Simple Harmonic Motion (SHM) and Waves can be challenging to revise for NEET Physics because they involve several equations, graphs and special cases. Questions may test your understanding of displacement, velocity, acceleration, energy changes, time periods, wave speed and standing-wave patterns. Memorising formulas without knowing when to apply them can also make numerical problems difficult to solve.
To prepare effectively, you need to connect each equation with its underlying concept and identify the conditions in which it applies. The following notes explain the key concepts through concise pointers, formula tables and comparisons, helping you revise important topics and practise NEET-level questions.
Simple Harmonic Motion is a type of periodic motion in which the restoring force or acceleration is directly proportional to displacement from the mean position and acts in the opposite direction.
|
Type of motion |
Meaning |
Example |
|
Periodic motion |
Motion that repeats after equal intervals of time |
Earth revolving around the Sun |
|
Oscillatory motion |
To-and-fro motion about a mean position |
A swinging pendulum |
|
Simple Harmonic Motion |
Oscillatory motion with restoring force proportional to displacement and directed towards the mean position |
An ideal spring-block system |
Conditions for SHM:
The body moves about a stable mean position.
The restoring force acts towards the mean position.
The restoring force is proportional to displacement: (F\propto -x).
Damping is neglected in ideal SHM.
For a particle oscillating with amplitude (A), angular frequency (\omega) and phase constant (\phi):
|
Quantity |
Equation |
Key point |
|
Displacement |
(x=A\sin(\omega t+\phi)) |
Depends on time and phase |
|
Velocity |
(v=A\omega\cos(\omega t+\phi)) |
Maximum at the mean position |
|
Acceleration |
(a=-\omega^2x) |
Always directed towards the mean position |
|
Restoring force |
(F=-m\omega^2x) |
Opposite to displacement |
|
Angular frequency |
(\omega=2\pi f=\frac{2\pi}{T}) |
Measured in rad/s |
|
Frequency |
(f=\frac{1}{T}) |
Number of oscillations per second |
|
Maximum speed |
(v_{\max}=A\omega) |
At the mean position |
|
Maximum acceleration |
(a_{\max}=A\omega^2) |
At the extreme positions |
The displacement equation may also be written using cosine. The choice depends on the initial position and phase of the particle.
|
Quantity |
Mean position ((x=0)) |
Extreme position ((x=\pm A)) |
|
Displacement |
Zero |
Maximum magnitude |
|
Velocity |
Maximum magnitude |
Zero |
|
Acceleration |
Zero |
Maximum magnitude |
|
Restoring force |
Zero |
Maximum magnitude |
|
Kinetic energy |
Maximum |
Zero |
|
Potential energy |
Minimum |
Maximum |
Remember:
The particle does not remain at rest at the mean position; it crosses it with maximum speed.
At an extreme position, the particle momentarily stops before reversing direction.
Acceleration and restoring force always point towards the mean position.
In ideal SHM, the total mechanical energy remains constant. Kinetic energy and potential energy keep converting into each other during oscillation.
|
Energy or quantity |
Formula |
|
Total energy |
(E=\frac12m\omega^2A^2) |
|
Potential energy |
(U=\frac12m\omega^2x^2) |
|
Kinetic energy |
(K=\frac12m\omega^2(A^2-x^2)) |
|
Kinetic energy using velocity |
(K=\frac12mv^2) |
|
Total energy using spring constant |
(E=\frac12kA^2) |
|
Potential energy using spring constant |
(U=\frac12kx^2) |
Here, (m) is mass, (k) is the spring constant, (A) is amplitude and (x) is displacement from the mean position.
|
Graph |
Relationship |
Shape or behaviour |
|
DisplacementтАУtime |
(x=A\sin(\omega t+\phi)) |
Sinusoidal |
|
VelocityтАУtime |
(v=A\omega\cos(\omega t+\phi)) |
Sinusoidal, phase-different from displacement |
|
AccelerationтАУtime |
(a=-\omega^2x) |
Opposite in phase to displacement |
|
Potential energyтАУdisplacement |
(U\propto x^2) |
Upward-opening parabola |
|
Kinetic energyтАУdisplacement |
(K\propto A^2-x^2) |
Downward-opening parabola |
|
Total energyтАУdisplacement |
(E=\frac12m\omega^2A^2) |
Constant horizontal line |
|
System |
Time period |
Important condition |
|
Spring-block system |
(T=2\pi\sqrt{\frac{m}{k}}) |
Ideal spring and small oscillations |
|
Simple pendulum |
(T=2\pi\sqrt{\frac{l}{g}}) |
Small angular displacement |
|
Physical pendulum |
(T=2\pi\sqrt{\frac{I}{mgd}}) |
Small oscillations |
|
Two masses connected by a spring |
(T=2\pi\sqrt{\frac{\mu}{k}}) |
(\mu=\frac{m_1m_2}{m_1+m_2}) is the reduced mass |
For a physical pendulum, (I) is the moment of inertia about the pivot and (d) is the distance between the pivot and the centre of mass.
|
Combination |
Equivalent spring constant |
|
Springs in series |
(\frac{1}{k_{\text{eq}}}=\frac{1}{k_1}+\frac{1}{k_2}) |
|
Two springs in series |
(k_{\text{eq}}=\frac{k_1k_2}{k_1+k_2}) |
|
Springs in parallel |
(k_{\text{eq}}=k_1+k_2) |
NEET tip: For a spring-block system, (T\propto\sqrt{m}) and (T\propto\frac{1}{\sqrt{k}}). Increasing the mass increases the time period, while increasing the spring constant decreases it.
