Starting from the displacement equation
The motion is defined the moment we write the NCERT displacement equation (Eq. 13.4):
$$x(t) = A\cos(\omega t + \varphi)$$
Here $A$ is the amplitude, $\omega$ the angular frequency, and $(\omega t + \varphi)$ the phase. Everything in this topic is obtained by differentiating this one expression with respect to time — velocity is the first derivative, acceleration the second. There is no new physics to assume; the velocity and acceleration are forced on us by the displacement. If you are still building the displacement equation itself, revisit simple harmonic motion first.
Velocity in SHM
Differentiating the displacement once with respect to time (NCERT Eq. 13.10) gives the instantaneous velocity (Eq. 13.9):
$$v(t) = \frac{dx}{dt} = -A\omega\sin(\omega t + \varphi)$$
The negative sign reflects that, while the displacement is positive and increasing toward the extreme, the cosine is falling, so the velocity points back toward the mean position. The same result follows from the reference-circle picture in SHM and uniform circular motion, where $v$ is the projection of the tangential speed $\omega A$.
To get velocity as a function of position rather than time, eliminate the trigonometric term. Using $\sin^2 + \cos^2 = 1$ with $\cos(\omega t+\varphi) = x/A$:
$$v = \pm\,\omega\sqrt{A^2 - x^2}$$
The speed relation reads off its own extremes. At the mean position $x = 0$, the square root is largest, so the speed peaks at $v_{\max} = A\omega$. At the extremes $x = \pm A$, the square root vanishes and the body is momentarily at rest. The body is therefore fastest precisely where the restoring force is zero, and stationary precisely where the force is greatest.
Acceleration in SHM
Differentiating the velocity with respect to time (NCERT Eq. 13.12) gives the acceleration (Eq. 13.11):
$$a(t) = \frac{dv}{dt} = -\omega^2 A\cos(\omega t + \varphi) = -\omega^2 x$$
The second form, $a = -\omega^2 x$, is the heart of the chapter. NCERT highlights the property directly: for $x > 0$, $a < 0$; for $x < 0$, $a > 0$. Whatever the value of $x$ between $-A$ and $A$, the acceleration is always directed toward the centre. This linear, opposing dependence of $a$ on $x$ is the operational definition of SHM and the bridge to the force law $F = -m\omega^2 x = -kx$.
Its magnitude is largest at the extremes: $a_{\max} = \omega^2 A$ at $x = \pm A$, and zero at the mean position $x = 0$ — the exact opposite arrangement to the speed.
Master comparison: x, v, a
The three quantities share one period $T$ and one amplitude scale, differing only in their peak values, where those peaks occur, and their phase. Read them together rather than memorising in isolation.
| Quantity | As function of time | As function of x | Maximum value | Where maximum | Where zero | Phase vs x |
|---|---|---|---|---|---|---|
Displacement x |
$A\cos(\omega t+\varphi)$ | $x$ | $A$ | Extremes $x=\pm A$ | Mean $x=0$ | Reference (0) |
Velocity v |
$-A\omega\sin(\omega t+\varphi)$ | $\pm\omega\sqrt{A^2-x^2}$ | $v_{\max}=A\omega$ | Mean $x=0$ | Extremes $x=\pm A$ | Leads by $\pi/2$ |
Acceleration a |
$-\omega^2 A\cos(\omega t+\varphi)$ | $-\omega^2 x$ | $a_{\max}=\omega^2 A$ | Extremes $x=\pm A$ | Mean $x=0$ | Antiphase ($\pi$) |
Two ratios fall straight out of the maxima and are worth carrying into the exam hall: $\dfrac{a_{\max}}{v_{\max}} = \dfrac{\omega^2 A}{\omega A} = \omega$, so $\omega = a_{\max}/v_{\max}$ and $T = 2\pi\,v_{\max}/a_{\max}$. Given any two of $A$, $\omega$, $v_{\max}$, $a_{\max}$, the rest follow.
The x-t, v-t and a-t graphs
Setting $\varphi = 0$ for clarity, NCERT writes the trio as $x = A\cos\omega t$, $v = -A\omega\sin\omega t$, $a = -\omega^2 A\cos\omega t$. All three vary sinusoidally with the same period $T$; only their amplitudes and phases differ. Plotted one above the other on a shared time axis, the shifts become visible at a glance.
