Special Relativity Recap for Electromagnetism
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You should be comfortable with the Lorentz transformation for spacetime coordinates and the basic postulates of special relativity. Familiarity with the vector nature of electric and magnetic fields in classical electrodynamics is assumed.
Why this matters
Special relativity is not merely a correction to electromagnetism; it is the framework that explains why the two are inseparable.
In previous units, we treated electric and magnetic fields as distinct entities governed by separate laws. However, when we examine how these fields transform between inertial frames moving at relativistic speeds, we discover that what appears as a purely electric field in one frame may manifest as a combination of electric and magnetic fields in another. This lecture serves as a critical orientation, bridging the gap between the static laws of Electromagnetism I and the unified tensor formulation we will encounter in the next lecture. By understanding the kinematic constraints imposed by the speed of light, we prepare the conceptual ground for viewing the electromagnetic field as a single, covariant object.
The Relativistic Worldview
Imagine two observers, Alice and Bob, moving relative to each other at a significant fraction of the speed of light. Alice holds a stationary charge. She sees only an electric field radiating outward. Bob, however, sees that charge moving. According to classical intuition, a moving charge should generate a magnetic field. Yet, Alice insists there is no magnetic field. Who is right? The answer is that both are correct within their own inertial frames. The electric and magnetic fields are not absolute properties of the charge itself but are frame-dependent components of a single underlying physical reality. This is the core insight of special relativity applied to electromagnetism: the separation of \(\mathbf{E}\) and \(\mathbf{B}\) is an artifact of the observer's state of motion. The fields mix under Lorentz transformations, much like space and time mix to form spacetime. This unification resolves apparent paradoxes in classical electrodynamics and ensures that the laws of physics remain consistent for all inertial observers.
Lorentz Transformations of Fields
To quantify this mixing, we apply the Lorentz transformation to the field components. Consider a boost along the \(x\)-axis with velocity \(v\). The components of the electric and magnetic fields parallel to the direction of motion remain unchanged, while the perpendicular components mix. This behaviour is analogous to how spatial coordinates transform in special relativity. The transformation laws ensure that the invariants of the electromagnetic field, \(E^2 - c^2B^2\) and \(\mathbf{E} \cdot \mathbf{B}\), remain consistent across frames. These relations are derived from the requirement that Maxwell's equations retain their form in all inertial frames, a principle known as Lorentz covariance. By mastering these transformation rules, we gain the ability to predict how fields appear to different observers without needing to solve the full set of Maxwell's equations in each frame.
Here, \(\gamma = 1/\sqrt{1 - v^2/c^2}\) is the Lorentz factor. Notice the symmetry: electric fields generate magnetic fields and vice versa, scaled by the velocity and the speed of light. This coupling is the mathematical expression of the physical unity of electromagnetism.
Invariants and Physical Meaning
While the individual components of \(\mathbf{E}\) and \(\mathbf{B}\) change between frames, certain combinations remain invariant. These invariants provide a frame-independent description of the electromagnetic field. The most important invariant is the difference between the squared magnitudes of the electric and magnetic fields. When \(\mathbf{E} \cdot \mathbf{B} = 0\) and this quantity is positive, there exists a frame where the magnetic field vanishes, implying the field is purely electric in that frame. If it is negative (again with \(\mathbf{E} \cdot \mathbf{B} = 0\)), there exists a frame where the electric field vanishes, implying the field is purely magnetic. This classification helps us understand the physical nature of the field independent of the observer's motion. Another invariant is the dot product of the electric and magnetic fields, and a field for which both invariants vanish is called null; electromagnetic waves are the standard example.
These invariants are crucial for analyzing radiation and field configurations. For instance, in a plane electromagnetic wave, both invariants vanish, indicating that the electric and magnetic fields are perpendicular with \(E = cB\) in all inertial frames. This property is a direct consequence of the relativistic structure of the field and cannot be fully appreciated without the framework of special relativity.