A wave transfers energy from one point to another without the overall transfer of matter. The particles of the medium may oscillate as the disturbance travels through it.
|
Wave type |
Particle motion |
Example |
|
Transverse wave |
Perpendicular to the direction of propagation |
Waves on a stretched string |
|
Longitudinal wave |
Parallel to the direction of propagation |
Sound in air |
|
Mechanical wave |
Requires a material medium |
Sound and waves on a string |
|
Electromagnetic wave |
Does not require a material medium |
Light waves |
|
Quantity |
Formula |
Meaning |
|
Wave speed |
(v=f\lambda) |
Speed equals frequency multiplied by wavelength |
|
Frequency |
(f=\frac{1}{T}) |
Oscillations per second |
|
Angular frequency |
(\omega=2\pi f) |
Angular rate of oscillation |
|
Wave number |
(k=\frac{2\pi}{\lambda}) |
Spatial frequency |
|
Wave equation travelling in (+x) direction |
(y=A\sin(\omega t-kx+\phi)) |
One common phase convention |
|
Wave equation travelling in (-x) direction |
(y=A\sin(\omega t+kx+\phi)) |
One common phase convention |
In the wave equation, (A) is amplitude, (\omega) is angular frequency, (k) is wave number and (\phi) is the initial phase.
The speed of a transverse wave on a stretched string depends on the tension and linear mass density.
[
v=\sqrt{\frac{F_T}{\mu}}
]
Here, (F_T) is the tension in the string and (\mu) is the mass per unit length.
Key points:
Greater tension increases wave speed.
Greater linear mass density decreases wave speed.
For a given medium under fixed conditions, wave speed is determined by the medium, while frequency is determined by the source.
When a wave enters another medium, its frequency remains unchanged, but its speed and wavelength may change.
For a sinusoidal transverse wave on a string:
[
P_{\text{avg}}=\frac12\mu\omega^2A^2v
]
The average power depends on the square of the amplitude and angular frequency, along with the medium's linear mass density and wave speed.
Standing waves form when two waves of the same frequency and amplitude travel in opposite directions and superpose. The resulting pattern contains fixed points called nodes and points of maximum oscillation called antinodes.
|
Feature |
Node |
Antinode |
|
Displacement amplitude |
Zero |
Maximum |
|
Particle motion |
No oscillation in the ideal standing-wave pattern |
Maximum oscillation |
|
Separation between adjacent points of the same type |
Node to next node: (\lambda/2) |
Antinode to next antinode: (\lambda/2) |
|
Distance between adjacent node and antinode |
(\lambda/4) |
(\lambda/4) |
Both ends of the string are nodes. The allowed frequencies are:
[
f_n=\frac{nv}{2L},\qquad n=1,2,3,\ldots
]
|
Mode |
Frequency |
Wavelength |
|
Fundamental |
(f_1=\frac{v}{2L}) |
(\lambda_1=2L) |
|
Second harmonic |
(f_2=\frac{v}{L}=2f_1) |
(\lambda_2=L) |
|
Third harmonic |
(f_3=\frac{3v}{2L}=3f_1) |
(\lambda_3=\frac{2L}{3}) |
|
(n)th harmonic |
(f_n=nf_1) |
(\lambda_n=\frac{2L}{n}) |
Here, (L) is the vibrating length of the string and (v) is the wave speed.
Organ pipes are classified according to their end conditions. An open end is a displacement antinode, while a closed end is a displacement node.
|
Pipe type |
Fundamental frequency |
Allowed frequencies |
|
Open at both ends |
(f_1=\frac{v}{2L}) |
(f_n=\frac{nv}{2L}), (n=1,2,3,\ldots) |
|
Closed at one end |
(f_1=\frac{v}{4L}) |
(f_n=\frac{(2n-1)v}{4L}), (n=1,2,3,\ldots) |
Important differences:
An open pipe supports all harmonics: (f_1,2f_1,3f_1,\ldots).
A pipe closed at one end supports only odd harmonics: (f_1,3f_1,5f_1,\ldots).
For the same length and wave speed, the fundamental frequency of an open pipe is twice that of a closed pipe.
For a pipe with an open end, the displacement antinode lies slightly outside the physical opening. This effect is accounted for using end correction.
|
Concept |
Formula or key point |
|
End correction for one open end |
(e\approx0.6r) |
|
Effective length of an open pipe |
(L_{\text{eff}}=L+2e) |
|
Effective length of a pipe closed at one end |
(L_{\text{eff}}=L+e) |
|
Resonance |
Occurs when the driving frequency matches a natural frequency of the system |
Here, (r) is the radius of the pipe. These end-correction relations are approximate and apply to common circular-pipe cases.
