An electromagnetic wave propagating in vacuum has electric and magnetic fields given by \(\vec{E}(\vec{x}, t)=\vec{E}_{0} \cos (\vec{k} \cdot \vec{x}-\omega t)\) and \(\vec{B}(\vec{x}, t)=\vec{B}_{0} \cos (\vec{k} \cdot \vec{x}-\omega t)\) where \(\vec{B}_{0}\) is given by \(\vec{B}_{0}=\vec{k} \times \vec{E}_{0} / \omega\) and the wave vector \(\vec{k}\) is perpendicular to both \(\vec{E}_{0}\) and \(\vec{B}_{0} .\) The magnitude of \(\vec{k}\) and the angular frequency \(\omega\) satisfy the dispersion relation, \(\omega /|\vec{k}|=\left(\mu_{0} \epsilon_{0}\right)^{-1 / 2},\) where \(\mu_{0}\) and \(\epsilon_{0}\) are the permeability and permittivity of free space, respectively. Such a wave transports energy in both its electric and magnetic fields. Calculate the ratio of the energy densities of the magnetic and electric fields, \(u_{B} / u_{E}\), in this wave. Simplify your final answer as much as possible.

Short Answer

Expert verified
Answer: The ratio of magnetic to electric field energy densities in an electromagnetic wave propagating in a vacuum is \(\dfrac{\mu_0}{\epsilon_0}\).

Step by step solution

01

1. Write the formula for magnetic field energy density

The energy density of the magnetic field is given by the following expression: \(u_B = \dfrac{1}{2\mu_0} |\vec{B}|^2\)
02

2. Write the formula for electric field energy density

The energy density of the electric field is given by the following expression: \(u_E = \dfrac{1}{2\epsilon_0} |\vec{E}|^2\)
03

3. Calculate the ratio of energy densities

To find the ratio of energy densities (\(\dfrac{u_B}{u_E}\)), we can divide the magnetic field energy density by the electric field energy density: \(\dfrac{u_B}{u_E} = \dfrac{\dfrac{1}{2\mu_0} |\vec{B}|^2}{\dfrac{1}{2\epsilon_0} |\vec{E}|^2}\)
04

4. Simplify the expression using given relationships between \(\vec{B}_0\) and \(\vec{E}_0\)

We can simplify the expression using the relationship \(\vec{B}_0 = \dfrac{\vec{k} \times \vec{E}_0}{\omega}\): \(|\vec{B}_0| = \dfrac{|\vec{k}||\vec{E}_0|}{\omega}\) We will square this equation and then substitute into the expression for the ratio: \(\dfrac{u_B}{u_E} = \dfrac{\dfrac{1}{2\mu_0} \left(\dfrac{|\vec{k}||\vec{E}_0|}{\omega}\right)^2}{\dfrac{1}{2\epsilon_0} |\vec{E}_0|^2}\)
05

5. Simplify the ratio of energy densities using the dispersion relation

We can simplify the expression further by using the dispersion relation, \(\omega / |\vec{k}| = \left(\mu_0 \epsilon_0\right)^{-1 / 2}\): \(\omega = |\vec{k}| \left(\mu_0 \epsilon_0\right)^{-1 / 2}\) Now, we will square this equation and substitute it into the expression for the ratio: \(\dfrac{u_B}{u_E} = \dfrac{\dfrac{1}{2\mu_0} \left(\dfrac{|\vec{k}||\vec{E}_0|}{|\vec{k}|\left(\mu_0 \epsilon_0\right)^{-1 / 2}}\right)^2}{\dfrac{1}{2\epsilon_0} |\vec{E}_0|^2}\)
06

