we give it another name as well, namely, the phase. So, when you write cosθ, the variable θ is

the argument of the cosine function, but it is also referred to as the phase of the cosine function.

1

87

Chapter 27 Oscillations: Introduction, Mass on a Spring

In order for an expression involving the cosine function to be at all meaningful, the phase of the

cosine must have units of angle (for instance, radians or degrees).

A Block Attached to the End of a Spring

Consider a block of mass m on a frictionless horizontal surface. The block is attached, by means

of an ideal massless horizontal spring having force constant k, to a wall. A person has pulled the

block out, directly away from the wall, and released it from rest. The block oscillates back and

forth (toward and away from the wall), on the end of the spring. We would like to find equations

that give the block’s position, velocity, and acceleration as functions of time. We start by

applying Newton’s 2nd Law to the block. Before drawing the free body diagram we draw a

sketch to help identify our one-dimensional coordinate system. We will call the horizontal

position of the point at which the spring is attached, the position x of the block. The origin of our

coordinate system will be the position at which the spring is neither stretched nor compressed.

When the position x is positive, the spring is stretched and exerts a force, on the block, in the

x

− direction. When the position of x is negative, the spring is compressed and exerts a force, on

the block, in the +x direction.

k

m

+x

x=0

Equilibrium Position

1

88

Chapter 27 Oscillations: Introduction, Mass on a Spring

Now we draw the free body diagram of the block:

FN

a

F

x

S = k

m

F

+x

= mg

g

and apply Newton’s 2nd Law:

1

a

=

∑F

m

1

a =

(− kx)

m

k

a = −

x

m

This equation, relating the acceleration of the block to its position x, can be considered to be an

equation relating the position of the block to time if we substitute for a using:

dv

a =

dt

and

dx

v =

dt

so

d dx

a =

dt dt

which is usually written

2

d x

a =

(27-1)

2

dt

and read “d squared x by dt squared” or “the second derivative of x with respect to t .”

k

Substituting this expression for a into a = −

x (the result we derived from Newton’s 2nd Law

m

above) yields

1

89

Chapter 27 Oscillations: Introduction, Mass on a Spring

d 2 x

k

= −

x (27-2)

dt 2

m

We know in advance that the position of the block depends on time. That is to say, x is a

function of time. This equation, equation 27-2, tells us that if you take the second derivative of x

with respect to time you get x itself, times a negative constant (−k/m).

We can find the an expression for x in terms of t that solves 27-2 by the method of “guess and

check.” Grossly, we’re looking for a function whose second derivative is essentially the negative

of itself. Two functions meet this criterion, the sine and the cosine. Either will work. We

arbitrarily choose to use the cosine function. We include some constants in our trial solution

(our guess) to be determined during the “check” part of our procedure. Here’s our trial solution:

 2π rad 

x = x

cos

max

t 

T

Here’s how we have arrived at this trial solution: Having established that x, depends on the

cosine of a multiple of the time variable, we let the units be our guide. We need the time t to be

part of the argument of the cosine, but we can’t take the cosine of something unless that

2π rad

something has units of angle. The constant

, with the constant T having units of time

T

(we’ll use seconds), makes it so that the argument of the cosine has units of radians. It is,

2π rad

however, more than just the units that motivates us to choose the ratio

as the constant.

T

To make the argument of the cosine have units of radians, all we need is a constant with units of

2π rad

radians per second. So why write it as

? Here’s the explanation: The block goes back

T

and forth. That is, it repeats its motion over and over again as time goes by. Starting with the

block at its maximum distance from the wall, the block moves toward the wall, reaches its

closest point of approach to the wall and then comes back out to its maximum distance from the

wall. At that point, it’s right back where it started from. We define the constant value of time T

to be the amount of time that it takes for one iteration of the motion.