Preparation for Covariance
The next step in our journey is to express these transformation laws in a compact, coordinate-free manner. We will introduce the electromagnetic field tensor, a four-dimensional object that encapsulates all six components of the electric and magnetic fields. This tensor formulation allows us to write Maxwell's equations in a form that is explicitly Lorentz covariant, meaning they look the same in every inertial frame. This is not just a mathematical convenience; it reveals the deep connection between electromagnetism and the geometry of spacetime. By treating the field as a tensor, we align electromagnetism with the broader framework of relativistic field theory, setting the stage for understanding gauge symmetry and the quantum nature of the photon. This lecture thus serves as the final conceptual bridge before we dive into the formalism of the field tensor.
A common misconception is that the magnetic field is a "relativistic correction" to the electric field, implying it is less fundamental. In reality, both fields are equally fundamental components of the electromagnetic field tensor. The distinction between electric and magnetic is frame-dependent, and neither is more "real" than the other. This perspective is essential for understanding phenomena such as the magnetic force between currents, which can be viewed as a relativistic effect of electrostatic forces in a different frame. C
Worked example
Problem. A point charge is at rest in frame \(S\), so \(\mathbf{B} = 0\) there. At a point directly above it the field is \(\mathbf{E} = E_0\hat{\mathbf{y}}\) with \(E_0 = 1.0 \times 10^{4}\ \mathrm{V\,m^{-1}}\). Frame \(S'\) moves at \(v = 0.6c\) along \(+x\). Find \(\mathbf{E}'\) and \(\mathbf{B}'\) at that event, and check both invariants.
- Lorentz factor: \(\gamma = 1/\sqrt{1 - 0.6^2} = 1/0.8 = 1.25\).
- Electric field: \(E'_x = E_x = 0\), \(E'_y = \gamma(E_y - vB_z) = 1.25\,E_0 = 1.25 \times 10^{4}\ \mathrm{V\,m^{-1}}\), \(E'_z = 0\).
- Magnetic field: \(B'_y = \gamma(B_y + vE_z/c^2) = 0\) and \(B'_z = \gamma(B_z - vE_y/c^2) = -1.25 \times 0.6\,E_0/c = -0.75\,E_0/c = -2.5 \times 10^{-5}\ \mathrm{T}\).
- Sign check: in \(S'\) the charge moves along \(-x\), and \(\mathbf{v}\times\mathbf{E}/c^2\) with \(\mathbf{v} = -v\hat{\mathbf{x}}\) points along \(-\hat{\mathbf{z}}\), as found.
- Invariants: \(E'^2 - c^2B'^2 = E_0^2(1.25^2 - 0.75^2) = E_0^2\), the same as in \(S\); \(\mathbf{E}' \cdot \mathbf{B}' = 0\), also unchanged.
Units check. \(E_0/c\) has units \(\mathrm{V\,m^{-1}}/(\mathrm{m\,s^{-1}}) = \mathrm{V\,s\,m^{-2}} = \mathrm{T}\).
Three quick tests
- What is the value of the invariant \(I_1 = E^2 - c^2 B^2\) for a plane electromagnetic wave?
Answer
It is zero, because \(E = cB\) in a plane wave, so \(E^2 - c^2 B^2 = 0\). - If a frame exists where the magnetic field is zero, what can you say about the invariant \(I_1\)?
Answer
\(I_1\) must be positive, as \(E^2 - c^2(0)^2 = E^2 > 0\). - Why is the electromagnetic field tensor necessary for a covariant formulation of Maxwell's equations?
Answer
It allows the six field components to be grouped into a single object that transforms linearly under Lorentz transformations, ensuring the equations retain their form in all inertial frames.
Problem set for PU-204 →
Each derivation in this unit ends with five graded problems with full solutions.
Lecture notes checked line by line by the editor; every number in the worked example was recomputed.