6. Final simplification

With careful simplification, we reach the final expression for the ratio of energy densities: \(\dfrac{u_B}{u_E} = \dfrac{\mu_0}{\epsilon_0}\) The ratio of magnetic to electric field energy densities in the electromagnetic wave propagating in a vacuum is \(\dfrac{\mu_0}{\epsilon_0}\).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Magnetic Field Energy Density
Understanding the concept of magnetic field energy density (\textbf{u}_B) is essential for grasping the dynamics of electromagnetic waves. Energy density refers to the amount of energy stored in a given system or region of space per unit volume. In the context of a magnetic field, the energy density is expressed mathematically as:
\[\begin{equation} u_B = \frac{1}{2\mu_0} |\vec{B}|^2\end{equation}\] Where \(\mu_0\) represents the permeability of free space and \(|\vec{B}|\) is the magnitude of the magnetic field vector. This quantity becomes significant when analyzing how much energy is carried by the magnetic component of an electromagnetic wave. In vacuum, the energy is solely due to the fields as there are no particles to carry kinetic or potential energy.
Furthermore, the factor of \(\frac{1}{2}\) arises from the averaging over a full cycle of the sinusoidal wave function, which gives us a clearer picture of the 'steady state' energy in the wave. This consideration is important when comparing the magnetic energy density to the electric energy density in an electromagnetic wave.
To put this into a real-world context, consider that all electronic devices that emit electromagnetic waves, like radios or MRI machines, rely on the principles of magnetic field energy density to operate effectively. In these devices, control over the energy transferred by the electromagnetic waves is crucial for their functionality.
Electric Field Energy Density
Parallel to the concept of magnetic field energy density, the electric field energy density (\textbf{u}_E) plays a symmetric role in the context of electromagnetic waves. It quantifies the amount of electrical energy stored per unit volume and is given by:
\[\begin{equation} u_E = \frac{1}{2\epsilon_0} |\vec{E}|^2\end{equation}\]Here, \(\epsilon_0\) is the permittivity of free space, and \(|\vec{E}|\) is the magnitude of the electric field vector. Just as with magnetic field energy density, the prefactor of \(\frac{1}{2}\) accounts for the average energy stored over a complete cycle of the wave.
Understanding electric field energy density is crucial for various applications, including the transmission of power and information through the electromagnetic spectrum. For instance, the intensity of light, one form of electromagnetic radiation, depends on the electric field energy density; thereby, it has direct implications for technologies such as optical fibers and lasers.
The comparison of electric and magnetic field energy densities also reveals insights into the interplay between electric and magnetic fields as they propagate through space. It's this balance of energies that governs the stable propagation of light and radio waves through the vacuum of space.
Dispersion Relation
The dispersion relation is a fundamental concept linking the properties of wave-like phenomena to their propagation through different mediums. In the vacuum, the dispersion relation for electromagnetic waves is expressed as:
\[\begin{equation} \frac{\omega}{|\vec{k}|} = \left(\mu_0 \epsilon_0\right)^{-1 / 2}\end{equation}\] This relationship connects the angular frequency \(\omega\) and the wave vector \(|\vec{k}|\), which are intrinsic properties of the wave, to the physical constants \(\mu_0\) and \(\epsilon_0\), which characterize the medium—in this case, the vacuum.
In simpler terms, the dispersion relation tells us how the phase speed of the wave depends on its frequency. For electromagnetic waves in a vacuum, this relation reveals that all frequencies travel at the same speed—the speed of light. This is because the vacuum is non-dispersive and does not separate light into different colors as a prism would do to visible light.
The concept of dispersion is crucial for understanding wave behavior in various disciplinary contexts beyond vacuum, such as in fiber optics, acoustics, and even quantum mechanics. For instance, the color spectrum displayed when light passes through a glass prism is a direct consequence of the dispersion relation changing with the medium, revealing its pivotal role in the study of wave phenomena.
Wave Propagation in Vacuum
Wave propagation in vacuum is characterized by the motion of waves through empty space, devoid of any medium. For electromagnetic waves, this process is governed by Maxwell's equations, which describe how electric and magnetic fields evolve and propagate in space and time.
In a vacuum, electromagnetic waves propagate without losing energy to the medium, allowing them to travel at the speed of light (approximately \( 3 \times 10^8 \) meters per second). This occurs because there are no charged particles that can absorb the wave's energy and no material to cause scattering or absorption. The result is a clean, unimpeded path for the electromagnetic wave represented by the equation:
\[\begin{equation} c = \left(\mu_0 \epsilon_0\right)^{-1 / 2}\end{equation}\] Where 'c' is the speed of light. Electromagnetic wave propagation forms the basis of many modern technologies—GPS systems, telecommunications, and space exploration, to name a few, all leverage this core principle of physics.
This concept of wave propagation also allows us to understand astronomical phenomena, as light from distant stars and galaxies travels through the vacuum of space to reach us, revealing the nature and motion of these celestial bodies. Hence, wave propagation in a vacuum is not just a foundational concept in physics but also an essential element in explaining the observable universe.

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Most popular questions from this chapter

A solenoid with 200 turns and a cross-sectional area of \(60 \mathrm{~cm}^{2}\) has a magnetic field of \(0.60 \mathrm{~T}\) along its axis. If the field is confined within the solenoid and changes at a rate of \(0.20 \mathrm{~T} / \mathrm{s}\), the magnitude of the induced potential difference in the solenoid will be a) 0.0020 V. b) \(0.02 \mathrm{~V}\). c) 0.001 V. d) \(0.24 \mathrm{~V}\).

A \(100 .-V\) battery is connected in series with a \(500 .-\Omega\) resistor. According to Faraday's Law of Induction, current can never change instantaneously, so there is always some "stray" inductance. Suppose the stray inductance is \(0.200 \mu \mathrm{H}\). How long will it take the current to build up to within \(0.500 \%\) of its final value of \(0.200 \mathrm{~A}\) after the resistor is con- nected to the battery?

A metal loop has an area of \(0.100 \mathrm{~m}^{2}\) and is placed flat on the ground. There is a uniform magnetic field pointing due west, as shown in the figure. This magnetic field initially has a magnitude of \(0.123 \mathrm{~T}\), which decreases steadily to \(0.075 \mathrm{~T}\) during a period of \(0.579 \mathrm{~s}\). Find the potential difference induced in the loop during this time.

A rectangular conducting loop with dimensions \(a\) and \(b\) and resistance \(R\), is placed in the \(x y\) -plane. A magnetic field of magnitude \(B\) passes through the loop. The magnetic field is in the positive \(z\) -direction and varies in time according to \(B=B_{0}\left(1+c_{1} t^{3}\right),\) where \(c_{1}\) is a constant with units of \(1 / \mathrm{s}^{3}\) What is the direction of the current induced in the loop, and what is its value at \(t=1 \mathrm{~s}\) (in terms of \(a, b, R, B_{0},\) and \(\left.c_{1}\right) ?\)

Which of the following will induce a current in a loop of wire in a uniform magnetic field? a) decreasing the strength of the field b) rotating the loop about an axis parallel to the field c) moving the loop within the field d) all of the above e) none of the above

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