E12 Linear Physical Systems Analysis
March 5, 2026

The second-order differential equation \[\ddot{x} + a \dot{x} + b x = 0\] usually has the solution \(x(t) =e^{s t}\) where \(s\) satisfies the characteristic equation \[s^2 + a s + b = 0 \implies s_{1,2} = \frac{-a \pm \sqrt{a^2-4b}}{2}\]
\[x(t) = K_1 e^{s_1 t} + K_2 e^{s_2 t} \qquad K_1,K_2 \in \mathbb{R}\]
| Case 1a: \(s_1,s_2 < 0\) | Case 1b: \(s_1< 0<s_2\) | Case 1c: \(s_1, s_2 > 0\) |
|---|---|---|
| Both roots negative | One positive, one negative | Both roots positive |
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\[ \begin{aligned} x(t) &= P e^{s_1 t} + \overline{P} e^{s_2 t} \qquad P \in \mathbb{C} \\ &= e^{rt} \left( A \cos \omega t + B \cos \omega t \right) \qquad A,B \in \mathbb{R} \\ s_{1,2} &= r \pm i \omega \end{aligned} \]
| Case 2a: \(r < 0\) | Case 2b: \(r = 0\) | Case 2c: \(r > 0\) |
|---|---|---|
| Real part negative | Real part zero | Real part positive |
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\[ x(t) = (C_1 + C_2t) e^{rt} \]
| Case 3a: \(r < 0\) | Case 3b: \(r = 0\) |
|---|---|
| Nonzero repeated roots | Repeated roots at zero |
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The differential equation \[m \ddot{x} + b \dot{x} + k x = 0\]
admits solutions of the form \(e^{st}\) where \(s\) must be a root of the characteristic polynomial \[m s^2 + b s + k.\] The roots will, in general, be complex, and are given by \[s_{1,2} = \frac{-b \pm \sqrt{b^2-4mk}}{2m}.\] Then, the solution can usually be written as \[x(t) = A e^{s_1t} + B e^{s_2 t}\] where \(A\) and \(B\) are, in general, complex.
If \(b^2-4mk >0\), the two roots are real and are given by the real numbers \[s_{1,2} = \frac{-b \pm \sqrt{b^2-4mk}}{2m}\] and the solution can be written as \[\boxed{x(t) = K_1 e^{s_1 t} + K_2 e^{s_2 t}} \qquad \text{with }K_1,K_2,s_1,s_2 \in \mathbb{R}\]
If \(b^2-4mk <0\), the two roots are complex and are given by the complex numbers \[ s_{1,2} = \frac{-b \pm \sqrt{b^2-4mk}}{2m} = r \pm i \omega, \] \[ \text{ where } \quad r = -\frac{b}{2m}, \quad \omega = \frac{1}{2m}\sqrt{4mk-b^2}\] and the solution can be written as \[x(t) = P e^{s_1 t} + \overline{P} e^{s_2 t} \qquad \text{with }P,s_1,s_2 \in \mathbb{C}\] or, alternatively, as \[\boxed{x(t) = e^{rt} \left( K_3 \cos \omega t + K_4 \sin \omega t \right)} \qquad \text{with }K_3,K_4,r,\omega \in \mathbb{R}\] or, alternatively, as \[x(t) = e^{rt} C_1 \cos \left( \omega t + \phi_1 \right) \qquad \text{with }C_1,\phi_1,r,\omega \in \mathbb{R}\] or, alternatively, as \[x(t) = e^{rt} C_2 \sin \left( \omega t + \phi_2 \right) \qquad \text{with }C_2,\phi_2,r,\omega \in \mathbb{R}\]
If \(b^2-4mk =0\), the two roots are repeated \[ s_1 = s_2 = \frac{-b \pm \sqrt{{b^2-4mk}}}{2m} = -b/2m = r\] and the solution can be written as (take MATH 43/44 to see why) \[\boxed{x(t) = (C_3 + C_4t) e^{rt}} \qquad \text{with }C_3,C_4,r \in \mathbb{R}\]
Let’s examine solutions to \[m \ddot{x} + b \dot{x} + k x = 0, \qquad x(0) = 1, \dot{x}(0) = 0\] With \(k=2\), \(m=3\), and \(b\) allowed to vary from \(0\) to \(6\).
| Value of \(b\) | Motion |
|---|---|
| \(0.0\) | ![]() |
| \(0.5\) | ![]() |
| \(1.0\) | ![]() |
| \(1.5\) | ![]() |
| \(2.0\) | ![]() |
| \(2.5\) | ![]() |
| \(3.0\) | ![]() |
| \(3.5\) | ![]() |
| \(4.0\) | ![]() |
| \(4.5\) | ![]() |
| \(5.0\) | ![]() |
| \(5.5\) | ![]() |
| \(6.0\) | ![]() |
The system \(m \ddot{x} + b \dot{x} + kx = f(t)\) has a free response that depends on the roots of the characteristic polynomial \(m s^2 + b s + k\).
In general, these roots are complex, so we can plot them on the complex plane.