Now consider the cosine function. We chose it because its second derivative is the negative of

itself, but it is looking better and better as a function that gives the position of the block as a

function of time because it too repeats itself as its phase (the argument of the cosine) continually

increases. Suppose the phase starts out as 0 at time 0. The cosine of 0 radians is 1, the biggest

the cosine ever gets. We can make this correspond to the block being at its maximum distance

from the wall. As the phase increases, the cosine gets smaller, then goes negative, eventually

reaching the value −1 when the phase is π radians. This could correspond to the block being

closest to the wall. Then, as the phase continues to increase, the cosine increases until, when the

phase is 2π, the cosine is back up to 1 corresponding to the block being right back where it

started from. From here, as the phase of the cosine continues to increase from 2π to 4π, the

1

90

Chapter 27 Oscillations: Introduction, Mass on a Spring

cosine again takes on all the values that it took on from 0 to 2π. The same thing happens again

as the phase increases from 4π to 6π, from 8π to 10π, etc.

2π rad

Getting back to that constant

that we “guessed” should be in the phase of the cosine in

T

our trial solution for x(t):

 2π rad 

x = x

cos

max

t 

T

With T being defined as the time it takes for the block to go back and forth once, look what

happens to the phase of the cosine as the stopwatch reading continually increases. Starting from

2π rad

0, as t increases from 0 to T, the phase of the cosine,

t , increases from 0 to 2π radians.

T

So, just as the block, from time 0 to time T, goes though one cycle of its motion, the cosine, from

time 0 to time T, goes through one cycle of its pattern. As the stopwatch reading increases from

T to 2T, the phase of the cosine increases from 2π rad to 4π rad. The block undergoes the second

cycle of its motion and the cosine function used to determine the position of the block goes

through the second cycle of its pattern. The idea holds true for any time t —as the stopwatch

reading continues to increase, the cosine function keeps repeating its cycle in exact

synchronization with the block, as it must if its value is to accurately represent the position of the

2π rad

block as a function of time. Again, it is no coincidence. We chose the constant

in the

T

phase of the cosine so that things would work out this way.

A few words on jargon are in order before we move on. The time T that it takes for the block to

complete one full cycle of its motion is referred to as the period of the oscillations of the block.

 2π rad 

Now how about that other constant, the “x

x =

max” in our educated guess

x

cos

?

max

t 

T

Again, the units were our guide. When you take the cosine of an angle, you get a pure number, a

value with no units. So, we need the xmax there to give our function units of distance (we’ll use

meters). We can further relate xmax to the motion of the block. The biggest the cosine of the

phase can ever get is 1, thus, the biggest xmax times the cosine of the phase can ever get is xmax.

 2π rad 

So, in the expression x = x

cos

, with x being the position of the block at any time t,

max

t 

T

xmax must be the maximum position of the block, the position of the block, relative to its

equilibrium position, when it is as far from the wall as it ever gets.

 2π rad 

Okay, we’ve given a lot of reasons why x = x

cos

should well describe the motion

max

t 

T

of the block, but unless it is consistent with Newton’s 2nd Law, that is, unless it satisfies equation

27-2:

1

91

Chapter 27 Oscillations: Introduction, Mass on a Spring

d 2x

k

= −

x

dt 2

m

which we derived from Newton’s 2nd Law, it is no good. So, let’s plug it into equation 27-2 and

2

d x

see if it works. First, let’s take the second derivative

of our trial solution with respect to t

2

dt

(so we can plug it and x itself directly into equation 27-2):

Given

 2π rad 

x = x

cos

,

max

t 

T

the first derivative is

dx

 2π rad  π

=

2 rad

xmax − sin

t 

dt

T

 T

dx

2π rad

 2π rad 

= −

x

sin

max

t 

dt

T

T

The second derivative is then

d 2x

2π rad

 2π rad  π

= −

2 rad

x

cos

2

max

t 

dt

T

T

T

2

d 2x

 2π rad 

 2π rad 

= −

 x

cos

2

max

t 

dt

T

T

 2π rad 

Now we are ready to substitute this and x itself, x = x

cos

, into the differential

max

t 

T

d 2x

k

equation

= −

x (equation 27-2) stemming from Newton’s 2nd Law of Motion. The

dt 2

m

substitution yields:

2

2π rad 

 2π rad 

k

 2π rad 

− 

 x

cos

max

t  = −

x

cos

max

t 

T

T

m

T

1

92

Chapter 27 Oscillations: Introduction, Mass on a Spring

which we copy here for your convenience.

2

2π rad 

 2π rad 

k

 2π rad 

− 

 x

cos

max

t  = −

x

cos

max

t 

T

T

m

T