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Physics LibreTexts

23.3: Energy and the Simple Harmonic Oscillator

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Let’s consider the block-spring system of Example 23.2 in which the block is initially stretched an amount x0>0 from the equilibrium position and is released from rest, vx,0=0. We shall consider three states: state 1, the initial state; state 2, at an arbitrary time in which the position and velocity are non-zero; and state 3, when the object first comes back to the equilibrium position. We shall show that the mechanical energy has the same value for each of these states and is constant throughout the motion. Choose the equilibrium position for the zero point of the potential energy.

State 1: all the energy is stored in the object-spring potential energy, U1=(1/2)kx20. The object is released from rest so the kinetic energy is zero, K1=0 The total mechanical energy is then

E1=U1=12kx20

State 2: at some time t , the position and x -component of the velocity of the object are given by

x(t)=x0cos(kmt)vx(t)=kmx0sin(kmt)

The kinetic energy is

K2=12mv2=12kx20sin2(kmt)

and the potential energy is

U2=12kx2=12kx20cos2(kmt)

The mechanical energy is the sum of the kinetic and potential energies

E2=K2+U2=12mv2x+12kx2=12kx20(cos2(kmt)+sin2(kmt))=12kx20

where we used the identity that cos2ω0t+sin2ω0t=1 and that ω0=k/m (Equation (23.2.6)).

The mechanical energy in state 2 is equal to the initial potential energy in state 1, so the mechanical energy is constant. This should come as no surprise; we isolated the object spring system so that there is no external work performed on the system and no internal non-conservative forces doing work.

clipboard_ea7c48775e301d7cc729ecc789f61441a.png
Figure 23.5 State 3 at equilibrium and in motion

State 3: now the object is at the equilibrium position so the potential energy is zero, U3 = 0 , and the mechanical energy is in the form of kinetic energy (Figure 23.5).

E3=K3=12mv2eq

Because the system is closed, mechanical energy is constant,

E1=E3

Therefore the initial stored potential energy is released as kinetic energy,

12kx20=12mv2eq

and the x -component of velocity at the equilibrium position is given by

vx,eq=±kmx0

Note that the plus-minus sign indicates that when the block is at equilibrium, there are two possible motions: in the positive x -direction or the negative x -direction. If we take x0>0, then the block starts moving towards the origin, and Vx,eq will be negative the first time the block moves through the equilibrium position.

We can show more generally that the mechanical energy is constant at all times as follows. The mechanical energy at an arbitrary time is given by

E=K+U=12mv2x+12kx2

Differentiate Equation (23.3.10)

dEdt=mvxdvxdt+kxdxdt=vx(md2xdt2+kx)

Now substitute the simple harmonic oscillator equation of motion, (Equation (23.2.1) ) into Equation (23.3.11) yielding

dEdt=0

demonstrating that the mechanical energy is a constant of the motion.

Simple Pendulum: Force Approach

A pendulum consists of an object hanging from the end of a string or rigid rod pivoted about the point P . The object is pulled to one side and allowed to oscillate. If the object has negligible size and the string or rod is massless, then the pendulum is called a simple pendulum. Consider a simple pendulum consisting of a massless string of length l and a point-like object of mass m attached to one end, called the bob. Suppose the string is fixed at the other end and is initially pulled out at an angle θ0 from the vertical and released from rest (Figure 23.6). Neglect any dissipation due to air resistance or frictional forces acting at the pivot.

clipboard_ed40d7edff676361d217cec20dd9a3209.png
Figure 23.6 Simple pendulum

Let’s choose polar coordinates for the pendulum as shown in Figure 23.7a along with the free-body force diagram for the suspended object (Figure 23.7b). The angle θ is defined with respect to the equilibrium position. When θ>0, the bob is has moved to the right, and when θ<0, the bob has moved to the left. The object will move in a circular arc centered at the pivot point. The forces on the object are the tension in the string T=Tˆr and gravity mg. The gravitation force on the object has ˆr- and ˆθ- component given by

mg=mg(cosθˆrsinθˆθ)

clipboard_e2cd7e1b7c1fbb7423b248db32ee09bb3.png clipboard_e41f345f6ea4e66767f01f6e2155b37f6.png
Figure 23.7 (b) free-body force diagram