We’ve seen that something special happens when the damping coefficient \(b\) crosses some critical value. What is this critical value?
\(m \ddot{x} + b \dot{x} + kx = 0\) has the solutions \(e^{st}\) when \[m s^2 + b s + k = 0 \implies s = \frac{-b \pm \sqrt{b^2-4mk}}{2m}\]
Recall that if — and only if — \(s \in \mathbb{C}\), then \(e^{st}\) will oscillate in time! (\(e^{i\theta} = \cos \theta + ...\))
There is a critical value of \(b = \sqrt{4mk}\) that demarcates qualitatively different behavior.
| Zeta \(\zeta\) | \(b\) | Name | Typical Motion and roots of \(m s^2 + b s + k\) |
|---|---|---|---|
| \(\zeta = 0\) | \(b=0\) | Undamped | ![]() |
| \(\zeta < 1\) | \(b < \sqrt{4mk}\) | Underdamped | ![]() |
| \(\zeta = 1\) | \(b = \sqrt{4mk}\) | Critically damped | ![]() |
| \(\zeta > 1\) | \(b > \sqrt{4mk}\) | Overdamped | ![]() |
Recall that the natural frequency is given by \(\sqrt{k/m}\). From now on, we will call this the ‘undamped natural frequency’ and use the symbol \(\boxed{\omega_n}\).
\[ m \ddot{x} + b \dot{x} + kx = 0 \] \[ \phantom{m} \ddot{x} + \frac{b}{m} \dot{x} + \frac{k}{m}x = 0 \] \[ \phantom{m} \ddot{x} + \overbrace{\frac{{\color{green}{b}}}{m} \cdot \frac{\sqrt{m}}{{\color{green}{\sqrt{m}}}} \cdot \frac{\sqrt{k}}{{\color{green}{\sqrt{k}}}} \cdot \frac{2}{{\color{green}{2}}}}^{b/m} \dot{x} + \left(\frac{\sqrt{k}}{\sqrt{m}}\right)^2 x = 0 \] \[ \phantom{m} \ddot{x} + \frac{{\color{green}{b}}}{{\color{brown}{\sqrt{m}}}} \cdot \frac{{1}}{{\color{green}{\sqrt{m}}}} \cdot \frac{{\color{brown}{\sqrt{k}}}}{{\color{green}{\sqrt{k}}}} \cdot \frac{2}{{\color{green}{2}}} \dot{x} + \left(\frac{{\color{brown}{\sqrt{k}}}}{{\color{brown}{\sqrt{m}}}}\right)^2 x = 0 \] \[ {\color{green}{\frac{b}{2\sqrt{mk}}}} \text{ is the damping ratio } \zeta \] \[ {\color{brown}{\sqrt{\frac{k}{m}}}} \text{ is the undamped natural frequency } \omega_n \] \[ \implies \boxed{\ddot{x} + 2 {\color{green}{\zeta}}{\color{brown}{\omega_n}} x + {\color{brown}{\omega^2_n}} x = 0} \]
We know that a system governed by \(m \ddot{x} + kx = 0\) has the free response \[ \begin{aligned} \textstyle x(t) &= \textstyle A \cos \left( t \sqrt{k/m} \right) + B \sin \left( t \sqrt{k/m} \right) \\ &= A \cos \omega_n t + B \sin \omega_n t \end{aligned} \] where \(A, B \in \mathbb{R}\) can be found using the initial conditions.
At what frequency does the system governed by \[m \ddot{x} + b \dot{x} + kx = 0 \tag{1}\] oscillate naturally?
Hint: Equation 1 is identical to \(\ddot{x} + 2 \zeta \omega_n x + \omega_n^2 x = 0\)
Underdamped second order systems (with \(\zeta < 1\)) have a time constant that characterizes how quickly or slowly they decay.

Solutions are multiples of \(x(t) = e^{({\color{blue}{r}} \pm i {\color{brown}{\omega}} )t}\).
When \(m \ddot{x} + b \dot{x} + k x = 0\) is written in the form \[\ddot{x} + 2 \zeta \omega_n x + \omega_n^2 x = 0,\]
the roots of the characteristic polynomial \[s^2 + 2 \zeta \omega_n s + \omega_n^2\] are \[s = - \zeta \omega_n \pm i \omega_n \sqrt{1-\zeta^2}\]
with the solution for \(x(t)\) given by \[x(t) = e^{- {\color{blue}{\zeta \omega_n}}t} \left( A \cos \left( t\, {\color{brown}{\omega_n \sqrt{1-\zeta^2}}} \right) + B \sin \left( t\, {\color{brown}{\omega_n \sqrt{1-\zeta^2}}} \right) \right)\]
Consider a spring-mass system starting from \(x = 0, \dot{x}=0\) that is subjected to a step function force \(f(t) = u_s(t)\)
\[\ddot{x} + 2 \zeta \omega_n \dot{x} + \omega_n^2 x = u_s(t)\]

Q. How does a spring-mass-damper system respond to a step-function force applied to it?
Approach:
\[ m \ddot{x} + b \dot{x} + k x = u_s(t) \] \[ \mathcal{L}\left[ m \ddot{x} + b \dot{x} + k x \right] = \mathcal{L} \left[ u_s(t) \right] \] \[ m s^2 X + b s X + k X = \frac{1}{s} \] \[ \left( m s^2 + b s + k \right) X = \frac{1}{s} \] \[ X(s) = \frac{1}{s} \frac{1}{ m s^2 + b s + k} \]
Consider a spring-mass system starting from \(x = 0, \dot{x}=0\) that is subjected to a impulse function force \(f(t) = \delta(t)\)
\[\ddot{x} + 2 \zeta \omega_n \dot{x} + \omega_n^2 x = \delta(t)\]

Q. How does a spring-mass-damper system respond to a Dirac Delta-function force applied to it?
Approach:
\[ m \ddot{x} + b \dot{x} + k x = \delta(t) \] \[ \mathcal{L}\left[ m \ddot{x} + b \dot{x} + k x \right] = \mathcal{L} \left[ \delta(t) \right] \] \[ m s^2 X + b s X + k X = 1 \] \[ \left( m s^2 + b s + k \right) X = 1 \] \[ X(s) = \frac{1}{ m s^2 + b s + k} \]
E12 • Spring 2026 • Lecture 14 • March 5, 2026