The geometry of Figure 1 is the whole story. Where displacement peaks at $+A$ (turning point), velocity crosses zero and acceleration dips to $-\omega^2 A$ — the body is stopped and being pulled hardest back. Where displacement crosses zero (mean position), velocity reaches its $\pm A\omega$ extreme and acceleration is zero — fastest, force-free.
The phase relationships
The shifts in Figure 1 are exact and quotable. Writing each curve as a cosine of an advanced phase:
$$v = A\omega\cos\!\left(\omega t + \varphi + \tfrac{\pi}{2}\right), \qquad a = \omega^2 A\cos\!\left(\omega t + \varphi + \pi\right)$$
So velocity leads displacement by $\pi/2$, and acceleration is in antiphase ($\pi$) with displacement. Velocity and acceleration in turn differ by $\pi/2$. NCERT states it in the same words: with respect to the displacement plot, the velocity plot has a phase difference of $\pi/2$ and the acceleration plot a phase difference of $\pi$.
The v–x ellipse
Plotting velocity against displacement removes time entirely. Squaring the speed relation, $v^2 = \omega^2(A^2 - x^2)$, and rearranging:
$$\frac{x^2}{A^2} + \frac{v^2}{A^2\omega^2} = 1$$
This is the standard equation of an ellipse — semi-axis $A$ along the displacement direction and semi-axis $A\omega$ along the velocity direction. The particle traces this closed loop once per period: it sweeps clockwise, touching $v=\pm A\omega$ at the mean position and $x = \pm A$ at the turning points.
The a–x straight line
Acceleration against displacement is the simplest plot of all. Because $a = -\omega^2 x$ is linear in $x$, the graph is a straight line through the origin with slope $-\omega^2$. The negative slope encodes the restoring nature — acceleration and displacement always have opposite signs.
The line $a = -\omega^2 x$ becomes Newton's law $F = -kx$ once you multiply by mass — see the force law for SHM for the $k = m\omega^2$ connection.
Worked example
A body oscillates with SHM according to $x = 5\cos\!\left(2\pi t + \tfrac{\pi}{4}\right)$ (SI units). At $t = 1.5\ \text{s}$, find the (a) displacement, (b) speed and (c) acceleration of the body.
Read off the constants. Amplitude $A = 5\ \text{m}$, angular frequency $\omega = 2\pi\ \text{s}^{-1}$, so period $T = 2\pi/\omega = 1\ \text{s}$. The phase at $t = 1.5\ \text{s}$ is $2\pi(1.5) + \pi/4 = 3\pi + \pi/4$.
(a) Displacement. $x = 5\cos(3\pi + \pi/4) = 5(-0.707) = -3.535\ \text{m}$.
(b) Speed. Using $v = -A\omega\sin(\omega t+\varphi)$: $v = -(5)(2\pi)\sin(3\pi+\pi/4) = -(5)(2\pi)(-0.707) = 10\pi(0.707) \approx 22\ \text{m s}^{-1}$.
(c) Acceleration. Using $a = -\omega^2 x$: $a = -(2\pi)^2(-3.535) = -(2\pi)^2(-3.535) \approx 140\ \text{m s}^{-2}$. Note how using $a = -\omega^2 x$ — rather than re-evaluating a trig function — turns part (c) into a one-line substitution of the part (a) answer.
Velocity & acceleration in SHM, in one breath
- Differentiate $x = A\cos(\omega t+\varphi)$ once for $v = -A\omega\sin(\omega t+\varphi)$, again for $a = -\omega^2 A\cos(\omega t+\varphi) = -\omega^2 x$.
- Speed in terms of position: $v = \pm\omega\sqrt{A^2-x^2}$ — the $\pm$ matters; it is a speed, not a velocity.
- $v_{\max} = A\omega$ at the mean position; $a_{\max} = \omega^2 A$ at the extremes. Opposite ends, always.
- Phase: velocity leads $x$ by $\pi/2$; acceleration is $\pi$ out of phase with $x$; $v$ and $a$ differ by $\pi/2$.
- $v$ vs $x$ is an ellipse $\dfrac{x^2}{A^2} + \dfrac{v^2}{A^2\omega^2} = 1$; $a$ vs $x$ is a straight line of slope $-\omega^2$.
- Shortcut: $\omega = a_{\max}/v_{\max}$ and $T = 2\pi v_{\max}/a_{\max}$.