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15 Flashcards in this deck.
Transverse Waves: In transverse waves, the oscillations occur perpendicular to the direction of wave propagation. Imagine a rope being flicked up and down; the waves move horizontally while the displacement is vertical. Common examples include electromagnetic waves (such as light) and waves on a string.
Longitudinal Waves: In longitudinal waves, the oscillations occur parallel to the direction of wave propagation. Sound waves in air are a primary example, where compressions and rarefactions move in the same direction as the wave travels.
For transverse waves, the displacement ($y$) can be described as: $$ y(x, t) = A \sin(kx - \omega t + \phi) $$ where $A$ is amplitude, $k = \frac{2\pi}{\lambda}$ is the wave number, $\omega = 2\pi f$ is the angular frequency, and $\phi$ is the phase constant.
For longitudinal waves, the pressure variation ($P$) can be modeled similarly: $$ P(x, t) = P_0 \sin(kx - \omega t + \phi) $$ where $P_0$ is the maximum pressure variation.
Only transverse waves, such as light waves, can be polarized. For instance, polarized sunglasses reduce glare by allowing only certain orientations of light waves to pass through.
Starting with Newton's second law and Hooke's law, we can derive the wave equation for transverse waves on a string:
$$ \frac{\partial^2 y}{\partial t^2} = \frac{T}{\mu} \frac{\partial^2 y}{\partial x^2} $$where $T$ is the tension in the string and $\mu$ is the linear mass density. This partial differential equation describes how transverse waves propagate through the string.
For longitudinal waves in a medium, the wave equation is derived from the equations of motion and the relation between pressure and density:
$$ \frac{\partial^2 \xi}{\partial t^2} = \frac{B}{\rho} \frac{\partial^2 \xi}{\partial x^2} $$where $\xi$ is the displacement, $B$ is the bulk modulus, and $\rho$ is the density of the medium. This equation characterizes the propagation of longitudinal waves, such as sound, in the medium.
For transverse waves on a string with tension $T$ and linear mass density $\mu$, the dispersion relation is:
$$ \omega = \sqrt{\frac{T}{\mu}} k $$indicating that wave speed ($v = \omega / k$) is constant and independent of frequency. However, in more complex media, wave speed can vary with frequency, leading to dispersion.
For longitudinal waves in gases, the speed of sound depends on temperature and is given by:
$$ v = \sqrt{\frac{\gamma R T}{M}} $$where $\gamma$ is the adiabatic index, $R$ is the universal gas constant, $T$ is the temperature, and $M$ is the molar mass. This shows that in gases, wave speed is influenced by thermodynamic properties.
The power ($P$) transported by a wave is given by:
$$ P = \frac{1}{2} \mu \omega^2 A^2 v $$for transverse waves on a string, where $\mu$ is the linear mass density, $\omega$ is the angular frequency, $A$ is the amplitude, and $v$ is the wave speed.
For longitudinal waves, the power can be expressed as:
$$ P = \frac{1}{2} \rho \omega^2 A^2 v $$where $\rho$ is the density of the medium. These equations illustrate how power depends on medium properties, frequency, amplitude, and speed.
The reflection coefficient ($R$) and transmission coefficient ($T$) for transverse waves at a boundary are given by:
$$ R = \frac{Z_2 - Z_1}{Z_2 + Z_1} $$ $$ T = \frac{2Z_2}{Z_2 + Z_1} $$where $Z_1$ and $Z_2$ are the impedances of the first and second media, respectively.
Similarly, for longitudinal waves, the coefficients are calculated based on acoustic impedances, affecting sound transmission and reflection through different materials.
Both transverse and longitudinal waves can exhibit interference, which is fundamental in applications like noise-canceling headphones (longitudinal) and optical coatings (transverse).
For transverse waves on a string fixed at both ends, standing waves form with nodes and antinodes, determined by the string's length and wave speed. Similarly, longitudinal standing waves occur in air columns in musical instruments, affecting sound production.
Example Problem: A string fixed at both ends has a length of 2 meters and supports the third harmonic mode of vibration. If the tension in the string is 50 N and its linear mass density is 0.01 kg/m, calculate the frequency of the third harmonic.
Solution: For a string fixed at both ends, the wavelength of the nth harmonic is:
$$ \lambda_n = \frac{2L}{n} $$where $L = 2$ m and $n = 3$. Thus, $$ \lambda_3 = \frac{2 \times 2}{3} = \frac{4}{3} \text{ m} $$
The wave speed ($v$) on the string is: $$ v = \sqrt{\frac{T}{\mu}} = \sqrt{\frac{50}{0.01}} = \sqrt{5000} \approx 70.71 \text{ m/s} $$
The frequency ($f$) of the third harmonic is: $$ f = \frac{v}{\lambda} = \frac{70.71}{\frac{4}{3}} \approx 53.03 \text{ Hz} $$>
Therefore, the frequency of the third harmonic is approximately 53.03 Hz.
Aspect | Transverse Waves | Longitudinal Waves |
---|---|---|
Oscillation Direction | Perpendicular to propagation | Parallel to propagation |
Examples | Light waves, electromagnetic waves, waves on a string | Sound waves, seismic P-waves, compression waves in springs |
Medium Requirements | Requires a medium that can sustain shear stress (usually solids) | Can travel through solids, liquids, and gases |
Energy Transmission | Energy is transferred perpendicular to wave direction | Energy is transferred in the same direction as wave propagation |
Polarization | Can be polarized | Cannot be polarized |
Wave Speed Dependence | Typically independent of frequency in ideal conditions | Can depend on medium properties like temperature and pressure |
1. Mnemonic for Wave Types: "Transverse Thinks Perpendicular" helps remember that transverse waves oscillate perpendicular to their direction of travel.
2. Visual Aids: Draw diagrams showing the oscillation directions relative to wave propagation to differentiate wave types effectively.
3. Practice Problems: Regularly solve problems involving both wave types to reinforce your understanding and application skills for the AP exam.
1. Gravitational waves, predicted by Einstein's theory of general relativity, are transverse waves that ripple through the fabric of spacetime itself.
2. The auroras (Northern and Southern Lights) are caused by transverse electromagnetic waves interacting with Earth's magnetosphere.
3. In certain metamaterials, scientists have engineered waves that exhibit both transverse and longitudinal characteristics, leading to unique wave manipulation capabilities.
Mistake 1: Confusing the direction of oscillation with the direction of wave propagation.
Incorrect: Believing that in longitudinal waves, oscillations occur perpendicular to wave travel.
Correct: Recognizing that in longitudinal waves, oscillations are parallel to wave propagation.
Mistake 2: Assuming all waves can be polarized.
Incorrect: Trying to polarize sound waves.
Correct: Understanding that only transverse waves, like light, can undergo polarization.
Mistake 3: Ignoring medium requirements when analyzing wave behavior.
Incorrect: Applying transverse wave equations to sound waves in gases.
Correct: Using longitudinal wave principles for sound in various media.