linear coupled oscillators
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k
x=0
m
Figure 1: A Single Spring and Mass System
1. A Single Spring & Mass Oscillator
1.1. Description of the Model
Before we discuss the coupled oscillators, we will review the simple problem of asingle spring and mass oscillator. This system consists of a single mass attachedto a spring, and allowed to slide on a horizontal surface. A picture of this canbe seen in Figure 1. For simplicity, we will ignore any damping forces acting onthe mass, such as air resistance, or friction. With these assumptions, we needonly consider the force that the spring exerts on the mass. We will assume thatthe spring obeys Hookes law, and thus exerts a linear restoring force on the
mass. This means that when the mass is displaced by a distance x from its
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equilibrium position, the spring exerts a force Fs = kx on the mass. We willrestrict our system to one-dimensional motion along the x-axis.
1.2. Finding the General Solution
We can describe the state of our system at any time in terms of the masssdisplacement from equilibrium x(t), and velocity v(t) = dx
dt. Given initial con-
ditions for the system, x(0) and v(0), we would like to be able to solve for themasses position as a function of time.
Newtons Second Law
Newtons second law is an important tool in solving this problem as well as themore complex problem of the coupled oscillators. Newtons second law says thatthe sum of the forces acting on a body is equal to the product of the objectsmass and its acceleration. Mathematically this is stated as, F = ma. In ourcase the displacement of the mass is x(t), so the acceleration is d
2xdt2
. So we stateNewtons second law as:
F = m
d2x
dt2
And we know that the net force acting on the mass is simply the force due tothe spring, which we know to be:
Fs = kx
So we write Newtons Second Law for our spring and mass system as:
Fs = kx = m d2
xdt2
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Which is rearranged:mx + kx = 0
This equation is traditionally rewritten in the form:
x +
k
m
x = 0 (1)
Now we make a simple substitution to write the equation in a simpler form.
=
k
m(2)
which is known as the natural frequency of the mass. The reason for this willbe revealed later. Now we have the second order differential equation:
x + 2x = 0 (3)
This is the final form of our differential equation describing the motion of themass.
The Method of the Lucky Guess
We will solve this equation in a way that at first seems to be a bit of a swindle,but in fact is a common technique for solving differential equations. We guess asolution. Though this is not a completely random guess, but rather, an educatedguess. Our guess is:
x = et
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where must be found. Taking the first and second derivatives of our guess, weget:
x = et
andx = 2et
which we substitute back into Equation 2 and simplify, giving us the character-istic polynomial p().
p() = 2 + 2 = 0 (4)
which we solve for
= i
and obtain our solution.x = eit (5)
But this is not the form we want it in. So we expand it using Eulers formula.
x = cos t + i sin t (6)
Now we use a theorem from differential equations that states that for complexvalued solutions of a linear differential equation, both the real and imaginaryparts of the complex solution, are solutions. And we form our general solutionby taking a linear combination of these two solutions.
x(t) = C1 cos t + C2 sin t (7)
Using trigonometry, we can rewrite our general solution in a more useful form:
x = A cos(t ) (8)
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0 5 10 15
1
0.5
0
0.5
1
t
x
Figure 2: Simple Harmonic Motion: x(t) = A cos(t ), A = 1, = 1, = 0
1.3. Analysis of ResultsFrom our solution, we now know that the masses motion has an amplitude of A,an angular frequency of , and a phase shift of radians. Now we can see whythe substitution for in Equation 2 was made. As we can see in Equation 8,the natural frequency is the angular frequency of the masses motion. A graphof the masss motion where A = 1, = 1, and = 0 can be seen in Figure 2.
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1 2
Ck kk
x=0 x=0
m m
Figure 3: Coupled Oscillators
2. Coupled Oscillators
2.1. Description of the Model
Now that we have reviewed the concepts of simple harmonic motion, we are
ready to discuss the problem of the coupled oscillators. As seen in Figure 3, wehave two spring and mass oscillators with stiffness constants k, and masses mcoupled together by a third spring of stiffness kc. Also it should be noted thatkc
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2.2. Finding the General Solution
Now we would like to find the general solution for the motion of the two masses.
Their positions are given by x1(t) and x2(t).