Our concern is with the tangential component of the gravitational force,

Fθ=mgsinθ

The sign in Equation (23.3.14) is crucial; the tangential force tends to restore the pendulum to the equilibrium value θ=0. If θ>0,Fθ<0 and if θ<0,Fθ>0 where we are that because the string is flexible, the angle θ is restricted to the range π/2<θ<π/2. (For angles |θ|>π/2 the string would go slack.) In both instances the tangential component of the force is directed towards the equilibrium position. The tangential component of acceleration is

aθ=lα=ld2θdt2

Newton’s Second Law, Fθ=maθ, yields

mglsinθ=ml2d2θdt2

We can rewrite this equation is the form

d2θdt2=glsinθ

This is not the simple harmonic oscillator equation although it still describes periodic motion. In the limit of small oscillations, sinθθ, Equation (23.3.17) becomes

d2θdt2glθ

This equation is similar to the object-spring simple harmonic oscillator differential equation

d2xdt2=kmx

By comparison with Equation (23.2.6) the angular frequency of oscillation for the pendulum is approximately

ω0gl

with period

T=2πω02πlg

The solutions to Equation (23.3.18) can be modeled after Equation (23.2.21). With the initial conditions that the pendulum is released from rest, dθdt(t=0)=0, at a small angle θ(t=0)=θ0, the angle the string makes with the vertical as a function of time is given by

θ(t)=θ0cos(ω0t)=θ0cos(2πTt)=θ0cos(glt)

The z -component of the angular velocity of the bob is

ωz(t)=dθdt(t)=glθ0sin(glt)

Keep in mind that the component of the angular velocity ωz=dθ/dt changes with time in an oscillatory manner (sinusoidally in the limit of small oscillations). The angular frequency ω0 is a parameter that describes the system. The z -component of the angular velocity ωz(t) besides being time-dependent, depends on the amplitude of oscillation θ0. In the limit of small oscillations, ω0 does not depend on the amplitude of oscillation.

The fact that the period is independent of the mass of the object follows algebraically from the fact that the mass appears on both sides of Newton’s Second Law and hence cancels. Consider also the argument that is attributed to Galileo: if a pendulum, consisting of two identical masses joined together, were set to oscillate, the two halves would not exert forces on each other. So, if the pendulum were split into two pieces, the pieces would oscillate the same as if they were one piece. This argument can be extended to simple pendula of arbitrary masses.

Simple Pendulum: Energy Approach

We can use energy methods to find the differential equation describing the time evolution of the angle θ. When the string is at an angle θ with respect to the vertical, the gravitational potential energy (relative to a choice of zero potential energy at the bottom of the swing where θ=0 as shown in Figure 23.8) is given by

U=mgl(1cosθ)

The θ -component of the velocity of the object is given by vθ=l(dθ/dt) so the kinetic energy is

K=12mv2=12m(ldθdt)2

clipboard_edc3fe31ec6250e1cb865a44ea72bb960.png
Figure 23.8 Energy diagram for simple pendulum

The mechanical energy of the system is then

E=K+U=12m(ldθdt)2+mgl(1cosθ)

Because we assumed that there is no non-conservative work (i.e. no air resistance or frictional forces acting at the pivot), the energy is constant, hence

0=dEdt=12m2l2dθdtd2θdt2+mglsinθdθdt=ml2dθdt(d2θdt2+glsinθ)

There are two solutions to this equation; the first one dθ/dt=0 is the equilibrium solution. That the z -component of the angular velocity is zero means the suspended object is not moving. The second solution is the one we are interested in

d2θdt2+glsinθ=0

which is the same differential equation (Equation (23.3.16)) that we found using the force method.