Sound is a mechanical wave, so it requires a medium to travel. Its speed depends on the properties of that medium and the conditions under which the sound propagates.
|
Medium or condition |
Formula or relationship |
|
General relation |
(v=\sqrt{\frac{B}{\rho}}) |
|
Ideal gas |
(v=\sqrt{\frac{\gamma P}{\rho}}) |
|
Ideal gas using temperature |
(v=\sqrt{\frac{\gamma RT}{M}}) |
|
Speed in air with Celsius temperature (t) |
(v\approx331+0.6t\ \text{m/s}) |
Here, (B) is the bulk modulus, (\rho) is density, (\gamma) is the ratio of specific heats, (P) is pressure, (R) is the universal gas constant, (T) is absolute temperature and (M) is molar mass.
Remember:
In a given gas, sound speed increases with absolute temperature.
Sound generally travels faster in solids than in gases, though the exact speed depends on the material and wave type.
Frequency determines pitch, while amplitude and intensity are related to perceived loudness.
|
Characteristic |
What it indicates |
Main factor |
|
Pitch |
How high or low a sound seems |
Frequency |
|
Loudness |
How loud or soft a sound seems |
Intensity and the sensitivity of the ear |
|
Quality or timbre |
Helps distinguish sounds from different sources |
Waveform and harmonic content |
|
Intensity |
Sound power passing through a unit area |
Power and area |
For a point source radiating uniformly in a free field, intensity decreases with the square of the distance:
[
I\propto\frac{1}{r^2}
]
This inverse-square relationship assumes negligible absorption and reflection.
Beats occur when two sound waves of slightly different frequencies superpose. The resulting sound alternates between louder and softer because of periodic changes in amplitude.
|
Quantity |
Formula |
||
|
Beat frequency |
(f_b= |
f_1-f_2 |
) |
|
Number of beats per second |
Equal to the absolute difference between the two frequencies |
||
|
Approximate beat period |
(T_b=\frac{1}{f_b}), when (f_b\neq0) |
Tuning fork questions:
If beats are heard when a tuning fork is sounded with a known frequency, the unknown frequency may differ from the known frequency by the beat frequency.
If wax is added to a tuning fork, its mass increases and its frequency generally decreases.
If a tuning fork is filed, its mass decreases and its frequency generally increases.
Use the direction of the frequency change, along with the beat count, to identify the unknown frequency.
Interference occurs when two or more waves superpose. Depending on their phase difference, they may reinforce or weaken each other.
|
Condition |
Path difference |
Phase difference |
Result |
|
Constructive interference |
(\Delta x=n\lambda) |
(\Delta\phi=2n\pi) |
Maximum intensity |
|
Destructive interference |
(\Delta x=(2n+1)\frac{\lambda}{2}) |
(\Delta\phi=(2n+1)\pi) |
Minimum intensity for equal amplitudes |
Here, (n=0,1,2,\ldots). The simple conditions assume coherent waves with the same frequency.
For two waves with amplitudes (A_1) and (A_2) and phase difference (\Delta\phi):
[
A_R=\sqrt{A_1^2+A_2^2+2A_1A_2\cos\Delta\phi}
]
For coherent waves in the same medium, intensity is proportional to the square of amplitude. Therefore:
[
I\propto A_R^2
]
For equal amplitudes (A):
|
Interference condition |
Resultant amplitude |
|
Constructive |
(A_R=2A) |
|
Destructive |
(A_R=0) |
Complete cancellation occurs only when the interfering waves have equal amplitudes and are exactly out of phase.
Use this combined table for a final formula check before solving numerical questions.
|
Topic |
Formula |
|
SHM displacement |
(x=A\sin(\omega t+\phi)) |
|
SHM acceleration |
(a=-\omega^2x) |
|
Maximum SHM speed |
(v_{\max}=A\omega) |
|
SHM total energy |
(E=\frac12m\omega^2A^2) |
|
Spring-block time period |
(T=2\pi\sqrt{\frac{m}{k}}) |
|
Simple pendulum time period |
(T=2\pi\sqrt{\frac{l}{g}}) |
|
Wave speed |
(v=f\lambda) |
|
Wave speed on a string |
(v=\sqrt{\frac{F_T}{\mu}}) |
|
String fundamental frequency |
(f_1=\frac{v}{2L}) |
|
Open-pipe fundamental frequency |
(f_1=\frac{v}{2L}) |
|
Closed-pipe fundamental frequency |
(f_1=\frac{v}{4L}) |
|
Beat frequency |
(f_b= |
|
Constructive interference |
(\Delta x=n\lambda) |
|
Destructive interference |
(\Delta x=(2n+1)\frac{\lambda}{2}) |
|
Sound intensity from a point source |
(I\propto\frac{1}{r^2}) |
Revise Simple Harmonic Motion (SHM) and Waves for NEET by focusing on motion, energy changes, time periods, wave speed, standing waves, organ pipes, beats and interference. Review the key equations, understand when each formula applies, and practise numerical questions to strengthen your conceptual understanding and improve problem-solving accuracy.