Newtons Second Law
As we did for the spring and mass system, we apply Newtons second law to thetwo mass system to obtain two second order differential equations describing themotion of the masses.
mx
1 + kx1
kc(x2
x1) = 0mx2 + kx2 kc(x1 x2) = 0
We rewrite these in the traditional form.
x1 +
k + kc
m
x1
kc
m
x2 = 0 (9)
x
2+k + kc
mx2 kc
mx1 = 0 (10)
Note that these equations cannot be easily solved as we did for the single springand mass. Each equation has a coupling term, which complicates matters, andprevents us from solving each equation separately. To make these equationseasily solvable, we switch from our coordinates x1 and x2, to coordinates q1,and q2. These new coordinates are known as normal coordinates. To make thischange, we first add the two equations together, and then subtract them, to
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obtain two new equations. Adding Equation 9 and Equation 10, we obtain:
(x1 + x2) +
kc
m (x1 + x2) = 0 (11)
Subtracting Equation 9 and Equation 10, we obtain:
(x1 x2) +
k + 2kc
m
(x1 x2) = 0 (12)
Now we change to our normal coordinates q1 and q2. We will also make asubstitution for 1 and 2, the normal frequencies of the system. It turns outthat these normal frequencies are the frequencies at which the masses oscillatein their normal modes of vibration. This will be further explained later.
q1 = x1 + x2 1 =
k
m(13)
q2 = x1 x2 2 =
k + 2kc
m(14)
Which we substitute into Equation 11 and Equation 12.
q1 + 21q1 = 0 (15)
q2 + 22q2 = 0 (16)
Now we have our equations in a much simpler form. In fact these equations areexactly the same as Equation 3, for the single spring and mass oscillator. Since
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they are not coupled, they can be solved separately in the same way Equation 3was. The solution is therefore:
q1(t) = C1 cos 1t + C2 sin 1t (17)q2(t) = C3 cos 2t + C4 sin 2t (18)
Now we use the relationship
x1 =q1 + q2
2
x2 =q1 q2
2to give the general solution for x1 and x2.
x1(t) = C1 cos 1t + C2 sin 1t + C3 cos 2t + C4 sin 2t (19)
x2(t) = C1 cos 1t + C2 sin 1t C3 cos 2tC4 sin 2t (20)
2.3. Behavior of the System
Now that we have the general solution for our coupled oscillators, we can giveour system some initial conditions, and solve for the motion of the masses. Letus assume that we displace m1 by a distance A, and m2 by a distance B, andthe masses are released from rest. This is the most general case for the massesmotion. So our initial conditions are stated as:
x1(0) = A x
1(0) = 0
x2(0) = B x2(0) = 0
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After substituting these values into Equation 19 and Equation 20 we can solvefor the constants C1, C2, C3, and C4.
C2 = C4 = 0
C1 =A + B
2
C3 =AB
2
So our solution is:
x1 =
A + B
2 cos 1t +
AB
2 cos 2t (21)
x2 =A + B
2cos 1t
AB
2cos 2t (22)
While these equations give us a solution that we can graph to see the behaviorof the masses, we would like to have our solution in a form that shows moreclearly how the masses will behave. First we will consider the motion of the firstmass, x1. We substitute e
it in for cos t.
xc =1
2
(A + B)ei1t + (AB)ei2t
and we remember that x1 = Re(xc). Now we will make a substitution for 1and 2 and use the properties of exponents to further simplify our equation.
=1 + 2
2 =
1 2
2(23)
1 = + 2 = (24)
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Which gives us:
xc =1
2
(A + B)ei(+)t + (AB)ei()t
xc =1
2eit
(A + B)eit + (AB)eit
Using Eulers formula, we expand the equation:
xc =1
2(cos t + i sin t)((A + B)(cos t + i sin t) + (AB)(cos t i sin t))
This is simplified to:
xc = A cos t cos t B sin t sin t + i(A cos t sin t + B cos t sin t)
Now we use the fact that x1 = Re(xc).
x1 = A cos t cos t B sin t sin t (25)
In a similar manner, x2 is found to be:
x2 = B cos t cos t A sin t sin t (26)
With these solutions it is easier to interpret the motion of the masses.
2.4. Normal modes
There are two normal modes of vibration for this system. The symmetric normalmode occurs when both masses are displaced an equal amount in the samedirection and released from rest. The non-symmetric mode occurs when bothmasses are displaced an equal distance from their equilibrium positions but inopposite directions.