We can find the time t1 that the object first reaches the bottom of the circular arc by setting θ(t1)=0 in Equation (23.3.22)

0=θ0cos(glt1)

This zero occurs when the argument of the cosine satisfies

glt1=π2

The z -component of the angular velocity at time t1 is therefore

dθdt(t1)=glθ0sin(glt1)=glθ0sin(π2)=glθ0

Note that the negative sign means that the bob is moving in the negative ˆθ-direction when it first reaches the bottom of the arc. The θ-component of the velocity at time t1 is therefore

vθ(t1)v1=ldθdt(t1)=lglθ0sin(glt1)=lgθ0sin(π2)=lgθ0(23.3.32)

We can also find the components of both the velocity and angular velocity using energy methods. When we release the bob from rest, the energy is only potential energy

E=U0=mgl(1cosθ0)mglθ202

where we used the approximation that cosθ01θ20/2. When the bob is at the bottom of the arc, the only contribution to the mechanical energy is the kinetic energy given by

K1=12mv21

Because the energy is constant, we have that U0=K1 or

mglθ202=12mv21

We can solve for the θ -component of the velocity at the bottom of the arc

vθ,1=±glθ0

The two possible solutions correspond to the different directions that the motion of the bob can have when at the bottom. The z -component of the angular velocity is then

dθdt(t1)=v1l=±glθ0

in agreement with our previous calculation.

If we do not make the small angle approximation, we can still use energy techniques to find the θ-component of the velocity at the bottom of the arc by equating the energies at the two positions

mgl(1cosθ0)=12mv21

vθ,1=±2gl(1cosθ0)

Simple Pendulum: Energy Approach

We can use energy methods to find the differential equation describing the time evolution of the angle θ. When the string is at an angle θ with respect to the vertical, the gravitational potential energy (relative to a choice of zero potential energy at the bottom of the swing where θ=0 as shown in Figure 23.8) is given by

U=mgl(1cosθ)

The θ -component of the velocity of the object is given by vθ=l(dθ/dt) so the kinetic energy is

K=12mv2=12m(ldθdt)2

clipboard_edc3fe31ec6250e1cb865a44ea72bb960.png
Figure 23.8 Energy diagram for simple pendulum

The mechanical energy of the system is then

E=K+U=12m(ldθdt)2+mgl(1cosθ)

Because we assumed that there is no non-conservative work (i.e. no air resistance or frictional forces acting at the pivot), the energy is constant, hence

0=dEdt=12m2l2dθdtd2θdt2+mglsinθdθdt=ml2dθdt(d2θdt2+glsinθ)

There are two solutions to this equation; the first one dθ/dt=0 is the equilibrium solution. That the z -component of the angular velocity is zero means the suspended object is not moving. The second solution is the one we are interested in

d2θdt2+glsinθ=0

which is the same differential equation (Equation (23.3.16)) that we found using the force method.

We can find the time t1 that the object first reaches the bottom of the circular arc by setting θ(t1)=0 in Equation (23.3.22)

0=θ0cos(glt1)

This zero occurs when the argument of the cosine satisfies

glt1=π2

The z -component of the angular velocity at time t1 is therefore

dθdt(t1)=glθ0sin(glt1)=glθ0sin(π2)=glθ0

Note that the negative sign means that the bob is moving in the negative ˆθ-direction when it first reaches the bottom of the arc. The θ-component of the velocity at time t1 is therefore

vθ(t1)v1=ldθdt(t1)=lglθ0sin(glt1)=lgθ0sin(π2)=lgθ0(23.3.32)

We can also find the components of both the velocity and angular velocity using energy methods. When we release the bob from rest, the energy is only potential energy

E=U0=mgl(1cosθ0)mglθ202

where we used the approximation that cosθ01θ20/2. When the bob is at the bottom of the arc, the only contribution to the mechanical energy is the kinetic energy given by

K1=12mv21

Because the energy is constant, we have that U0=K1 or

mglθ202=12mv21

We can solve for the θ -component of the velocity at the bottom of the arc

vθ,1=±glθ0

The two possible solutions correspond to the different directions that the motion of the bob can have when at the bottom. The z -component of the angular velocity is then

dθdt(t1)=v1l=±glθ0

in agreement with our previous calculation.

If we do not make the small angle approximation, we can still use energy techniques to find the θ-component of the velocity at the bottom of the arc by equating the energies at the two positions

mgl(1cosθ0)=12mv21

vθ,1=±2gl(1cosθ0)


This page titled 23.3: Energy and the Simple Harmonic Oscillator is shared under a not declared license and was authored, remixed, and/or curated by Peter Dourmashkin (MIT OpenCourseWare) via source content that was edited to the style and standards of the LibreTexts platform.

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