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The Symmetric Mode
First we will consider the symmetric mode of vibration where A = B. So our
initial conditions are:
x1(0) = A x
1(0) = 0
x2(0) = A x
2(0) = 0
So Equation 25 and Equation 26 become:
x1 = A(cos t cos t sin t sin t)
x2 = A(cos t cos t sin t sin t)
Notice that x1=x2. We then use the Addition Formula from trigonometry:
x1 = x2 = A cos(t + t)
This is further simplified by replacing (Equation 23) and (Equation 24) with1.
x1 = x2 = A cos 1t (27)
This is simple harmonic motion of frequency 1. This can be understood byrealizing that the coupling spring is never stretched or compressed. In effect wehave two independent spring and mass systems oscillating in SHM with theirnatural frequencies. A graph of the motions of the two masses can be seen inFigure 4. Notice that both masses have exactly the same motion.
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0 2 4 6 8 101
0
1
t
x1
0 2 4 6 8 101
0
1
t
x2
Figure 4: The Symmetric Mode: x1 = x2 = A cos 1t
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The Anti-Symmetric Mode
Now we consider the second normal mode, known as the anti-symmetric mode.
We displace each mass by an equal distance in opposite directions. Our initialconditions are:
x1(0) = A x
1(0) = 0
x2(0) = A x
2(0) = 0
which gives us the equations of motion
x1(t) = A(cos t cos t sin t sin t)
x2(t) = A(cos t cos t sin t sin t)
Noticex1 = x2
The motion of the masses is symmetric but opposite. We replace and with2 and arrive at the solution:
x1 = A cos 2 (28)
x2 = A cos 2 (29)
In the anti-symmetric mode, the masses oscillate with a frequency 2, whilethe masses oscillated with a frequency 1 for the symmetric mode of vibration.2 > 1 (Equation 13 and Equation 14), which means that for the second normalmode, the masses are oscillating more rapidly. This is caused by the couplingspring, which was not affecting the masses for the symmetric mode. A graph ofthe motion can be seen in Figure 5. Notice that the two masses have exactlyopposite motions. Their motion is again SHM of frequency 2.
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0 2 4 6 8 101
0
1
t
x1
0 2 4 6 8 101
0
1
t
x2
Figure 5: The Anti-Symmetric Mode: x1 = x2 = A cos 2
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General Behavior
Now that we have completed our analysis of the two normal modes of the system,we can discuss the more general behavior of the system where no symmetry ispresent. Let us give our system the initial conditions:
x1(0) = A x
1(0) = 0
x2(0) = 0 x
2(0) = 0
By substituting these values into our general solution (Equation 25 and Equa-tion 26) we get:
x1 = A cos t cos t (30)
x2 = A sin t sin t (31)
We can now clearly see that m1 and m2 display a beating phenomenon, where is the beat frequency and is the frequency of the rapid oscillations, andthe amplitude is A. This can be seen in Figure 6. Notice that the peaks of x1correspond to the troughs of x2. Each mass oscillates between the maximum
amplitude A and an amplitude of zero. If we give the system initial conditions ofx1(0) = A and x2(0) = B and the two masses are released from rest, we can see asimilar behavior. This is shown in Figure 7. Again, the peaks ofx1 occur at thesame times as the troughs of x2. However, neither masss oscillations ever reachan amplitude of zero. This is because neither mass started at its equilibriumposition. Here each mass oscillates between the maximum amplitude A and theminimum amplitude B. The energy of the system is continuously oscillating
between m1 and m2, while the total energy of the system remains constant.
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0 20 40 60 801
0
1
t
x1
0 20 40 60 801
0
1
t
x2
Figure 6: x1(0) = A, x2(0) = 0
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0 20 40 60 801
0
1
t
x1
0 20 40 60 801
0
1
t
x2
Figure 7: x1(0) = A, x2(0) = B
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3. Conclusion
Having completed our analysis, we have found the normal modes of the system,
as well as its normal frequencies. And we have determined the general behaviorof the system. We can see that given two different initial displacements for m1and m2, the energy of the system oscillates back and forth between the twomasses continuously, never reaching a steady state of motion for either mass.
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References
[A.P. French, 1971] French, Vibrations and Waves
[Blanchard, Devaney, Hall, 1998] Blanchard, Devaney, Hall, Differential Equa-tions
[Dave Arnold, 1999] Arnold, Ordinary Differential Equations using Matlab
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